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 82 83 84 85 86 87 88 89 90 91 92 93 94 95 96 97 98 99 100 101 102 103 104 105 106 107 108 109 110 111 112 113 114 115 116 117 118 119 120 121 122 123 124 125 126 127 128 129 130 131 132 133 134 135 136 137 138 139 140 141 142 143 144 145 146 147 148 149 150 151 152 153 154 155 156 157 158 159 160 161 162 163 164 165 166 167 168 169 170 171 172 173 174 175 176 177 178 179 180 181 182 183 184 185 186 187 188 189 190 191 192 193 194 195 196 197 198 199 200 201 202 203 204 205 206 207 208 209 210 211 212 213 214 215 216 217 218 219 220 221 222 223 224 225 226 227 228 229 230 231 232 233 234 235 236 237 238 239 240 241 242 243 244 245 246 247 248 249 250 251 252 253 254 255 256 257 258 259 260 261 262 263 264 265 266 267 268 269 270 271 272 273 274 275 276 277 278 279 280 281 282 283 284 285 286 287 288 289 290 291 292 293 294 295 296 297 298 299 300 301 302 303 304 305 306 307 308 309 310 311 312 313 314 315 316 317 318 319 320 321 322 323 324 325 326 327 328 329 330 331 332 333 334 335 336 337 338 339 340 341 342 343 344 345 346 347 348 349 350 351 352 353 354 355 356 357 358 359 360 361 362 363 364 365 366 367 368 369 370 371 372 373 374 375 376 377 378 379 380 381 382 383 384 385 386 387 388 389 390 391 392 393 394 395 396 397 398 399 400 401 402 403 404 405 406 407 408 409 410 411 412 413 414 415 416 417 418 419 420 421 422 423 424 425 426 427 428 429 430 431 432 433 434 435 436 437 438 439 440 441 442 443 444 445 446 447 448 449 450 451 452 453 454 455 456 457 458 459 460 461 462 463 464 465 466 467 468 469 470 471 472 473 474 475 476 477 478 479 480 481 482 483 484 485 486 487 488 489 490 491 492 493 494 495 496 497 498 499 500 501 502 503 504 505 506 507 508 509 510 511 512 513 514 515 516 517 518 519 520 521 522 523 524 525 526 527 528 529 530 531 532 533 534 535 536 537 538 539 540 541 542 543 544 545 546 547 548 549 550 551 552 553 554 555 556 557 558 559 560 561 562 563 564 565 566 567 568 569 570 571 572 573 574 575 576 577 578 579 580 581 582 583 584 585 586 587 588 589 590 591 592 593 594 595 596 597 598 599 600 601 602 603 604 605 606 607 608 609 610 611 612 613 614 615 616 617 618 619 620 621
|
/*
Copyright 2013-2016, 2018-2020 Frederic Vincent, Thibaut Paumard
This file is part of Gyoto.
Gyoto is free software: you can redistribute it and/or modify
it under the terms of the GNU General Public License as published by
the Free Software Foundation, either version 3 of the License, or
(at your option) any later version.
Gyoto is distributed in the hope that it will be useful,
but WITHOUT ANY WARRANTY; without even the implied warranty of
MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
GNU General Public License for more details.
You should have received a copy of the GNU General Public License
along with Gyoto. If not, see <http://www.gnu.org/licenses/>.
*/
#include "GyotoPhoton.h"
#include "GyotoDynamicalDisk3D.h"
#include "GyotoUtils.h"
#include "GyotoFactoryMessenger.h"
#include "GyotoKerrBL.h"
#include "GyotoKerrKS.h"
#include <iostream>
#include <iomanip>
#include <fstream>
#include <cstdlib>
#include <fstream>
#include <cstring>
#include <cmath>
#include <limits>
#include <sstream>
#include <dirent.h>
using namespace std;
using namespace Gyoto;
using namespace Gyoto::Astrobj;
#include "GyotoProperty.h"
GYOTO_PROPERTY_START(DynamicalDisk3D)
GYOTO_PROPERTY_FILENAME(DynamicalDisk3D, File, file)
GYOTO_PROPERTY_DOUBLE(DynamicalDisk3D, tinit, tinit)
GYOTO_PROPERTY_DOUBLE(DynamicalDisk3D, dt, dt)
GYOTO_PROPERTY_BOOL(DynamicalDisk3D,
TemperatureGrid, IntensityGrid, temperature)
GYOTO_PROPERTY_DOUBLE(DynamicalDisk3D, PLindex, PLindex)
GYOTO_PROPERTY_BOOL(DynamicalDisk3D,
WithVelocity, NoVelocity, withVelocity)
GYOTO_PROPERTY_DOUBLE(DynamicalDisk3D, FloorTemperature, floorTemperature)
GYOTO_PROPERTY_END(DynamicalDisk3D, Disk3D::properties)
DynamicalDisk3D::DynamicalDisk3D() :
Disk3D(),
spectrumBB_(NULL),
temperature_(1),
dirname_(NULL),
tinit_(0.),
dt_(1.),
nb_times_(1),
PLindex_(3),
novel_(0),
floortemperature_(0),
emission_array_(NULL),
velocity_array_(NULL),
absorption_array_(NULL)
{
GYOTO_DEBUG << "DynamicalDisk3D Construction" << endl;
spectrumBB_ = new Spectrum::BlackBody();
}
DynamicalDisk3D::DynamicalDisk3D(const DynamicalDisk3D& o) :
Disk3D(o),
spectrumBB_(NULL),
temperature_(o.temperature_),
dirname_(NULL),
tinit_(o.tinit_),
dt_(o.dt_),
nb_times_(o.nb_times_),
PLindex_(o.PLindex_),
novel_(o.novel_),
floortemperature_(o.floortemperature_),
emission_array_(NULL),
velocity_array_(NULL),
absorption_array_(NULL)
{
GYOTO_DEBUG << "DynamicalDisk3D Copy" << endl;
if (o.spectrumBB_()) spectrumBB_=o.spectrumBB_->clone();
if (o.dirname_){
//dirname_ copy
size_t length = strlen(o.dirname_)+1;
dirname_ = new char[length];
memcpy(dirname_, o.dirname_, length);
}
if (o.emission_array_ && o.velocity_array_){
// emission_array_ and velocity_array_ copy
size_t naxes[4];
getEmissquantNaxes(naxes);
size_t nnu=naxes[0], nphi=naxes[1], nz=naxes[2], nr=naxes[3];
// Allocate
emission_array_ = new double*[nb_times_];
velocity_array_ = new double*[nb_times_];
// Copy
size_t nel1=nnu*nphi*nz*nr,
nel2=3*nphi*nz*nr,
szt=nel1*sizeof(double),
szv=nel2*sizeof(double);
for (int i=1; i<=nb_times_; i++) {
emission_array_[i-1] = new double[nel1];
velocity_array_[i-1] = new double[nel2];
memcpy(emission_array_[i-1], o.emission_array_[i-1], szt);
memcpy(velocity_array_[i-1], o.velocity_array_[i-1], szv);
}
// If absorption is given, copy
if (o.absorption_array_){
absorption_array_ = new double*[nb_times_];
for (int i=1; i<=nb_times_; i++) {
absorption_array_[i-1] = new double[nel1];
memcpy(absorption_array_[i-1], o.absorption_array_[i-1], szt);
}
}
}
}
DynamicalDisk3D* DynamicalDisk3D::clone() const
{ return new DynamicalDisk3D(*this); }
bool DynamicalDisk3D::isThreadSafe() const {
// spectrumBB_ is not handled by a property.
return Disk3D::isThreadSafe()
&& (!spectrumBB_ || spectrumBB_ -> isThreadSafe());
}
DynamicalDisk3D::~DynamicalDisk3D() {
GYOTO_DEBUG << "DynamicalDisk3D Destruction" << endl;
if (emission_array_) delete [] emission_array_;
if (absorption_array_) delete [] absorption_array_;
if (velocity_array_) delete [] velocity_array_;
}
double const * DynamicalDisk3D::getVelocity() const { return Disk3D::getVelocity(); }
void DynamicalDisk3D::copyQuantities(int iq) {
if (iq<1 || iq>nb_times_)
GYOTO_ERROR("In DynamicalDisk3D::copyQuantities: incoherent value of iq");
setEmissquant(emission_array_[iq-1]);
if (absorption_array_) opacity(absorption_array_[iq-1]);
setVelocity(velocity_array_[iq-1]);
}
void DynamicalDisk3D::getVelocity(double const pos[4], double vel[4]) {
if (novel_){
// Velocity of emitted particle is not provided (only bulk velocity
// is known). Then put velocity to default, redshift factor will
// be constant.
vel[0]=1.;vel[1]=0.;vel[2]=0.;vel[3]=0.;
}else{
double rcur=pos[1];
double risco;
switch (gg_->coordKind()) {
case GYOTO_COORDKIND_SPHERICAL:
{
string kin = gg_->kind();
if (kin == "KerrBL")
risco = static_cast<SmartPointer<Metric::KerrBL> >(gg_) -> getRms();
else if (kin == "Minkowski")
risco = 6.;
else
risco=0., GYOTO_ERROR("In DynamicalDisk3D::getVelocity: bad metric");
break;
}
default:
GYOTO_ERROR("DynamicalDisk3D::getVelocity: bad COORDKIND");
risco=0.;
}
if (rcur<risco){
//default velocity, emission will be 0 there anyway
vel[0]=1.;
for (int ii=1;ii<4;ii++)
vel[ii]=0.;
}else{
double time = pos[0], tcomp=tinit_;
int ifits=1;
while(time>tcomp && ifits<nb_times_){
tcomp+=dt_;
ifits++;
}
if (ifits==1 || ifits==nb_times_){
copyQuantities(ifits);
Disk3D::getVelocity(pos,vel);
}else{
double vel1[4], vel2[4];
copyQuantities(ifits-1);
Disk3D::getVelocity(pos,vel1);
copyQuantities(ifits);
Disk3D::getVelocity(pos,vel2);
for (int ii=0;ii<4;ii++){ // 1st order interpol
double t1 = tinit_+(ifits-2)*dt_;
vel[ii]=vel1[ii]+(vel2[ii]-vel1[ii])/dt_*(time-t1);
}
}
}
}
}
double DynamicalDisk3D::emission1date(double nu, double dsem,
state_t const &,
double const co[8]) const{
GYOTO_DEBUG << endl;
double * emiss = const_cast<double*>(getEmissquant());
double risco;
switch (gg_->coordKind()) {
case GYOTO_COORDKIND_SPHERICAL:
{
string kin = gg_->kind();
if (kin == "KerrBL")
risco = static_cast<SmartPointer<Metric::KerrBL> >(gg_) -> getRms();
else if (kin == "Minkowski")
risco = 6.;
else
risco=0., GYOTO_ERROR("In DynamicalDisk3D::getVelocity: bad metric");
break;
}
default:
GYOTO_ERROR("DynamicalDisk3D::emission1date(): bad COORDKIND"
", should be BL corrdinates");
risco=0.;
}
double rcur=co[1];
if (rcur*fabs(sin(co[2])) > rout() || rcur < risco) return 0.;
size_t i[4]; // {i_nu, i_phi, i_z, i_r}
getIndices(i,co,nu);
size_t naxes[4];
getEmissquantNaxes(naxes);
size_t nnu=naxes[0], nphi=naxes[1], nz=naxes[2];
double emissq = emiss[i[3]*nphi*nz*nnu+i[2]*nphi*nnu+i[1]*nnu+i[0]];
//This is a quantity from which emiss. coef. j_nu is known
//this is temperature in K if temperature_=1
//or directly j_nu, up to the nu dependence, if temperature_=0
double Ires=-1.; // emitted specific intensity
if (!flag_radtransf_){ // optically thick case
if (temperature_){
spectrumBB_->temperature(emissq);
Ires=(*spectrumBB_)(nu);
//cout << "in emis: " << emissq << " " << Ires << endl;
}else{
Ires=emissq;
}
}else{// // optically thin case
if (temperature_){
// cout << "in DD3 Ires= " << rcur << " " << th << " " << emissq << " " << floortemperature_ << " ";
if (emissq<floortemperature_){
//cout << "return 0 " << emissq << " " << floortemperature_ << endl;
//throwwError("test dynad3d");
Ires=0.;
}else{
// BB radiation
spectrumBB_->temperature(emissq);
Ires=(*spectrumBB_)(nu);
//cout << "return " << emissq << " " << Ires << endl;
// BELOW: BREMS computation for 2012 RWI paper
// //SI value of cylindrical r coordinate:
// double dist_unit = gg_->unitLength();
// /*
// Following fact (in SI units) is defined by:
// fact=RR/(Mm*kappa*gamma)
// with:
// RR=8.3144621; // Perfect gas constant in SI
// Mm=6e-4; //This is N_avogadro*M_atomicmassunit/gamma in kg/mol
// kappa=3e10; // p = kappa*density^gamma
// gamma=1.66667;
// [see DynaDisk3D.i]
// */
// double fact=2.77149e-07;
// //See DynaDisk3D.i, or paper, for relation between emissq and density
// double density=pow(fact*emissq,1.5);// 1.5 is 1/(gamma-1)
// //density is in SI units, kg/m^3
// /*** Computing emission coef: ***/
// //Emission coef jnu for thermal bremsstrahlung
// // (see RybickiLightman 5.14a)
// /*
// fact2=1/4pi * 2^5*pi*e^6/(3*me*c^3) * sqrt(2pi/(3*kB*me)) * 1/mu^2
// in SI, with: me=electron mass, e=electron charge, kB=boltzman,
// mu=atomic mass unit
// Anyway this factor has no importance,
// we are interested in relative values
// */
// double fact2=7.83315e-12;
// double hok=4.79924e-11; //planck cst / boltzman cst
// double jnu = fact2 * 1./sqrt(emissq) * density*density
// * exp(-hok*nu/emissq);
// //Elementary intensity added by current dsem segment of worldline
// //in SI units:
// Ires=jnu*dsem*dist_unit; // usd e.g. for 3D RWI computation
// //cout << "stuff: " << density << " " << fact2 << " " << emissq << " " << dsem << " " << jnu << endl;
}
// cout << Ires << endl; // TEST
}else{
//Ires=Iem; // used e.g. for GC blob computation
double dist_unit = gg_->unitLength()*100.; // unit length in cgs
double jnu = emissq*pow(nu,-(PLindex_-1.)/2.);
Ires=jnu*dsem*dist_unit;
}
}
return Ires;
}
double DynamicalDisk3D::emission(double nu, double dsem,
state_t const &cph,
double const co[8]) const {
GYOTO_DEBUG << endl;
double time = co[0], tcomp=tinit_;
int ifits=1;
while(time>tcomp && ifits<nb_times_){
tcomp+=dt_;
ifits++;
}
if (ifits==1 || ifits==nb_times_){
const_cast<DynamicalDisk3D*>(this)->copyQuantities(ifits); //awful trick to avoid problems with constness of function emission -> to improve
return emission1date(nu,dsem,cph,co);
}else{
double I1, I2;
const_cast<DynamicalDisk3D*>(this)->copyQuantities(ifits-1);
I1=emission1date(nu,dsem,cph,co);
const_cast<DynamicalDisk3D*>(this)->copyQuantities(ifits);
I2=emission1date(nu,dsem,cph,co);
double t1 = tinit_+(ifits-2)*dt_;
return I1+(I2-I1)/dt_*(time-t1);
}
return 0.;
}
double DynamicalDisk3D::transmission1date(double nu, double dsem,
state_t const &,
double const co[8]) const{
GYOTO_DEBUG << endl;
if (!flag_radtransf_) return 0.;
double risco;
switch (gg_->coordKind()) {
case GYOTO_COORDKIND_SPHERICAL:
{
string kin = gg_->kind();
if (kin == "KerrBL")
risco = static_cast<SmartPointer<Metric::KerrBL> >(gg_) -> getRms();
else if (kin == "Minkowski")
risco = 6.;
else
risco=0., GYOTO_ERROR("In DynamicalDisk3D::getVelocity: bad metric");
break;
}
default:
GYOTO_ERROR("DynamicalDisk3D::emission1date(): bad COORDKIND"
", should be BL corrdinates");
risco=0.;
}
double rcur=co[1];
if (rcur*fabs(sin(co[2])) > rout() || rcur < risco) return 0.;
size_t i[4]; // {i_nu, i_phi, i_z, i_r}
getIndices(i,co,nu);
size_t naxes[4];
getEmissquantNaxes(naxes);
size_t nnu=naxes[0], nphi=naxes[1], nz=naxes[2];
if (temperature_){
double * emiss = const_cast<double*>(getEmissquant());
double emissq = emiss[i[3]*nphi*nz*nnu+i[2]*nphi*nnu+i[1]*nnu+i[0]];
//emissq is local temperature in K
//cout << "in trans DD3: " << rcur << " " << th << " " << emissq << " " << floortemperature_ << endl;
if (emissq<floortemperature_) return 1.;
else return 0.;
// BELOW: absorption for RWI 2012 paper
// spectrumBB_->temperature(emissq);
// double BnuT=(*spectrumBB_)(nu); //Planck function
// double jnu=emission1date(nu,dsem,NULL,co); // Emission coef * ds
// double alphanu=0.; //absorption coef.
// if (BnuT==0.){
// /*
// BnuT can be 0 in the region close to ISCO where density
// decreases very fast. Then jnu should be 0 too (density~0).
// If both are 0, then nothing happens (no absorption, no emission,
// it's free space). Thus leave alphanu=0.
// If jnu!=0 then alphanu is not defined, this should not happen.
// */
// if (jnu!=0.){
// cout << "r= " << rcur << " " << emissq << " " << jnu << " " << BnuT << endl;
// GYOTO_ERROR("In DynamicalDisk3D::"
// "transmission1date absorption coef. undefined!");
// }
// }else{
// alphanu=jnu/BnuT;
// }
// //Thermal emission assumed, use Kirchhoff alphanu=jnu/Bnu
// return exp(-alphanu); // the dsem factor is already included
// //in alphanu via jnu=emission1date(...,dsem,...)
}else{
if (absorption_array_){
double * abs = const_cast<double*>(opacity());
double absq = abs[i[3]*nphi*nz*nnu+i[2]*nphi*nnu+i[1]*nnu+i[0]];
double dist_unit = gg_->unitLength()*100.; //dist unit in cgs
double alphanu=absq*pow(nu,-(PLindex_+4.)/2.);
return exp(-alphanu*dsem*dist_unit);
}else{
GYOTO_ERROR("In DynamicalDisk3D: in non-BB optically thin case, "
"opacity should be provided");
}
}
GYOTO_ERROR("BUG: should not reach this point!");
return 0.; // avoid pedantic warning
}
double DynamicalDisk3D::transmission(double nuem, double dsem, state_t const &cp, double const *co) const {
GYOTO_DEBUG << endl;
double time = co[0], tcomp=tinit_;
int ifits=1;
while(time>tcomp && ifits<nb_times_){
tcomp+=dt_;
ifits++;
}
if (ifits==1 || ifits==nb_times_){
const_cast<DynamicalDisk3D*>(this)->copyQuantities(ifits); //awful trick to avoid problems with constness of function transmission -> to improve
return transmission1date(nuem,dsem,cp,co);
}else{
double I1, I2;
const_cast<DynamicalDisk3D*>(this)->copyQuantities(ifits-1);
I1=transmission1date(nuem,dsem,cp,co);
const_cast<DynamicalDisk3D*>(this)->copyQuantities(ifits);
I2=transmission1date(nuem,dsem,cp,co);
double t1 = tinit_+(ifits-2)*dt_;
return I1+(I2-I1)/dt_*(time-t1);
}
return double(flag_radtransf_);
}
void DynamicalDisk3D::metric(SmartPointer<Metric::Generic> gg) {
//Metric must be KerrBL (see emission function)
string kin = gg->kind();
if (kin != "KerrBL" && kin != "Minkowski")
GYOTO_ERROR
("DynamicalDisk3D::metric(): metric must be KerrBL");
Disk3D::metric(gg);
}
void DynamicalDisk3D::file(std::string const &content) {
#ifdef GYOTO_USE_CFITSIO
int withopacity=0;
dirname_ = new char[strlen(content.c_str())+1];
strcpy(dirname_,content.c_str());
DIR *dp;
struct dirent *dirp;
if((dp = opendir(dirname_)) == NULL) {
GYOTO_ERROR("In DynamicalDisk3D.C constructor : bad dirname_");
}
nb_times_=0;
while ((dirp = readdir(dp)) != NULL) {
nb_times_++;
}
nb_times_-=2; //for directories . and ..
/*
NB: ***Caution***, here it is assumed that dirname_
contains ONLY the FITS files, nothing else.
*/
closedir(dp);
GYOTO_DEBUG << "FITS directory, number of FITS files= " <<
dirname_ << " " << nb_times_ << endl;
if (nb_times_<1)
GYOTO_ERROR("In DynamicalDisk3D.C: bad nb_times_ value");
//check whether absorption is provided
{
// make declarations local (avoid warning)
ostringstream stream_name ;
stream_name << dirname_ << "data3D0001.fits.gz";
string filename = stream_name.str();
fitsRead(filename);
}
if (opacity()) {
//cout << "WITH OPACITY" << endl;
withopacity=1;
}
//initialize emission, absorption, velocity arrays
emission_array_ = new double*[nb_times_] ;
if (withopacity) absorption_array_ = new double*[nb_times_] ;
else absorption_array_=NULL;
velocity_array_ = new double*[nb_times_] ;
double nu0b=0., zminb=0., zmaxb=0., rinb=0., routb=0.;
size_t nnub=0, nphib=0, nzb=0, nrb=0;
//fill in the arrays
for (int i=1; i<=nb_times_; i++) {
ostringstream stream_name ;
stream_name << dirname_ << "data3D"
<< setw(4) << setfill('0')
<< i << ".fits.gz" ;
string filename = stream_name.str();
GYOTO_DEBUG << "Reading FITS file: " << filename << endl ;
fitsRead(filename);
size_t naxes[4];
getEmissquantNaxes(naxes);
size_t nnu=naxes[0], nphi=naxes[1],
nz=naxes[2], nr=naxes[3];
size_t nel1=nnu*nphi*nz*nr, nel2=3*nr*nz*nphi;
//save emission
if (getEmissquant()){
double * emtemp = const_cast<double*>(getEmissquant());
emission_array_[i-1] = new double[nel1];
for (size_t j=0;j<nel1;j++)
emission_array_[i-1][j]=emtemp[j];
}else {
GYOTO_ERROR("In DynamicalDisk3D::file(fname): "
"Emission must be supplied");
}
//save absorption (if any)
if (withopacity){
if (opacity()){
double * abstemp = const_cast<double*>(opacity());
absorption_array_[i-1] = new double[nel1];
for (size_t j=0;j<nel1;j++)
absorption_array_[i-1][j]=abstemp[j];
//cout << "SAVING ABS ARRAY" << endl;
}else{
GYOTO_ERROR("In DynamicalDisk3D::file(fname): "
"Absorption should be supplied here");
}
}
//save velocity
if (getVelocity()){
double * veltemp = const_cast<double*>(getVelocity());
velocity_array_[i-1] = new double[nel2];
for (size_t j=0;j<nel2;j++)
velocity_array_[i-1][j]=veltemp[j];
}else{
GYOTO_ERROR("In DynmicalDisk::file(fname): "
"Velocity must be supplied");
}
//check grid is constant
if (i==1){
nu0b=nu0();nnub=nnu;
nphib=nphi;
zminb=zmin();zmaxb=zmax();nzb=nz;
rinb=rin();routb=rout();nrb=nr;
}
if (
nu0()!=nu0b || nnu!=nnub
|| nphi!=nphib
|| zmin()!=zminb || zmax()!=zmaxb || nz!=nzb
|| rin()!=rinb || rout()!=routb || nr!=nrb
) GYOTO_ERROR("DynamicalDisk3D::file(fname) Grid is not constant!");
}
#else
GYOTO_ERROR("This Gyoto has no FITS i/o");
#endif
}
std::string DynamicalDisk3D::file() const {return dirname_;}
void DynamicalDisk3D::tinit(double t) {tinit_=t;}
double DynamicalDisk3D::tinit()const{return tinit_;}
void DynamicalDisk3D::dt(double t) {dt_=t;}
double DynamicalDisk3D::dt()const{return dt_;}
void DynamicalDisk3D::PLindex(double t) {PLindex_=t;}
double DynamicalDisk3D::PLindex()const{return PLindex_;}
void DynamicalDisk3D::floorTemperature(double t) {floortemperature_=t;}
double DynamicalDisk3D::floorTemperature()const{return floortemperature_;}
void DynamicalDisk3D::temperature(bool t) {temperature_=t;}
bool DynamicalDisk3D::temperature() const {return temperature_;}
void DynamicalDisk3D::withVelocity(bool t) {novel_=!t;}
bool DynamicalDisk3D::withVelocity() const {return !novel_;}
|