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<!doctype book PUBLIC "-//Davenport//DTD DocBook V3.0//EN" [
]>
<book>
<bookinfo>
<date>$Date: 1999/12/04 19:08:16 $</date>
<title>The Linux System Administrators' Guide</title>
<subtitle>Version 0.6.2</subtitle>
<author>
<firstname>Lars</firstname>
<surname>Wirzenius</surname>
<affiliation>
<address>
<email>liw@iki.fi</email>
</address>
</affiliation>
</author>
<author>
<firstname>Joanna</firstname>
<surname>Oja</surname>
<affiliation>
<address>
<email>viu@iki.fi</email>
</address>
</affiliation>
</author>
<abstract> <para>An introduction to system administration of a Linux
system for novices.</para> </abstract>
<legalnotice>
<para>Copyright 1993--1998 Lars Wirzenius.</para>
<para>Trademarks are owned by their owners.</para>
<para>Permission is granted to make and distribute verbatim
copies of this manual provided the copyright notice and this
permission notice are preserved on all copies.</para>
<para>Permission is granted to process the document source
code through TeX or other formatters and print the results,
and distribute the printed document, provided the printed
document carries copying permission notice identical to this one,
including the references to where the source code can be found
and the official home page.</para>
<para>Permission is granted to copy and distribute modified
versions of this manual under the conditions for verbatim
copying, provided that the entire resulting derived work is
distributed under the terms of a permission notice identical to
this one. </para>
<para>Permission is granted to copy and distribute translations
of this manual into another language, under the above conditions
for modified versions.</para>
<para>The author would appreciate a notification of modifications,
translations, and printed versions. Thank you.</para>
</legalnotice>
</bookinfo>
<toc></toc>
<preface>
<title>Dedication</title>
<para>This place is dedicated to a future dedication.</para>
</preface>
<preface>
<title>Source and pre-formatted versions available</title>
<para>The source code and and other machine readable formats
of this book can be found on the Internet via anonymous
FTP at the Linux Documentation Project home page <ulink
url="http://sunsite.unc.edu/LDP/">http://sunsite.unc.edu/LDP/</ulink>,
or at the home page of this book at <ulink
url="http://www.iki.fi/viu/linux/sag/">http://www.iki.fi/viu/linux/sag/</ulink>.
Available are at least PostScript and TeX .DVI formats.</para>
</preface>
<chapter>
<title>Introduction</title>
<blockquote><para><quote>In the beginning, the file was without
form, and void; and emptiness was upon the face of the bits.
And the Fingers of the Author moved upon the face of the
keyboard. And the Author said, Let there be words, and there
were words.</quote></para></blockquote>
<para>This manual, the Linux System Administrators' Guide,
describes the system administration aspects of using Linux.
It is intended for people who know next to nothing about system
administration (as in ``what is it?''), but who have already
mastered at least the basics of normal usage. This manual also
doesn't tell you how to install Linux; that is described in the
Installation and Getting Started document. See below for more
information about Linux manuals.</para>
<para>System administration is all the things that one has to
do to keep a computer system in a useable shape. It includes
things like backing up files (and restoring them if necessary),
installing new programs, creating accounts for users (and deleting
them when no longer needed), making certain that the filesystem
is not corrupted, and so on. If a computer were, say, a house,
system administration would be called maintenance, and would
include cleaning, fixing broken windows, and other such things.
System administration is not called maintenance, because that
would be too simple.
<footnote><para>There are some people who
<emphasis>do</emphasis> call it that, but that's
just because they have never read this manual, poor
things.</para></footnote>
</para>
<para>The structure of this manual is such that many of the
chapters should be usable independently, so that if you need
information about, say, backups, you can read just that chapter.
This hopefully makes the book easier to use as a reference manual,
and makes it possible to read just a small part when needed,
instead of having to read everything. However, this manual is
first and foremost a tutorial, and a reference manual only as
a lucky coincidence.</para>
<para>This manual is not intended to be used completely by itself.
Plenty of the rest of the Linux documentation is also important
for system administrators. After all, a system administrator is
just a user with special privileges and duties. A very important
resource are the manual pages, which should always be consulted
when a command is not familiar.</para>
<para>While this manual is targeted at Linux, a general principle
has been that it should be useful with other UNIX based operating
systems as well. Unfortunately, since there is so much variance
between different versions of UNIX in general, and in system
administration in particular, there is little hope to cover
all variants. Even covering all possibilities for Linux is
difficult, due to the nature of its development.</para>
<para>There is no one official Linux distribution, so different
people have different setups, and many people have a setup they
have built up themselves. This book is not targeted at any
one distribution, even though I use the Debian GNU/Linux system
almost exclusively. When possible, I have tried to point out
differences, and explain several alternatives.</para>
<para>I have tried to describe how things work, rather than just
listing ``five easy steps'' for each task. This means that there
is much information here that is not necessary for everyone,
but those parts are marked as such and can be skipped if you
use a preconfigured system. Reading everything will, naturally,
increase your understanding of the system and should make using
and administering it more pleasant.</para>
<para>Like all other Linux related development, the work was
done on a volunteer basis: I did it because I thought it might
be fun and because I felt it should be done. However, like all
volunteer work, there is a limit to how much effort I have been
able to spend, and also on how much knowledge and experience
I have. This means that the manual is not necessarily as good
as it would be if a wizard had been paid handsomely to write it
and had spent a few years to perfect it. I think, of course,
that it is pretty nice, but be warned.</para>
<para>One particular point where I have cut corners is that I
have not covered very thoroughly many things that are already
well documented in other freely available manuals. This applies
especially to program specific documentation, such as all the
details of using <command>mkfs</command>. I only describe the
purpose of the program, and as much of its usage as is necessary
for the purposes of this manual. For further information,
I refer the gentle reader to these other manuals. Usually,
all of the referred to documentation is part of the full Linux
documentation set.</para>
<para>Lars has tried to make this manual as good as possible
and I would like, as a current maintainer, to keep up the good
work. I would really like to hear from you if you have any
ideas on how to make it better. Bad language, factual errors,
ideas for new areas to cover, rewritten sections, information
about how various UNIX versions do things, I am interested in
all of it. My contact information is available via the World
Wide Web at <ulink url="http://www.iki.fi/viu/">
http://www.iki.fi/viu/</ulink>.
</para>
<para>Many people have helped me with this book, directly or
indirectly. I would like to especially thank Matt Welsh for
inspiration and LDP leadership, Andy Oram for getting me to work
again with much-valued feedback, Olaf Kirch for showing me that it
can be done, and Adam Richter at Yggdrasil and others for showing
me that other people can find it interesting as well.</para>
<para>Stephen Tweedie, H. Peter Anvin, Remy Card, Theodore
Ts'o, and Stephen Tweedie have let me borrow their work (and
thus make the book look thicker and much more impressive):
a comparison between the xia and ext2 filesystems, the device
list and a description of the ext2 filesystem. These aren't
part of the book any more. I am most grateful for this, and
very apologetic for the earlier versions that sometimes lacked
proper attribution.</para>
<para>In addition, I would like to thank Mark Komarinski for
sending his material in 1993 and the many system administration
columns in Linux Journal. They are quite informative and
inspirational.</para>
<para>Many useful comments have been sent by a large number
of people. My miniature black hole of an archive doesn't let
me find all their names, but some of them are, in alphabetical
order: Paul Caprioli, Ales Cepek, Marie-France Declerfayt,
Dave Dobson, Olaf Flebbe, Helmut Geyer, Larry Greenfield and
his father, Stephen Harris, Jyrki Havia, Jim Haynes, York Lam,
Timothy Andrew Lister, Jim Lynch, Michael J. Micek, Jacob Navia,
Dan Poirier, Daniel Quinlan, Jouni K Seppnen, Philippe Steindl,
G.B. Stotte. My apologies to anyone I have forgotten.</para>
<para>META need to add typographical conventsions and LDP blurb
here.</para>
<sect1>
<title>The Linux Documentation Project</title>
<para>The Linux Documentation Project, or LDP, is a loose team
of writers, proofreaders, and editors who are working together
to provide complete documentation for the Linux operating system.
The overall coordinator of the project is Greg Hankins.</para>
<para>This manual is one in a set of several being
distributed by the LDP, including a Linux Users' Guide,
System Administrators' Guide, Network Administrators' Guide,
and Kernel Hackers' Guide. These manuals are all available
in source format, .dvi format, and postscript output
by anonymous FTP from sunsite.unc.edu, in the directory
<filename>/pub/Linux/docs/LDP</filename>.</para>
<para>We encourage anyone with a penchant for writing or editing
to join us in improving Linux documentation. If you have
Internet e-mail access, you can contact Greg Hankins at
<email>gregh@sunsite.unc.edu</email>.</para>
</sect1>
</chapter>
<chapter>
<title>Overview of a Linux System</title>
<blockquote><para><quote>God looked over everything he
had made, and saw that it was very good. </quote> (Genesis
1:31)</para></blockquote>
<para>This chapter gives an overview of a Linux system. First,
the major services provided by the operating system are described.
Then, the programs that implement these services are described
with a considerable lack of detail. The purpose of this chapter
is to give an understanding of the system as a whole, so that
each part is described in detail elsewhere.</para>
<sect1>
<title>Various parts of an operating system</title>
<para>A UNIX operating system consists
of a <glossterm>kernel</glossterm> and some
<glossterm>system programs</glossterm>. There are also some
<glossterm>application programs</glossterm> for doing work.
The kernel is the heart of the operating system.
<footnote><para>In fact, it is often mistakenly considered
to be the operating system itself, but it is not.
An operating system provides many more services than a
plain kernel.</footnote>
It keeps track of files on the disk, starts programs and runs
them concurrently, assigns memory and other resources to various
processes, receives packets from and sends packets to the network,
and so on. The kernel does very little by itself, but it provides
tools with which all services can be built. It also prevents
anyone from accessing the hardware directly, forcing everyone
to use the tools it provides. This way the kernel provides
some protection for users from each other. The tools provided
by the kernel are used via <glossterm>system calls<glossterm>;
see manual page section 2 for more information on these. </para>
<para>The system programs use the tools provided by the kernel to
implement the various services required from an operating system.
System programs, and all other programs, run `on top of the
kernel', in what is called the <glossterm>user mode</glossterm>.
The difference between system and application programs is
one of intent: applications are intended for getting useful
things done (or for playing, if it happens to be a game),
whereas system programs are needed to get the system working.
A word processor is an application; <command>telnet</command>
is a system program. The difference is often somewhat blurry,
however, and is important only to compulsive categorizers.</para>
<para>An operating system can also contain compilers and their
corresponding libraries (GCC and the C library in particular under
Linux), although not all programming languages need be part of
the operating system. Documentation, and sometimes even games,
can also be part of it. Traditionally, the operating system has
been defined by the contents of the installation tape or disks;
with Linux it is not as clear since it is spread all over the
FTP sites of the world.</para>
</sect1>
<sect1>
<title>Important parts of the kernel</title>
<para>The Linux kernel consists of several important parts: process
management, memory management, hardware device drivers, filesystem
drivers, network management, and various other bits and pieces.
<xref linkend="kerneloverview">
shows some of them.</para>
<figure id="kerneloverview" float="1">
<title>Some of the more important parts of the Linux kernel</title>
<graphic fileref="overview-kernel"></graphic>
</figure>
<para>Probably the most important parts of the kernel (nothing else
works without them) are memory management and
process management. Memory management takes care of assigning
memory areas and swap space areas to processes, parts of the
kernel, and for the buffer cache. Process management creates
processes, and implements multitasking by switching the
active process on the processor.</para>
<para>At the lowest level, the kernel contains a hardware device
driver for each kind of hardware it supports. Since the world is
full of different kinds of hardware, the number of hardware device
drivers is large. There are often many otherwise similar pieces
of hardware that differ in how they are controlled by software.
The similarities make it possible to have general classes of
drivers that support similar operations; each member of the class
has the same interface to the rest of the kernel but differs in
what it needs to do to implement them. For example, all disk
drivers look alike to the rest of the kernel, i.e., they all
have operations like `initialize the drive', `read sector N',
and `write sector N'.</para>
<para>Some software services provided by the kernel itself have
similar properties, and can therefore be abstracted into classes.
For example, the various network protocols have been abstracted
into one programming interface, the BSD socket library. Another
example is the <glossterm>virtual filesystem</glossterm> (VFS)
layer that abstracts the filesystem operations away from their
implementation. Each filesystem type provides an implementation
of each filesystem operation. When some entity tries to use
a filesystem, the request goes via the VFS, which routes the
request to the proper filesystem driver.</para>
</sect1>
<sect1>
<title>Major services in a UNIX system</title>
<para>This section describes some of the more important UNIX
services, but without much detail. They are described more
thoroughly in later chapters.</para>
<sect2>
<title><command>init</command></title>
<para>The single most important service in a UNIX system is
provided by <command>init</command>. <command>init</command>
is started as the first process of every UNIX system, as the last
thing the kernel does when it boots. When <command>init</command>
starts, it continues the boot process by doing various startup
chores (checking and mounting filesystems, starting daemons,
etc).</para>
<para>The exact list of things that <command>init</command>
does depends on which flavor it is; there are several to choose
from. <command>init</command> usually provides the concept of
<glossterm>single user mode</glossterm>, in which no one can
log in and root uses a shell at the console; the usual mode is
called <glossterm>multiuser mode</glossterm>. Some flavors
generalize this as <glossterm>run levels</glossterm>; single
and multiuser modes are considered to be two run levels, and
there can be additional ones as well, for example, to run X on
the console.</para>
<para>In normal operation, <command>init</command> makes sure
<command>getty</command> is working (to allow users to log in),
and to adopt orphan processes (processes whose parent has died; in
UNIX <emphasis>all</emphasis> processes <emphasis>must</emphasis>
be in a single tree, so orphans must be adopted).</para>
<para>When the system is shut down, it is <command>init</command>
that is in charge of killing all other processes, unmounting all
filesystems and stopping the processor, along with anything else
it has been configured to do.</para>
</sect2>
<sect2>
<title>Logins from terminals</title>
<para>Logins from terminals (via serial lines) and the console
(when not running X) are provided by the <command>getty</command>
program. <command>init</command> starts a separate instance
of <command>getty</command> for each terminal for which
logins are to be allowed. <command>getty</command> reads
the username and runs the <command>login</command> program,
which reads the password. If the username and password
are correct, <command>login</command> runs the shell.
When the shell terminates, i.e., the user logs out, or when
<command>login</command> terminated because the username
and password didn't match, <command>init</command> notices
this and starts a new instance of <command>getty</command>.
The kernel has no notion of logins, this is all handled by the
system programs.</para>
</sect2>
<sect2>
<title>Syslog</title>
<para>The kernel and many system programs produce error, warning, and
other messages. It is often important that these messages can
be viewed later, even much later, so they should be written to
a file. The program doing this is <command>syslog</command>. It can be
configured to sort the messages to different files according to
writer or degree of importance. For example, kernel messages
are often directed to a separate file from the others, since
kernel messages are often more important and need to be read
regularly to spot problems.</para>
</sect2>
<sect2>
<title>Periodic command execution: <command>cron</command> and
<command>at</command></title>
<para>Both users and system administrators often need
to run commands periodically. For example, the system
administrator might want to run a command to clean the
directories with temporary files (<filename>/tmp</filename>
and <filename>/var/tmp</filename>) from old files, to keep the
disks from filling up, since not all programs clean up after
themselves correctly.</para>
<para>The <command>cron</command> service is set up to do this.
Each user has a <filename>crontab</filename> file, where he
lists the commands he wants to execute and the times they should
be executed. The <command>cron</command> daemon takes care of
starting the commands when specified.</para>
<para>The <command>at</command> service is similar to
<command>cron</command>, but it is once only: the command is
executed at the given time, but it is not repeated.</para>
</sect2>
<sect2>
<title>Graphical user interface</title>
<para>UNIX and Linux don't incorporate the user interface
into the kernel; instead, they let it be implemented by user
level programs. This applies for both text mode and graphical
environments.</para>
<para>This arrangement makes the system more flexible, but has
the disadvantage that it is simple to implement a different
user interface for each program, making the system harder to
learn.</para>
<para>The graphical environment primarily used with Linux
is called the X Window System (X for short). X also does
not implement a user interface; it only implements a window
system, i.e., tools with which a graphical user interface can
be implemented. The three most popular user interface styles
implemented over X are Athena, Motif, and Open Look.</para>
</sect2>
<sect2>
<title>Networking</title>
<para>Networking is the act of connecting two or more computers
so that they can communicate with each other. The actual methods
of connecting and communicating are slightly complicated, but
the end result is very useful.</para>
<para>UNIX operating systems have many networking features.
Most basic services (filesystems, printing, backups, etc) can
be done over the network. This can make system administration
easier, since it allows centralized administration, while
still reaping in the benefits of microcomputing and distributed
computing, such as lower costs and better fault tolerance.</para>
<para>However, this book merely glances at networking; see the
<citetitle>Linux Network Administrators' Guide</citetitle> for
more information, including a basic description of how networks
operate.</para>
</sect2>
<sect2>
<title>Network logins</title>
<para>Network logins work a little differently than normal logins.
There is a separate physical serial line for each terminal via
which it is possible to log in. For each person logging in via
the network, there is a separate virtual network connection,
and there can be any number of these.
<footnote><para>Well, at least there can be many. Network
bandwidth still being a scarce resource, there is still
some practical upper limit to the number of concurrent
logins via one network connection. </para></footnote>
It is therefore not possible to run a separate
<command>getty</command> for each possible virtual connection.
There are also several different ways to log in via a network,
<command>telnet</command> and <command>rlogin</command> being
the major ones in TCP/IP networks.</para>
<para>Network logins have, instead of a herd of
<command>getty</command>s, a single daemon per way of logging in
(<command>telnet</command> and <command>rlogin</command> have
separate daemons) that listens for all incoming login attempts.
When it notices one, it starts a new instance of itself to
handle that single attempt; the original instance continues to
listen for other attempts. The new instance works similarly
to <command>getty</command>.</para>
</sect2>
<sect2>
<title>Network file systems</title>
<para>One of the more useful things that can be done with
networking services is sharing files via a <glossterm>network
file system</glossterm>. The one usually used is called the
Network File System, or NFS, developed by Sun.</para>
<para>With a network file system any file operations done by
a program on one machine are sent over the network to another
computer. This fools the program to think that all the files
on the other computer are actually on the computer the program
is running on. This makes information sharing extremely simple,
since it requires no modifications to programs.</para>
</sect2>
<sect2>
<title>Mail</title>
<para>Electronic mail is usually the most important method for
communicating via computer. An electronic letter is stored in a
file using a special format, and special mail programs are used
to send and read the letters.</para>
<para>Each user has an <glossterm>incoming mailbox</glossterm>
(a file in the special format), where all new mail is stored.
When someone sends mail, the mail program locates the receiver's
mailbox and appends the letter to the mailbox file. If the
receiver's mailbox is in another machine, the letter is sent to
the other machine, which delivers it to the mailbox as it best
sees fit.</para>
<para>The mail system consists of many programs. The
delivery of mail to local or remote mailboxes is done by one
program (the <glossterm>mail transfer agent</glossterm> or
<glossterm>MTA</glossterm>, e.g., <command>sendmail</command>
or <command>smail</command>), while the programs users use
are many and varied (<glossterm>mail user agent</glossterm>
or <glossterm>MUA</glossterm>, e.g., <command>pine</command>
or <command>elm</command>). The mailboxes are usually stored
in <filename>/var/spool/mail</filename>.</para>
</sect2>
<sect2>
<title>Printing</title>
<para>Only one person can use a printer at one time, but it is
uneconomical not to share printers between users. The printer is
therefore managed by software that implements a <glossterm>print
queue</glossterm>: all print jobs are put into a queue and
whenever the printer is done with one job, the next one is sent
to it automatically. This relieves the users from organizing
the print queue and fighting over control of the printer.
<footnote><para>Instead, they form a new queue
<emphasis>at</emphasis> the printer, waiting for their
printouts, since no one ever seems to be able to get the
queue software to know exactly when anyone's printout is
really finished. This is a great boost to intra-office
social relations.</para></footnote>
</para>
<para>The print queue software also <glossterm>spools</glossterm>
the printouts on disk, i.e., the text is kept in a file while
the job is in the queue. This allows an application program
to spit out the print jobs quickly to the print queue software;
the application does not have to wait until the job is actually
printed to continue. This is really convenient, since it
allows one to print out one version, and not have to wait for
it to be printed before one can make a completely revised new
version.</para>
</sect2>
<sect2>
<title>The filesystem layout</title>
<para>The filesystem is divided into many parts;
usually along the lines of a root filesystem with
<filename>/bin</filename>, <filename>/lib</filename>,
<filename>/etc</filename>, <filename>/dev</filename>, and
a few others; a <filename>/usr</filename> filesystem with
programs and unchanging data; a <filename>/var</filename>
filesystem with changing data (such as log files); and a
<filename>/home</filename> filesystem for everyone's personal
files. Depending on the hardware configuration and the decisions
of the system administrator, the division can be different;
it can even be all in one filesystem.</para>
<para><xref linkend="dir-tree-overview"> describes the filesystem
layout in some detail; the Linux Filesystem Standard covers it
in somewhat more detail.</para>
</sect2>
</sect1>
</chapter>
<chapter id="dir-tree-overview">
<title>Overview of the Directory Tree</title>
<blockquote><para><quote> Two days later, there was Pooh, sitting
on his branch, dangling his legs, and there, beside him, were
four pots of honey...</quote> (A.A. Milne) </para></blockquote>
<para>This chapter describes the important parts of a standard
Linux directory tree, based on the FSSTND filesystem
standard. It outlines the normal way of breaking the directory
tree into separate filesystems with different purposes and gives
the motivation behind this particular split. Some alternative
ways of splitting are also described.</para>
<sect1>
<title>Background</title>
<para>This chapter is loosely based on the <citetitle>Linux
filesystem standard</citetitle>, FSSTND, version 1.2 (see
the bibliography), which attempts to set a standard for how
the directory tree in a Linux system is organized. Such a
standard has the advantage that it will be easier to write or
port software for Linux, and to administer Linux machines, since
everything will be in their usual places. There is no authority
behind the standard that forces anyone to comply with it, but it
has got the support of most, if not all, Linux distributions.
It is not a good idea to break with the FSSTND without very
compelling reasons. The FSSTND attempts to follow Unix tradition
and current trends, making Linux systems familiar to those with
experience with other Unix systems, and vice versa.</para>
<para>This chapter is not as detailed as the FSSTND. A system
administrator should also read the FSSTND for a complete
understanding.</para>
<para>This chapter does not explain all files in detail.
The intention is not to describe every file, but to give
an overview of the system from a filesystem point of view.
Further information on each file is available elsewhere in this
manual or the manual pages.</para>
<para>The full directory tree is intended to be breakable
into smaller parts, each on its own disk or partition,
to accomodate to disk size limits and to ease backup
and other system administration. The major parts are the
root, <filename>/usr</filename>, <filename>/var</filename>, and
<filename>/home</filename> filesystems (see
<xref linkend="fstree">). Each part has a different purpose.
The directory tree has been designed so that it works well in
a network of Linux machines which may share some parts of the
filesystems over a read-only device (e.g., a CD-ROM), or over
the network with NFS.</para>
<figure id="fstree" float="1">
<title>Parts of a Unix directory tree. Dashed lines indicate partition limits.</title>
<graphic fileref="fstree"></graphic>
</figure>
<para>The roles of the different parts of the directory tree are
described below.
<itemizedlist>
<listitem> <para>The root filesystem is specific for
each machine (it is generally stored on a local disk,
although it could be a ramdisk or network drive as well)
and contains the files that are necessary for booting
the system up, and to bring it up to such a state that
the other filesystems may be mounted. The contents of
the root filesystem will therefore be sufficient for
the single user state. It will also contain tools for
fixing a broken system, and for recovering lost files
from backups.</para> </listitem>
<listitem><para> The <filename>/usr</filename> filesystem
contains all commands, libraries, manual pages, and
other unchanging files needed during normal operation.
No files in <filename>/usr</filename> should be specific
for any given machine, nor should they be modified during
normal use. This allows the files to be shared over
the network, which can be cost-effective since it saves
disk space (there can easily be hundreds of megabytes in
<filename>/usr</filename>), and can make administration
easier (only the master <filename>/usr</filename> needs to
be changed when updating an application, not each machine
separately). Even if the filesystem is on a local disk,
it could be mounted read-only, to lessen the chance of
filesystem corruption during a crash.</para></listitem>
<listitem> <para>The <filename>/var</filename>
filesystem contains files that change, such as spool
directories (for mail, news, printers, etc), log
files, formatted manual pages, and temporary files.
Traditionally everything in <filename>/var</filename>
has been somewhere below <filename>/usr</filename>, but
that made it impossible to mount <filename>/usr</filename>
read-only.<para></listitem>
<listitem> <para> The <filename>/home</filename>
filesystem contains the users' home directories, i.e., all
the real data on the system. Separating home directories
to their own directory tree or filesystem makes backups
easier; the other parts often do not have to be backed
up, or at least not as often (they seldom change).
A big <filename>/home</filename> might have to be
broken on several filesystems, which requires adding an
extra naming level below <filename>/home</filename>,
e.g., <filename>/home/students</filename> and
<filename>/home/staff</filename>.</para></listitem>
</itemizedlist> </para>
<para>Although the different parts have been called filesystems
above, there is no requirement that they actually be on separate
filesystems. They could easily be kept in a single one if the
system is a small single-user system and the user wants to keep
things simple. The directory tree might also be divided into
filesystems differently, depending on how large the disks are, and
how space is allocated for various purposes. The important part,
though, is that all the standard <emphasis>names</emphasis>
work; even if, say, <filename>/var</filename> and
<filename>/usr</filename> are actually on the same
partition, the names <filename>/usr/lib/libc.a</filename>
and <filename>/var/log/messages</filename> must work, for
example by moving files below <filename>/var</filename>
into <filename>/usr/var</filename>, and
making <filename>/var</filename> a symlink to
<filename>/usr/var</filename>.</para>
<para>The Unix filesystem structure groups files according to purpose,
i.e., all commands are in one place, all data files in another,
documentation in a third, and so on. An alternative would be to
group files files according to the program they belong to, i.e.,
all Emacs files would be in one directory, all TeX in another,
and so on. The problem with the latter approach is that it
makes it difficult to share files (the program directory often
contains both static and shareable and changing and
non-shareable files), and sometimes to even find the files
(e.g., manual pages in a huge number of places, and making the
manual page programs find all of them is a maintenance
nightmare).</para>
</sect1>
<sect1>
<title>The root filesystem</title>
<para>The root filesystem should generally be small, since
it contains very critical files and a small, infrequently
modified filesystem has a better chance of not getting corrupted.
A corrupted root filesystem will generally mean that the system
becomes unbootable except with special measures (e.g., from a
floppy), so you don't want to risk it.</para>
<para>The root directory generally doesn't contain any files, except
perhaps the standard boot image for the system, usually called
<filename>/vmlinuz</filename>. All other files are in subdirectories in the
root filesystems:
<glosslist>
<glossentry>
<glossterm><filename>/bin</filename></glossterm>
<glossdef><para>Commands needed during bootup
that might be used by normal users (probably after
bootup).</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/sbin</filename></glossterm>
<glossdef><para>Like <filename>/bin</filename>,
but the commands are not intended for normal
users, although they may use them if necessary and
allowed.</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/etc</filename></glossterm>
<glossdef><para>Configuration files specific to the
machine.</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/root</filename></glossterm>
<glossdef><para>The home directory for user
root.</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/lib</filename></glossterm>
<glossdef><para>Shared libraries needed by the programs
on the root filesystem.</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/lib/modules</filename></glossterm>
<glossdef><para>Loadable kernel modules, especially
those that are needed to boot the system when
recovering from disasters (e.g., network and filesystem
drivers).</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/dev</filename></glossterm>
<glossdef><para>Device files.</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/tmp</filename></glossterm>
<glossdef><para>Temporary files. Programs running after
bootup should use <filename>/var/tmp</filename>, not
<filename>/tmp</filename>, since the former is probably
on a disk with more space.</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/boot</filename></glossterm>
<glossdef><para>Files used by the bootstrap loader,
e.g., LILO. Kernel images are often kept here instead
of in the root directory. If there are many kernel
images, the directory can easily grow rather big, and it
might be better to keep it in a separate filesystem.
Another reason would be to make sure the kernel
images are within the first 1024 cylinders of an IDE
disk.</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/mnt</filename></glossterm>
<glossdef><para>Mount point for temporary mounts by
the system administrator. Programs aren't supposed
to mount on <filename>/mnt</filename> automatically.
<filename>/mnt</filename> might be divided into
subdirectories (e.g., <filename>/mnt/dosa</filename>
might be the floppy drive using an MS-DOS filesystem,
and <filename>/mnt/exta</filename> might be the same
with an ext2 filesystem).</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/proc</filename>, <filename>/usr</filename>, <filename>/var</filename>, <filename>/home</filename></glossterm>
<glossdef><para>Mount points for the other
filesystems.</para></glossdef></glossentry>
</glosslist>
</para>
</sect1>
<sect1>
<title>The <filename>/etc</filename> directory</title>
<para>The <filename>/etc</filename> directory contains a lot
of files. Some of them are described below. For others, you
should determine which program they belong to and read the manual
page for that program. Many networking configuration files are
in <filename>/etc</filename> as well, and are described in the
<citetitle>Networking Administrators' Guide</citetitle>.
<glosslist>
<glossentry>
<glossterm><filename>/etc/rc</filename> or <filename>/etc/rc.d</filename> or <filename>/etc/rc?.d</filename></glossterm>
<glossdef><para>Scripts or directories of scripts
to run at startup or when changing the run level.
See the chapter on <command>init</command> for further
information. </para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/etc/passwd</filename></glossterm>
<glossdef><para>The user database, with fields giving
the username, real name, home directory, encrypted
password, and other information about each user.
The format is documented in the <command>passwd</command> manual page.
</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/etc/fdprm</filename></glossterm>
<glossdef><para>Floppy disk parameter table.
Describes what different floppy disk formats look
like. Used by <command>setfdprm</command>. See the
<command>setfdprm</command> manual page for more
information. </para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/etc/fstab</filename></glossterm>
<glossdef><para>Lists the filesystems mounted
automatically at startup by the <command>mount
-a</command> command (in <filename>/etc/rc</filename>
or equivalent startup file). Under Linux, also contains
information about swap areas used automatically by
<command>swapon -a</command>. See <xref linkend="mount-and-umount"> and the
<command>mount</command> manual page for more information.
</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/etc/group</filename></glossterm>
<glossdef><para>Similar to
<filename>/etc/passwd</filename>, but
describes groups instead of users. See the
<command>group</command> manual page for more information.
</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/etc/inittab</filename></glossterm>
<glossdef><para>Configuration file for
<command>init</command>. </para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/etc/issue</filename></glossterm>
<glossdef><para>Output by <command>getty</command> before
the login prompt. Usually contains a short description or
welcoming message to the system. The contents are up to
the system administrator. </para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/etc/magic</filename></glossterm>
<glossdef><para>The configuration file
for <command>file</command>. Contains the
descriptions of various file formats based on
which <command>file</command> guesses the type of
the file. See the <filename>magic</filename> and
<command>file</command> manual pages for more information.
</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/etc/motd</filename></glossterm>
<glossdef><para>The message of the day, automatically
output after a successful login. Contents are up to the
system administrator. Often used for getting information
to every user, such as warnings about planned downtimes.
</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/etc/mtab</filename></glossterm>
<glossdef><para>List of currently mounted filesystems.
Initially set up by the bootup scripts, and updated
automatically by the <command>mount</command>
command. Used when a list of mounted filesystems is
needed, e.g., by the <command>df</command> command.
</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/etc/shadow</filename></glossterm>
<glossdef><para>Shadow password file on systems
with shadow password software installed.
Shadow passwords move the encrypted password
from <filename>/etc/passwd</filename> into
<filename>/etc/shadow</filename>; the latter is not
readable by anyone except root. This makes it harder
to crack passwords. </para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/etc/login.defs</filename></glossterm>
<glossdef><para>Configuration file for
the <command>login</command> command.
</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/etc/printcap</filename></glossterm>
<glossdef><para>Like <filename>/etc/termcap</filename>,
but intended for printers. Different syntax.
</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/etc/profile</filename>, <filename>/etc/csh.login</filename>, <filename>/etc/csh.cshrc</filename></glossterm>
<glossdef><para>Files executed at login or startup time
by the Bourne or C shells. These allow the system
administrator to set global defaults for all users.
See the manual pages for the respective shells.
</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/etc/securetty</filename></glossterm>
<glossdef><para>Identifies secure terminals, i.e.,
the terminals from which root is allowed to log in.
Typically only the virtual consoles are listed, so
that it becomes impossible (or at least harder) to gain
superuser privileges by breaking into a system over a
modem or a network. </para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/etc/shells</filename></glossterm>
<glossdef><para>Lists trusted shells. The
<command>chsh</command> command allows users to change
their login shell only to shells listed in this file.
<command>ftpd</command>, the server process that provides
FTP services for a machine, will check that the user's
shell is listed in <filename>/etc/shells</filename>
and will not let people log in unles the shell is
listed there. </para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/etc/termcap</filename></glossterm>
<glossdef><para>The terminal capability database.
Describes by what ``escape sequences'' various terminals
can be controlled. Programs are written so that instead
of directly outputting an escape sequence that only
works on a particular brand of terminal, they look up
the correct sequence to do whatever it is they want to
do in <filename>/etc/termcap</filename>. As a result
most programs work with most kinds of terminals.
See the <filename>termcap</filename>, curs_termcap,
and <filename>terminfo</filename> manual pages for
more information. </para></glossdef></glossentry>
</glosslist>
</para>
</sect1>
<sect1>
<title>The <filename>/dev</filename> directory</title>
<para>The <filename>/dev</filename> directory contains
the special device files for all the devices. The device
files are named using special conventions; these are
described in the <citetitle>Device list</citetitle> (see
XXX). The device files are created during installation,
and later with the <command>/dev/MAKEDEV</command> script.
The <command>/dev/MAKEDEV.local</command> is a script written
by the system administrator that creates local-only device
files or links (i.e., those that are not part of the standard
<command>MAKEDEV</command>, such as device files for some
non-standard device driver).</para>
</sect1>
<sect1>
<title>The <filename>/usr</filename> filesystem</title>
<para>The <filename>/usr</filename> filesystem is often
large, since all programs are installed there. All files
in <filename>/usr</filename> usually come from a Linux
distribution; locally installed programs and other stuff goes
below <filename>/usr/local</filename>. This makes it possible
to update the system from a new version of the distribution,
or even a completely new distribution, without having to
install all programs again. Some of the subdirectories of
<filename>/usr</filename> are listed below (some of the less
important directories have been dropped; see the FSSTND for
more information).
<glosslist>
<glossentry>
<glossterm><filename>/usr/X11R6</filename></glossterm>
<glossdef><para>The X Window System, all files.
To simplify the development and installation of
X, the X files have not been integrated into the
rest of the system. There is a directory tree
below <filename>/usr/X11R6</filename> similar
to that below <filename>/usr</filename> itself.
</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/usr/X386</filename></glossterm>
<glossdef><para>Similar to
<filename>/usr/X11R6</filename>, but for X11 Release 5.
</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/usr/bin</filename></glossterm>
<glossdef><para>Almost all user commands.
Some commands are in <filename>/bin</filename>
or in <filename>/usr/local/bin</filename>.
</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/usr/sbin</filename></glossterm>
<glossdef><para>System administration commands that are
not needed on the root filesystem, e.g., most server
programs. </para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/usr/man</filename>, <filename>/usr/info</filename>, <filename>/usr/doc</filename></glossterm>
<glossdef><para>Manual pages, GNU Info documents, and
miscellaneous other documentation files, respectively.
</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/usr/include</filename></glossterm>
<glossdef><para>Header files for the C
programming language. This should actually be below
<filename>/usr/lib</filename> for consistency, but the
tradition is overwhelmingly in support for this name.
</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/usr/lib</filename></glossterm>
<glossdef><para>Unchanging data files for programs and
subsystems, including some site-wide configuration
files. The name <filename>lib</filename> comes from library;
originally libraries of programming subroutines
were stored in <filename>/usr/lib</filename>.
</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/usr/local</filename></glossterm>
<glossdef><para>The place for locally installed software
and other files. </para></glossdef></glossentry>
</glosslist></para>
</sect1>
<sect1>
<title>The <filename>/var</filename> filesystem</title>
<para>The <filename>/var</filename> contains data that is changed when the system is
running normally. It is specific for each system, i.e., not
shared over the network with other computers.
<glosslist>
<glossentry>
<glossterm><filename>/var/catman</filename></glossterm>
<glossdef><para>A cache for man pages that are formatted
on demand. The source for manual pages is usually
stored in <filename>/usr/man/man*</filename>; some
manual pages might come with a pre-formatted version,
which is stored in <filename>/usr/man/cat*</filename>.
Other manual pages need to be formatted when they are
first viewed; the formatted version is then stored
in <filename>/var/man</filename> so that the next
person to view the same page won't have to wait for
it to be formatted. (<filename>/var/catman</filename>
is often cleaned in the same way temporary directories
are cleaned.)</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/var/lib</filename></glossterm>
<glossdef><para>Files that change while the system is
running normally.</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/var/local</filename></glossterm>
<glossdef><para>Variable data for programs that are
installed in <filename>/usr/local</filename> (i.e.,
programs that have been installed by the system
administrator). Note that even locally installed
programs should use the other <filename>/var</filename>
directories if they are appropriate, e.g.,
<filename>/var/lock</filename>.</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/var/lock</filename></glossterm>
<glossdef><para>Lock files. Many programs
follow a convention to create a lock file in
<filename>/var/lock</filename> to indicate that they
are using a particular device or file. Other programs
will notice the lock file and won't attempt to use the
device or file.</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/var/log</filename></glossterm>
<glossdef><para>Log files from various
programs, especially <command>login</command>
(<filename>/var/log/wtmp</filename>, which logs all logins
and logouts into the system) and <command>syslog</command>
(<filename>/var/log/messages</filename>, where all
kernel and system program message are usually stored).
Files in <filename>/var/log</filename> can often grow
indefinitely, and may require cleaning at regular
intervals.</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/var/run</filename></glossterm>
<glossdef><para>Files that contain information about the
system that is valid until the system is next booted.
For example, <filename>/var/run/utmp</filename>
contains information about people currently logged
in.</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/var/spool</filename></glossterm>
<glossdef><para>Directories for mail,
news, printer queues, and other queued work.
Each different spool has its own subdirectory
below <filename>/var/spool</filename>,
e.g., the mailboxes of the users are in
<filename>/var/spool/mail</filename>.</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/var/tmp</filename></glossterm>
<glossdef><para>Temporary files that are large
or that need to exist for a longer time than
what is allowed for <filename>/tmp</filename>.
(Although the system administrator might not allow
very old files in <filename>/var/tmp</filename>
either.)</para></glossdef></glossentry>
</glosslist></para>
</sect1>
<sect1>
<title>The <filename>/proc</filename> filesystem</title>
<para>The <filename>/proc</filename> filesystem contains
a illusionary filesystem. It does not exist on a disk.
Instead, the kernel creates it in memory. It is used to provide
information about the system (originally about processes, hence
the name). Some of the more important files and directories are
explained below. The <filename>/proc</filename> filesystem is
described in more detail in the <filename>proc</filename> manual page.
<glosslist>
<glossentry>
<glossterm><filename>/proc/1</filename></glossterm>
<glossdef><para>A directory with information about
process number 1. Each process has a directory below
<filename>/proc</filename> with the name being its process
identification number. </para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/proc/cpuinfo</filename></glossterm>
<glossdef><para>Information about the processor,
such as its type, make, model, and perfomance.
</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/proc/devices</filename></glossterm>
<glossdef><para>List of device drivers configured into the
currently running kernel. </para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/proc/dma</filename></glossterm>
<glossdef><para>Shows which DMA channels are being used
at the moment. </para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/proc/filesystems</filename></glossterm>
<glossdef><para>Filesystems configured into the kernel.
</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/proc/interrupts</filename></glossterm>
<glossdef><para>Shows which interrupts are
in use, and how many of each there have been.
</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/proc/ioports</filename></glossterm>
<glossdef><para>Which I/O ports are in use at the moment.
</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/proc/kcore</filename></glossterm>
<glossdef><para>An image of the physical memory of
the system. This is exactly the same size as your
physical memory, but does not really take up that much
memory; it is generated on the fly as programs access it.
(Remember: unless you copy it elsewhere, nothing under
<filename>/proc</filename> takes up any disk space
at all.) </para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/proc/kmsg</filename></glossterm>
<glossdef><para>Messages output by the kernel.
These are also routed to <command>syslog</command>.
</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/proc/ksyms</filename></glossterm>
<glossdef><para>Symbol table for the kernel.
</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/proc/loadavg</filename></glossterm>
<glossdef><para>The `load average' of the system; three
meaningless indicators of how much work the system has
to do at the moment. </para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/proc/meminfo</filename></glossterm>
<glossdef><para>Information about memory usage, both
physical and swap. </para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/proc/modules</filename></glossterm>
<glossdef><para>Which kernel modules are loaded at
the moment. </para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/proc/net</filename></glossterm>
<glossdef><para>Status information about network
protocols. </para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/proc/self</filename></glossterm>
<glossdef><para>A symbolic link to the process
directory of the program that is looking at
<filename>/proc</filename>. When two processes look at
<filename>/proc</filename>, they get different links.
This is mainly a convenience to make it easier
for programs to get at their process directory.
</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/proc/stat</filename></glossterm>
<glossdef><para>Various statistics about the system, such
as the number of page faults since the system was booted.
</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/proc/uptime</filename></glossterm>
<glossdef><para>The time the system has been up.
</para></glossdef></glossentry>
<glossentry>
<glossterm><filename>/proc/version</filename></glossterm>
<glossdef><para>The kernel version.
</para></glossdef></glossentry>
</glosslist></para>
<para>Note that while the above files tend to be easily
readable text files, they can sometimes be formatted in a way
that is not easily digestable. There are many commands that
do little more than read the above files and format them for
easier understanding. For example, the <command>free</command>
program reads <filename>/proc/meminfo</filename> and converts
the amounts given in bytes to kilobytes (and adds a little more
information, as well).</para>
</sect1>
</chapter>
<chapter>
<title>Using Disks and Other Storage Media</title>
<blockquote><para><quote>On a clear disk you can seek forever.
</quote></para></blockquote>
<!--
% the following metas need too much work for the next version
%
% \meta copying a directory/disk verbatim
%
% \meta disaster recovery: program to scan for ext2 superblocks
%
% \meta explain lost+found; how to fix a filesystem; what to do when
% there is a bad block; identifying the file that has the bad block
%
% \meta chart that shows characteristics of various fs: max size,
% max file size, usable as root, max name length, speed, support
%
% \meta
% Recovering from a bad MBR or super block.
% Manually remounting (ro->rw, rw->ro, when, why)
% automounting
% MD patches
% Why does Linux read/write disk in background?
% how to mount a dos disk so that everyone can access it?
% supermount
% ide disks map away bad sectors (until they're too many, then
% use badblocks)
% mounting: mountee root becomes mount point, e.g. permissions/ownership
% linux has maximum of 15 partitions (not inherent in partition
% scheme!)
% max ext2 part size is 2TB, file 2 GB
% ext2 fragmentation
% list important device files for disks et al as a table
-->
<para>When you install or upgrade your system, you need to do a
fair amount of work on your disks. You have to make filesystems
on your disks so that files can be stored on them and reserve
space for the different parts of your system.</para>
<para>This chapter explains all these initial activities. Usually,
once you get your system set up, you won't have to go through
the work again, except for using floppies. You'll need to come
back to this chapter if you add a new disk or want to fine-tune
your disk usage.<para>
<para>The basic tasks in administering disks are:
<itemizedlist>
<listitem><para>
Format your disk. This does various things to prepare it for
use, such as checking for bad sectors. (Formatting is nowadays
not necessary for most hard disks.)</para></listitem>
<listitem><para>
Partition a hard disk, if you want to use it for several
activities that aren't supposed to interfere with one another.
One reason for partitioning is to store different operating
systems on the same disk. Another reason is to keep user
files separate from system files, which simplifies back-ups
and helps protect the system files from corruption.
</para></listitem>
<listitem><para>
Make a filesystem (of a suitable type) on each disk or partition.
The disk means
nothing to Linux until you make a filesystem; then files can
be created and accessed on it.
</para></listitem>
<listitem><para>
Mount different filesystems to form a single tree structure, either
automatically, or manually as needed. (Manually mounted filesystems
usually need to be unmounted manually as well.)
</para></listitem>
</itemizedlist>
<para><xref linkend="memory-management"> contains information
about virtual memory and disk caching, of which you also need
to be aware when using disks.</para>
<sect1>
<title>Two kinds of devices</title>
<para>UNIX, and therefore Linux, recognizes two different
kinds of device: random-access block devices (such as disks),
and character devices (such as tapes and serial lines),
some of which may be serial, and some random-access. Each
supported device is represented in the filesystem as a
<glossterm>device file</glossterm>.
When you read or write a device file, the
data comes from or goes to the device it represents. This way
no special programs (and no special application programming
methodology, such as catching interrupts or polling a serial
port) are necessary to access devices; for example, to send a
file to the printer, one could just say
<screen>
<prompt>$</prompt> <userinput>cat filename > /dev/lp1</userinput>
<prompt>$</prompt>
</screen>
and the contents of the file are printed (the file must, of
course, be in a form that the printer understands). However,
since it is not a good idea to have several people cat their
files to the printer at the same time, one usually uses a special
program to send the files to be printed (usually <command>lpr</command>).
This program makes sure that only one file is being printed
at a time, and will automatically send files to the printer as
soon as it finishes with the previous file. Something similar
is needed for most devices. In fact, one seldom needs to worry
about device files at all.</para>
<para>Since devices show up as files in the filesystem (in the
<filename>/dev</filename> directory), it is easy
to see just what device files exist, using <command>ls</command> or
another suitable command. In the output of <command>ls -l</command>, the
first column contains the type of the file and its
permissions. For example, inspecting a serial device
gives on my system
<screen>
<prompt>$</prompt> <userinput>ls -l /dev/cua0</userinput>
<computeroutput>crw-rw-rw- 1 root uucp 5, 64 Nov 30 1993 /dev/cua0</computeroutput>
<prompt>$</prompt>
</screen>
The first character in the first column, i.e.,
`<literal>c</literal>' in <literal>crw-rw-rw-</literal>
above, tells an informed user the type of the file, in this
case a character device. For ordinary files, the first
character is `<literal>-</literal>', for directories
it is `<literal>d</literal>', and for block devices
`<literal>b</literal>'; see the <command>ls</command> man page
for further information.</para>
<para>Note that usually all device files exist even though the
device itself might be not be installed. So just because you
have a file <filename>/dev/sda</filename>, it doesn't mean that you really do
have an SCSI hard disk. Having all the device files makes the
installation programs simpler, and makes it easier to add new
hardware (there is no need to find out the correct parameters
for and create the device files for the new device).</para>
</sect1>
<sect1>
<title>Hard disks</title>
<para>This subsection introduces terminology related to hard
disks. If you already know the terms and concepts, you can skip
this subsection.</para>
<para>See <xref linkend="hd-schematic"> for a schematic picture
of the important parts in a hard disk. A hard disk consists of
one or more circular <glossterm>platters</glossterm>,
<footnote><para>The platters are made of a hard
substance, e.g., aluminium, which gives the hard disk
its name.</para></footnote>
of which either or both <glossterm>surfaces</glossterm> are coated
with a magnetic substance used for recording the data. For each
surface, there is a <glossterm>read-write head</glossterm> that
examines or alters the recorded data. The platters rotate on
a common axis; a typical rotation speed is 3600 rotations per
minute, although high-performance hard disks have higher speeds.
The heads move along the radius of the platters; this movement
combined with the rotation of the platters allows the head to
access all parts of the surfaces.</para>
<para>The processor (CPU) and the actual disk communicate through
a <glossterm>disk controller</glossterm>. This relieves the rest of the computer
from knowing how to use the drive, since the controllers for
different types of disks can be made to use the same interface
towards the rest of the computer. Therefore, the computer can
say just ``hey disk, gimme what I want'', instead of a long and
complex series of electric signals to move the head to the proper
location and waiting for the correct position to come under
the head and doing all the other unpleasant stuff necessary.
(In reality, the interface to the controller is still complex,
but much less so than it would otherwise be.) The controller
can also do some other stuff, such as caching, or automatic bad
sector replacement.</para>
<para>The above is usually all one needs to understand about the
hardware. There is also a bunch of other stuff, such as the
motor that rotates the platters and moves the heads, and the
electronics that control the operation of the mechanical
parts, but that is mostly not relevant for understanding the
working principle of a hard disk.</para>
<para>The surfaces are usually divided into concentric rings,
called <glossterm>tracks</glossterm>, and these in turn are
divided into <glossterm>sectors</glossterm>. This division
is used to specify locations on the hard disk and to allocate
disk space to files. To find a given place on the hard disk,
one might say ``surface 3, track 5, sector 7''. Usually the
number of sectors is the same for all tracks, but some hard disks
put more sectors in outer tracks (all sectors are of the same
physical size, so more of them fit in the longer outer tracks).
Typically, a sector will hold 512 bytes of data. The disk itself
can't handle smaller amounts of data than one sector.</para>
<figure id="hd-schematic" float="1">
<title>A schematic picture of a hard disk.</title>
<graphic fileref="hd-schematic"></graphic>
</figure>
<para>Each surface is divided into tracks (and sectors) in
the same way. This means that when the head for one surface
is on a track, the heads for the other surfaces are also on
the corresponding tracks. All the corresponding tracks taken
together are called a <glossterm>cylinder</glossterm>. It takes
time to move the heads from one track (cylinder) to another,
so by placing the data that is often accessed together (say, a
file) so that it is within one cylinder, it is not necessary to
move the heads to read all of it. This improves performance.
It is not always possible to place files like this; files
that are stored in several places on the disk are called
<glossterm>fragmented</glossterm>.</para>
<para>The number of surfaces (or heads, which is the same thing),
cylinders, and sectors vary a lot; the specification of the
number of each is called the <glossterm>geometry</glossterm> of a hard disk. The
geometry is usually stored in a special, battery-powered memory
location called the <glossterm>CMOS RAM</glossterm>, from where the operating
system can fetch it during bootup or driver initialization.</para>
<para>Unfortunately, the BIOS
<footnote><para>The BIOS is some built-in software stored on
ROM chips. It takes care, among other things, of the
initial stages of booting.</para></footnote>
has a design limitation, which makes it
impossible to specify a track number that is larger than 1024 in
the CMOS RAM,
which is too little for a large hard disk. To overcome this,
the hard disk controller lies about the geometry, and
<glossterm>translates the addresses</glossterm> given by the computer into something
that fits reality. For example, a hard disk might have 8 heads,
2048 tracks, and 35 sectors per track.
<footnote><para>The numbers are completely
imaginary.</para></footnote>
Its controller could lie to the computer and claim that it
has 16 heads, 1024 tracks, and 35 sectors per track, thus not
exceeding the limit on tracks, and translates the address that
the computer gives it by halving the head number, and doubling
the track number. The math can be more complicated in reality,
because the numbers are not as nice as here (but again, the
details are not relevant for understanding the principle).
This translation distorts the operating system's view of how
the disk is organized, thus making it impractical to use the
all-data-on-one-cylinder trick to boost performance.</para>
<para>The translation is only a problem for IDE disks. SCSI disks
use a sequential sector number (i.e., the controller translates
a sequential sector number to a head, cylinder, and sector
triplet), and a completely different method for the CPU to talk
with the controller, so they are insulated from the problem.
Note, however, that the computer might not know the real geometry
of an SCSI disk either.</para>
<para>Since Linux often will not know the real geometry of a disk,
its filesystems don't even try to keep files within a single
cylinder. Instead, it tries to assign sequentially numbered
sectors to files, which almost always gives similar performance.
The issue is further complicated by on-controller caches, and
automatic prefetches done by the controller.</para>
<para>Each hard disk is represented by a separate device
file. There can (usually) be only two or four IDE hard
disks. These are known as <filename>/dev/hda</filename>,
<filename>/dev/hdb</filename>, <filename>/dev/hdc</filename>,
and <filename>/dev/hdd</filename>, respectively. SCSI
hard disks are known as <filename>/dev/sda</filename>,
<filename>/dev/sdb</filename>, and so on. Similar naming
conventions exist for other hard disk types; see XXX (device
list) for more information. Note that the device files for
the hard disks give access to the entire disk, with no regard
to partitions (which will be discussed below), and it's easy to
mess up the partitions or the data in them if you aren't careful.
The disks' device files are usually used only to get access to the
master boot record (which will also be discussed below).</para>
</sect1>
<sect1>
<title>Floppies</title>
<para>A floppy disk consists of a flexible membrane covered on one
or both sides with similar magnetic substance as a hard disk.
The floppy disk itself doesn't have a read-write head, that is
included in the drive. A floppy corresponds to one platter in
a hard disk, but is removable and one drive can be used to
access different floppies, whereas the hard disk is one
indivisible unit.</para>
<para>Like a hard disk, a floppy is divided into tracks and sectors
(and the two corresponding tracks on either side of a floppy
form a cylinder), but there are many fewer of them than on a
hard disk.</para>
<para>A floppy drive can usually use several different types of disks;
for example, a 3.5 inch drive can use both 720 kB and
1.44 MB disks. Since the drive has to operate a bit differently
and the operating system must know how big the disk is, there
are many device files for floppy drives, one per combination of
drive and disk type.
Therefore, <filename>/dev/fd0H1440</filename> is the first floppy drive (fd0),
which must be a 3.5 inch drive,
using a 3.5 inch, high density disk (H) of
size 1440 kB (1440), i.e., a normal 3.5 inch HD floppy.
For more information on the naming conventions for the floppy
devices, see XXX (device list).</para>
<para>The names for floppy drives are complex, however, and Linux
therefore has a special floppy device type that automatically
detects the type of the disk in the drive. It works by
trying to read the first sector of a newly inserted floppy
using different floppy types until it finds the correct one.
This naturally requires that the floppy is formatted first.
The automatic devices are called <filename>/dev/fd0</filename>,
<filename>/dev/fd1</filename>, and so on.</para>
<para>The parameters the automatic device uses to access a disk can
also be set using the program <command>setfdprm</command>. This can be
useful if you need to use disks that do not follow any usual
floppy sizes, e.g., if they have an unusual number of sectors,
or if the autodetecting for some reason fails and the proper
device file is missing.</para>
<para>Linux can handle many nonstandard floppy disk formats
in addition to all the standard ones. Some of these require
using special formatting programs. We'll skip these disk
types for now, but in the mean time you can examine the
<filename>/etc/fdprm</filename> file. It specifies the settings
that <command>setfdprm</command> recognizes.</para>
<para>The operating system must know when a disk has been changed in
a floppy drive, for example, in order to avoid using cached
data from the previous disk. Unfortunately, the signal line
that is used for this is sometimes broken, and worse, this won't
always be noticeable when using the drive from within MS-DOS.
If you are experiencing weird problems using floppies, this might
be the reason. The only way to correct it is to repair the
floppy drive.</para>
</sect1>
<sect1>
<title>CD-ROM's</title>
<para>A CD-ROM drive uses an optically read, plastic coated disk.
The information is recorded on the surface of the
disk
<footnote><para>That is, the surface inside
the disk, on the metal disk inside the plastic
coating.</para></footnote>
in small `holes' aligned along a spiral from the center to the
edge. The drive directs a laser beam along the spiral to read
the disk. When the laser hits a hole, the laser is reflected in
one way; when it hits smooth surface, it is reflected in another
way. This makes it easy to code bits, and therefore information.
The rest is easy, mere mechanics.</para>
<para>CD-ROM drives are slow compared to hard disks. Whereas a
typical hard disk will have an average seek time less than
15 milliseconds, a fast CD-ROM drive can use tenths of a second
for seeks. The actual data transfer rate is fairly high at
hundreds of kilobytes per second. The slowness means that
CD-ROM drives are not as pleasant to use instead of hard disks
(some Linux distributions provide `live' filesystems on CD-ROM's,
making it unnecessary to copy the files to the hard disk, making
installation easier and saving a lot of hard disk space), although
it is still possible. For installing new software, CD-ROM's are
very good, since it maximum speed is not essential during
installation.</para>
<para>There are several ways to arrange data on a CD-ROM. The most
popular one is specified by the international standard ISO 9660.
This standard specifies a very minimal filesystem, which is
even more crude than the one MS-DOS uses. On the other hand,
it is so minimal that every operating system should be able to
map it to its native system.</para>
<para>For normal UNIX use, the ISO 9660 filesystem is not usable, so
an extension to the standard has been developed, called
the Rock Ridge extension. Rock Ridge allows longer filenames,
symbolic links, and a lot of other goodies, making a CD-ROM
look more or less like any contemporary UNIX filesystem.
Even better, a Rock Ridge filesystem is still a valid ISO 9660
filesystem, making it usable by non-UNIX systems as well.
Linux supports both ISO 9660 and the Rock Ridge extensions;
the extensions are recognized and used automatically.</para>
<para>The filesystem is only half the battle, however. Most CD-ROM's
contain data that requires a special program to access, and
most of these programs do not run under Linux (except, possibly,
under dosemu, the Linux MS-DOS emulator).</para>
<para>A CD-ROM drive is accessed via the corresponding device file.
There are several ways to connect a CD-ROM drive to the computer:
via SCSI, via a sound card, or via EIDE. The hardware hacking
needed to do this is outside the scope of this book, but the
type of connection decides the device file. See XXX (device-list)
for enlightment.</para>
</sect1>
<sect1>
<title>Tapes</title>
<para>A tape drive uses a tape, similar
<footnote><para>But completely
different, of course.</para></footnote>
to cassettes used for music. A tape is serial in nature, which
means that in order to get to any given part of it, you first have
to go through all the parts in between. A disk can be accessed
randomly, i.e., you can jump directly to any place on the disk.
The serial access of tapes makes them slow.</para>
<para>On the other hand, tapes are relatively cheap to make,
since they do not need to be fast. They can also easily be made
quite long, and can therefore contain a large amount of data.
This makes tapes very suitable for things like archiving and
backups, which do not require large speeds, but benefit from
low costs and large storage capacities.</para>
</sect1>
<sect1>
<title>Formatting</title>
<para><glossterm>Formatting</glossterm> is the process of writing marks on the
magnetic media that are used to mark tracks and sectors.
Before a disk is formatted, its magnetic surface is a complete
mess of magnetic signals. When it is formatted, some order is
brought into the chaos by essentially drawing lines where the
tracks go, and where they are divided into sectors. The
actual details are not quite exactly like this, but that is
irrelevant. What is important is that a disk cannot be used
unless it has been formatted.</para>
<para>The terminology is a bit confusing here: in MS-DOS, the word
formatting is used to cover also the process of creating a
filesystem (which will be discussed below). There, the two
processes are often combined, especially for floppies. When
the distinction needs to be made, the real formatting is
called <glossterm>low-level formatting</glossterm>, while making the filesystem
is called <glossterm>high-level formatting</glossterm>. In UNIX circles,
the two are called formatting and making a filesystem, so
that's what is used in this book as well.</para>
<para>For IDE and some SCSI disks the formatting is actually
done at the factory and doesn't need to be repeated; hence most
people rarely need to worry about it. In fact, formatting a
hard disk can cause it to work less well, for example because
a disk might need to be formatted in some very special way to
allow automatic bad sector replacement to work.</para>
<para>Disks that need to be or can be formatted often require a
special program anyway, because the interface to the formatting
logic inside the drive is different from drive to drive.
The formatting program is often either on the controller BIOS,
or is supplied as an MS-DOS program; neither of these can easily
be used from within Linux.</para>
<para>During formatting one might encounter bad spots on the
disk, called <glossterm>bad blocks</glossterm> or <glossterm>bad
sectors</glossterm>. These are sometimes handled by the drive
itself, but even then, if more of them develop, something needs
to be done to avoid using those parts of the disk. The logic to
do this is built into the filesystem; how to add the information
into the filesystem is described below. Alternatively, one
might create a small partition that covers just the bad part of
the disk; this approach might be a good idea if the bad spot is
very large, since filesystems can sometimes have trouble with
very large bad areas.</para>
<para>Floppies are formatted with <command>fdformat</command>. The floppy device
file to use is given as the parameter. For example, the
following command would format a high density,
3.5 inch floppy in the first floppy drive:
<screen>
<prompt>$</prompt> <userinput>fdformat /dev/fd0H1440</userinput>
<computeroutput>Double-sided, 80 tracks, 18 sec/track. Total capacity 1440 kB.</computeroutput>
<computeroutput>Formatting ... done</computeroutput>
<computeroutput>Verifying ... done</computeroutput>
<prompt>$</prompt>
</screen>
Note that if you want to use an autodetecting device (e.g.,
<filename>/dev/fd0</filename>), you <emphasis>must</emphasis> set the parameters of the device
with <command>setfdprm</command> first. To achieve the same effect as
above, one would have to do the following:
<screen>
<prompt>$</prompt> <userinput>setfdprm /dev/fd0 1440/1440</userinput>
<prompt>$</prompt> <userinput>fdformat /dev/fd0</userinput>
<computeroutput>Double-sided, 80 tracks, 18 sec/track. Total capacity 1440 kB.</computeroutput>
<computeroutput>Formatting ... done</computeroutput>
<computeroutput>Verifying ... done</computeroutput>
<prompt>$</prompt>
</screen>
It is usually more convenient to choose the correct device file
that matches the type of the floppy. Note that it is unwise to
format floppies to contain more information than what they are
designed for.</para>
<para><command>fdformat</command> will also validate the floppy, i.e., check it
for bad blocks. It will try a bad block several times (you
can usually hear this, the drive noise changes dramatically).
If the floppy is only marginally bad (due to dirt on the
read/write head, some errors are false signals), <command>fdformat</command> won't
complain, but a real error will abort the validation process.
The kernel will print log messages for each I/O error it
finds; these will go to the console or, if <command>syslog</command>
is being used, to the file <filename>/usr/log/messages</filename>. <command>fdformat</command>
itself won't tell where the error is (one usually doesn't care,
floppies are cheap enough that a bad one is automatically thrown
away).
<screen>
<prompt>$</prompt> <userinput>fdformat /dev/fd0H1440</userinput>
<computeroutput>Double-sided, 80 tracks, 18 sec/track. Total capacity 1440 kB.</computeroutput>
<computeroutput>Formatting ... done</computeroutput>
<computeroutput>Verifying ... read: Unknown error</computeroutput>
<prompt>$</prompt>
</screen>
The <command>badblocks</command> command can be used to search any disk or
partition for bad blocks (including a floppy). It does not
format the disk, so it can be used to check even existing
filesystems. The example below checks a 3.5 inch
floppy with two bad blocks.
<screen>
<prompt>$</prompt> <userinput>badblocks /dev/fd0H1440 1440</userinput>
<computeroutput>718</computeroutput>
<computeroutput>719</computeroutput>
<prompt>$</prompt>
</screen>
<command>badblocks</command> outputs the block numbers of the bad
blocks it finds. Most filesystems can avoid such bad blocks. They
maintain a list of known bad blocks, which is initialized when the
filesystem is made, and can be modified later. The initial search
for bad blocks can be done by the <command>mkfs</command> command
(which initializes the filesystem), but later checks should be
done with <command>badblocks</command> and the new blocks should
be added with <command>fsck</command>. We'll describe <command>mkfs</command>
and <command>fsck</command> later.</para>
<para>Many modern disks automatically notice bad blocks, and attempt
to fix them by using a special, reserved good block instead.
This is invisible to the operating system. This feature should
be documented in the disk's manual, if you're curious if it
is happening. Even such disks can fail, if the number of bad
blocks grows too large, although chances are that by then the disk
will be so rotten as to be unusable.</para>
</sect1>
<sect1>
<title>Partitions</title>
<para>A hard disk can be divided into several
<glossterm>partitions</glossterm>. Each partition functions as if
it were a separate hard disk. The idea is that if you have one
hard disk, and want to have, say, two operating systems on it,
you can divide the disk into two partitions. Each operating
system uses its partition as it wishes and doesn't touch the
other one's. This way the two operating systems can co-exist
peacefully on the same hard disk. Without partitions one would
have to buy a hard disk for each operating system.</para>
<para>Floppies are not partitioned. There is no technical reason
against this, but since they're so small, partitions would be
useful only very rarely. CD-ROM's are usually also not
partitioned, since it's easier to use them as one big
disk, and there is seldom a need to have several operating
systems on one.</para>
<sect2>
<title>The MBR, boot sectors and partition table</title>
<para>The information about how a hard disk has been partitioned
is stored in its first sector (that is, the first sector of the
first track on the first disk surface). The first sector is the
<glossterm>master boot record</glossterm> (MBR) of the disk; this
is the sector that the BIOS reads in and starts when the machine
is first booted. The master boot record contains a small program
that reads the partition table, checks which partition is active
(that is, marked bootable), and reads the first sector of that
partition, the partition's <glossterm>boot sector</glossterm>
(the MBR is also a boot sector, but it has a special status and
therefore a special name). This boot sector contains another
small program that reads the first part of the operating system
stored on that partition (assuming it is bootable), and then
starts it.</para>
<para>The partitioning scheme is not built into the hardware, or
even into the BIOS. It is only a convention that many
operating systems follow. Not all operating systems do follow
it, but they are the exceptions. Some operating
systems support partitions, but they occupy one partition on
the hard disk, and use their internal partitioning method
within that partition. The latter type exists peacefully
with other operating systems (including Linux), and does not
require any special measures, but an operating system
that doesn't support partitions cannot co-exist on the same
disk with any other operating system.</para>
<para>As a safety precaution, it is a good idea to write down the
partition table on a piece of paper, so that if it ever corrupts
you don't have to lose all your files. (A bad partition table
can be fixed with <command>fdisk</command>). The relevant information
is given by the <command>fdisk -l</command> command:
<screen>
<prompt>$</prompt> <userinput>fdisk -l /dev/hda</userinput>
<computeroutput></computeroutput>
<computeroutput>Disk /dev/hda: 15 heads, 57 sectors, 790 cylinders</computeroutput>
<computeroutput>Units = cylinders of 855 * 512 bytes</computeroutput>
<computeroutput></computeroutput>
<computeroutput> Device Boot Begin Start End Blocks Id System</computeroutput>
<computeroutput>/dev/hda1 1 1 24 10231+ 82 Linux swap</computeroutput>
<computeroutput>/dev/hda2 25 25 48 10260 83 Linux native</computeroutput>
<computeroutput>/dev/hda3 49 49 408 153900 83 Linux native</computeroutput>
<computeroutput>/dev/hda4 409 409 790 163305 5 Extended</computeroutput>
<computeroutput>/dev/hda5 409 409 744 143611+ 83 Linux native</computeroutput>
<computeroutput>/dev/hda6 745 745 790 19636+ 83 Linux native</computeroutput>
<prompt>$</prompt>
</screen>
</sect2>
<sect2>
<title>Extended and logical partitions</title>
<para>The original partitioning scheme for PC hard disks allowed
only four partitions. This quickly turned out to be too little
in real life, partly because some people want more than four
operating systems (Linux, MS-DOS, OS/2, Minix, FreeBSD, NetBSD, or
Windows/NT, to name a few), but primarily because sometimes it
is a good idea to have several partitions for one
operating system. For example, swap space is usually best put
in its own partition for Linux instead of in the main
Linux partition for reasons of speed (see below).</para>
<para>To overcome this design problem, <glossterm>extended partitions</glossterm> were
invented. This trick allows partitioning a <glossterm>primary
partition</glossterm> into sub-partitions. The
primary partition thus subdivided is the <glossterm>extended partition</glossterm>; the
subpartitions are <glossterm>logical partitions</glossterm>. They behave
like primary
<footnote><para>Illogical?</para></footnote>
partitions, but are created differently. There is no speed
difference between them.</para>
<para>The partition structure of a hard disk might look like that
in <xref linkend="hard-disk-layout">. The disk is divided into
three primary partitions, the second of which is divided into
two logical partitions. Part of the disk is not partitioned
at all. The disk as a whole and each primary partition has a
boot sector.</para>
<figure id="hard-disk-layout" float="1">
<title>A sample hard disk partitioning.</title>
<graphic fileref="hd-layout"></graphic>
</figure>
</sect2>
<sect2>
<title>Partition types</title>
<para>The partition tables (the one in the MBR, and the ones for
extended partitions) contain one byte per partition that
identifies the type of that partition. This attempts to
identify the operating system that uses the partition, or what
it uses it for. The purpose is to make it possible to avoid
having two operating systems accidentally using the same
partition. However, in reality, operating systems do not
really care about the partition type byte; e.g., Linux
doesn't care at all what it is. Worse, some of them use it
incorrectly; e.g., at least some versions of DR-DOS ignore the
most significant bit of the byte, while others don't.</para>
<para>There is no standardization agency to specify what each byte
value means, but some commonly accepted ones are included in
in <xref linkend="partition-ids">. The same list is
available in the Linux <command>fdisk</command> program.</para>
<table id="partition-ids">
<title>Partition types (from the Linux <command>fdisk</command> program).</title>
<tgroup cols=6>
<tbody>
<row>
<entry>0</entry> <entry>Empty</entry>
<entry>40</entry> <entry>Venix 80286</entry>
<entry>94</entry> <entry>Amoeba BBT</entry>
</row>
<row>
<entry>1</entry> <entry>DOS 12-bit FAT</entry>
<entry>51</entry> <entry>Novell?</entry>
<entry>a5</entry> <entry>BSD/386</entry>
</row>
<row>
<entry>2</entry> <entry>XENIX root</entry>
<entry>52</entry> <entry>Microport</entry>
<entry>b7</entry> <entry>BSDI fs</entry>
</row>
<row>
<entry>3</entry> <entry>XENIX usr</entry>
<entry>63</entry> <entry>GNU HURD</entry>
<entry>b8</entry> <entry>BSDI swap</entry>
</row>
<row>
<entry>4</entry> <entry>DOS 16-bitf <32M</entry>
<entry>64</entry> <entry>Novell</entry>
<entry>c7</entry> <entry>Syrinx</entry>
</row>
<row>
<entry>5</entry> <entry>Extended</entry>
<entry>75</entry> <entry>PC/IX</entry>
<entry>db</entry> <entry>CP/M</entry>
</row>
<row>
<entry>6</entry> <entry>DOS 16-bit >=32M</entry>
<entry>80</entry> <entry>Old MINIX</entry>
<entry>e1</entry> <entry>DOS access</entry>
</row>
<row>
<entry>7</entry> <entry>OS/2 HPFS</entry>
<entry>81</entry> <entry>Linux/MINIX</entry>
<entry>e3</entry> <entry>DOS R/O</entry>
</row>
<row>
<entry>8</entry> <entry>AIX</entry>
<entry>82</entry> <entry>Linux swap</entry>
<entry>f2</entry> <entry>DOS secondary</entry>
</row>
<row>
<entry>9</entry> <entry>AIX bootable</entry>
<entry>83</entry> <entry>Linux native</entry>
<entry>ff</entry> <entry>BBT</entry>
</row>
<row>
<entry>a</entry> <entry>OS/2 Boot Manag</entry>
<entry>93</entry> <entry>Amoeba</entry>
<entry></entry> <entry></entry>
</row>
</tbody>
</tgroup>
</table>
</sect2>
<sect2>
<title>Partitioning a hard disk</title>
<para>There are many programs for creating and removing
partitions. Most operating systems have their own, and it
can be a good idea to use each operating system's own, just
in case it does something unusual that the others can't.
Many of the programs are called <command>fdisk</command>,
including the Linux one, or variations thereof. Details on
using the Linux <command>fdisk</command> are given on its
man page. The <command>cfdisk</command> command is similar
to <command>fdisk</command>, but has a nicer (full screen)
user interface.</para>
<para>When using IDE disks, the boot partition (the partition
with the bootable kernel image files) must be completely
within the first 1024 cylinders. This is because the disk is
used via the BIOS during boot (before the system goes into
protected mode), and BIOS can't handle more than 1024 cylinders.
It is sometimes possible to use a boot partition that is only
partly within the first 1024 cylinders. This works as long
as all the files that are read with the BIOS are within the
first 1024 cylinders. Since this is difficult to arrange,
it is <emphasis>a very bad idea</emphasis> to do it; you never know when
a kernel update or disk defragmentation will result in an
unbootable system. Therefore, make sure your boot partition
is completely within the first 1024 cylinders.</para>
<para>Some newer versions of the BIOS and IDE disks can, in fact,
handle disks with more than 1024 cylinders. If you have such
a system, you can forget about the problem; if you aren't quite
sure of it, put it within the first 1024 cylinders.</para>
<para>Each partition should have an even number of sectors,
since the Linux filesystems use a 1 kilobyte block size, i.e.,
two sectors. An odd number of sectors will result in the
last sector being unused. This won't result in any problems,
but it is ugly, and some versions of <command>fdisk</command>
will warn about it.</para>
<para>Changing a partition's size usually requires first backing up
everything you want to save from that partition (preferably the
whole disk, just in case), deleting the partition, creating
new partition, then restoring everything to the new partition.
If the partition is growing, you may need to adjust the sizes
(and backup and restore) of the adjoining partitions as well.</para>
<para>Since changing partition sizes is painful, it is preferable to
get the partitions right
the first time, or have an effective and easy to use backup
system. If you're installing from a media that does not require
much human intervention (say, from CD-ROM, as opposed to floppies),
it is often easy to play with different configuration at first.
Since you don't already have data to back up, it is not so
painful to modify partition sizes several times.</para>
<para>There is a program for MS-DOS, called
<command>fips</command>, which resizes an MS-DOS partition without
requiring the backup and restore, but for other filesystems it
is still necessary.</para>
</sect2>
<sect2>
<title>Device files and partitions</title>
<para>Each partition and extended partition has its own
device file. The naming convention for these files is that a
partition's number is appended after the name of the whole disk,
with the convention that 1-4 are primary partitions (regardless
of how many primary partitions there are) and 5-8 are logical
partitions (regardless of within which primary partition
they reside). For example, <filename>/dev/hda1</filename>
is the first primary partition on the first IDE hard disk, and
<filename>/dev/sdb7</filename> is the third extended partition on
the second SCSI hard disk. The device list in XXX (device list)
gives more information.</para>
</sect2>
</sect1>
<sect1>
<title>Filesystems</title>
<sect2>
<title>What are filesystems?</title>
<para>A <glossterm>filesystem</glossterm> is the methods and
data structures that an operating system uses to keep track
of files on a disk or partition; that is, the way the files
are organized on the disk. The word is also used to refer to a
partition or disk that is used to store the files or the type of
the filesystem. Thus, one might say ``I have two filesystems''
meaning one has two partitions on which one stores files, or
that one is using the ``extended filesystem'', meaning the type
of the filesystem.</para>
<para>The difference between a disk or partition and the filesystem
it contains is important. A few programs (including,
reasonably enough, programs that create filesystems) operate
directly on the raw sectors of a disk or partition; if there
is an existing file system there it will be destroyed or
seriously corrupted. Most programs operate on a filesystem,
and therefore won't work on a partition that doesn't contain
one (or that contains one of the wrong type).</para>
<para>Before a partition or disk can be used as a filesystem, it
needs to be initialized, and the bookkeeping data structures need
to be written to the disk. This process is called
<glossterm>making a filesystem</glossterm>.</para>
<para>Most UNIX filesystem types have a similar general
structure, although the exact details vary quite a bit.
The central concepts are <glossterm>superblock</glossterm>,
<glossterm>inode</glossterm>, <glossterm>data block</glossterm>,
<glossterm>directory block</glossterm>, and <glossterm>indirection
block</glossterm>. The superblock contains information
about the filesystem as a whole, such as its size (the exact
information here depends on the filesystem). An inode contains
all information about a file, except its name. The name is
stored in the directory, together with the number of the inode.
A directory entry consists of a filename and the number of
the inode which represents the file. The inode contains the
numbers of several data blocks, which are used to store the
data in the file. There is space only for a few data block
numbers in the inode, however, and if more are needed, more
space for pointers to the data blocks is allocated dynamically.
These dynamically allocated blocks are indirect blocks; the name
indicates that in order to find the data block, one has to find
its number in the indirect block first.</para>
<para>UNIX filesystems usually allow one to create a
<glossterm>hole</glossterm> in a file (this is done with
<function>lseek</function>; check the manual page), which means
that the filesystem just pretends that at a particular place in
the file there is just zero bytes, but no actual disk sectors are
reserved for that place in the file (this means that the file
will use a bit less disk space). This happens especially often
for small binaries, Linux shared libraries, some databases, and
a few other special cases. (Holes are implemented by storing a
special value as the address of the data block in the indirect
block or inode. This special address means that no data block
is allocated for that part of the file, ergo, there is a hole
in the file.)</para>
<para>Holes are moderately useful. On the author's system,
a simple measurement showed a potential for about 4 MB of
savings through holes of about 200 MB total used disk space.
That system, however, contains relatively few programs and no
database files.</para>
</sect2>
<sect2>
<title>Filesystems galore</title>
<para>Linux supports several types of filesystems. As of this
writing the most important ones are:
<glosslist>
<glossentry>
<glossterm>minix</glossterm>
<glossdef><para>
The oldest, presumed to be the most reliable, but quite
limited in features (some time stamps are missing, at
most 30 character filenames) and restricted in
capabilities (at most 64 MB per filesystem).
</para></glossdef></glossentry>
<glossentry>
<glossterm>xia</glossterm>
<glossdef><para>
A modified version of the minix filesystem that lifts
the limits on the filenames and filesystem sizes,
but does not otherwise introduce new features. It is
not very popular, but is reported to work very well.
</para></glossdef></glossentry>
<glossentry>
<glossterm>ext2</glossterm>
<glossdef><para>
The most featureful of the native Linux filesystems,
currently also the most popular one. It is designed to
be easily upwards compatible, so that new versions
of the filesystem code do not require re-making the
existing filesystems.
</para></glossdef></glossentry>
<glossentry>
<glossterm>ext</glossterm>
<glossdef><para>
An older version of ext2 that wasn't upwards
compatible. It is hardly ever used in new installations
any more, and most people have converted to ext2.
</para></glossdef></glossentry>
</glosslist>
</para>
<para>In addition, support for several foreign filesystem exists,
to make it easier to exchange files with other operating
systems. These foreign filesystems work just like native
ones, except that they may be lacking in some usual UNIX
features, or have curious limitations, or other oddities.
<glosslist>
<glossentry>
<glossterm>msdos</glossterm>
<glossdef><para>
Compatibility with MS-DOS (and OS/2 and Windows NT)
FAT filesystems.
</para></glossdef></glossentry>
<glossentry>
<glossterm>usmdos</glossterm>
<glossdef><para>
Extends the msdos filesystem driver under
Linux to get long filenames, owners,
permissions, links, and device files. This allows a normal
msdos filesystem to be used as if it were a
Linux one, thus removing the need for a separate
partition for Linux.
</para></glossdef></glossentry>
<glossentry>
<glossterm>iso9660</glossterm>
<glossdef><para>
The standard CD-ROM filesystem; the popular Rock Ridge
extension to the CD-ROM standard that allows longer file
names is supported automatically.
</para></glossdef></glossentry>
<glossentry>
<glossterm>nfs</glossterm>
<glossdef><para>
A networked filesystem that allows sharing a filesystem
between many computers to allow easy access to the
files from all of them.
</para></glossdef></glossentry>
<glossentry>
<glossterm>hpfs</glossterm>
<glossdef><para>
The OS/2 filesystem.
</para></glossdef></glossentry>
<glossentry>
<glossterm>sysv</glossterm>
<glossdef><para>
SystemV/386, Coherent, and Xenix filesystems.
</para></glossdef></glossentry>
</glosslist>
</para>
<para>The choice of filesystem to use depends on the situation. If
compatibility or other reasons make one of the non-native
filesystems necessary, then that one must be used. If one can
choose freely, then it is probably wisest to use ext2, since
it has all the features but does not suffer from lack of
performance.</para>
<para>There is also the proc filesystem, usually accessible as
the <filename>/proc</filename> directory, which is not really a
filesystem at all, even though it looks like one. The
proc filesystem makes it easy to access certain kernel
data structures, such as the process list (hence the name).
It makes these
data structures look like a filesystem, and that filesystem
can be manipulated with all the usual file tools. For example,
to get a listing of all processes one might use the
command
<screen>
<prompt>$</prompt> <userinput>ls -l /proc</userinput>
<computeroutput>total 0
dr-xr-xr-x 4 root root 0 Jan 31 20:37 1
dr-xr-xr-x 4 liw users 0 Jan 31 20:37 63
dr-xr-xr-x 4 liw users 0 Jan 31 20:37 94
dr-xr-xr-x 4 liw users 0 Jan 31 20:37 95
dr-xr-xr-x 4 root users 0 Jan 31 20:37 98
dr-xr-xr-x 4 liw users 0 Jan 31 20:37 99
-r--r--r-- 1 root root 0 Jan 31 20:37 devices
-r--r--r-- 1 root root 0 Jan 31 20:37 dma
-r--r--r-- 1 root root 0 Jan 31 20:37 filesystems
-r--r--r-- 1 root root 0 Jan 31 20:37 interrupts
-r-------- 1 root root 8654848 Jan 31 20:37 kcore
-r--r--r-- 1 root root 0 Jan 31 11:50 kmsg
-r--r--r-- 1 root root 0 Jan 31 20:37 ksyms
-r--r--r-- 1 root root 0 Jan 31 11:51 loadavg
-r--r--r-- 1 root root 0 Jan 31 20:37 meminfo
-r--r--r-- 1 root root 0 Jan 31 20:37 modules
dr-xr-xr-x 2 root root 0 Jan 31 20:37 net
dr-xr-xr-x 4 root root 0 Jan 31 20:37 self
-r--r--r-- 1 root root 0 Jan 31 20:37 stat
-r--r--r-- 1 root root 0 Jan 31 20:37 uptime
-r--r--r-- 1 root root 0 Jan 31 20:37 version</computeroutput>
<prompt>$</prompt>
</screen>
(There will be a few extra files that don't correspond to
processes, though. The above example has been shortened.)</para>
<para>Note that even though it is called a filesystem, no part of
the proc filesystem touches any disk. It exists only in the
kernel's imagination. Whenever anyone tries to look at any
part of the proc filesystem, the kernel makes it look as if
the part existed somewhere, even though it doesn't. So, even
though there is a multi-megabyte <filename>/proc/kcore</filename> file,
it doesn't take any disk space.
</sect2>
<sect2>
<title>Which filesystem should be used?</title>
<para>There is usually little point in using many different
filesystems. Currently, ext2fs is the most popular one, and
it is probably the wisest choice. Depending on the overhead
for bookkeeping structures, speed, (perceived) reliability,
compatibility, and various other reasons, it may be advisable
to use another file system. This needs to be decided on a
case-by-case basis.</para>
</sect2>
<sect2>
<title>Creating a filesystem</title>
<para>Filesystems are created, i.e., initialized, with the <command>mkfs</command>
command. There is actually a separate program for each filesystem
type. <command>mkfs</command> is just a front end that runs the appropriate
program depending on the desired filesystem type. The type is
selected with the <option>-t fstype</option> option.</para>
<para>The programs called by <command>mkfs</command> have slightly
different command line interfaces. The common and most important
options are summarized below; see the manual pages for more.
<glosslist>
<glossentry>
<glossterm><option>-t fstype</option></glossterm>
<glossdef><para>
Select the type of the filesystem.
</para></glossdef></glossentry>
<glossentry>
<glossterm><option>-c</option></glossterm>
<glossdef><para>
Search for bad blocks and initialize the bad
block list accordingly.
</para></glossdef></glossentry>
<glossentry>
<glossterm>-l filename</glossterm>
<glossdef><para>
Read the initial bad block list from the name file.
</para></glossdef></glossentry>
</glosslist>
</para>
<para>To create an ext2 filesystem on a floppy, one would give the
following commands:
<screen>
<prompt>$</prompt> <userinput>fdformat -n /dev/fd0H1440</userinput>
<computeroutput>Double-sided, 80 tracks, 18 sec/track. Total capacity 1440 kB.
Formatting ... done</computeroutput>
<prompt>$</prompt> <userinput>badblocks /dev/fd0H1440 1440 $>$ bad-blocks</userinput>
<prompt>$</prompt> <userinput>mkfs -t ext2 -l bad-blocks /dev/fd0H1440</userinput>
<computeroutput>mke2fs 0.5a, 5-Apr-94 for EXT2 FS 0.5, 94/03/10
360 inodes, 1440 blocks
72 blocks (5.00%) reserved for the super user
First data block=1
Block size=1024 (log=0)
Fragment size=1024 (log=0)
1 block group
8192 blocks per group, 8192 fragments per group
360 inodes per group
Writing inode tables: done
Writing superblocks and filesystem accounting information: done</computeroutput>
<prompt>$</prompt>
</screen>
First, the floppy was formatted (the <option>-n</option> option
prevents validation, i.e., bad block checking). Then bad blocks
were searched with <command>badblocks</command>, with the output
redirected to a file, <filename>bad-blocks</filename>. Finally,
the filesystem was created, with the bad block list initialized
by whatever <command>badblocks</command> found.</para>
<para>The <option>-c</option> option could have been used with
<command>mkfs</command> instead of <command>badblocks</command>
and a separate file. The example below does that.
<screen>
<prompt>$</prompt> <userinput>mkfs -t ext2 -c /dev/fd0H1440</userinput>
<computeroutput>mke2fs 0.5a, 5-Apr-94 for EXT2 FS 0.5, 94/03/10
360 inodes, 1440 blocks
72 blocks (5.00%) reserved for the super user
First data block=1
Block size=1024 (log=0)
Fragment size=1024 (log=0)
1 block group
8192 blocks per group, 8192 fragments per group
360 inodes per group
Checking for bad blocks (read-only test): done
Writing inode tables: done
Writing superblocks and filesystem accounting information: done</computeroutput>
<prompt>$</prompt>
</screen>
The <option>-c</option> option is more convenient than a separate use of
<command>badblocks</command>, but <command>badblocks</command> is necessary for checking
after the filesystem has been created.</para>
<para>The process to prepare filesystems on hard disks or
partitions is the same as for floppies, except that the formatting
isn't needed.</para>
</sect2>
<sect2 id="mount-and-umount">
<title>Mounting and unmounting</title>
<para>Before one can use a filesystem, it has to be <glossterm>mounted</glossterm>.
The operating system then does various bookkeeping things to
make sure that everything works. Since all files in UNIX are
in a single directory tree, the mount operation will make it
look like the contents of the new filesystem are the contents of
an existing subdirectory in some already mounted filesystem.</para>
<para>For example, <xref linkend="hd-mount-root"> shows three
separate filesystems, each with their own root directory.
When the last two filesystems are mounted below <filename>/home</filename>
and <filename>/usr</filename>, respectively, on the first filesystem, we
can get a single directory tree, as in
<xref linkend="hd-mount-all">.</para>
<figure id="hd-mount-root" float="1">
<title>Three separate filesystems.</title>
<graphic fileref="hd-mount-separate"></graphic>
</figure>
<figure id="hd-mount-all" float="1">
<title><filename>/home</filename> and <filename>/usr</filename> have been mounted.</title>
<graphic fileref="hd-mount-mounted"></graphic>
</figure>
<para>The mounts could be done as in the following example:
<screen>
<prompt>$</prompt> <userinput>mount /dev/hda2 /home</userinput>
<prompt>$</prompt> <userinput>mount /dev/hda3 /usr</userinput>
<prompt>$</prompt>
</screen>
The <command>mount</command> command takes two arguments.
The first one is the device file corresponding to the disk
or partition containing the filesystem. The second one is
the directory below which it will be mounted. After these
commands the contents of the two filesystems look just
like the contents of the <filename>/home</filename> and
<filename>/usr</filename> directories, respectively. One would
then say that ``<filename>/dev/hda2</filename> <glossterm>is
mounted on</glossterm> <filename>/home</filename>'', and
similarly for <filename>/usr</filename>. To look at either
filesystem, one would look at the contents of the directory
on which it has been mounted, just as if it were any other
directory. Note the difference between the device file,
<filename>/dev/hda2</filename>, and the mounted-on directory,
<filename>/home</filename>. The device file gives access to the
raw contents of the disk, the mounted-on directory gives access
to the files on the disk. The mounted-on directory is called
the <glossterm>mount point</glossterm>.</para>
<para>Linux supports many filesystem types. <command>mount</command> tries to
guess the type of the filesystem. You can also use the
<option>-t fstype</option> option to specify the type directly;
this is sometimes necessary, since the heuristics <command>mount</command>
uses do not always work. For example, to mount an MS-DOS
floppy, you could use the following command:
<screen>
<prompt>$</prompt> <userinput>mount -t msdos /dev/fd0 /floppy</userinput>
<prompt>$</prompt>
</screen>
</para>
<para>The mounted-on directory need not be empty, although it
must exist. Any files in it, however, will be inaccessible by
name while the filesystem is mounted. (Any files that have
already been opened will still be accessible. Files that
have hard links from other directories can be accessed using
those names.) There is no harm done with this, and it can even
be useful. For instance, some people like to have <filename>/tmp</filename>
and <filename>/var/tmp</filename> synonymous, and make <filename>/tmp</filename> be a symbolic
link to <filename>/var/tmp</filename>. When the system is booted, before
the <filename>/var</filename> filesystem is mounted, a <filename>/var/tmp</filename> directory
residing on the root filesystem is used instead. When <filename>/var</filename>
is mounted, it will make the <filename>/var/tmp</filename> directory on the root
filesystem inaccessible. If <filename>/var/tmp</filename> didn't exist on the
root filesystem, it would be impossible to use temporary files
before mounting <filename>/var</filename>.</para>
<para>If you don't intend to write anything to the filesystem, use
the <option>-r</option> switch for <command>mount</command> to do a <glossterm>readonly
mount</glossterm>. This will make the kernel stop any attempts at
writing to the filesystem, and will also stop the kernel from
updating file access times in the inodes. Read-only mounts
are necessary for unwritable media, e.g., CD-ROM's.</para>
<para>The alert reader has already noticed a slight
logistical problem. How is the first filesystem (called the <glossterm>root
filesystem</glossterm>, because it contains the root directory) mounted,
since it obviously can't be mounted on another filesystem?
Well, the answer is that it is done by magic.
<footnote><para>For more
information, see the kernel source or the Kernel Hackers'
Guide.</para></footnote>
The root filesystem is magically mounted at boot time,
and one can rely on it to always be mounted. If the
root filesystem can't be mounted, the system does not boot.
The name of the filesystem that is magically mounted as root
is either compiled into the kernel, or set using LILO or
<command>rdev</command>.</para>
<para>The root filesystem is usually first mounted readonly.
The startup scripts will then run <command>fsck</command>
to verify its validity, and if there are no problems, they
will <glossterm>re-mount</glossterm> it so that writes will
also be allowed. <command>fsck</command> must not be run on a
mounted filesystem, since any changes to the filesystem while
<command>fsck</command> is running <emphasis>will</emphasis>
cause trouble. Since the root filesystem is mounted readonly
while it is being checked, <command>fsck</command> can fix any
problems without worry, since the remount operation will flush
any metadata that the filesystem keeps in memory.</para>
<para>On many systems there are other filesystems that should
also be mounted automatically at boot time. These are specified
in the <filename>/etc/fstab</filename> file; see the fstab man
page for details on the format. The details of exactly when the
extra filesystems are mounted depend on many factors, and can be
configured by each administrator if need be; see
<xref linkend="boots-and-shutdowns">.</para>
<para>When a filesystem no longer needs to be mounted, it can be
unmounted with <command>umount</command>.
<footnote><para>It should of course be
<command>unmount</command>, but the n mysteriously disappeared in
the 70's, and hasn't been seen since. Please return it to Bell
Labs, NJ, if you find it.</footnote>
<command>umount</command> takes one argument:
either the device file or the mount point.
For example, to unmount the directories of
the previous example, one could use the commands
<screen>
<prompt>$</prompt> <userinput>umount /dev/hda2</userinput>
<prompt>$</prompt> <userinput>umount /usr</userinput>
<prompt>$</prompt>
</screen>
</para>
<para>See the man page for further instructions on how to
use the command. It is imperative that you always unmount a
mounted floppy. <emphasis>Don't just pop the floppy out of
the drive!</emphasis> Because of disk caching, the data is
not necessarily written to the floppy until you unmount it,
so removing the floppy from the drive too early might cause the
contents to become garbled. If you only read from the floppy,
this is not very likely, but if you write, even accidentally,
the result may be catastrophic.</para>
<para>Mounting and unmounting requires super user privileges, i.e.,
only root can do it. The reason for this is that if any
user can mount a floppy on any directory, then it is rather easy
to create a floppy with, say, a Trojan horse disguised as
<filename>/bin/sh</filename>, or any other often used program. However, it is
often necessary to allow users to use floppies, and there are
several ways to do this:
<itemizedlist>
<listitem><para>Give the users the root password. This is
obviously bad security, but is the easiest solution. It works
well if there is no need for security anyway, which is the case
on many non-networked, personal systems.</para></listitem>
<listitem><para>Use a program such as <command>sudo</command> to allow users to
use mount. This is still bad security, but doesn't
directly give super user privileges to
everyone.
<footnote><para>It requires several seconds of hard
thinking on the users' behalf.</para></footnote>
</para></listitem>
<listitem><para>Make the users use <command>mtools</command>, a package for manipulating
MS-DOS filesystems, without mounting them. This works
well if MS-DOS floppies are all that is needed,
but is rather awkward otherwise.
</para></listitem>
<listitem><para>List the floppy devices and their allowable mount points
together with the suitable options in <filename>/etc/fstab</filename>.
</itemizedlist>
The last alternative can be implemented by adding a line like
the following to the <filename>/etc/fstab</filename> file:
<screen>
/dev/fd0 /floppy msdos user,noauto 0 0
</screen>
The columns are: device file to mount, directory to mount
on, filesystem type, options, backup frequency (used by
<command>dump</command>), and <command>fsck</command> pass number
(to specify the order in which filesystems should be checked
upon boot; 0 means no check).</para>
<para>The <option>noauto</option> option stops this mount to be done
automatically when the system is started (i.e., it stops
<command>mount -a</command> from mounting it). The <option>user</option> option
allows any user to mount the filesystem, and, because of security
reasons, disallows execution of programs (normal or setuid)
and interpretation of device files from the mounted filesystem.
After this, any user can mount a floppy with an msdos
filesystem with the following command:
<screen>
<prompt>$</prompt> <userinput>mount /floppy</userinput>
<prompt>$</prompt>
</screen>
The floppy can (and needs to, of course) be unmounted with
the corresponding <command>umount</command> command.</para>
<para>If you want to provide access to several types of floppies,
you need to give several mount points. The settings can be
different for each mount point. For example, to give access
to both MS-DOS and ext2 floppies, you could have the following
to lines in <filename>/etc/fstab</filename>:
<screen>
/dev/fd0 /dosfloppy msdos user,noauto 0 0
/dev/fd0 /ext2floppy ext2 user,noauto 0 0
</screen>
For MS-DOS filesystems (not just floppies), you probably want
to restrict access to it by using the <option>uid</option>,
<option>gid</option>, and <option>umask</option> filesystem
options, described in detail on the <command>mount</command>
manual page. If you aren't careful, mounting an MS-DOS filesystem
gives everyone at least read access to the files in it, which
is not a good idea.</para>
</sect2>
<sect2>
<title>Checking filesystem integrity with <command>fsck</command></title>
<para>Filesystems are complex creatures, and as such, they
tend to be somewhat error-prone. A filesystem's correctness and
validity can be checked using the <command>fsck</command> command.
It can be instructed to repair any minor problems it finds, and to
alert the user if there any unrepairable problems. Fortunately,
the code to implement filesystems is debugged quite effectively,
so there are seldom any problems at all, and they are usually
caused by power failures, failing hardware, or operator errors;
for example, by not shutting down the system properly.</para>
<para>Most systems are setup to run <command>fsck</command>
automatically at boot time, so that any errors are detected
(and hopefully corrected) before the system is used. Use of
a corrupted filesystem tends to make things worse: if the
data structures are messed up, using the filesystem will
probably mess them up even more, resulting in more data loss.
However, <command>fsck</command> can take a while to run on big
filesystems, and since errors almost never occur if the system
has been shut down properly, a couple of tricks are used to
avoid doing the checks in such cases. The first is that if
the file <filename>/etc/fastboot</filename> exists, no checks
are made. The second is that the ext2 filesystem has a special
marker in its superblock that tells whether the filesystem
was unmounted properly after the previous mount. This allows
<command>e2fsck</command> (the version of <command>fsck</command>
for the ext2 filesystem) to avoid checking the filesystem if
the flag indicates that the unmount was done (the assumption
being that a proper unmount indicates no problems). Whether the
<filename>/etc/fastboot</filename> trick works on your system
depends on your startup scripts, but the ext2 trick works
every time you use <command>e2fsck</command>. It has to be
explicitly bypassed with an option to <command>e2fsck</command>
to be avoided. (See the <command>e2fsck</command> man page for
details on how.)</para>
<para>The automatic checking only works for the
filesystems that are mounted automatically at boot time.
Use <command>fsck</command> manually to check other filesystems,
e.g., floppies.</para>
<para>If <command>fsck</command> finds unrepairable problems,
you need either in-depth knowlege of how filesystems work in
general, and the type of the corrupt filesystem in particular,
or good backups. The latter is easy (although sometimes tedious)
to arrange, the former can sometimes be arranged via a friend,
the Linux newsgroups and mailing lists, or some other source of
support, if you don't have the know-how yourself. I'd like to
tell you more about it, but my lack of education and experience
in this regard hinders me. The <command>debugfs</command>
program by Theodore T'so should be useful.</para>
<para><command>fsck</command> must only be run on unmounted
filesystems, never on mounted filesystems (with the exception of
the read-only root during startup). This is because it accesses
the raw disk, and can therefore modify the filesystem without the
operating system realizing it. There <emphasis>will</emphasis>
be trouble, if the operating system is confused.</para>
</sect2>
<sect2>
<title>Checking for disk errors with <command>badblocks</command></title>
<para>It can be a good idea to periodically check for bad blocks.
This is done with the <command>badblocks</command> command. It outputs
a list of the numbers of all bad blocks it can find. This list
can be fed to <command>fsck</command> to be recorded
in the filesystem data structures so that the operating system
won't try to use the bad blocks for storing data.
The following example will show how this could be done.
<screen>
<prompt>$</prompt> <userinput>badblocks /dev/fd0H1440 1440 > bad-blocks</userinput>
<prompt>$</prompt> <userinput>fsck -t ext2 -l bad-blocks /dev/fd0H1440</userinput>
<computeroutput>Parallelizing fsck version 0.5a (5-Apr-94)
e2fsck 0.5a, 5-Apr-94 for EXT2 FS 0.5, 94/03/10
Pass 1: Checking inodes, blocks, and sizes
Pass 2: Checking directory structure
Pass 3: Checking directory connectivity
Pass 4: Check reference counts.
Pass 5: Checking group summary information.
/dev/fd0H1440: ***** FILE SYSTEM WAS MODIFIED *****
/dev/fd0H1440: 11/360 files, 63/1440 blocks</computeroutput>
<prompt>$</prompt>
</screen>
If badblocks reports a block that was already used,
<command>e2fsck</command> will try to move the block to another
place. If the block was really bad, not just marginal, the
contents of the file may be corrupted.</para>
</sect2>
<sect2>
<title>Fighting fragmentation</title>
<para>When a file is written to disk, it can't always be written
in consecutive blocks. A file that is not stored in
consecutive blocks is <glossterm>fragmented</glossterm>. It takes longer
to read a fragmented file, since the disk's read-write head
will have to move more. It is desireable to avoid fragmentation,
although it is less of a problem in a system with a good buffer
cache with read-ahead.</para>
<para>The ext2 filesystem attempts to keep fragmentation at a
minimum, by keeping all blocks in a file close together, even if
they can't be stored in consecutive sectors. Ext2 effectively
always allocates the free block that is nearest to other blocks
in a file. For ext2, it is therefore seldom necessary to worry
about fragmentation. There is a program for defragmenting an
ext2 filesystem, see XXX (ext2-defrag) in the bibliography.</para>
<para>There are many MS-DOS defragmentation programs that
move blocks around in the filesystem to remove fragmentation.
For other filesystems, defragmentation must be done by backing
up the filesystem, re-creating it, and restoring the files
from backups. Backing up a filesystem before defragmening is
a good idea for all filesystems, since many things can go wrong
during the defragmentation.</para>
</sect2>
<sect2>
<title>Other tools for all filesystems</title>
<para>Some other tools are also useful for managing filesystems.
<command>df</command> shows the free disk space on one or more
filesystems; <command>du</command> shows how much disk space a
directory and all its files contain. These can be used to hunt
down disk space wasters.</para>
<para><command>sync</command> forces all unwritten blocks
in the buffer cache (see <xref linkend="buffer-cache">) to
be written to disk. It is seldom necessary to do this by
hand; the daemon process <command>update</command> does
this automatically. It can be useful in catastrophies,
for example if <command>update</command> or its helper
process <command>bdflush</command> dies, or if you must
turn off power <emphasis>now</emphasis> and can't wait for
<command>update</command> to run.</para>
</sect2>
<sect2>
<title>Other tools for the ext2 filesystem</title>
<para>In addition to the filesystem creator (<command>mke2fs</command>) and
checker (<command>e2fsck</command>) accessible directly or via the
filesystem type independent front ends, the ext2
filesystem has some additional tools that can be useful.</para>
<para><command>tune2fs</command> adjusts filesystem parameters. Some of the
more interesting parameters are:
<itemizedlist>
<listitem><para>
A maximal mount count. <command>e2fsck</command> enforces a check when
filesystem has been mounted too many times, even if
the clean flag is set. For a system that is used for
developing or testing the system, it might be a good
idea to reduce this limit.
</para></listitem>
<listitem><para>
A maximal time between checks. <command>e2fsck</command> can also enforce
a maximal time between two checks, even if the clean
flag is set, and the filesystem hasn't been mounted very
often. This can be disabled, however.
</para></listitem>
<listitem><para>
Number of blocks reserved for root. Ext2
reserves some blocks for root so that if the
filesystem fills up, it is still possible to do system
administration without having to delete anything. The
reserved amount is by default 5 percent, which on most disks
isn't enough to be wasteful. However, for floppies there
is no point in reserving any blocks.
</para></listitem>
</itemizedlist>
See the <command>tune2fs</command> manual page for more
information.</para>
<para><command>dumpe2fs</command> shows information about an ext2 filesystem, mostly
from the superblock. <xref linkend="dumpe2fs-output"> shows
a sample output. Some of the information in the output is
technical and requires understanding of how the filesystem
works (see appendix XXX ext2fspaper), but much of
it is readily understandable even for layadmins.</para>
<figure id="dumpe2fs-output" float="1">
<title>Sample output from <command>dumpe2fs</command></title>
<literallayout>
dumpe2fs 0.5b, 11-Mar-95 for EXT2 FS 0.5a, 94/10/23
Filesystem magic number: 0xEF53
Filesystem state: clean
Errors behavior: Continue
Inode count: 360
Block count: 1440
Reserved block count: 72
Free blocks: 1133
Free inodes: 326
First block: 1
Block size: 1024
Fragment size: 1024
Blocks per group: 8192
Fragments per group: 8192
Inodes per group: 360
Last mount time: Tue Aug 8 01:52:52 1995
Last write time: Tue Aug 8 01:53:28 1995
Mount count: 3
Maximum mount count: 20
Last checked: Tue Aug 8 01:06:31 1995
Check interval: 0
Reserved blocks uid: 0 (user root)
Reserved blocks gid: 0 (group root)
Group 0:
Block bitmap at 3, Inode bitmap at 4, Inode table at 5
1133 free blocks, 326 free inodes, 2 directories
Free blocks: 307-1439
Free inodes: 35-360
</literallayout>
</figure>
<para><command>debugfs</command> is a filesystem debugger.
It allows direct access to the filesystem data structures
stored on disk and can thus be used to repair a disk that is so
broken that <command>fsck</command> can't fix it automatically.
It has also been known to be used to recover deleted files.
However, <command>debugfs</command> very much requires that
you understand what you're doing; a failure to understand can
destroy all your data.</para>
<para><command>dump</command> and <command>restore</command> can be used to back up an
ext2 filesystem. They are ext2 specific versions of the
traditional UNIX backup tools. See <xref linkend="backups">
for more information on backups.</para>
</sect2>
</sect1>
<sect1>
<title>Disks without filesystems</title>
<para>Not all disks or partitions are used as filesystems.
A swap partition, for example, will not have a filesystem on it.
Many floppies are used in a tape-drive emulating fashion, so that
a <command>tar</command> or other file is written directly on
the raw disk, without a filesystem. Linux boot floppies don't
contain a filesystem, only the raw kernel.</para>
<para>Avoiding a filesystem has the advantage of making more of
the disk usable, since a filesystem always has some bookkeeping
overhead. It also makes the disks more easily compatible
with other systems: for example, the <command>tar</command>
file format is the same on all systems, while filesystems are
different on most systems. You will quickly get used to disks
without filesystems if you need them. Bootable Linux floppies
also do not necessarily have a filesystem, although that is
also possible.</para>
<para>One reason to use raw disks is to make image copies of them.
For instance, if the disk contains a partially damaged filesystem,
it is a good idea to make an exact copy of it before trying to
fix it, since then you can start again if your fixing breaks things
even more. One way to do this is to use <command>dd</command>:
<screen>
<prompt>$</prompt> <userinput>dd if=/dev/fd0H1440 of=floppy-image</userinput>
<computeroutput>2880+0 records in
2880+0 records out</computeroutput>
<prompt>$</prompt> <userinput>dd if=floppy-image of=/dev/fd0H1440</userinput>
<computeroutput>2880+0 records in
2880+0 records out</computeroutput>
<prompt>$</prompt>
</screen>
The first <command>dd</command> makes an exact image of the
floppy to the file <filename>floppy-image</filename>, the second
one writes the image to the floppy. (The user has presumably
switched the floppy before the second command. Otherwise the
command pair is of doubtful usefulness.)</para>
</sect1>
<sect1>
<title>Allocating disk space</title>
<sect2>
<title>Partitioning schemes</title>
<para>It is not easy to partition a disk in the best possible way.
Worse, there is no universally correct way to do it; there are
too many factors involved.</para>
<para>The traditional way is to have a (relatively) small
root filesystem, which contains <filename>/bin</filename>,
<filename>/etc</filename>, <filename>/dev</filename>,
<filename>/lib</filename>, <filename>/tmp</filename>, and other
stuff that is needed to get the system up and running. This way,
the root filesystem (in its own partition or on its own disk)
is all that is needed to bring up the system. The reasoning is
that if the root filesystem is small and is not heavily used,
it is less likely to become corrupt when the system crashes, and
you will therefore find it easier to fix any problems caused by
the crash. Then you create separate partitions or use separate
disks for the directory tree below <filename>/usr</filename>, the
users' home directories (often under <filename>/home</filename>),
and the swap space. Separating the home directories (with the
users' files) in their own partition makes backups easier, since
it is usually not necessary to backup programs (which reside
below <filename>/usr</filename>). In a networked environment it
is also possible to share <filename>/usr</filename> among several
machines (e.g., by using NFS), thereby reducing the total disk
space required by several tens or hundreds of megabytes times
the number of machines.</para>
<para>The problem with having many partitions is that it splits
the total amount of free disk space into many small pieces.
Nowadays, when disks and (hopefully) operating systems are
more reliable, many people prefer to have just one partition
that holds all their files. On the other hand, it can be less
painful to back up (and restore) a small partition.</para>
<!--
% \meta more reasons for many partitions: users/temp files/spools
% can't fill up all disks, readonly partitions less likely to corrupt,
% fsck is faster, limits losses a filesystem goes really wrong,
% logging must not be disturbed, boots from >1023 cylinders do not
% work on all BIOS's, /usr/local won't be disturbed by an upgrade,
% easy to divide backup on many tapes, spare (scratch) partition for
% experimentation (e.g., a new Linux distribution), scratch can
% also be used to backup root during upgrades
-->
<para>For a small hard disk (assuming you don't do kernel
development), the best way to go is probably to have just one
partition. For large hard disks, it is probably
better to have a few large partitions, just in case
something does go wrong. (Note that `small' and `large' are
used in a relative sense here; your needs for disk space
decide what the threshold is.)</para>
<para>If you have several disks, you might wish to have the
root filesystem (including <filename>/usr</filename>) on one,
and the users' home directories on another.</para>
<para>It is a good idea to be prepared to experiment a bit
with different partitioning schemes (over time, not just
while first installing the system). This is a bit of work,
since it essentially requires you to install the system from
scratch several times, but it is the only way to be sure you do
it right.</para>
</sect2>
<sect2>
<title>Space requirements</title>
<para>The Linux distribution you install will give some indication
of how much disk space you need for various configurations.
Programs installed separately may also do the same. This will
help you plan your disk space usage, but you should prepare
for the future and reserve some extra space for things you will
notice later that you need.</para>
<para>The amount you need for user files depends on what your
users wish to do. Most people seem to need as much space for
their files as possible, but the amount they will live happily
with varies a lot. Some people do only light text processing
and will survive nicely with a few megabytes, others do heavy
image processing and will need gigabytes.</para>
<para>By the way, when comparing file sizes given in
kilobytes or megabytes and disk space given in megabytes, it
can be important to know that the two units can be different.
Some disk manufacturers like to pretend that a kilobyte is 1000
bytes and a megabyte is 1000 kilobytes, while all the rest of
the computing world uses 1024 for both factors. Therefore,
my 345 MB hard disk was really a 330 MB hard disk.
<footnote><para>Sic transit discus mundi.</para></footnote>
</para>
<para>Swap space allocation is discussed in <xref
linkend="swap-allocation">.</para>
</sect2>
<sect2>
<title>Examples of hard disk allocation</title>
<para>I used to have a 109 MB hard disk. Now I am using a 330 MB
hard disk. I'll explain how and why I partitioned these
disks.</para>
<para>The 109 MB disk I partitioned in a lot of ways, when my
needs and the operating systems I used changed; I'll explain
two typical scenarios. First, I used to run MS-DOS together
with Linux. For that, I needed about 20 MB of hard disk, or
just enough to have MS-DOS, a C compiler, an editor, a few other
utilities, the program I was working on, and enough free disk
space to not feel claustrophobic. For Linux, I had a 10 MB swap
partition, and the rest, or 79 MB, was a single partition with all
the files I had under Linux. I experimented with having separate
root, <filename>/usr</filename>, and <filename>/home</filename>
partitions, but there was never enough free disk space in one
piece to do much interesting.</para>
<para>When I didn't need MS-DOS anymore, I repartitioned the
disk so that I had a 12 MB swap partition, and again had the
rest as a single filesystem.</para>
<para>The 330 MB disk is partitioned into several partitions, like
this:
<informaltable>
<tgroup cols=2>
<tbody>
<row> <entry>5 MB</entry> <entry>root filesystem</entry> </row>
<row> <entry> 10 MB</entry> <entry>swap partition</entry> </row>
<row> <entry>180 MB</entry> <entry><filename>/usr</filename> filesystem</entry> </row>
<row> <entry>120 MB</entry> <entry><filename>/home</filename> filesystem</entry> </row>
<row> <entry> 15 MB</entry> <entry>scratch partition</entry> </row>
</tbody>
</tgroup>
</informaltable>
The scratch partition is for playing around with things that
require their own partition, e.g., trying different Linux
distributions, or comparing speeds of filesystems. When not
needed for anything else, it is used as swap space (I like to
have a lot of open windows).</para>
</sect2>
<sect2>
<title>Adding more disk space for Linux</title>
<para>Adding more disk space for Linux is easy, at least after the
hardware has been properly installed (the hardware installation
is outside the scope of this book). You format it if necessary,
then create the partitions and filesystem as described above,
and add the proper lines to <filename>/etc/fstab</filename>
so that it is mounted automatically.</para>
</sect2>
<sect2>
<title>Tips for saving disk space</title>
<para>The best tip for saving disk space is to avoid installing
unnecessary programs. Most Linux distributions have an
option to install only part of the packages they contain,
and by analyzing your needs you might notice that you don't
need most of them. This will help save a lot of disk space,
since many programs are quite large. Even if you do need a
particular package or program, you might not need all of it.
For example, some on-line documentation might be unnecessary,
as might some of the Elisp files for GNU Emacs, some of the
fonts for X11, or some of the libraries for programming.</para>
<para>If you cannot uninstall packages, you might look into
compression. Compression programs such as <command>gzip</command>
or <command>zip</command> will compress (and uncompress)
individual files or groups of files. The <command>gzexe</command>
system will compress and uncompress programs invisibly to the
user (unused programs are compressed, then uncompressed as they
are used). The experimental DouBle system will compress all
files in a filesystem, invisibly to the programs that use them.
(If you are familiar with products such as Stacker for MS-DOS,
the principle is the same.)</para>
</sect2>
</sect1>
</chapter>
<chapter id="memory-management">
<title>Memory Management</title>
<blockquote><para><quote>Minnet, jag har tappat mitt minne,
r jag svensk eller finne, kommer inte ihg...</quote>
(Bosse sterberg)
</para></blockquote>
<para> This section describes the Linux memory management
features, i.e., virtual memory and the disk buffer cache.
The purpose and workings and the things the system administrator
needs to take into consideration are described.</para>
<sect1>
<title>What is virtual memory?</title>
<para>Linux supports <glossterm>virtual memory</glossterm>, that
is, using a disk as an extension of RAM so that the effective
size of usable memory grows correspondingly. The kernel will
write the contents of a currently unused block of memory to the
hard disk so that the memory can be used for another purpose.
When the original contents are needed again, they are read back
into memory. This is all made completely transparent to the
user; programs running under Linux only see the larger amount of
memory available and don't notice that parts of them reside on
the disk from time to time. Of course, reading and writing the
hard disk is slower (on the order of a thousand times slower)
than using real memory, so the programs don't run as fast.
The part of the hard disk that is used as virtual memory is
called the <glossterm>swap space</glossterm>.</para>
<para>Linux can use either a normal file in the filesystem or a
separate partition for swap space. A swap partition is
faster, but it is easier to change the size of a swap file
(there's no need to repartition the whole hard disk, and
possibly install everything from scratch). When you know how
much swap space you need, you should go for a swap partition,
but if you are uncertain, you can use a swap file first, use
the system for a while so that you can get a feel for how much
swap you need, and then make a swap partition when you're
confident about its size.</para>
<para>You should also know that Linux allows one to use several swap
partitions and/or swap files at the same time. This means
that if you only occasionally need an unusual amount of swap space,
you can set up an extra swap file at such times, instead of
keeping the whole amount allocated all the time.</para>
<para>A note on operating system terminology: computer science usually
distinguishes between swapping (writing the whole process out to
swap space) and paging (writing only fixed size parts, usually
a few kilobytes, at a time). Paging is usually more efficient,
and that's what Linux does, but traditional Linux terminology
talks about swapping anyway.
<footnote><para>Thus quite needlessly annoying a
number of computer scientists something horrible.
</para></footnote>
</para>
</sect1>
<sect1>
<title>Creating a swap space</title>
<para>A swap file is an ordinary file; it is in no way special
to the kernel. The only thing that matters to the kernel is
that it has no holes, and that it is prepared for use with
<command>mkswap</command>. It must reside on a local disk,
however; it can't reside in a filesystem that has been mounted
over NFS due to implementation reasons.</para>
<para>The bit about holes is important. The swap file reserves
the disk space so that the kernel can quickly swap out a page
without having to go through all the things that are necessary
when allocating a disk sector to a file. The kernel merely
uses any sectors that have already been allocated to the file.
Because a hole in a file means that there are no disk sectors
allocated (for that place in the file), it is not good for the
kernel to try to use them.</para>
<para>One good way to create the swap file without holes is through
the following command:
<screen>
<prompt>$</prompt> <userinput>dd if=/dev/zero of=/extra-swap bs=1024 count=1024</userinput>
<computeroutput>1024+0 records in
1024+0 records out</computeroutput>
<prompt>$</prompt>
</screen>
where <filename>/extra-swap</filename> is the name of the swap
file and the size of is given after the <literal>count=</literal>.
It is best for the size to be a multiple of 4, because the
kernel writes out <glossterm>memory pages</glossterm>, which
are 4 kilobytes in size. If the size is not a multiple of 4,
the last couple of kilobytes may be unused.</para>
<para>A swap partition is also not special in any way. You create
it just like any other partition; the only difference is that
it is used as a raw partition, that is, it will not contain any
filesystem at all. It is a good idea to mark swap partitions
as type 82 (Linux swap); this will the make partition listings
clearer, even though it is not strictly necessary to the
kernel.</para>
<para>After you have created a swap file or a swap partition, you
need to write a signature to its beginning; this contains some
administrative information and is used by the kernel. The
command to do this is <command>mkswap</command>, used like this:
<screen>
<prompt>$</prompt> <userinput>mkswap /extra-swap 1024</userinput>
<computeroutput>Setting up swapspace, size = 1044480 bytes</computeroutput>
<prompt>$</prompt>
</screen>
Note that the swap space is still not in use yet: it exists,
but the kernel does not use it to provide virtual memory.</para>
<para>You should be very careful when using
<command>mkswap</command>, since it does not check that the
file or partition isn't used for anything else. <emphasis>You
can easily overwrite important files and partitions with
<command>mkswap</command>!</emphasis> Fortunately, you should
only need to use <command>mkswap</command> when you install
your system.</para>
<para>The Linux memory manager limits the size of each swap space to
about 127 MB (for various technical reasons, the actual limit
is (4096-10) * 8 * 4096 = 133890048$ bytes, or
127.6875 megabytes). You can, however, use up to
8 swap spaces simultaneously, for a total of almost
1 GB.
<footnote><para>A gigabyte here, a gigabyte there, pretty
soon we start talking about real memory.</para></footnote>
</para>
</sect1>
<sect1>
<title>Using a swap space</title>
<para>An initialized swap space is taken into use with
<command>swapon</command>. This command tells the kernel that
the swap space can be used. The path to the swap space is given
as the argument, so to start swapping on a temporary swap file
one might use the following command.
<screen>
<prompt>$</prompt> <userinput>swapon /extra-swap</userinput>
<prompt>$</prompt>
</screen>
Swap spaces can be used automatically by listing them in
the <filename>/etc/fstab</filename> file.
<screen>
/dev/hda8 none swap sw 0 0
/swapfile none swap sw 0 0
</screen>
The startup scripts will run the command <command>swapon
-a</command>, which will start swapping on all the swap
spaces listed in <command>/etc/fstab</command>. Therefore,
the <command>swapon</command> command is usually used only when
extra swap is needed.</para>
<para>You can monitor the use of swap spaces with
<command>free</command>. It will tell the total amount of swap
space used.
<screen>
<prompt>$</prompt> <userinput>free</userinput>
<computeroutput> total used free shared buffers
Mem: 15152 14896 256 12404 2528
-/+ buffers: 12368 2784
Swap: 32452 6684 25768</computeroutput>
<prompt>$</prompt>
</screen>
The first line of output (<literal>Mem:</literal>) shows the
physical memory. The total column does not show the physical
memory used by the kernel, which is usually about a megabyte.
The used column shows the amount of memory used (the second
line does not count buffers). The free column shows completely
unused memory. The shared column shows the amount of memory
shared by several processes; the more, the merrier. The buffers
column shows the current size of the disk buffer cache.</para>
<para>That last line (<literal>Swap:</literal>) shows similar
information for the swap spaces. If this line is all zeroes,
your swap space is not activated.</para>
<para>The same information is available via
<command>top</command>, or using the proc filesystem in file
<filename>/proc/meminfo</filename>. It is currently difficult
to get information on the use of a specific swap space.</para>
<para>A swap space can be removed from use with
<command>swapoff</command>. It is usually not necessary to do it,
except for temporary swap spaces. Any pages in use in the swap
space are swapped in first; if there is not sufficient physical
memory to hold them, they will then be swapped out (to some other
swap space). If there is not enough virtual memory to hold all
of the pages Linux will start to thrash; after a long while it
should recover, but meanwhile the system is unusable. You should
check (e.g., with <command>free</command>) that there is enough
free memory before removing a swap space from use.</para>
<para>All the swap spaces that are used automatically
with <command>swapon -a</command> can be removed from use
with <command>swapoff -a</command>; it looks at the file
<filename>/etc/fstab</filename> to find what to remove.
Any manually used swap spaces will remain in use.</para>
<para>Sometimes a lot of swap space can be in use even though
there is a lot of free physical memory. This can happen for
instance if at one point there is need to swap, but later a big
process that occupied much of the physical memory terminates
and frees the memory. The swapped-out data is not automatically
swapped in until it is needed, so the physical memory may remain
free for a long time. There is no need to worry about this,
but it can be comforting to know what is happening. </para>
</sect1>
<sect1>
<title>Sharing swap spaces with other operating systems</title>
<para>Virtual memory is built into many operating systems.
Since they each need it only when they are running, i.e., never at
the same time, the swap spaces of all but the currently running
one are being wasted. It would be more efficient for them to
share a single swap space. This is possible, but can require a
bit of hacking. The Tips-HOWTO contains some advice on how to
implement this. </para>
</sect1>
<sect1 id="swap-allocation">
<title>Allocating swap space</title>
<para>Some people will tell you that you should allocate twice as much
swap space as you have physical memory, but this is a bogus rule.
Here's how to do it properly:
<itemizedlist>
<listitem>
<para> Estimate your total memory needs. This is the largest
amount of memory you'll probably need at a time, that is the
sum of the memory requirements of all the programs you want to
run at the same time. This can be done by running at the same
time all the programs you are likely to ever be running at the
same time. </para>
<para>For instance, if you want to run X, you should allocate
about 8 MB for it, gcc wants several megabytes (some
files need an unusually large amount, up to tens of
megabytes, but usually about four should do), and so on.
The kernel will use about a megabyte by itself, and the
usual shells and other small utilities perhaps a few
hundred kilobytes (say a megabyte together). There is
no need to try to be exact, rough estimates are fine,
but you might want to be on the pessimistic side.</para>
<para>Remember that if there are going to be several people
using the system at the same time, they are all going
to consume memory. However, if two people run the same
program at the same time, the total memory consumption
is usually not double, since code pages and shared
libraries exist only once.</para>
<para>The <command>free</command> and <command>ps</command>
commands are useful for estimating the memory needs.
</listitem>
<listitem>
<para>Add some security to the estimate in step 1. This is because
estimates of program sizes will probably be wrong, because
you'll probably forget some programs you want to run, and to
make certain that you have some extra space just in case. A
couple of megabytes should be fine. (It is better to allocate
too much than too little swap space, but there's no need to
over-do it and allocate the whole disk, since unused swap space
is wasted space; see later about adding more swap.) Also,
since it is nicer to deal with even numbers, you can round the
value up to the next full megabyte.</para>
</listitem>
<listitem>
<para>Based on the computations above, you know how much memory
you'll be needing in total. So, in order to allocate swap
space, you just need to subtract the size of your physical
memory from the total memory needed, and you know how much
swap space you need. (On some versions of UNIX, you need to
allocate space for an image of the physical memory as well, so
the amount computed in step 2 is what you need and you shouldn't
do the subtraction.)</para>
</listitem>
<listitem>
<para>If your calculated swap space is very much larger than your
physical memory (more than a couple times larger), you should
probably invest in more physical memory, otherwise performance
will be too low.</para>
</itemizedlist>
<para>It's a good idea to have at least some swap space, even if
your calculations indicate that you need none. Linux uses
swap space somewhat aggressively, so that as much physical
memory as possible can be kept free. Linux will swap out
memory pages that have not been used, even if the memory
is not yet needed for anything. This avoids waiting for
swapping when it is needed: the swapping can be done
earlier, when the disk is otherwise idle.</para>
<para>Swap space can be divided among several disks. This
can sometimes improve performance, depending on the
relative speeds of the disks and the access patterns
of the disks. You might want to experiment with a few
schemes, but be aware that doing the experiments
properly is quite difficult. You should not believe
claims that any one scheme is superior to any other,
since it won't always be true.
</para>
</sect1>
<sect1 id="buffer-cache">
<title>The buffer cache</title>
<para>Reading from a disk
<footnote><para>Except a RAM disk, for obvious
reasons.</para></footnote>
is very slow compared to accessing (real) memory. In addition,
it is common to read the same part of a disk several times
during relatively short periods of time. For example, one
might first read an e-mail message, then read the letter into
an editor when replying to it, then make the mail program read
it again when copying it to a folder. Or, consider how often
the command <command>ls</command> might be run on a system with
many users. By reading the information from disk only once
and then keeping it in memory until no longer needed, one can
speed up all but the first read. This is called <glossterm>disk
buffering</glossterm>, and the memory used for the purpose is
called the <glossterm>buffer cache</glossterm>.</para>
<para>Since memory is, unfortunately, a finite, nay, scarce
resource, the buffer cache usually cannot be big enough (it
can't hold all the data one ever wants to use). When the cache
fills up, the data that has been unused for the longest time
is discarded and the memory thus freed is used for the new
data.</para>
<para>Disk buffering works for writes as well. On the one hand,
data that is written is often soon read again (e.g., a source
code file is saved to a file, then read by the compiler),
so putting data that is written in the cache is a good idea.
On the other hand, by only putting the data into the cache, not
writing it to disk at once, the program that writes runs quicker.
The writes can then be done in the background, without slowing
down the other programs.</para>
<para>Most operating systems have buffer caches (although
they might be called something else), but not all of
them work according to the above principles. Some are
<glossterm>write-through</glossterm>: the data is written to disk
at once (it is kept in the cache as well, of course). The cache
is called <glossterm>write-back</glossterm> if the writes are done
at a later time. Write-back is more efficient than write-through,
but also a bit more prone to errors: if the machine crashes,
or the power is cut at a bad moment, or the floppy is removed
from the disk drive before the data in the cache waiting to be
written gets written, the changes in the cache are usually lost.
This might even mean that the filesystem (if there is one) is
not in full working order, perhaps because the unwritten data
held important changes to the bookkeeping information.</para>
<para>Because of this, you should never turn off the
power without using a proper shutdown procedure (see <xref
linkend="boots-and-shutdowns">), or remove a floppy from the
disk drive until it has been unmounted (if it was mounted)
or after whatever program is using it has signaled that it
is finished and the floppy drive light doesn't shine anymore.
The <command>sync</command> command <glossterm>flushes</glossterm>
the buffer, i.e., forces all unwritten data to be written to disk,
and can be used when one wants to be sure that everything is
safely written. In traditional UNIX systems, there is a program
called <command>update</command> running in the background
which does a <command>sync</command> every 30 seconds, so
it is usually not necessary to use <command>sync</command>.
Linux has an additional daemon, <command>bdflush</command>,
which does a more imperfect sync more frequently to avoid the
sudden freeze due to heavy disk I/O that <command>sync</command>
sometimes causes.</para>
<para>Under Linux, <command>bdflush</command> is started by
<command>update</command>. There is usually no reason to worry
about it, but if <command>bdflush</command> happens to die for
some reason, the kernel will warn about this, and you should
start it by hand (<command>/sbin/update</command>).</para>
<para>The cache does not actually buffer files, but blocks, which
are the smallest units of disk I/O (under Linux, they are usually
1 kB). This way, also directories, super blocks, other filesystem
bookkeeping data, and non-filesystem disks are cached.</para>
<para>The effectiveness of a cache is primarily decided by its
size. A small cache is next to useless: it will hold so little
data that all cached data is flushed from the cache before it
is reused. The critical size depends on how much data is read
and written, and how often the same data is accessed. The only
way to know is to experiment.</para>
<para>If the cache is of a fixed size, it is not very good to have
it too big, either, because that might make the free memory too
small and cause swapping (which is also slow). To make the most
efficient use of real memory, Linux automatically uses all free
RAM for buffer cache, but also automatically makes the cache
smaller when programs need more memory.</para>
<para>Under Linux, you do not need to do anything to make use
of the cache, it happens completely automatically. Except for
following the proper procedures for shutdown and removing
floppies, you do not need to worry about it. </para>
</chapter>
<chapter id="boots-and-shutdowns">
<title>Boots And Shutdowns</title>
<blockquote><para><literallayout>
Start me up
Ah... you've got to... you've got to
Never, never never stop
Start it up
Ah... start it up, never, never, never
You make a grown man cry,
you make a grown man cry
(Rolling Stones)
</literallayout></para></blockquote>
<para> This section explains what goes on when a Linux system is
brought up and taken down, and how it should be done properly.
If proper procedures are not followed, files might be corrupted
or lost.</para>
<sect1>
<title>An overview of boots and shutdowns</title>
<para>The act of turning on a computer system and causing its
operating system to be loaded
<footnote><para>On early computers, it wasn't enough
to merely turn on the computer, you had to manually load the
operating system as well. These new-fangled thing-a-ma-jigs do
it all by themselves.</para></footnote>
is called <glossterm>booting</glossterm>. The name comes from
an image of the computer pulling itself up from its bootstraps,
but the act itself slightly more realistic.</para>
<para>During bootstrapping, the computer first loads a small piece
of code called the <glossterm>bootstrap loader</glossterm>, which
in turn loads and starts the operating system. The bootstrap
loader is usually stored in a fixed location on a hard disk
or a floppy. The reason for this two step process is that
the operating system is big and complicated, but the first
piece of code that the computer loads must be very small (a
few hundred bytes), to avoid making the firmware unnecessarily
complicated.</para>
<para>Different computers do the bootstrapping differently.
For PC's, the computer (its BIOS) reads in the first sector
(called the <glossterm>boot sector</glossterm>) of a floppy or
hard disk. The bootstrap loader is contained within this sector.
It loads the operating system from elsewhere on the disk (or
from some other place).</para>
<para>After Linux has been loaded, it initializes the hardware and
device drivers, and then runs <command>init</command>. <command>init</command>
starts other processes to allow users to log in, and do things.
The details of this part will be discussed below.</para>
<para>In order to shut down a Linux system, first all processes
are told to terminate (this makes them close any files and
do other necessary things to keep things tidy), then filesystems
and swap areas are unmounted, and finally a message is printed
to the console that the power can be turned off. If the proper
procedure is not followed, terrible things can and will happen;
most importantly, the filesystem buffer cache might not be flushed,
which means that all data in it is lost and the filesystem on
disk is inconsistent, and therefore possibly unusable.
</para>
</sect1>
<sect1>
<title>The boot process in closer look</title>
<para>You can boot Linux either from a floppy or from the hard
disk. The installation section in the Installation and
Getting Started guide (XXX citation)
tells you how to install Linux so you can boot it the way
you want to.</para>
<para>When a PC is booted, the BIOS will do various tests to
check that everything looks all right,
<footnote><para>This is called
the <glossterm>power on self test</glossterm>, or
<glossterm>POST</glossterm> for short.</para></footnote>
and will then start the actual booting. It will choose a disk
drive (typically the first floppy drive, if there is a floppy
inserted, otherwise the first hard disk, if one is installed
in the computer; the order might be configurable, however)
and will then read its very first sector. This is called the
<glossterm>boot sector</glossterm>; for a hard disk, it is also
called the <glossterm>master boot record</glossterm>, since a
hard disk can contain several partitions, each with their own
boot sectors.</para>
<para>The boot sector contains a small program (small enough to
fit into one sector) whose responsibility is to read the actual
operating system from the disk and start it. When booting Linux
from a floppy disk, the boot sector contains code that just reads
the first few hundred blocks (depending on the actual kernel
size, of course) to a predetermined place in memory. On a Linux
boot floppy, there is no filesystem, the kernel is just stored
in consecutive sectors, since this simplifies the boot process.
It is possible, however, to boot from a floppy with a filesystem,
by using LILO, the LInux LOader.</para>
<para>When booting from the hard disk, the code in the master
boot record will examine the partition table (also in the master
boot record), identify the active partition (the partition that is
marked to be bootable), read the boot sector from that partition,
and then start the code in that boot sector. The code in the
partition's boot sector does what a floppy disk's boot sector
does: it will read in the kernel from the partition and start it.
The details vary, however, since it is generally not useful to
have a separate partition for just the kernel image, so the
code in the partition's boot sector can't just read the disk
in sequential order, it has to find the sectors wherever the
filesystem has put them. There are several ways around this
problem, but the most common way is to use LILO. (The details
about how to do this are irrelevant for this discussion, however;
see the LILO documentation for more information; it is most
thorough.)</para>
<para>When booting with LILO, it will normally go right ahead
and read in and boot the default kernel. It is also possible
to configure LILO to be able to boot one of several kernels,
or even other operating systems than Linux, and it is possible
for the user to choose which kernel or operating system is to
be booted at boot time. LILO can be configured so that if one
holds down the <keycap>alt</keycap>, <keycap>shift</keycap>, or
<keycap>ctrl</keycap> key at boot time (when LILO is loaded),
LILO will ask what is to be booted and not boot the default
right away. Alternatively, LILO can be configured so that it
will always ask, with an optional timeout that will cause the
default kernel to be booted.</para>
<para>With LILO, it is also possible to give a <glossterm>kernel
command line argument</glossterm>, after the name of the kernel
or operating system.</para>
<para>Booting from floppy and from hard disk have both their
advantages, but generally booting from the hard disk is nicer,
since it avoids the hassle of playing around with floppies.
It is also faster. However, it can be more troublesome to install
the system to boot from the hard disk, so many people will first
boot from floppy, then, when the system is otherwise installed
and working well, will install LILO and start booting from the
hard disk.</para>
<para>After the Linux kernel has been read into the memory, by
whatever means, and is started for real, roughly the following
things happen:
<itemizedlist>
<listitem><para>
The Linux kernel is installed compressed, so it will first
uncompress itself. The beginning of the kernel image
contains a small program that does this.
</para></listitem>
<listitem><para>
If you have a super-VGA card that Linux
recognizes and that has some special text modes (such as 100
columns by 40 rows), Linux asks you which mode
you want to use. During the kernel compilation, it is
possible to preset a video mode, so that this is never asked.
This can also be done with LILO or <command>rdev</command>.
</para></listitem>
<listitem><para>
After this, the kernel checks what other hardware there is
(hard disks, floppies, network adapters, etc), and configures
some of its device drivers appropriately; while it does this,
it outputs messages about its findings. For example, when I
boot, I it looks like this:
<screen>
<computeroutput>
LILO boot:
Loading linux.
Console: colour EGA+ 80x25, 8 virtual consoles
Serial driver version 3.94 with no serial options enabled
tty00 at 0x03f8 (irq = 4) is a 16450
tty01 at 0x02f8 (irq = 3) is a 16450
lp_init: lp1 exists (0), using polling driver
Memory: 7332k/8192k available (300k kernel code, 384k reserved, 176k data)
Floppy drive(s): fd0 is 1.44M, fd1 is 1.2M
Loopback device init
Warning WD8013 board not found at i/o = 280.
Math coprocessor using irq13 error reporting.
Partition check:
hda: hda1 hda2 hda3
VFS: Mounted root (ext filesystem).
Linux version 0.99.pl9-1 (root@haven) 05/01/93 14:12:20
</computeroutput>
</screen>
The exact texts are different on different systems, depending
on the hardware, the version of Linux being used, and how
it has been configured.
</para></listitem>
<listitem><para> Then the kernel will try to mount the root
filesystem. The place is configurable at compilation time, or
any time with <command>rdev</command> or LILO. The filesystem
type is detected automatically. If the mounting of the root
filesystem fails, for example because you didn't remember to
include the corresponding filesystem driver in the kernel, the
kernel panics and halts the system (there isn't much it can do,
anyway). </para>
<para>The root filesystem is usually mounted read-only (this can
be set in the same way as the place). This makes it possible
to check the filesystem while it is mounted; it is not a good
idea to check a filesystem that is mounted read-write.
</para></listitem>
<listitem><para> After this, the kernel starts
the program <command>init</command> (located in
<filename>/sbin/init</filename>) in the background (this will
always become process number 1). <command>init</command> does
various startup chores. The exact things it does depends on how
it is configured; see <xref linkend="init"> for more information
(not yet written). It will at least start some essential
background daemons. </para></listitem>
<listitem><para> <command>init</command> then switches to
multi-user mode, and starts a <command>getty</command> for virtual
consoles and serial lines. <command>getty</command> is the
program which lets people log in via virtual consoles and serial
terminals. <command>init</command> may also start some other
programs, depending on how it is configured. </para></listitem>
<listitem><para> After this, the boot is complete, and the system
is up and running normally. </para></listitem>
</itemizedlist>
</para>
</sect1>
<sect1>
<title>More about shutdowns</title>
<para>It is important to follow the correct procedures when you shut
down a Linux system. If you fail do so, your filesystems probably
will become trashed and the files probably will become scrambled.
This is because Linux has a disk cache that won't write things
to disk at once, but only at intervals. This greatly improves
performance but also means that if you just turn off the power
at a whim the cache may hold a lot of data and that what is on
the disk may not be a fully working filesystem (because only
some things have been written to the disk).</para>
<para>Another reason against just flipping the power switch is that
in a multi-tasking system there can be lots of things going on
in the background, and shutting the power can be quite
disastrous. By using the proper shutdown sequence, you ensure
that all background processes can save their data.</para>
<para>The command for properly shutting down a Linux system
is <command>shutdown</command>. It is usually used in one of
two ways.</para>
<para>If you are running a system where you are the only user,
the usual way of using <command>shutdown</command> is to quit
all running programs, log out on all virtual consoles, log
in as root on one of them (or stay logged in as root if you
already are, but you should change to root's home directory or
the root directory, to avoid problems with unmounting), then
give the command <command>shutdown -h now</command> (substitute
<literal>now</literal> with a plus sign and a number in minutes
if you want a delay, though you usually don't on a single user
system).</para>
<para>Alternatively, if your system has many users, use the command
<command>shutdown -h +time message</command>, where <literal>time</literal>
is the
time in minutes until the system is halted, and <literal>message</literal>
is a short explanation of why the system is shutting down.
<screen>
<prompt>#</prompt> <userinput>shutdown -h +10 'We will install a new disk. System should
> be back on-line in three hours.'</userinput>
<prompt>#</prompt>
</screen>
This will warn everybody that the system will shut down in
ten minutes, and that they'd better get lost or lose data.
The warning is printed to every terminal on which someone is
logged in, including all <command>xterm</command>s:
<screen>
<computeroutput>
Broadcast message from root (ttyp0) Wed Aug 2 01:03:25 1995...
We will install a new disk. System should
be back on-line in three hours.
The system is going DOWN for system halt in 10 minutes !!
</computeroutput>
</screen>
The warning is automatically repeated a few times before the boot,
with shorter and shorter intervals as the time runs out.</para>
<para>When the real shutting down starts after any delays, all
filesystems (except the root one) are unmounted, user processes
(if anybody is still logged in) are killed, daemons are shut down,
all filesystem are unmounted, and generally everything settles
down. When that is done, <command>init</command> prints out a
message that you can power down the machine. Then, and only then,
should you move your fingers towards the power switch.</para>
<para>Sometimes, although rarely on any good system, it is
impossible to shut down properly. For instance, if the kernel
panics and crashes and burns and generally misbehaves, it might
be completely impossible to give any new commands, hence shutting
down properly is somewhat difficult, and just about everything
you can do is hope that nothing has been too severely damaged
and turn off the power. If the troubles are a bit less severe
(say, somebody hit your keyboard with an axe), and the kernel
and the <command>update</command> program still run normally,
it is probably a good idea to wait a couple of minutes to give
<command>update</command> a chance to flush the buffer cache,
and only cut the power after that.</para>
<para>Some people like to shut down using the command
<command>sync</command>
<footnote><para><command>sync</command> flushes the
buffer cache. </para></footnote>
three times, waiting for the disk I/O to stop, then turn off
the power. If there are no running programs, this is about
equivalent to using <command>shutdown</command>. However, it
does not unmount any filesystems and this can lead to problems
with the ext2fs ``clean filesystem'' flag. The triple-sync
method is <emphasis>not recommended</emphasis>.</para>
<para>(In case you're wondering: the reason for three syncs is
that in the early days of UNIX, when the commands were
typed separately, that usually gave sufficient time for most
disk I/O to be finished.)
</para>
</sect1>
<sect1>
<title>Rebooting</title>
<para>Rebooting means booting the system again. This can be
accomplished by first shutting it down completely, turning
power off, and then turning it back on. A simpler way is to
ask <command>shutdown</command> to reboot the system, instead
of merely halting it. This is accomplished by using the
<option>-r</option> option to <command>shutdown</command>,
for example, by giving the command <command>shutdown -r
now</command>.</para>
<para>Most Linux systems run <command>shutdown -r now</command>
when ctrl-alt-del is pressed on the keyboard. This reboots the
system. The action on ctrl-alt-del is configurable, however, and
it might be better to allow for some delay before the reboot on
a multiuser machine. Systems that are physically accessible to
anyone might even be configured to do nothing when ctrl-alt-del
is pressed. </para>
</sect1>
<sect1>
<title>Single user mode</title>
<para>The <command>shutdown</command> command can also be used
to bring the system down to single user mode, in which no one
can log in, but root can use the console. This is useful for
system administration tasks that can't be done while the system is
running normally.</para>
</sect1>
<sect1>
<title>Emergency boot floppies</title>
<para>It is not always possible to boot a computer from the hard disk.
For example, if you make a mistake in configuring LILO, you might
make your system unbootable. For these situations, you need an
alternative way of booting that will always work (as long as the
hardware works). For typical PC's, this means booting from the
floppy drive.</para>
<para>Most Linux distributions allow one to create an
<glossterm>emergency boot floppy</glossterm> during installation.
It is a good idea to do this. However, some such boot disks
contain only the kernel, and assume you will be using the programs
on the distribution's installation disks to fix whatever problem
you have. Sometimes those programs aren't enough; for example,
you might have to restore some files from backups made with
software not on the installation disks.</para>
<para>Thus, it might be necessary to create a custom root floppy
as well. The <citetitle>Bootdisk HOWTO</citetitle> by Graham
Chapman (XXX citation) contains instructions for doing this.
You must, of course, remember to keep your emergency boot and
root floppies up to date.</para>
<para>You can't use the floppy drive you use to mount the root
floppy for anything else. This can be inconvenient if you only
have one floppy drive. However, if you have enough memory, you
can configure your boot floppy to load the root disk to a ramdisk
(the boot floppy's kernel needs to be specially configured for
this). Once the root floppy has been loaded into the ramdisk,
the floppy drive is free to mount other disks. </para>
</chapter>
<chapter id="init">
<title><command>init</command></title>
<para>
<blockquote><para><quote>Uuno on numero yksi</quote>
(Slogan for a series of Finnish movies.)</para></blockquote>
<para> This chapter describes the <command>init</command> process,
which is the first user level process started by the kernel.
<command>init</command> has many important duties, such as
starting <command>getty</command> (so that users can log in),
implementing run levels, and taking care of orphaned processes.
This chapter explains how <command>init</command> is configured
and how you can make use of the different run levels.</para>
<sect1>
<title><command>init</command> comes first</title>
<para><command>init</command> is one of those programs that
are absolutely essential to the operation of a Linux system,
but that you still can mostly ignore. A good Linux distribution
will come with a configuration for <command>init</command>
that will work for most systems, and on these systems there is
nothing you need to do about <command>init</command>. Usually,
you only need to worry about <command>init</command> if you hook
up serial terminals, dial-in (not dial-out) modems, or if you
want to change the default run level.</para>
<para>When the kernel has started itself (has been loaded
into memory, has started running, and has initialized all
device drivers and data structures and such), it finishes its
own part of the boot process by starting a user level program,
<command>init</command>. Thus, <command>init</command> is always
the first process (its process number is always 1).</para>
<para>The kernel looks for <command>init</command>
in a few locations that have been historically used
for it, but the proper location for it (on a Linux
system) is <filename>/sbin/init</filename>. If the
kernel can't find <command>init</command>, it tries to run
<filename>/bin/sh</filename>, and if that also fails, the startup
of the system fails.</para>
<para>When <command>init</command> starts, it finishes the
boot process by doing a number of administrative tasks, such
as checking filesystems, cleaning up <filename>/tmp</filename>,
starting various services, and starting a <command>getty</command>
for each terminal and virtual console where users should be able
to log in (see <xref linkend="log-in-and-out">).</para>
<para>After the system is properly up, <command>init</command>
restarts <command>getty</command> for each terminal
after a user has logged out (so that the next user can log
in). <command>init</command> also adopts orphan processes: when
a process starts a child process and dies before its child, the
child immediately becomes a child of <command>init</command>.
This is important for various technical reasons, but it is good
to know it, since it makes it easier to understand process lists
and process tree graphs.
<footnote><para><command>init</command> itself is not
allowed to die. You can't kill <command>init</command>
even with SIGKILL. </para></footnote>
There are a few variants of <command>init</command>
available. Most Linux distributions
use <command>sysvinit</command> (written by Miquel
van Smoorenburg), which is based on the System V
<command>init</command> design. The BSD versions of Unix have
a different <command>init</command>. The primary difference
is run levels: System V has them, BSD does not (at least
traditionally). This difference is not essential. We'll look
at <command>sysvinit</command> only. </para>
</sect1>
<sect1>
<title>Configuring <command>init</command> to start <command>getty</command>: the <filename>/etc/inittab</filename> file</title>
<para>When it starts up, <command>init</command> reads the <filename>/etc/inittab</filename>
configuration file. While the system is running, it will
re-read it, if sent the HUP signal;
<footnote><para>Using the command <command>kill -HUP
1</command> as root, for example </para></footnote>
this feature makes it unnecessary to boot the system to make
changes to the <command>init</command> configuration take
effect.</para>
<para>The <filename>/etc/inittab</filename> file is
a bit complicated. We'll start with the simple case
of configuring <command>getty</command> lines. Lines in
<filename>/etc/inittab</filename> consist of four colon-delimited
fields:
<screen>
id:runlevels:action:process
</screen>
The fields are described below. In addition,
<filename>/etc/inittab</filename> can contain empty lines, and
lines that begin with a number sign (`<literal>#</literal>');
these are both ignored.
<glosslist>
<glossentry><glossterm>id</glossterm>
<glossdef><para>
This identifies the line in the file. For
<command>getty</command> lines, it specifies the terminal
it runs on (the characters after <filename>/dev/tty</filename>
in the device file name). For other lines,
it doesn't matter (except for length restrictions),
but it should be unique.
</para></glossdef></glossentry>
<glossentry><glossterm>runlevels</glossterm>
<glossdef><para>
The run levels the line should be considered
for. The run levels are given as single digits,
without delimiters. (Run levels are described
in the next section.)
</para></glossdef></glossentry>
<glossentry><glossterm>action</glossterm>
<glossdef><para>
What action should be taken by the line, e.g.,
<literal>respawn</literal> to run the command in the
next field again, when it exits, or <literal>once</literal>
to run it just once.
</para></glossdef></glossentry>
<glossentry><glossterm>process</glossterm>
<glossdef><para>
The command to run.
</para></glossdef></glossentry>
</glosslist>
To start a <command>getty</command> on the first virtual terminal
(<filename>/dev/tty1</filename>), in all the normal multi-user
run levels (2-5), one would write the following line:
<screen>
1:2345:respawn:/sbin/getty 9600 tty1
</screen>
The first field says that this is the line for <filename>/dev/tty1</filename>.
The second field says that it applies to run levels 2, 3, 4,
and 5. The third field means that the command should be run
again, after it exits (so that one can log in, log out, and
then log in again). The last field is the command that runs
<command>getty</command> on the first virtual terminal.
<footnote><para>Different versions of
<command>getty</command> are run differently. Consult
your manual page, and make sure it is the correct
manual page.</para></footnote>
</para>
<para>If you wanted to add terminals or dial-in modem lines to a
system, you'd add more lines to <filename>/etc/inittab</filename>,
one for each terminal or dial-in line. For more details, see the
manual pages <command>init</command>, <filename>inittab</filename>,
and <command>getty</command>.</para>
<para>If a command fails when it starts,
and <command>init</command> is configured to
<literal>restart</literal> it, it will use a lot of
system resources: <command>init</command> starts it,
it fails, <command>init</command> starts it, it fails,
<command>init</command> starts it, it fails, and so on, ad
infinitum. To prevent this, <command>init</command> will keep
track of how often it restarts a command, and if the frequency
grows to high, it will delay for five minutes before restarting
again. </para>
</sect1>
<sect1>
<title>Run levels</title>
<para>A <glossterm>run level</glossterm> is a state of
<command>init</command> and the whole system that defines what
system services are operating. Run levels are identified by
numbers, see <xref linkend="run-levels">. There is no consensus of how to use the
user defined run levels (2 through 5). Some system administrators
use run levels to define which subsystems are working, e.g.,
whether X is running, whether the network is operational, and
so on. Others have all subsystems always running or start and
stop them individually, without changing run levels, since run
levels are too coarse for controlling their systems. You need
to decide for yourself, but it might be easiest to follow the
way your Linux distribution does things.</para>
<table id="run-levels">
<title>Run level numbers</title>
<tgroup cols=2>
<tbody>
<row> <entry>0</entry> <entry>Halt the system.</entry> </row>
<row> <entry>1</entry> <entry>Single-user mode (for special administration).</entry> </row>
<row> <entry>2-5</entry> <entry>Normal operation (user defined).</entry> </row>
<row> <entry>6</entry> <entry>Reboot.</entry> </row>
</tbody>
</tgroup>
</table>
<para>Run levels are configured in <filename>/etc/inittab</filename> by lines like
the following:
<screen>
l2:2:wait:/etc/init.d/rc 2
</screen>
The first field is an arbitrary label, the second one means
that this applies for run level 2. The third field means
that <command>init</command> should run the command in the
fourth field once, when the run level is entered, and that
<command>init</command> should wait for it to complete. The
<filename>/etc/init.d/rc</filename> command runs whatever
commands are necessary to start and stop services to enter run
level 2.</para>
<para>The command in the fourth field does all the hard work of
setting up a run level. It starts services that aren't already
running, and stops services that shouldn't be running in the
new run level any more. Exactly what the command is, and how run
levels are configured, depends on the Linux distribution.</para>
<para>When <command>init</command> starts, it looks for a line
in <filename>/etc/inittab</filename> that specifies the default
run level:
<screen>
id:2:initdefault:
</screen>
You can ask <command>init</command> to go to a non-default run
level at startup by giving the kernel a command line argument
of <literal>single</literal> or <literal>emergency</literal>.
Kernel command line arguments can be given via LILO, for example.
This allows you to choose the single user mode (run level 1).</para>
<para>While the system is running, the <command>telinit</command>
command can change the run level. When the run level is
changed, <command>init</command> runs the relevant command from
<filename>/etc/inittab</filename>. </para>
</sect1>
<sect1>
<title>Special configuration in <filename>/etc/inittab</filename></title>
<para>The <filename>/etc/inittab</filename> has some special
features that allow <command>init</command> to react to special
circumstances. These special features are marked by special
keywords in the third field. Some examples:
<glosslist>
<glossentry><glossterm><literal>powerwait</literal></glossterm>
<glossdef><para>
Allows <command>init</command> to shut the system
down, when the power fails. This assumes the use of
a UPS, and software that watches the UPS and informs
<command>init</command> that the power is off.
</para></glossdef></glossentry>
<glossentry><glossterm><literal>ctrlaltdel</literal></glossterm>
<glossdef><para>
Allows <command>init</command> to reboot the system, when
the user presses ctrl-alt-del on the console keyboard.
Note that the system administrator can configure the
reaction to ctrl-alt-del to be something else instead,
e.g., to be ignored, if the system is in a public
location. (Or to start <command>nethack</command>.)
</para></glossdef></glossentry>
<glossentry><glossterm><literal>sysinit</literal></glossterm>
<glossdef><para>
Command to be run when the system is booted. This command
usually cleans up <filename>/tmp</filename>, for example.
</para></glossdef></glossentry>
</glosslist>
The list above is not exhaustive. See your
<filename>inittab</filename> manual page for all possibilities,
and for details on how to use the above ones. </para>
</sect1>
<sect1>
<title>Booting in single user mode</title>
<para>An important run level is <glossterm>single user mode</glossterm> (run level 1),
in which only the system administrator is using the machine
and as few system services, including logins, as possible are
running. Single user mode is necessary for a few administrative
tasks,
<footnote><para>It probably shouldn't be used for playing
<command>nethack</command>.</para></footnote>
such as running <command>fsck</command> on a
<filename>/usr</filename> partition, since this requires that
the partition be unmounted, and that can't happen, unless just
about all system services are killed.</para>
<para>A running system can be taken to single user mode by using
<command>telinit</command> to request run level 1. At bootup,
it can be entered by giving the word <literal>single</literal>
or <literal>emergency</literal> on the kernel command line: the
kernel gives the command line to <command>init</command> as well,
and <command>init</command> understands from that word that it
shouldn't use the default run level. (The kernel command line is
entered in a way that depends on how you boot the system.)</para>
<para>Booting into single user mode is sometimes necessary so
that one can run <command>fsck</command> by hand, before anything
mounts or otherwise touches a broken <filename>/usr</filename>
partition (any activity on a broken filesystem is likely to
break it more, so <command>fsck</command> should be run as soon
as possible).</para>
<para>The bootup scripts <command>init</command> runs
will automatically enter single user mode, if the automatic
<command>fsck</command> at bootup fails. This is an attempt to
prevent the system from using a filesystem that is so broken that
<command>fsck</command> can't fix it automatically. Such breakage
is relatively rare, and usually involves a broken hard disk or an
experimental kernel release, but it's good to be prepared.</para>
<para>As a security measure, a properly configured system
will ask for the root password before starting the shell in
single user mode. Otherwise, it would be simple to just enter
a suitable line to LILO to get in as root. (This will break if
<filename>/etc/passwd</filename> has been broken by filesystem
problems, of course, and in that case you'd better have a boot
floppy handy.)</para>
</chapter>
<chapter id="log-in-and-out">
<title>Logging In And Out</title>
<blockquote><para><quote>I don't care to belong to a club
that accepts people like me as a member.</quote>
(Groucho Marx)</para></blockquote>
<para>
This section describes what happens when a user logs
in or out. The various interactions of background processes,
log files, configuration files, and so on are described in
some detail.
</para>
<sect1>
<title>Logins via terminals</title>
<para><xref linkend="terminal-logins"> shows how logins happen via
terminals. First, <command>init</command> makes sure there is
a <command>getty</command> program for the terminal connection
(or console). <command>getty</command> listens at the terminal
and waits for the user to notify that he is ready to login in
(this usually means that the user must type something). When it
notices a user, <command>getty</command> outputs a welcome message
(stored in <filename>/etc/issue</filename>), and prompts for
the username, and finally runs the <command>login</command>
program. <command>login</command> gets the username as a
parameter, and prompts the user for the password. If these
match, <command>login</command> starts the shell configured
for the user; else it just exits and terminates the process
(perhaps after giving the user another chance at entering the
username and password). <command>init</command> notices that
the process terminated, and starts a new <command>getty</command>
for the terminal.
</para>
<figure id="terminal-logins" float="1">
<title>Logins via terminals: the interaction of <command>init</command>, <command>getty</command>, <command>login</command>, and the shell.</title>
<graphic fileref="logins-via-terminals"></graphic>
</figure>
<para> Note that the only new process is the
one created by <command>init</command> (using the
<function>fork</function> system call); <command>getty</command>
and <command>login</command> only replace the program running in
the process (using the <function>exec</function> system call).
</para>
<para> A separate program, for noticing the user, is needed
for serial lines, since it can be (and traditionally was)
complicated to notice when a terminal becomes active.
<command>getty</command> also adapts to the speed and other
settings of the connection, which is important especially for
dial-in connections, where these parameters may change from call
to call. </para>
<para> There are several versions of <command>getty</command>
and <command>init</command> in use, all with their good and
bad points. It is a good idea to learn about the versions on
your system, and also about the other versions (you could use the
Linux Software Map to search them). If you don't have dial-in's,
you probably don't have to worry about <command>getty</command>,
but <command>init</command> is still important. </para>
</sect1>
<sect1>
<title>Logins via the network</title>
<para>Two computers in the same network are usually linked via a
single physical cable. When they communicate over the network,
the programs in each computer that take part in the communication
are linked via a <glossterm>virtual connection</glossterm>, a sort
of imaginary cable. As far as the programs at either end of the
virtual connection are concerned, they have a monopoly on their
own cable. However, since the cable is not real, only imaginary,
the operating systems of both computers can have several virtual
connections share the same physical cable. This way, using just
a single cable, several programs can communicate without having
to know of or care about the other communications. It is even
possible to have several computers use the same cable; the virtual
connections exist between two computers, and the other computers
ignore those connections that they don't take part in. </para>
<para> That's a complicated and over-abstracted description of
the reality. It might, however, be good enough to understand
the important reason why network logins are somewhat different
from normal logins. The virtual connections are established
when there are two programs on different computers that wish
to communicate. Since it is in principle possible to login
from any computer in a network to any other computer, there is
a huge number of potential virtual communications. Because of
this, it is not practical to start a <command>getty</command>
for each potential login. </para>
<para> There is a single process inetd (corresponding to
<command>getty</command>) that handles all network logins.
When it notices an incoming network login (i.e., it notices
that it gets a new virtual connection to some other computer),
it starts a new process to handle that single login. The original
process remains and continues to listen for new logins. </para>
<para> To make things a bit more complicated, there is
more than one communication protocol for network logins.
The two most important ones are <command>telnet</command> and
<command>rlogin</command>. In addition to logins, there are many
other virtual connections that may be made (for FTP, Gopher, HTTP,
and other network services). It would be ineffective to have a
separate process listening for a particular type of connection,
so instead there is only one listener that can recognize the type
of the connection and can start the correct type of program to
provide the service. This single listener is called <command>inetd</command>;
see the <citetitle>Linux Network Administrators' Guide</citetitle>
for more information. </para>
</sect1>
<sect1>
<title>What <command>login</command> does</title>
<para>The <command>login</command> program takes care of
authenticating the user (making sure that the username and
password match), and of setting up an initial environment for
the user by setting permissions for the serial line and starting
the shell. </para>
<para> Part of the initial setup is outputting the contents of
the file <filename>/etc/motd</filename> (short for message of the
day) and checking for electronic mail. These can be disabled
by creating a file called <filename>.hushlogin</filename> in
the user's home directory. </para>
<para> If the file <filename>/etc/nologin</filename>
exists, logins are disabled. That file is typically
created by <command>shutdown</command> and relatives.
<command>login</command> checks for this file, and will
refuse to accept a login if it exists. If it does exist,
<command>login</command> outputs its contents to the terminal
before it quits. </para>
<para> <command>login</command> logs all failed login attempts in
a system log file (via <command>syslog</command>). It also logs
all logins by root. Both of these can be useful when tracking
down intruders. </para>
<para> Currently logged in people are listed in
<filename>/var/run/utmp</filename>. This file is valid only
until the system is next rebooted or shut down; it is cleared
when the system is booted. It lists each user and the terminal
(or network connection) he is using, along with some other useful
information. The <command>who</command>, <command>w</command>,
and other similar commands look in <filename>utmp</filename>
to see who are logged in. </para>
<para> All successful logins are recorded into
<filename>/var/log/wtmp</filename>. This file will grow without
limit, so it must be cleaned regularly, for example by having
a weekly <command>cron</command> job to clear it.
<footnote><para>Good Linux distributions do this out
of the box.</para></footnote>
The <command>last</command> command browses
<filename>wtmp</filename>. </para>
<para> Both <filename>utmp</filename> and
<filename>wtmp</filename> are in a binary format (see the
<filename>utmp</filename> manual page); it is unfortunately not
convenient to examine them without special programs. </para>
</sect1>
<sect1>
<title>X and xdm</title>
<para> XXX X implements logins via xdm; also: xterm -ls </para>
</sect1>
<sect1>
<title>Access control</title>
<para> The user database is traditionally contained in the
<filename>/etc/passwd</filename> file. Some systems use
<glossterm>shadow passwords</glossterm>, and have moved the
passwords to <command>/etc/shadow</command>. Sites with many
computers that share the accounts use NIS or some other method
to store the user database; they might also automatically copy
the database from one central location to all other computers.
</para>
<para> The user database contains not only the passwords, but
also some additional information about the users, such as their
real names, home directories, and login shells. This other
information needs to be public, so that anyone can read it.
Therefore the password is stored encrypted. This does have
the drawback that anyone with access to the encrypted password
can use various cryptographical methods to guess it, without
trying to actually log into the computer. Shadow passwords try
to avoid this by moving the password into another file, which
only root can read (the password is still stored encrypted).
However, installing shadow passwords later onto a system that
did not support them can be difficult. </para>
<para> With or without passwords, it is important to make
sure that all passwords in a system are good, i.e., not easily
guessable. The <command>crack</command> program can be used
to crack passwords; any password it can find is by definition
not a good one. While <command>crack</command> can be run
by intruders, it can also be run by the system adminstrator
to avoid bad passwords. Good passwords can also be enforced
by the <command>passwd</command> program; this is in fact more
effective in CPU cycles, since cracking passwords requires quite
a lot of computation. </para>
<para> The user group database is kept in
<filename>/etc/group</filename>; for systems with shadow
passwords, there can be a <filename>/etc/shadow.group</filename>.
</para>
<para> root usually can't login via most terminals
or the network, only via terminals listed in the
<filename>/etc/securetty</filename> file. This makes it necessary
to get physical access to one of these terminals. It is, however,
possible to log in via any terminal as any other user, and use
the <command>su</command> command to become root. </para>
</sect1>
<sect1>
<title>Shell startup</title>
<para> When an interactive login shell starts, it automatically
executes one or more pre-defined files. Different shells execute
different files; see the documentation of each shell for further
information. </para>
<para> Most shells first run some global file, for example, the
Bourne shell (<command>/bin/sh</command>) and its derivatives
execute <filename>/etc/profile</filename>; in addition,
they execute <filename>.profile</filename> in the user's
home directory. <filename>/etc/profile</filename> allows the
system administrator to have set up a common user environment,
especially by setting the <envar>PATH</envar> to include local
command directories in addition to the normal ones. On the other
hand, <filename>.profile</filename> allows the user to customize
the environment to his own tastes by overriding, if necessary,
the default environment. </para>
</chapter>
<chapter>
<title>Managing user accounts</title>
<blockquote><para><quote>The similarities of sysadmins and drug
dealers: both measure stuff in K's, and both have users.</quote>
(Old, tired computer joke.)</para></blockquote>
<para> This chapter explains how to create new user accounts,
how to modify the properties of those accounts, and how to remove
the accounts. Different Linux systems have different tools for
doing this.</para>
<sect1>
<title>What's an account?</title>
<para> When a computer is used by many people it is usually
necessary to differentiate between the users, for example, so that
their private files can be kept private. This is important even
if the computer can only be used by a single person at a time,
as with most microcomputers.
<footnote><para>It might be quite embarrassing if my
sister could read my love letters.</para></footnote>
Thus, each user is given a unique username, and that name is
used to log in. </para>
<para> There's more to a user than just a name, however. An
<glossterm>account</glossterm> is all the files, resources,
and information belonging to one user. The term hints at banks,
and in a commercial system each account usually has some money
attached to it, and that money vanishes at different speeds
depending on how much the user stresses the system. For example,
disk space might have a price per megabyte and day, and processing
time might have a price per second. </para>
</sect1>
<sect1>
<title>Creating a user</title>
<para> The Linux kernel itself treats users are mere numbers.
Each user is identified by a unique integer, the <glossterm>user
id</glossterm> or <glossterm>uid</glossterm>, because numbers are
faster and easier for a computer to process than textual names.
A separate database outside the kernel assigns a textual name,
the <glossterm>username</glossterm>, to each user id. The database
contains additional information as well. </para>
<para> To create a user, you need to add information about
the user to the user database, and create a home directory for
him. It may also be necessary to educate the user, and set up
a suitable initial environment for him. </para>
<para> Most Linux distributions come with a program for
creating accounts. There are several such programs available.
Two command line alternatives are <command>adduser</command>
and <command>useradd</command>; there may be a GUI tool as well.
Whatever the program, the result is that there is little if
any manual work to be done. Even if the details are many and
intricate, these programs make everything seem trivial. However,
<xref linkend="manual-adduser"> describes how to do it by hand.
</para>
<sect2>
<title><filename>/etc/passwd</filename> and other informative files</title>
<para> The basic user database in a Unix system is the text file,
<filename>/etc/passwd</filename> (called the <glossterm>password
file</glossterm>), which lists all valid usernames and their
associated information. The file has one line per username,
and is divided into seven colon-delimited fields:
<itemizedlist>
<listitem><para>Username.</para></listitem>
<listitem><para>Password, in an encrypted form.</para></listitem>
<listitem><para>Numeric user id.</para></listitem>
<listitem><para>Numeric group id.</para></listitem>
<listitem><para>Full name or other description of account.</para></listitem>
<listitem><para>Home directory.</para></listitem>
<listitem><para>Login shell (program to run at login).</para></listitem>
</itemizedlist>
The format is explained in more detail on the
<filename>passwd</filename> manual page. </para>
<para> Any user on the system may read the password file,
so that they can, for example, learn the name of another user.
This means that the password (the second field) is also available
to everyone. The password file encrypts the password, so in
theory there is no problem. However, the encryption is breakable,
especially if the password is weak (e.g., it is short or it can
be found in a dictionary). Therefore it is not a good idea to
have the password in the password file. </para>
<para>
Many Linux systems have <glossterm>shadow passwords</glossterm>. This is
an alternative way of storing the password: the encrypted
password is stored in a separate file, <filename>/etc/shadow</filename>,
which only root can read. The <filename>/etc/passwd</filename>
file only contains a special marker in the second field.
Any program that needs to verify a user is setuid, and
can therefore access the shadow password file. Normal
programs, which only use the other fields in the password
file, can't get at the password.
<footnote><para>Yes, this means that the
password file has all the information about a user
<emphasis>except</emphasis> his password. The wonder
of development.</para></footnote>
</para>
</sect2>
<sect2>
<title>Picking numeric user and group ids</title>
<para> On most systems it doesn't matter what the numeric user
and group ids are, but if you use the Network filesystem (NFS),
you need to have the same uid and gid on all systems. This
is because NFS also identifies users with the numeric uids.
If you aren't using NFS, you can let your account creation tool
pick them automatically. </para>
<para> If you are using NFS, you'll have to be invent a mechanism
for synchronizing account information. One alternative is to
the NIS system (see XXX network-admin-guide). </para>
<para> However, you should try to avoid re-using numeric uid's
(and textual usernames), because the new owner of the uid (or
username) may get access to the old owner's files (or mail,
or whatever). </para>
</sect2>
<!--
%\subsection{Managing groups}
%
% \meta Debian creates a new group for each user; give reason for this;
% give reasons against.
-->
<sect2>
<title>Initial environment: <filename>/etc/skel</filename></title>
<para> When the home directory for a new user is created, it is
initialized with files from the <filename>/etc/skel</filename>
directory. The system administrator can create files in
<filename>/etc/skel</filename> that will provide a nice
default environment for users. For example, he might create a
<filename>/etc/skel/.profile</filename> that sets the EDITOR
environment variable to some editor that is friendly towards
new users. </para>
<para> However, it is usually best to try to keep
<filename>/etc/skel</filename> as small as possible, since it
will be next to impossible to update existing users' files. For
example, if the name of the friendly editor changes, all existing
users would have to edit their <filename>.profile</filename>. The
system administrator could try to do it automatically, with a
script, but that is almost certain going to break someone's file.
</para>
<para> Whenever possible, it is better to put global configuration
into global files, such as <filename>/etc/profile</filename>. This
way it is possible to update it without breaking users'
own setups. </para>
</sect2>
<sect2 id="manual-adduser">
<title>Creating a user by hand</title>
<para> To create a new account manually, follow these steps:
<itemizedlist>
<listitem><para> Edit <filename>/etc/passwd</filename> with
<command>vipw</command> and add a new line for the new account. Be
careful with the syntax. <emphasis>Do not edit directly with an
editor!</emphasis> <command>vipw</command> locks the file, so
that other commands won't try to update it at the same time. You
should make the password field be `<literal>*</literal>', so
that it is impossible to log in. </para></listitem>
<listitem><para> Similarly, edit <filename>/etc/group</filename>
with <command>vigr</command>, if you need to create a new group
as well. </para></listitem>
<listitem><para> Create the home directory of the user with
<command>mkdir</command>. </para></listitem>
<listitem><para> Copy the files from
<filename>/etc/skel</filename> to the new home directory.
</para></listitem>
<listitem><para> Fix ownerships and permissions with
<command>chown</command> and <command>chmod</command>. The
<option>-R</option> option is most useful. The correct
permissions vary a little from one site to another, but usually
the following commands do the right thing:
<screen>
<userinput>cd /home/newusername
chown -R username.group .
chmod -R go=u,go-w .
chmod go= .</userinput>
</screen>
</para></listitem>
<listitem><para> Set the password with <command>passwd</command>.
</para></listitem>
</itemizedlist>
</para>
<para> After you set the password in the last step, the account
will work. You shouldn't set it until everything else has been
done, otherwise the user may inadvertently log in while you're
still copying the files. </para>
<para>
It is sometimes necessary to create dummy
accounts
<footnote><para>Surreal users?</para></footnote>
that are not used by people. For example, to set up an anonymous
FTP server (so that anyone can download files from it, without
having to get an account first), you need to create an account
called ftp. In such cases, it is usually not necessary to set
the password (last step above). Indeed, it is better not to, so
that no-one can use the account, unless they first become root,
since root can become any user. </para>
</sect2>
</sect1>
<!--
%\section{Educating a new user}
%
% \meta
% make sure they know how to get help
% large sites might want to write a small booklet (or even just
% a couple of pages) with important stuff: how to log in
% and out, how to change password, which systems there are,
% how to use mail, list of people that answer questions
-->
<sect1>
<title>Changing user properties</title>
<para>
There are a few commands for changing various
properties of an account (i.e., the relevant field
in <filename>/etc/passwd</filename>):
<glosslist>
<glossentry><glossterm><command>chfn</command></glossterm>
<glossdef><para> Change the full name field.
</para></glossdef></glossentry>
<glossentry><glossterm><command>chsh</command></glossterm>
<glossdef><para> Change the login shell.
</para></glossdef></glossentry>
<glossentry><glossterm><command>passwd</command></glossterm>
<glossdef><para>Change the password.
</para></glossdef></glossentry>
</glosslist>
The super-user may use these commands to change the properties
of any account. Normal users can only change the properties
of their own account. It may sometimes be necessary to disable
these commands (with <command>chmod</command>) for normal users,
for example in an environment with many novice users. </para>
<para>
Other tasks need to be done by hand. For example, to
change the username, you need to edit <filename>/etc/passwd</filename>
directly (with <command>vipw</command>, remember). Likewise, to add
or remove the user to more groups, you need to edit
<filename>/etc/group</filename> (with <command>vigr</command>). Such tasks tend to
be rare, however, and should be done with caution: for
example, if
you change the username, e-mail will no longer reach the
user, unless you also create a mail alias.
<footnote><para>The user's name might change due to
marriage, for example, and he might want to have his
username reflect his new name.</para></footnote>
</para>
</sect1>
<sect1>
<title>Removing a user</title>
<para> To remove a user, you first remove all
his files, mailboxes, mail aliases, print jobs,
<command>cron</command> and <command>at</command> jobs,
and all other references to the user. Then you remove the
relevant lines from <filename>/etc/passwd</filename> and
<filename>/etc/group</filename> (remember to remove the username
from all groups it's been added to). It may be a good idea to
first disable the account (see below), before you start removing
stuff, to prevent the user from using the account while it is
being removed. </para>
<para>
Remember that users may have files outside their home
directory. The <command>find</command> command can find them:
<screen>
find / -user username
</screen>
However, note that the above command will take a
<emphasis>long</emphasis> time, if you have large disks. If you
mount network disks, you need to be careful so that you won't
trash the network or the server. </para>
<para> Some Linux distributions come with special
commands to do this; look for <command>deluser</command> or
<command>userdel</command>. However, it is easy to do it by
hand as well, and the commands might not do everything. </para>
</sect1>
<sect1>
<title>Disabling a user temporarily</title>
<para> It is sometimes necessary to temporarily disable an
account, without removing it. For example, the user might not
have paid his fees, or the system administrator may suspect that
a cracker has got the password of that account. </para>
<para> The best way to disable an account is to change its shell
into a special program that just prints a message. This way,
whoever tries to log into the account, will fail, and will
know why. The message can tell the user to contact the system
administrator so that any problems may be dealt with. </para>
<para>
It would also be possible to change the username
or password to something else, but then the user
won't know what is going on. Confused users mean more
work.
<footnote><para>But they can be <emphasis>so</emphasis>
fun, if you're a BOFH.</para></footnote>
</para>
<para> A simple way to create the special programs is to write
`tail scripts':
<screen>
#!/usr/bin/tail +2
This account has been closed due to a security breach.
Please call 555-1234 and wait for the men in black to arrive.
</screen>
The first two characters (`<literal>#!</literal>') tell the
kernel that the rest of the line is a command that needs to be
run to interpret this file. The <command>tail</command> command
in this case outputs everything except the first line to the
standard output. </para>
<para>
If user billg is suspected of a security breach,
the system administrator would do something like this:
<screen>
<prompt>#</prompt> <userinput>chsh -s /usr/local/lib/no-login/security billg</userinput>
<prompt>#</prompt> <userinput>su - tester</userinput>
This account has been closed due to a security breach.
Please call 555-1234 and wait for the men in black to arrive.
<prompt>#</prompt>
</screen>
The purpose of the <command>su</command> is to test that the
change worked, of course. </para>
<para> Tail scripts should be kept in a separate directory,
so that their names don't interfere with normal user commands.
</para>
</sect1>
<!--
%\section{Accounting}
%
% \meta
% sac et al
-->
</chapter>
<chapter id="backups">
<title>Backups</title>
<blockquote><para><literallayout>
Hardware is indeterministically reliable.
Software is deterministically unreliable.
People are indeterministically unreliable.
Nature is deterministically reliable.
</literallayout></para></blockquote>
<para> This chapter explains about why, how, and when to make
backups, and how to restore things from backups.</para>
<sect1>
<title>On the importance of being backed up</title>
<para> Your data is valuable. It will cost you time and effort
re-create it, and that costs money or at least personal grief
and tears; sometimes it can't even be re-created, e.g., if it
is the results of some experiments. Since it is an investment,
you should protect it and take steps to avoid losing it. </para>
<para> There are basically four reasons why you might lose data:
hardware failures, software bugs, human action, or natural
disasters.
<footnote><para>The fifth reason is ``something
else''.</para></footnote>
Although modern hardware tends to be quite reliable, it can
still break seemingly spontaneously. The most critical piece
of hardware for storing data is the hard disk, which relies on
tiny magnetic fields remaining intact in a world filled with
electromagnetic noise. Modern software doesn't even tend to
be reliable; a rock solid program is an exception, not a rule.
Humans are quite unreliable, they will either make a mistake, or
they will be malicious and destroy data on purpose. Nature might
not be evil, but it can wreak havoc even when being good. All in
all, it is a small miracle that anything works at all. </para>
<para> Backups are a way to protect the investment in data.
By having several copies of the data, it does not matter as much
if one is destroyed (the cost is only that of the restoration
of the lost data from the backup). </para>
<para> It is important to do backups properly. Like everything
else that is related to the physical world, backups will fail
sooner or later. Part of doing backups well is to make sure
they work; you don't want to notice that your backups didn't work.
<footnote><para>Don't laugh. This has happened to
several people.</para></footnote>
Adding insult to injury, you might have a bad crash just as
you're making the backup; if you have only one backup medium,
it might destroyed as well, leaving you with the smoking ashes
of hard work.
<footnote><para>Been there, done that...</para></footnote>
Or you might notice, when trying to restore, that you forgot to
back up something important, like the user database on a 15000
user site. Best of all, all your backups might be working
perfectly, but the last known tape drive reading the kind of
tapes you used was the one that now has a bucketful of water
in it. </para>
<para> When it comes to backups, paranoia is in the job
description. </para>
</sect1>
<sect1>
<title>Selecting the backup medium</title>
<para> The most important decision regarding backups is the choice
of backup medium. You need to consider cost, reliability, speed,
availability, and usability. </para>
<para> Cost is important, since you should preferably have
several times more backup storage than what you need for the data.
A cheap medium is usually a must. </para>
<para> Reliability is extremely important, since a broken
backup can make a grown man cry. A backup medium must be able
to hold data without corruption for years. The way you use the
medium affects it reliability as a backup medium. A hard disk
is typically very reliable, but as a backup medium it is not
very reliable, if it is in the same computer as the disk you
are backing up. </para>
<para> Speed is usually not very important, if backups can be done
without interaction. It doesn't matter if a backup takes two
hours, as long as it needs no supervision. On the other hand,
if the backup can't be done when the computer would otherwise
be idle, then speed is an issue. </para>
<para> Availability is obviously necessary, since you can't
use a backup medium if it doesn't exist. Less obvious is the
need for the medium to be available even in the future, and on
computers other than your own. Otherwise you may not be able
to restore your backups after a disaster. </para>
<para> Usability is a large factor in how often backups are made.
The easier it is to make backups, the better. A backup medium
mustn't be hard or boring to use. </para>
<para> The typical alternatives are floppies and tapes.
Floppies are very cheap, fairly reliable, not very fast,
very available, but not very usable for large amounts of data.
Tapes are cheap to somewhat expensive, fairly reliable, fairly
fast, quite available, and, depending on the size of the tape,
quite comfortable. </para>
<para> There are other alternatives. They are usually not very
good on availability, but if that is not a problem, they can
be better in other ways. For example, magneto-optical disks
can have good sides of both floppies (they're random access,
making restoration of a single file quick) and tapes (contain
a lot of data). </para>
</sect1>
<sect1>
<title>Selecting the backup tool</title>
<para> There are many tools that can be used to make
backups. The traditional UNIX tools used for backups
are <command>tar</command>, <command>cpio</command>, and
<command>dump</command>. In addition, there are large number
of third party packages (both freeware and commercial) that
can be used. The choice of backup medium can affect the choice
of tool. </para>
<para> <command>tar</command> and <command>cpio</command> are
similar, and mostly equivalent from a backup point of view.
Both are capable of storing files on tapes, and retrieving
files from them. Both are capable of using almost any media,
since the kernel device drivers take care of the low level
device handling and the devices all tend to look alike to user
level programs. Some UNIX versions of <command>tar</command>
and <command>cpio</command> may have problems with unusual files
(symbolic links, device files, files with very long pathnames, and
so on), but the Linux versions should handle all files correctly.
</para>
<para> <command>dump</command> is different in that it reads
the filesystem directly and not via the filesystem. It is
also written specifically for backups; <command>tar</command>
and <command>cpio</command> are really for archiving files,
although they work for backups as well. </para>
<para> Reading the filesystem directly has some advantages.
It makes it possible to back files up without affecting their time
stamps; for <command>tar</command> and <command>cpio</command>,
you would have to mount the filesystem read-only first.
Directly reading the filesystem is also more effective, if
everything needs to be backed up, since it can be done with
much less disk head movement. The major disadvantage is that
it makes the backup program specific to one filesystem type;
the Linux <command>dump</command> program understands the ext2
filesystem only. </para>
<para> <command>dump</command> also directly supports
backup levels (which we'll be discussing below); with
<command>tar</command> and <command>cpio</command> this has to
be implemented with other tools. </para>
<para> A comparison of the third party backup tools is beyond
the scope of this book. The Linux Software Map lists many of
the freeware ones. </para>
</sect1>
<sect1>
<title>Simple backups</title>
<para> A simple backup scheme is to back up everything once,
then back up everything that has been modified since the
previous backup. The first backup is called a <glossterm>full
backup</glossterm>, the subsequent ones are <glossterm>incremental
backups</glossterm>. A full backup is often more laborius
than incremental ones, since there is more data to write to the
tape and a full backup might not fit onto one tape (or floppy).
Restoring from incremental backups can be many times more work
than from a full one. Restoration can be optimized so that
you always back up everything since the previous full backup;
this way, backups are a bit more work, but there should never
be a need to restore more than a full backup and an incremental
backup. </para>
<para> If you want to make backups every day and have six
tapes, you could use tape 1 for the first full backup (say, on
a Friday), and tapes 2 to 5 for the incremental backups (Monday
through Thursday). Then you make a new full backup on tape 6
(second Friday), and start doing incremental ones with tapes 2
to 5 again. You don't want to overwrite tape 1 until you've got
a new full backup, lest something happens while you're making
the full backup. After you've made a full backup to tape 6,
you want to keep tape 1 somewhere else, so that when your other
backup tapes are destroyed in the fire, you still have at least
something left. When you need to make the next full backup,
you fetch tape 1 and leave tape 6 in its place. </para>
<para> If you have more than six tapes, you can use the extra
ones for full backups. Each time you make a full backup, you
use the oldest tape. This way you can have full backups from
several previous weeks, which is good if you want to find an old,
now deleted file, or an old version of a file. </para>
<sect2>
<title>Making backups with <command>tar</command></title>
<para>
A full backup can easily be made with <command>tar</command>:
<screen>
<prompt>#</prompt> <userinput>tar --create --file /dev/ftape /usr/src</userinput>
<computeroutput>tar: Removing leading / from absolute path names in the archive</computeroutput>
<prompt>#</prompt>
</screen>
The example above uses the GNU version of <command>tar</command>
and its long option names. The traditional version of
<command>tar</command> only understands single character
options. The GNU version can also handle backups that don't
fit on one tape or floppy, and also very long paths; not all
traditional versions can do these things. (Linux only uses
GNU <command>tar</command>.) </para>
<para> If your backup doesn't fit on one tape, you need to use
the <option>--multi-volume</option> (<option>-M</option>) option:
<screen>
<prompt>#</prompt> <userinput>tar -cMf /dev/fd0H1440 /usr/src</userinput>
<computeroutput>tar: Removing leading / from absolute path names in the archive
Prepare volume #2 for /dev/fd0H1440 and hit return:</computeroutput>
<prompt>#</prompt>
</screen>
Note that you should format the floppies before you begin the
backup, or else use another window or virtual terminal and do
it when <command>tar</command> asks for a new floppy. </para>
<para> After you've made a backup, you should check that it is OK,
using the <option>--compare</option> (<option>-d</option>) option:
<screen>
<prompt>#</prompt> <userinput>tar --compare --verbose -f /dev/ftape</userinput>
<computeroutput>usr/src/
usr/src/linux
usr/src/linux-1.2.10-includes/
....</computeroutput>
<prompt>#</prompt>
</screen>
Failing to check a backup means that you will not notice that your
backups aren't working until after you've lost the original data.
</para>
<para> An incremental backup can be done with
<command>tar</command> using the <option>--newer</option>
(<option>-N</option>) option:
<screen>
<prompt>#</prompt> <userinput>tar --create --newer '8 Sep 1995' --file /dev/ftape /usr/src --verbose</userinput>
<computeroutput>tar: Removing leading / from absolute path names in the archive
usr/src/
usr/src/linux-1.2.10-includes/
usr/src/linux-1.2.10-includes/include/
usr/src/linux-1.2.10-includes/include/linux/
usr/src/linux-1.2.10-includes/include/linux/modules/
usr/src/linux-1.2.10-includes/include/asm-generic/
usr/src/linux-1.2.10-includes/include/asm-i386/
usr/src/linux-1.2.10-includes/include/asm-mips/
usr/src/linux-1.2.10-includes/include/asm-alpha/
usr/src/linux-1.2.10-includes/include/asm-m68k/
usr/src/linux-1.2.10-includes/include/asm-sparc/
usr/src/patch-1.2.11.gz</computeroutput>
<prompt>#</prompt>
</screen>
Unfortunately, <command>tar</command> can't notice when a file's
inode information has changed, for example, that it's permission
bits have been changed, or when its name has been changed.
This can be worked around using <command>find</command> and
comparing current filesystem state with lists of files that have
been previously backed up. Scripts and programs for doing this
can be found on Linux ftp sites. </para>
</sect2>
<sect2>
<title>Restoring files with <command>tar</command></title>
<para> The <option>--extract</option> (<option>-x</option>)
option for <command>tar</command> extracts files:
<screen>
<prompt>#</prompt> <userinput>tar --extract --same-permissions --verbose --file /dev/fd0H1440</userinput>
<computeroutput>usr/src/
usr/src/linux
usr/src/linux-1.2.10-includes/
usr/src/linux-1.2.10-includes/include/
usr/src/linux-1.2.10-includes/include/linux/
usr/src/linux-1.2.10-includes/include/linux/hdreg.h
usr/src/linux-1.2.10-includes/include/linux/kernel.h
...</computeroutput>
<prompt>#</prompt>
</screen>
You also extract only specific files or directories (which
includes all their files and subdirectories) by naming on the
command line:
<screen>
<prompt>#</prompt> <userinput>tar xpvf /dev/fd0H1440 usr/src/linux-1.2.10-includes/include/linux/hdreg.h</userinput>
<computeroutput>usr/src/linux-1.2.10-includes/include/linux/hdreg.h</computeroutput>
<prompt>#</prompt>
</screen>
Use the <option>--list</option> (<option>-t</option>) option,
if you just want to see what files are on a backup volume:
<screen>
<prompt>#</prompt> <userinput>tar --list --file /dev/fd0H1440</userinput>
<computeroutput>usr/src/
usr/src/linux
usr/src/linux-1.2.10-includes/
usr/src/linux-1.2.10-includes/include/
usr/src/linux-1.2.10-includes/include/linux/
usr/src/linux-1.2.10-includes/include/linux/hdreg.h
usr/src/linux-1.2.10-includes/include/linux/kernel.h
...</computeroutput>
<prompt>#</prompt>
</screen>
Note that <command>tar</command> always reads the backup volume
sequentially, so for large volumes it is rather slow. It is not
possible, however, to use random access database techniques when
using a tape drive or some other sequential medium. </para>
<para> <command>tar</command> doesn't handle deleted files
properly. If you need to restore a filesystem from a full and
an incremental backup, and you have deleted a file between
the two backups, it will exist again after you have done the
restore. This can be a big problem, if the file has sensitive
data that should no longer be available. </para>
</sect2>
</sect1>
<sect1>
<title>Multilevel backups</title>
<para> The simple backup method outlined in the previous section
is often quite adequate for personal use or small sites. For more
heavy duty use, multilevel backups are more appropriate. </para>
<para> The simple method has two backup levels: full and
incremental backups. This can be generalized to any number of
levels. A full backup would be level 0, and the different levels
of incremental backups levels 1, 2, 3, etc. At each incremental
backup level you back up everything that has changed since the
previous backup at the same or a previous level. </para>
<para> The purpose for doing this is that it allows a longer
<glossterm>backup history</glossterm> cheaply. In the example in
the previous section, the backup history went back to the previous
full backup. This could be extended by having more tapes, but
only a week per new tape, which might be too expensive. A longer
backup history is useful, since deleted or corrupted files are
often not noticed for a long time. Even a version of a file that
is not very up to date is better than no file at all. </para>
<para> With multiple levels the backup history can be extended
more cheaply. For example, if we buy ten tapes, we could use
tapes 1 and 2 for monthly backups (first Friday each month),
tapes 3 to 6 for weekly backups (other Fridays; note that there
can be five Fridays in one month, so we need four more tapes),
and tapes 7 to 10 for daily backups (Monday to Thursday).
With only four more tapes, we've been able to extend the backup
history from two weeks (after all daily tapes have been used)
to two months. It is true that we can't restore every version
of each file during those two months, but what we can restore
is often good enough. </para>
<para><xref linkend="backup-history-timeline"> shows which backup
level is used each day, and which backups can be restored from
at the end of the month. </para>
<figure id="backup-history-timeline" float="1">
<title>A sample multilevel backup schedule.</title>
<graphic fileref="backup-timeline"></graphic>
</figure>
<para> Backup levels can also be used to keep filesystem
restoration time to a minimum. If you have many incremental
backups with monotonously growing level numbers, you need to
restore all of them if you need to rebuild the whole filesystem.
Instead you can use level numbers that aren't monotonous, and
keep down the number of backups to restore. </para>
<para> To minimize the number of tapes needed to restore, you
could use a smaller level for each incremental tape. However,
then the time to make the backups increases (each backup copies
everything since the previous full backup). A better scheme is
suggested by the <command>dump</command> manual page and described
by the table XX (efficient-backup-levels). Use the following
succession of backup levels: 3, 2, 5, 4, 7, 6, 9, 8, 9, etc.
This keeps both the backup and restore times low. The most you
have to backup is two day's worth of work. The number of tapes
for a restore depends on how long you keep between full backups,
but it is less than in the simple schemes. </para>
<table id="efficient-backup-levels">
<title>Efficient backup scheme using many backup levels</title>
<tgroup cols=4>
<thead>
<row><entry>Tape</entry> <entry>Level</entry> <entry>Backup (days)</entry> <entry>Restore tapes</entry></row>
</thead>
<tbody>
<row><entry>1</entry> <entry>0</entry> <entry>n/a</entry> <entry>1</entry></row>
<row><entry>2</entry> <entry>3</entry> <entry>1</entry> <entry>1, 2</entry></row>
<row><entry>3</entry> <entry>2</entry> <entry>2</entry> <entry>1, 3</entry></row>
<row><entry>4</entry> <entry>5</entry> <entry>1</entry> <entry>1, 2, 4</entry></row>
<row><entry>5</entry> <entry>4</entry> <entry>2</entry> <entry>1, 2, 5</entry></row>
<row><entry>6</entry> <entry>7</entry> <entry>1</entry> <entry>1, 2, 5, 6</entry></row>
<row><entry>7</entry> <entry>6</entry> <entry>2</entry> <entry>1, 2, 5, 7</entry></row>
<row><entry>8</entry> <entry>9</entry> <entry>1</entry> <entry>1, 2, 5, 7, 8</entry></row>
<row><entry>9</entry> <entry>8</entry> <entry>2</entry> <entry>1, 2, 5, 7, 9</entry></row>
<row><entry>10</entry> <entry>9</entry> <entry>1</entry> <entry>1, 2, 5, 7, 9, 10</entry></row>
<row><entry>11</entry> <entry>9</entry> <entry>1</entry> <entry>1, 2, 5, 7, 9, 10, 11</entry></row>
<row><entry>...</entry> <entry>9</entry> <entry>1</entry> <entry>1, 2, 5, 7, 9, 10, 11, ...</entry></row>
</tbody>
</tgroup>
</table>
<para> A fancy scheme can reduce the amount of labor needed, but
it does mean there are more things to keep track of. You must
decide if it is worth it. </para>
<para> <command>dump</command> has built-in support for backup
levels. For <command>tar</command> and <command>cpio</command>
it must be implemented with shell scripts. </para>
</sect1>
<sect1>
<title>What to back up</title>
<para> You want to back up as much as possible. The major
exception is software that can be easily reinstalled,
<footnote><para>You get to decide what's easy.
Some people consider installing from dozens of floppies
easy.</para></footnote>
but even they may have configuration files that it is
important to back up, lest you need to do all the work to
configure them all over again. Another major exception is
the <filename>/proc</filename> filesystem; since that only
contains data that the kernel always generates automatically,
it is never a good idea to back it up. Expecially the
<filename>/proc/kcore</filename> file is unnecessary, since it
is just an image of your current physical memory; it's pretty
large as well. </para>
<para> Gray areas include the news spool, log files, and many
other things in <filename>/var</filename>. You must decide what
you consider important. </para>
<para> The obvious things to back up are user files
(<filename>/home</filename>) and system configuration files
(<filename>/etc</filename>, but possibly other things scattered
all over the filesystem). </para>
</sect1>
<sect1>
<title>Compressed backups</title>
<para> Backups take a lot of space, which can cost quite
a lot of money. To reduce the space needed, the backups
can be compressed. There are several ways of doing this.
Some programs have support for for compression built in; for
example, the <option>--gzip</option> (<option>-z</option>)
option for GNU <command>tar</command> pipes the whole backup
through the <command>gzip</command> compression program, before
writing it to the backup medium. </para>
<para> Unfortunately, compressed backups can cause trouble.
Due to the nature of how compression works, if a single bit is
wrong, all the rest of the compressed data will be unusable.
Some backup programs have some built in error correction, but no
method can handle a large number of errors. This means that if
the backup is compressed the way GNU <command>tar</command> does
it, with the whole output compressed as a unit, a single error
makes all the rest of the backup lost. Backups must be reliable,
and this method of compression is not a good idea. </para>
<para> An alternative way is to compress each file separately.
This still means that the one file is lost, but all other files
are unharmed. The lost file would have been corrupted anyway,
so this situation is not much worse than not using compression
at all. The <command>afio</command> program (a variant of
<command>cpio</command>) can do this. </para>
<para>
Compression takes some time, which may make the backup program
unable to write data fast enough for a tape drive.
<footnote><para>If a tape drive doesn't data fast enough,
it has to stop; this makes backups even slower, and can
be bad for the tape and the drive.</para></footnote>
This can be avoided by buffering the output (either internally, if
the backup program if smart enough, or by using another program),
but even that might not work well enough. This should only be
a problem on slow computers. </para>
</sect1>
</chapter>
<chapter>
<title>Keeping Time</title>
<blockquote><para><quote>Time is an illusion. Lunchtime double
so.</quote> (Douglas Adams.)</para></blockquote>
<para> This chapter explains how a Linux system keeps time,
and what you need to do to avoid causing trouble. Usually,
you don't need to do anything about time, but it is good to
understand it.</para>
<sect1>
<title>Time zones</title>
<para> Time measurement is based on mostly regular natural
phenomena, such as alternating light and dark periods caused
by the rotation of the planet. The total time taken by two
successive periods is constant, but the lengths of the light
and dark period vary. One simple constant is noon. </para>
<para> Noon is the time of the day when the Sun is at its
highest position. Since the Earth is round,
<footnote><para>According to
recent research.</para></footnote>
noon happens at different times in different places. This leads
to the concept of <glossterm>local time</glossterm>. Humans
measure time in many units, most of which are tied to natural
phenomena like noon. As long as you stay in the same place,
it doesn't matter that local times differ. </para>
<para> As soon as you need to communicate with distant places,
you'll notice the need for a common time. In modern times,
most of the places in the world communicate with most other
places in the world, so a global standard for measuring time
has been defined. This time is called <glossterm>universal
time</glossterm> (UT or UTC, formerly known as Greenwich Mean Time
or GMT, since it used to be local time in Greenwich, England).
When people with different local times need to communicate,
they can express times in universal time, so that there is no
confusion about when things should happen. </para>
<para> Each local time is called a time zone. While geography
would allow all places that have noon at the same time have the
same time zone, politics makes it difficult. For various reasons,
many countries use <glossterm>daylight savings time</glossterm>,
that is, they move their clocks to have more natural light
while they work, and then move the clocks back during winter.
Other countries do not do this. Those that do, do not agree when
the clocks should be moved, and they change the rules from year
to year. This makes time zone conversions definitely non-trivial.
</para>
<para> Time zones are best named by the location or by telling
the difference between local and universal time. In the US
and some other countries, the local time zones have a name and
a three letter abbreviation. The abbreviations are not unique,
however, and should not be used unless the country is also named.
It is better to talk about the local time in, say, Helsinki,
than about East European time, since not all countries in Eastern
Europe follow the same rules. </para>
<para> Linux has a time zone package that knows about all
existing time zones, and that can easily be updated when the
rules change. All the system administrator needs to do is to
select the appropriate time zone. Also, each user can set his
own time zone; this is important since many people work with
computers in different countries over the Internet. When the
rules for daylight savings time change in your local time zone,
make sure you'll upgrade at least that part of your Linux system.
Other than setting the system time zone and upgrading the time
zone data files, there is little need to bother about time.
</para>
</sect1>
<sect1>
<title>The hardware and software clocks</title>
<para> A personal computer has a battery driven hardware clock.
The battery ensures that the clock will work even if the rest of
the computer is without electricity. The hardware clock can be
set from the BIOS setup screen or from whatever operating system
is running. </para>
<para> The Linux kernel keeps track of time independently from
the hardware clock. During the boot, Linux sets its own clock
to the same time as the hardware clock. After this, both clocks
run independently. Linux maintains its own clock because looking
at the hardware is slow and complicated. </para>
<para> The kernel clock always shows universal time. This way,
the kernel does not need to know about time zones at all. The
simplicity results in higher reliability and makes it easier
to update the time zone information. Each process handles time
zone conversions itself (using standard tools that are part of
the time zone package). </para>
<para> The hardware clock can be in local time or in universal
time. It is usually better to have it in universal time,
because then you don't need to change the hardware clock when
daylight savings time begins or ends (UTC does not have DST).
Unfortunately, some PC operating systems, including MS-DOS,
Windows, and OS/2, assume the hardware clock shows local time.
Linux can handle either, but if the hardware clock shows local
time, then it must be modified when daylight savings time begins
or ends (otherwise it wouldn't show local time). </para>
</sect1>
<sect1>
<title>Showing and setting time</title>
<para> In the Debian system, the system time zone is determined
by the symbolic link <filename>/etc/localtime</filename>.
This link points at a time zone data file that describes
the local time zone. The time zone data files are stored in
<filename>/usr/lib/zoneinfo</filename>. Other Linux distributions
may do this differently. </para>
<para> A user can change his private time zone by setting the
TZ environment variable. If it is unset, the system time zone
is assumed. The syntax of the TZ variable is described in the
<function>tzset</function> manual page. </para>
<para>
The <command>date</command> command shows the current date and
time.
<footnote><para>Beware of the <command>time</command> command, which does
not show the current time.</para></footnote>
For example:
<screen>
<prompt>$</prompt> <userinput>date</userinput>
<computeroutput>Sun Jul 14 21:53:41 EET DST 1996</computeroutput>
<prompt>$</prompt>
</screen>
That time is Sunday, 14th of July, 1996, at about ten before
ten at the evening, in the time zone called ``EET DST''
(which might be East European Daylight Savings Time).
<command>date</command> can also show the univeral time:
<screen>
<prompt>$</prompt> <userinput>date -u</userinput>
Sun Jul 14 18:53:42 UTC 1996
<computeroutput>Sun Jul 14 18:53:42 UTC 1996</computeroutput>
<prompt>$</prompt>
</screen>
<command>date</command> is also used to set the kernel's software
clock:
<screen>
<prompt>#</prompt> <userinput>date 07142157</userinput>
<computeroutput>Sun Jul 14 21:57:00 EET DST 1996</computeroutput>
<prompt>#</prompt> <userinput>date</userinput>
<computeroutput>Sun Jul 14 21:57:02 EET DST 1996</computeroutput>
<prompt>#</prompt>
</screen>
See the <command>date</command> manual page for more details;
the syntax is a bit arcane. Only root can set the time.
While each user can have his own time zone, the clock is the
same for everyone. </para>
<para> <command>date</command> only shows or sets the software
clock. The <command>clock</command> commands syncronizes
the hardware and software clocks. It is used when the system
boots, to read the hardware clock and set the software clock.
If you need to set both clocks, you first set the software clock
with <command>date</command>, and then the hardware clock with
<command>clock -w</command>. </para>
<para> The <option>-u</option> option to <command>clock</command>
tells it that the hardware clock is in universal time.
You <emphasis>must</emphasis> use the <option>-u</option>
option correctly. If you don't, your computer will be quite
confused about what the time is. </para>
<para> The clocks should be changed with care. Many parts of a
Unix system require the clocks to work correctly. For example,
the <command>cron</command> daemon runs commands periodically.
If you change the clock, it can be confused of whether
it needs to run the commands or not. On one early Unix
system, someone set the clock twenty years into the future,
and <command>cron</command> wanted to run all the periodic
commands for twenty years all at once. Current versions of
<command>cron</command> can handle this correctly, but you should
still be careful. Big jumps or backward jumps are more dangeours
than smaller or forward ones. </para>
</sect1>
<sect1>
<title>When the clock is wrong</title>
<para> The Linux software clock is not always accurate. It is
kept running by a periodic <glossterm>timer interrupt</glossterm>
generated by PC hardware. If the system has too many processes
running, it may take too long to service the timer interrupt, and
the software clock starts slipping behind. The hardware clock
runs independently and is usually more accurate. If you boot
your computer often (as is the case for most systems that aren't
servers), it will usually keep fairly accurate time. </para>
<para> If you need to adjust the hardware clock, it is usually
simplest to reboot, go into the BIOS setup screen, and do it
from there. This avoids all trouble that changing system time
might cause. If doing it via BIOS is not an option, set the new
time with <command>date</command> and <command>clock</command>
(in that order), but be prepared to reboot, if some part of the
system starts acting funny. </para>
<para> A networked computer (even if just over the modem) can
check its own clock automatically, by comparing it to some other
computer's time. If the other computer is known to keep very
accurate time, then both computers will keep accurate time.
This can be done by using the <command>rdate</command> and
<command>netdate</command> commands. Both check the time of a
remote computer (<command>netdate</command> can handle several
remote computers), and set the local computer's time to that.
By running one these commands regularly, your computer will keep
as accurate time as the remote computer. </para>
<para> XXX say something intelligent about NTP </para>
</sect1>
</chapter>
<glossary>
<title>Glossary (DRAFT)</title>
<blockquote><para><quote>The Librarian of the Unseen University
had unilaterally decided to aid comprehension
by producing an Orang-utan/Human Dictionary.
He'd been working on it for three months.
It wasn't easy. He'd got as far as `Oook.'</quote>
(Terry Pratchett, ``Men At Arms'')</para></blockquote>
<para> This is a short list of word definitions for concepts
relating to Linux and system administration. </para>
<glossentry>
<glossterm>ambition</glossterm>
<glossdef><para>
The act of writing funny sentences in the hope of getting them
into the Linux cookie file.
</para></glossdef>
</glossentry>
<glossentry>
<glossterm>application program</glossterm>
<glossdef><para>
Software that does something useful. The results of using an
application program is what the computer was bought for.
See also system program, operating system.
</para></glossdef>
</glossentry>
<glossentry>
<glossterm>daemon</glossterm>
<glossdef><para>
A process lurking in the background, usually unnoticed, until
something triggers it into action. For example, the <command>update</command>
daemon wakes up every thirty seconds or so to flush the buffer
cache, and the <command>sendmail</command> daemon awakes whenever someone sends
mail.
</para></glossdef>
</glossentry>
<glossentry>
<glossterm>file system</glossterm>
<glossdef><para>
The methods and data structures that an operating
system uses to keep track of files on a disk or partition;
the way the files are organized on the disk. Also used about
a partition or disk that is used to store the files
or the type of the filesystem.
</para></glossdef>
</glossentry>
<glossentry>
<glossterm>glossary</glossterm>
<glossdef><para>
A list of words and explanations of what they do. Not
to be confused with a dictionary, which is also a list of
words and explanations.
</para></glossdef>
</glossentry>
<glossentry>
<glossterm>kernel</glossterm>
<glossdef><para>
Part of an operating system that implements the interaction with
hardware and the sharing of resources. See also system program.
</para></glossdef>
</glossentry>
<glossentry>
<glossterm>operating system</glossterm>
<glossdef><para>
Software that shares a computer system's resources (processor,
memory, disk space, network bandwidth, and so on) between
users and the application programs they run. Controls access
to the system to provide security. See also kernel, system program,
application program.
</para></glossdef>
</glossentry>
<glossentry>
<glossterm>system call</glossterm>
<glossdef><para>
The services provided by the kernel to application programs,
and the way in which they are invoked. See section 2 of the
manual pages.
</para></glossdef>
</glossentry>
<glossentry>
<glossterm>system program</glossterm>
<glossdef><para>
Programs that implement high level functionality of an operating
system, i.e., things that aren't directly dependent on the
hardware. May sometimes require special privileges to run
(e.g., for delivering electronic mail), but often just commonly
thought of as part of the system (e.g., a compiler). See also
application program, kernel, operating system.
</para></glossdef>
</glossentry>
</glossary>
</book>
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