Array GreyBodyDustEmissivity::emissivity(const DustMix* mix, const Array& Jv) const
{
// get basic information about the wavelength grid
WavelengthGrid* lambdagrid = find<WavelengthGrid>();
int Nlambda = lambdagrid->Nlambda();
// get basic information about the dust mix
int Npop = mix->Npop();
// accumulate the emissivities at the equilibrium temperature for all populations in the dust mix
Array ev(Nlambda);
for (int c=0; c<Npop; c++)
{
double T = mix->equilibrium(Jv,c);
PlanckFunction B(T);
for (int ell=0; ell<Nlambda; ell++)
{
ev[ell] += mix->sigmaabs(ell,c) * B(lambdagrid->lambda(ell));
}
}
// convert emissivity from "per hydrogen atom" to "per unit mass"
ev /= mix->mu();
return ev;
}
void InstrumentFrame::calibrateAndWriteDataFrames(int ell, QList<Array*> farrays, QStringList fnames)
{
PeerToPeerCommunicator* comm = find<PeerToPeerCommunicator>();
if (!comm->isRoot()) return;
Units* units = find<Units>();
WavelengthGrid* lambdagrid = find<WavelengthGrid>();
// conversion from bolometric luminosities (units W) to monochromatic luminosities (units W/m)
// --> divide by delta-lambda
double dlambda = lambdagrid->dlambda(ell);
// correction for the area of the pixels of the images; the units are now W/m/sr
// --> divide by area
double xpresang = 2.0*atan(_xpres/(2.0*_distance));
double ypresang = 2.0*atan(_ypres/(2.0*_distance));
double area = xpresang*ypresang;
// calibration step 3: conversion of the flux per pixel from monochromatic luminosity units (W/m/sr)
// to flux density units (W/m3/sr) by taking into account the distance
// --> divide by fourpid2
double fourpid2 = 4.0*M_PI*_distance*_distance;
// conversion from program SI units (at this moment W/m3/sr) to the correct output units
// --> multiply by unit conversion factor
double unitfactor = units->osurfacebrightness(lambdagrid->lambda(ell), 1.);
// perform the conversion, in place
foreach (Array* farr, farrays)
{
(*farr) *= (unitfactor / (dlambda * area * fourpid2));
}
// write a FITS file for each array
for (int q = 0; q < farrays.size(); q++)
{
QString filename = find<FilePaths>()->output(_instrument->instrumentName()
+ "_" + fnames[q] + "_" + QString::number(ell) + ".fits");
find<Log>()->info("Writing " + fnames[q] + " flux " + QString::number(ell)
+ " to FITS file " + filename + "...");
FITSInOut::write(filename, *(farrays[q]), _Nxp, _Nyp, 1,
units->olength(_xpres), units->olength(_ypres),
units->usurfacebrightness(), units->ulength());
}
}
void SED::write(const QString& filename) const
{
WavelengthGrid* lambdagrid = find<WavelengthGrid>();
Units* units = find<Units>();
ofstream file(filename.toLocal8Bit().constData());
file << setprecision(8) << scientific;
for (int ell=0; ell<lambdagrid->Nlambda(); ell++)
{
double lambda = lambdagrid->lambda(ell);
double dlambda = lambdagrid->dlambda(ell);
file << units->owavelength(lambda)
<< '\t'
<< _Lv[ell]/dlambda*lambda
<< endl;
}
file.close();
}
void InstrumentFrame::calibrateAndWriteDataFrames(int ell, QList<Array*> farrays, QStringList fnames)
{
Units* units = find<Units>();
WavelengthGrid* lambdagrid = find<WavelengthGrid>();
// conversion from bolometric luminosities (units W) to monochromatic luminosities (units W/m)
// --> divide by delta-lambda
double dlambda = lambdagrid->dlambda(ell);
// correction for the area of the pixels of the images; the units are now W/m/sr
// --> divide by area
double xpresang = 2.0*atan(_xpres/(2.0*_distance));
double ypresang = 2.0*atan(_ypres/(2.0*_distance));
double area = xpresang*ypresang;
// calibration step 3: conversion of the flux per pixel from monochromatic luminosity units (W/m/sr)
// to flux density units (W/m3/sr) by taking into account the distance
// --> divide by fourpid2
double fourpid2 = 4.0*M_PI*_distance*_distance;
// conversion from program SI units (at this moment W/m3/sr) to the correct output units
// --> multiply by unit conversion factor
double unitfactor = units->osurfacebrightness(lambdagrid->lambda(ell), 1.);
// Perform the conversion, in place
foreach (Array* farr, farrays)
{
(*farr) *= (unitfactor / (dlambda * area * fourpid2));
}
// Write a FITS file for each array
for (int q = 0; q < farrays.size(); q++)
{
QString filename = _instrument->instrumentName() + "_" + fnames[q] + "_" + QString::number(ell);
QString description = fnames[q] + " flux " + QString::number(ell);
// Create the image and save it
Image image(this, _Nxp, _Nyp, 1, _xpres, _ypres, "surfacebrightness");
image.saveto(this, *(farrays[q]), filename, description);
}
}
void PerspectiveInstrument::write()
{
Units* units = find<Units>();
WavelengthGrid* lambdagrid = find<WavelengthGrid>();
int Nlambda = find<WavelengthGrid>()->Nlambda();
// Put the data cube in a list of f-array pointers, as the sumResults function requires
QList< Array* > farrays;
farrays << &_ftotv;
// Sum the flux arrays element-wise across the different processes
sumResults(farrays);
// Multiply each sample by lambda/dlamdba and by the constant factor 1/(4 pi s^2)
// to obtain the surface brightness and convert to output units (such as W/m2/arcsec2)
double front = 1. / (4.*M_PI*_s*_s);
for (int ell=0; ell<Nlambda; ell++)
{
double lambda = lambdagrid->lambda(ell);
double dlambda = lambdagrid->dlambda(ell);
for (int i=0; i<_Nx; i++)
{
for (int j=0; j<_Ny; j++)
{
int m = i + _Nx*j + _Nx*_Ny*ell;
_ftotv[m] = units->osurfacebrightness(lambda, _ftotv[m]*front/dlambda);
}
}
}
// Write a FITS file containing the data cube
QString filename = _instrumentname + "_total";
Image image(this, _Nx, _Ny, Nlambda, _s, _s, "surfacebrightness");
image.saveto(this, _ftotv, filename, "total flux");
}
void QuasarSED::setupSelfBefore()
{
StellarSED::setupSelfBefore();
WavelengthGrid* lambdagrid = find<WavelengthGrid>();
double Nlambda = lambdagrid->Nlambda();
Array jv(Nlambda);
for (int ell=0; ell<Nlambda; ell++)
{
double lambda = lambdagrid->lambda(ell);
lambda *= 1e6; // conversion from m to micron (the Quasar SED is defined using microns)
double j = 0.0;
double a = 1.0;
double b = 0.003981072;
double c = 0.001258926;
double d = 0.070376103;
if (lambda<0.001)
j = 0.0;
else if (lambda<0.01)
j = a*pow(lambda,0.2);
else if (lambda<0.1)
j = b*pow(lambda,-1.0);
else if (lambda<5.0)
j = c*pow(lambda,-1.5);
else if (lambda<1000.0)
j = d*pow(lambda,-4.0);
else
j = 0.0;
jv[ell] = j;
}
setemissivities(jv);
}
void SPHStarburstComp::setupSelfBefore()
{
StellarComp::setupSelfBefore();
// cache the random generator
_random = find<Random>();
// local constant for units
const double pc = Units::pc();
// vectors storing the particle attributes (r and h are data members since we need those after setup)
std::vector<double> SFRv;
std::vector<double> Zv;
std::vector<double> logCv;
std::vector<double> Pv;
std::vector<double> fPDRv;
// load the SPH star particles
QString filepath = find<FilePaths>()->input(_filename);
QFile infile(filepath);
if (!infile.open(QIODevice::ReadOnly|QIODevice::Text))
throw FATALERROR("Could not open the SPH HII region data file " + filepath);
find<Log>()->info("Reading SPH HII region particles from file " + filepath + "...");
int Nparts = 0;
double SFRtot = 0;
while (!infile.atEnd())
{
// read a line, split it in columns, and skip empty and comment lines
QList<QByteArray> columns = infile.readLine().simplified().split(' ');
if (!columns.isEmpty() && !columns[0].startsWith('#'))
{
// get the column values; missing or illegal values default to zero
_rv.push_back(Vec(columns.value(0).toDouble()*pc,
columns.value(1).toDouble()*pc,
columns.value(2).toDouble()*pc));
_hv.push_back(columns.value(3).toDouble()*pc);
SFRv.push_back(columns.value(4).toDouble()); // star formation rate in Msun / yr
Zv.push_back(columns.value(5).toDouble()); // metallicity as dimensionless fraction
logCv.push_back(columns.value(6).toDouble()); // log compactness (Groves 2008) as dimensionless value
Pv.push_back(columns.value(7).toDouble()); // ISM pressure in Pa
fPDRv.push_back(columns.value(8).toDouble()); // dimensionless photo-dissociation region covering fraction
Nparts++;
SFRtot += columns.value(4).toDouble();
}
}
infile.close();
double Mtot = SFRtot * 1.e7; // total stellar mass from total sfr over the last 10 Myr
find<Log>()->info(" Total number of SPH HII region particles: " + QString::number(Nparts));
find<Log>()->info(" Total stellar mass: " + QString::number(Mtot) + " Msun");
find<Log>()->info("Filling the vectors with the SEDs of the particles... ");
// construct the library of SED models
MappingsSEDFamily map(this);
// construct a temporary matrix Lvv with the luminosity of each particle at each wavelength
// and also the permanent vector _Ltotv with the total luminosity for every wavelength bin
int Nlambda = find<WavelengthGrid>()->Nlambda();
ArrayTable<2> Lvv(Nlambda,Nparts);
_Ltotv.resize(Nlambda);
double Ltot = 0;
for (int i=0; i<Nparts; i++)
{
const Array& Lv = map.luminosities(SFRv[i], Zv[i], logCv[i], Pv[i], fPDRv[i]);
for (int ell=0; ell<Nlambda; ell++)
{
Lvv[ell][i] = Lv[ell];
_Ltotv[ell] += Lv[ell];
Ltot += Lv[ell];
}
}
find<Log>()->info(" HII luminosity: " + QString::number(Ltot/Units::Lsun()) + " Lsun");
// construct the permanent vectors _Xvv with the normalized cumulative luminosities (per wavelength bin)
_Xvv.resize(Nlambda,0);
for (int ell=0; ell<Nlambda; ell++)
{
NR::cdf(_Xvv[ell], Lvv[ell]);
}
// if requested, write a data file with the luminosities per wavelength
if (_writeLuminosities)
{
Units* units = find<Units>();
WavelengthGrid* lambdagrid = find<WavelengthGrid>();
// Create a text file
TextOutFile file(this, "HII_luminosities", "HII luminosities");
// Write the header
file.addColumn("lambda (" + units->uwavelength() + ")");
file.addColumn("luminosity (" + units->ubolluminosity() + ")");
// Write the body
for (int ell=0; ell<Nlambda; ell++)
{
file.writeRow(QList<double>() << units->owavelength(lambdagrid->lambda(ell))
<< units->obolluminosity(_Ltotv[ell]));
}
}
}
void PanDustSystem::write() const
{
DustSystem::write();
// If requested, output the interstellar radiation field in every dust cell to a data file
if (_writeISRF)
{
WavelengthGrid* lambdagrid = find<WavelengthGrid>();
Units* units = find<Units>();
// Create a text file
TextOutFile file(this, "ds_isrf", "ISRF");
// Write the header
file.writeLine("# Mean field intensities for all dust cells with nonzero absorption");
file.addColumn("dust cell index", 'd');
file.addColumn("x coordinate of cell center (" + units->ulength() + ")", 'g');
file.addColumn("y coordinate of cell center (" + units->ulength() + ")", 'g');
file.addColumn("z coordinate of cell center (" + units->ulength() + ")", 'g');
for (int ell=0; ell<_Nlambda; ell++)
file.addColumn("J_lambda (W/m3/sr) for lambda = "
+ QString::number(units->owavelength(lambdagrid->lambda(ell)))
+ " " + units->uwavelength(), 'g');
// Write one line for each dust cell with nonzero absorption
for (int m=0; m<_Ncells; m++)
{
double Ltotm = Labs(m);
if (Ltotm>0.0)
{
QList<double> values;
Position bfr = _grid->centralPositionInCell(m);
values << m << units->olength(bfr.x()) << units->olength(bfr.y()) << units->olength(bfr.z());
for (auto J : meanintensityv(m)) values << J;
file.writeRow(values);
}
}
}
// If requested, output temperate map(s) along coordiate axes cuts
if (_writeTemp)
{
// construct a private class instance to do the work (parallelized)
WriteTemp wt(this);
Parallel* parallel = find<ParallelFactory>()->parallel();
// get the dimension of the dust grid
int dimDust = _grid->dimension();
// Create an assigner that assigns all the work to the root process
RootAssigner* assigner = new RootAssigner(0);
assigner->assign(Np);
// For the xy plane (always)
{
wt.setup(1,1,0);
parallel->call(&wt, assigner);
wt.write();
}
// For the xz plane (only if dimension is at least 2)
if (dimDust >= 2)
{
wt.setup(1,0,1);
parallel->call(&wt, assigner);
wt.write();
}
// For the yz plane (only if dimension is 3)
if (dimDust == 3)
{
wt.setup(0,1,1);
parallel->call(&wt, assigner);
wt.write();
}
}
}
void PanDustSystem::write() const
{
DustSystem::write();
PeerToPeerCommunicator* comm = find<PeerToPeerCommunicator>();
bool dataParallel = comm->dataParallel();
// If requested, output the interstellar radiation field in every dust cell to a data file
if (_writeISRF)
{
WavelengthGrid* lambdagrid = find<WavelengthGrid>();
Units* units = find<Units>();
// Create a text file
TextOutFile file(this, "ds_isrf", "ISRF");
// Write the header
file.writeLine("# Mean field intensities for all dust cells with nonzero absorption");
file.addColumn("dust cell index", 'd');
file.addColumn("x coordinate of cell center (" + units->ulength() + ")", 'g');
file.addColumn("y coordinate of cell center (" + units->ulength() + ")", 'g');
file.addColumn("z coordinate of cell center (" + units->ulength() + ")", 'g');
for (int ell=0; ell<_Nlambda; ell++)
file.addColumn("J_lambda (W/m3/sr) for lambda = "
+ QString::number(units->owavelength(lambdagrid->lambda(ell)))
+ " " + units->uwavelength(), 'g');
// Write one line for each dust cell with nonzero absorption
for (int m=0; m<_Ncells; m++)
{
if (!dataParallel)
{
double Ltotm = Labs(m);
if (Ltotm>0.0)
{
QList<double> values;
Position bfr = _grid->centralPositionInCell(m);
values << m << units->olength(bfr.x()) << units->olength(bfr.y()) << units->olength(bfr.z());
for (auto J : meanintensityv(m)) values << J;
file.writeRow(values);
}
}
else // for distributed mode
{
QList<double> values;
Position bfr = _grid->centralPositionInCell(m);
values << m << units->olength(bfr.x()) << units->olength(bfr.y()) << units->olength(bfr.z());
// the correct process gets Jv
Array Jv(_Nlambda);
if (_assigner->validIndex(m)) Jv = meanintensityv(m);
// and broadcasts it
int sender = _assigner->rankForIndex(m);
comm->broadcast(Jv,sender);
if (Jv.sum()>0)
{
for (auto J : Jv) values << J;
file.writeRow(values);
}
}
}
}
// If requested, output temperature map(s) along coordinate axes and temperature data for each dust cell
if (_writeTemp)
{
// Parallelize the calculation over the threads
Parallel* parallel = find<ParallelFactory>()->parallel();
// If the necessary data is distributed over the processes, do the calculation on all processes.
// Else, let the root do everything.
bool isRoot = comm->isRoot();
// Output temperature map(s) along coordinate axes
{
// Construct a private class instance to do the work (parallelized)
WriteTempCut wt(this);
// Get the dimension of the dust grid
int dimDust = _grid->dimension();
// For the xy plane (always)
{
wt.setup(1,1,0);
if (dataParallel) parallel->call(&wt, Np);
else if (isRoot) parallel->call(&wt, Np);
wt.write();
}
// For the xz plane (only if dimension is at least 2)
if (dimDust >= 2)
{
wt.setup(1,0,1);
if (dataParallel) parallel->call(&wt, Np);
else if (isRoot) parallel->call(&wt, Np);
wt.write();
}
// For the yz plane (only if dimension is 3)
if (dimDust == 3)
{
wt.setup(0,1,1);
if (dataParallel) parallel->call(&wt, Np);
else if (isRoot) parallel->call(&wt, Np);
wt.write();
}
}
// Output a text file with temperature data for each dust cell
{
find<Log>()->info("Calculating indicative dust temperatures for each cell...");
// Construct a private class instance to do the work (parallelized)
WriteTempData wt(this);
// Call the body on the right cells. If everything is available, no unnecessary communication will be done.
if (dataParallel)
{
// Calculate the temperature for the cells owned by this process
parallel->call(&wt, _assigner);
}
else if (isRoot)
{
// Let root calculate it for everything
parallel->call(&wt, _Ncells);
}
wt.write();
}
}
}
void SingleFrameInstrument::calibrateAndWriteDataCubes(QList< Array*> farrays, QStringList fnames)
{
WavelengthGrid* lambdagrid = find<WavelengthGrid>();
int Nlambda = lambdagrid->Nlambda();
// calibration step 1: conversion from bolometric luminosities (units W) to monochromatic luminosities (units W/m)
for (int ell=0; ell<Nlambda; ell++)
{
double dlambda = lambdagrid->dlambda(ell);
for (int i=0; i<_Nxp; i++)
{
for (int j=0; j<_Nyp; j++)
{
int m = i + _Nxp*j + _Nxp*_Nyp*ell;
foreach (Array* farr, farrays)
{
(*farr)[m] /= dlambda;
}
}
}
}
// calibration step 2: correction for the area of the pixels of the images; the units are now W/m/sr
double xpresang = 2.0*atan(_xpres/(2.0*_distance));
double ypresang = 2.0*atan(_ypres/(2.0*_distance));
double area = xpresang*ypresang;
foreach (Array* farr, farrays)
{
(*farr) /= area;
}
// calibration step 3: conversion of the flux per pixel from monochromatic luminosity units (W/m/sr)
// to flux density units (W/m3/sr) by taking into account the distance
double fourpid2 = 4.0*M_PI*_distance*_distance;
foreach (Array* farr, farrays)
{
(*farr) /= fourpid2;
}
// conversion from program SI units (at this moment W/m3/sr) to the correct output units;
// we use lambda*flambda for the surface brightness (in units like W/m2/arcsec2)
Units* units = find<Units>();
for (int ell=0; ell<Nlambda; ell++)
{
double lambda = lambdagrid->lambda(ell);
for (int i=0; i<_Nxp; i++)
{
for (int j=0; j<_Nyp; j++)
{
int m = i + _Nxp*j + _Nxp*_Nyp*ell;
foreach (Array* farr, farrays)
{
(*farr)[m] = units->obolsurfacebrightness(lambda*(*farr)[m]);
}
}
}
}