/usr/include/Gyoto/GyotoDirectionalDisk.h is in libgyoto2-dev 0.2.3-1.
This file is owned by root:root, with mode 0o644.
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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 | /**
* \file GyotoDirectionalDisk.h
* \brief Geometrically thin disk read from FITS file
*
* This class describes a disk contained in the z=0 (equatorial)
* plane. The flux emitted
* at radius r, making an angle i with respect to the local normal,
* at frequency nu is given in a FITS file.
*
* The target of ray-traced Gyoto::Photon
*/
/*
Copyright 2014 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/>.
*/
#ifndef __GyotoDirectionalDisk_H_
#define __GyotoDirectionalDisk_H_
#include <iostream>
#include <fstream>
#include <iomanip>
namespace Gyoto{
namespace Astrobj { class DirectionalDisk; }
}
//#include <GyotoMetric.h>
#include <GyotoThinDisk.h>
/**
* \class Gyoto::Astrobj::DirectionalDisk
* \brief Geometrically thin disk read from FITS file
*
* This class describes a disk contained in the z=0 (equatorial)
* plane. The flux emitted
* at radius r, making an angle i with respect to the local normal,
* at frequency nu is given in a FITS file.
*
*/
class Gyoto::Astrobj::DirectionalDisk : public Astrobj::ThinDisk {
friend class Gyoto::SmartPointer<Gyoto::Astrobj::DirectionalDisk>;
private:
std::string filename_; ///< Optional FITS file name containing the arrays
/**
* An array of dimensionality double[nr_][ni_][nnu_]. In FITS
* format, the first dimension is nu, the second cosi (direction cosine),
* and the third r. There is no phi dependence.
*/
double * emission_; ///< I<SUB>ν</SUB>(ν, r, cosi;)
double * radius_; ///< Radius vector
double * cosi_; ///< Direction cosine vector
double * freq_; ///< Frequencies vector
size_t nnu_; ///< Number of frequencies provided in DirectionalDisk::emission_
size_t ni_; ///< Number of direction cosine
size_t nr_; ///< Number of radius values
// Constructors - Destructor
// -------------------------
public:
DirectionalDisk(); ///< Standard constructor
DirectionalDisk(const DirectionalDisk& ) ;///< Copy constructor
virtual DirectionalDisk* clone () const; ///< Cloner
virtual ~DirectionalDisk() ; ///< Destructor
// Accessors
// ---------
public:
#ifdef GYOTO_USE_CFITSIO
/// Read parameters and arrays from FITS file
virtual void fitsRead(std::string filename_);
/// Write parameters and arrays to FITS file
virtual void fitsWrite(std::string filename_);
#endif
/// Set DirectionalDisk::emission_
/**
* The pointer is copied directly, not the array content.
*
* This is a low-level function. Beware that:
* - previously allocated array will not be freed automatically;
* - array attached when the destructor is called will be freed.
*/
void setEmission(double * pattern);
void radius(double * pattern);
/**
* DirectionalDisk::emission_ is freed if not NULL, reallocated, and
* pattern is copied into emission_.
*
* Finally, DirectionalDisk::nnu_, DirectionalDisk::ni_, and
* DirectionalDisk::nr_ are set according to naxes.
*
* \param pattern Array to copy as emission_. May be NULL in which
* case emission_ is simply deallocated and set to NULL.
*
* \param naxes { nnu_, ni_, nr_ }.
*/
virtual void copyIntensity(double const * const pattern = NULL,
size_t const naxes[3] = NULL);
virtual double const * getIntensity() const;///< Get DirectionalDisk::emission_
virtual void getIntensityNaxes( size_t naxes[3] ) const ; ///< Get DirectionalDisk::nnu_, DirectionalDisk::ni_, and DirectionalDisk::nr_
virtual void copyGridRadius(double const * const pattern = NULL,
size_t nr = 0 );
virtual double const * getGridRadius() const; ///< Get DirectionalDisk::radius_
virtual void copyGridCosi(double const * const pattern = NULL,
size_t ni = 0 );
virtual double const * getGridCosi() const; ///< Get DirectionalDisk::cosi_
virtual void copyGridFreq(double const * const pattern = NULL,
size_t ni = 0 );
virtual double const * getGridFreq() const; ///< Get DirectionalDisk::freq_
virtual int setParameter(std::string name,
std::string content,
std::string unit);
protected:
void getIndices(size_t i[3], double const co[4], double cosi, double nu=0.) const ;
///< Get emission_ cell corresponding to position co[4]
public:
using ThinDisk::emission;
virtual double emission(double nu_em, double dsem,
double c_ph[8], double c_obj[8]) const;
public:
#ifdef GYOTO_USE_XERCES
virtual void fillElement(FactoryMessenger *fmp) const ;
virtual void setParameters(FactoryMessenger *fmp);
#endif
};
#endif
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