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/**
* \file GyotoPlasmoid.h
* \brief Plasmoid sphere formed by magnetic reconnection following a Star orbit, emitting synchrotron,
* with two distributions of electrons:
* one thermal at "low" temperature and one kappa at "high" temperature
*
*/
/*
Copyright 2019 Frederic Vincent, Thibaut Paumard, Nicolas Aimar
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 __GyotoPlasmoid_H_
#define __GyotoPlasmoid_H_
namespace Gyoto{
namespace Astrobj { class Plasmoid; }
}
#include <iostream>
#include <fstream>
#include <iomanip>
#include <GyotoMetric.h>
#include <GyotoUniformSphere.h>
#include <GyotoFitsRW.h>
#include <GyotoKappaDistributionSynchrotronSpectrum.h>
//#include <GyotoThermalSynchrotronSpectrum.h>
#ifdef GYOTO_USE_CFITSIO
#include <fitsio.h>
#endif
#ifdef GYOTO_USE_XERCES
#include <GyotoRegister.h>
#endif
#include <string>
/**
* \class Gyoto::Astrobj::Plasmoid
* \brief Plasmoid Shere of plasma emitting synchrotron, following
* a trajectory specified in getVelocity (non-geodesic a priori)
*
*/
class Gyoto::Astrobj::Plasmoid :
public FitsRW,
public Gyoto::Astrobj::UniformSphere{
friend class Gyoto::SmartPointer<Gyoto::Astrobj::Plasmoid>;
// Data :
// -----
private:
double* posIni_; // 4-position of the plasmoid in spherical coordinates
double* fourveldt_; // 4-velocity of the plasmoid in spherical coordinates (dxi/dt, not dtau)
std::string flag_; // type of motion "helical" or "equatorial"
bool posSet_;
double t_inj_;
double radiusMax_; // Maximun radius of the Plasmoid in geometrical units
std::string varyRadius_;
// FITS FILE Quantities
std::string filename_;
double* freq_array_;
double* jnu_array_;
double* anu_array_;
// Constructors - Destructor
// -------------------------
public:
GYOTO_OBJECT; // This object has a (non-inherited) Property list
/**
* Create Plasmoid object with undefined initial conditions. One needs to
* set the coordinate system, the metric, the type of motion, and the initial position
* and velocity before integrating the orbit. initCoord()
* can be used for that.
*/
Plasmoid(); ///< Default constructor
Plasmoid(const Plasmoid& orig); ///< Copy constructor
virtual Plasmoid * clone() const ;
virtual ~Plasmoid() ; ///< Destructor
public:
virtual std::string className() const ; ///< "Plasmoid"
virtual std::string className_l() const ; ///< "inflate_star"
public:
void motionType(std::string const type);
SmartPointer<Metric::Generic> metric() const;
void metric(SmartPointer<Metric::Generic> gg);
void initPosition(std::vector<double> const &v);
std::vector<double> initPosition() const;
void initVelocity(std::vector<double> const &v);
std::vector<double> initVelocity() const;
void initCoord(std::vector<double> const &v);
std::vector<double> initCoord() const;
void radiusMax(double rr);
double radiusMax() const;
void Radius(std::string vary);
virtual void radiativeQ(double Inu[], double Taunu[],
double const nu_em[], size_t nbnu,
double dsem, state_t const &coord_ph,
double const coord_obj[8]=NULL) const;
void getCartesian(double const * const dates, size_t const n_dates,
double * const x, double * const y,
double * const z, double * const xprime=NULL,
double * const yprime=NULL,
double * const zprime=NULL);
void getVelocity(double const pos[4], double vel[4]);
int Impact(Gyoto::Photon* ph, size_t index,
Astrobj::Properties *data=NULL);
void file(std::string const &f);
std::vector<size_t> fitsRead(std::string filename);
};
#endif
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