File: simulation

package info (click to toggle)
debian-astro 5.0
  • links: PTS, VCS
  • area: main
  • in suites: forky, sid, trixie
  • size: 264 kB
  • sloc: makefile: 20
file content (81 lines) | stat: -rw-r--r-- 3,042 bytes parent folder | download
1
2
3
4
5
6
7
8
9
10
11
12
13
14
15
16
17
18
19
20
21
22
23
24
25
26
27
28
29
30
31
32
33
34
35
36
37
38
39
40
41
42
43
44
45
46
47
48
49
50
51
52
53
54
55
56
57
58
59
60
61
62
63
64
65
66
67
68
69
70
71
72
73
74
75
76
77
78
79
80
81
Format: https://blends.debian.org/blends/1.1
Task: Simulation
Install: true
Description: Simulation packages for astronomy
 This metapackage will install packages for celestial, astronomical and
 cosmological simulations.

Recommends: splash

Recommends: gyoto

Recommends: lorene

Recommends: yorick-yao

Recommends: python3-yt

Recommends: geant321
Why: taken from ascl

Recommends: cloudy
WNPP: 725891

Recommends: mocassin

Recommends: mpgrafic

Recommends: visit
WNPP: 395573
Homepage: https://visit-dav.github.io/visit-website/
Pkg-Description: Interactive parallel visualization and graphical analysis tool
 VisIt is a free interactive parallel visualization and graphical
 analysis tool for viewing scientific data.  Users can quickly generate
 visualizations from their data, animate them through time, manipulate
 them, and save the resulting images for presentations.  VisIt contains
 a rich set of visualization features so that you can view your data in
 a variety of ways.  It can be used to visualize scalar and vector
 fields defined on two- and three-dimensional (2D and 3D) structured and
 unstructured meshes.
 .
 VisIt was designed to handle very large data set sizes in the terascale
 range and yet can also handle small data sets in the kilobyte range.

Recommends: inhomog
WNPP: 872509
Homepage: https://bitbucket.org/broukema/inhomog
Pkg-Description: kinematical backreaction and average scale factor evolution
 This is a library (shared + static) and a front-end example program
 used for relativistic cosmology. The front-end `inhomog' provides
 command-line numerical exploration of a key question in present-day
 observational cosmology (is dark energy just an artefact of not
 modelling structure formation properly?) and the library is aimed for
 use by more computationally intensive simulations studying the same
 family of questions.

Recommends: splotch
WNPP: 892482
Homepage: http://wwwmpa.mpa-garching.mpg.de/~kdolag/Splotch/
Pkg-Description : Ray tracer to visualize SPH simulations
 This is some software for high performance visualization of huge
 scientific data.

Recommends: disperse
WNPP: 898834
Homepage: http://www2.iap.fr/users/sousbie/web/html/indexd41d.html
Pkg-Description: Automatic feature identification in 2D and 3D
 DisPerSE stands for "Discrete Persistent Structures Extractor" and
 its main purpose is the automatic identification of persistent
 topological features such as peaks, voids, walls and in particular
 filamentary structures within sampled distributions in 2D, 3D, and
 possibly more...

Recommends: python3-einsteinpy
WNPP: 925241
Homepage: https://github.com/einsteinpy/einsteinpy
Pkg-Description: Python Library for General Relativity
 EinsteinPy is an open source pure Python package dedicated to
 problems arising in General Relativity and relativistic physics, such
 as goedesics plotting for schwarzschild space-time model, calculation
 of schwarzschild radius for any mass given, symbolic calculation of
 various functions related to GR such as christoffel symbols.