A toroidal accretion structure. More...

#include <GyotoPolishDoughnut.h>

Inheritance diagram for Gyoto::Astrobj::PolishDoughnut:

Classes
class	intersection_t
	double intersection(double) Functor class More...

class	outerradius_t
	double outerradius(double) Functor class More...

Public Types
typedef Gyoto::SmartPointer< Gyoto::SmartPointee >	Subcontractor_t(Gyoto::FactoryMessenger *, std::vector< std::string > const &)
	A subcontractor builds an object upon order from the Factory.

Public Member Functions
virtual Property const *	getProperties () const
	Get list of properties.

void	fillProperty (Gyoto::FactoryMessenger *fmp, Property const &p) const
	Output a single Property to XML.

	PolishDoughnut ()
	Default constructor.

	PolishDoughnut (const PolishDoughnut &)
	Copy constructor.

virtual PolishDoughnut *	clone () const
	Cloner.

virtual	~PolishDoughnut ()
	Destructor.

double	getL0 () const
	Get PolishDoughnut::l0_.

double	lambda () const
	Get PolishDoughnut::lambda_.

void	lambda (double lambda)
	Set PolishDoughnut::lambda_.

double	centralEnthalpyPerUnitVolume () const
	Get PolishDoughnut::central_enthalpy_cgs_.

double	centralEnthalpyPerUnitVolume (std::string const &unit) const
	Get PolishDoughnut::central_enthalpy_cgs_ in specified unit.

void	centralEnthalpyPerUnitVolume (double density)
	Set PolishDoughnut::central_enthalpy_cgs_.

void	centralEnthalpyPerUnitVolume (double density, std::string const &unit)
	Set PolishDoughnut::central_enthalpy_cgs_ in specified unit.

double	centralTemp () const
	Get PolishDoughnut::central_temperature_.

void	centralTemp (double val)
	Set PolishDoughnut::central_temperature_.

double	beta () const
	Get PolishDoughnut::beta_.

void	beta (double beta)
	Set PolishDoughnut::beta_.

void	magnetizationParameter (double rr)

double	magnetizationParameter () const

void	spectralOversampling (size_t)
	Set PolishDoughnut::spectral_oversampling_.

size_t	spectralOversampling () const
	Get PolishDoughnut::spectral_oversampling_.

bool	changeCusp () const
	Get PolishDoughnut::komissarov_.

void	changeCusp (bool t)
	Set PolishDoughnut::komissarov_.

bool	bremsstrahlung () const
	Get PolishDoughnut::bremsstrahlung_.

void	bremsstrahlung (bool brems)
	Set PolishDoughnut::bremsstrahlung_.

bool	angleAveraged () const
	Get PolishDoughnut::angle_averaged_.

void	angleAveraged (bool komis)
	Set PolishDoughnut::angle_averaged_.

void	nonThermalDeltaExpo (std::vector< double > const &v)

std::vector< double >	nonThermalDeltaExpo () const

void	angmomrinner (std::vector< double > const &v)

std::vector< double >	angmomrinner () const

void	adafparams (std::vector< double > const &v)

std::vector< double >	adafparams () const

void	adaf (bool t)

bool	adaf () const

void	setParameter (Gyoto::Property const &p, std::string const &name, std::string const &content, std::string const &unit)
	Set parameter by Property (and name)

double	getWsurface () const
	Get PolishDoughnut::W_surface_.

double	getWcentre () const
	Get PolishDoughnut::W_centre_.

double	getRcusp () const
	Get PolishDoughnut::r_cusp_.

double	getRcentre () const
	Get PolishDoughnut::r_centre_.

virtual void	metric (Gyoto::SmartPointer< Gyoto::Metric::Generic >)
	Set the Metric gg_.

int	Impact (Photon ph, size_t index, Astrobj::Properties data)
	Does a photon at these coordinates impact the object?

virtual double	operator() (double const coord[4])
	Function defining the object interior.

virtual void	safetyValue (double val)
	Set Standard::safety_value_.

virtual double	safetyValue () const
	Get Standard::safety_value_.

double	deltaInObj () const
	Get Generic::delta_inobj_.

void	deltaInObj (double val)
	Set Generic::delta_inobj_.

virtual double	operator() (double const data[])=0
	The actual function.

virtual double	giveDelta (double coord[8])
	Maximum δ inside object.

virtual SmartPointer< Metric::Generic >	metric () const
	Get the Metric gg_.

virtual double	rMax ()
	Get maximal distance from center of coordinate system.

virtual double	rMax () const
	Get maximal distance from center of coordinate system.

virtual double	rMax (std::string const &unit)
	Get rmax_ is specified unit.

virtual double	rMax (std::string const &unit) const
	Get rmax_ is specified unit.

virtual void	rMax (double val)
	Set maximal distance from center of coordinate system.

virtual void	rMax (double val, std::string const &unit)
	Set maximal distance from center of coordinate system.

virtual double	deltaMax (double coord[8])
	Get max step constraint for adaptive integration.

	GYOTO_OBJECT_ACCESSORS_UNIT (deltaMaxInsideRMax)

void	opticallyThin (bool flag)
	Set whether the object is optically thin.

bool	opticallyThin () const
	Query whether object is optically thin.

void	showshadow (bool flag)

bool	showshadow () const

void	redshift (bool flag)

bool	redshift () const

virtual Gyoto::Quantity_t	getDefaultQuantities ()
	Which quantities to compute if know was requested.

virtual void	setParameters (FactoryMessenger *fmp)
	Main loop in Subcontractor_t function.

virtual void	processHitQuantities (Photon ph, state_t const &coord_ph_hit, double const coord_obj_hit, double dt, Astrobj::Properties *data) const
	Fills Astrobj::Properties.

virtual void	processHitQuantities (Photon ph, double coord_ph_hit, double coord_obj_hit, double dt, Astrobj::Properties data) const =delete

virtual double	emission (double nu_em, double dsem, state_t const &coord_ph, double const coord_obj[8]=NULL) const
	Specific intensity I_ν

virtual double	emission (double nu_em, double dsem, double coord_ph[8], double coord_obj[8]=NULL) const =delete
	Obsolete, update your code;.

virtual void	emission (double Inu[], double const nu_em[], size_t nbnu, double dsem, state_t const &coord_ph, double const coord_obj[8]=NULL) const
	Specific intensity I_ν for several values of ν_em

virtual void	emission (double Inu[], double nu_em[], size_t nbnu, double dsem, double coord_ph[8], double coord_obj[8]=NULL) const =delete
	Obsolete, update your code.

virtual void	radiativeQ (double Inu[], double Taunu[], double nu_em[], size_t nbnu, double dsem, double coord_ph[8], double coord_obj[8]=NULL) const =delete

virtual void	radiativeQ (double Inu, double Qnu, double Unu, double Vnu, Eigen::Matrix4d Onu, double const nuem, size_t nbnu, double dsem, state_t const &cph, double const *co) const
	Compute the increment of Stokes parameters and transmission matrix. Polarised version of RadiaveQ.

virtual double	integrateEmission (double nu1, double nu2, double dsem, state_t const &c_ph, double const c_obj[8]=NULL) const
	∫_ν₁^ν₂ I_ν dν (or j_ν)

virtual double	integrateEmission (double nu1, double nu2, double dsem, double c_ph[8], double c_obj[8]=NULL) const =delete
	Obsolete, update your code.

virtual void	integrateEmission (double I, double const boundaries, size_t const chaninds, size_t nbnu, double dsem, double cph, double *co) const =delete
	Obsolete, update your code.

virtual double	transmission (double nuem, double dsem, state_t const &coord_ph, double const coord_obj[8]) const
	Transmission: exp( α_ν * ds_em )

virtual double	transmission (double nuem, double dsem, state_t const &coord) const =delete
	Obsolete, update your code.

virtual double	transmission (double nuem, double dsem, double coord[8]) const =delete
	Obsolete, update your code.

Eigen::Matrix4d	Omatrix (double alphanu[4], double rnu[3], double Chi, double dsem) const

Eigen::Matrix4d	Omatrix (double alphaInu, double alphaQnu, double alphaUnu, double alphaVnu, double rQnu, double rUnu, double rVnu, double Chi, double dsem) const

Eigen::Matrix4d	Omatrix (double alphanu[4], double rnu[3], double sin2Chi, double cos2Chi, double dsem) const

Eigen::Matrix4d	Omatrix (double alphaInu, double alphaQnu, double alphaUnu, double alphaVnu, double rQnu, double rUnu, double rVnu, double sin2Chi, double cos2Chi, double dsem) const

Eigen::Matrix4d	Pmatrix (double alphaInu, double alphaQnu, double alphaUnu, double alphaVnu, double rQnu, double rUnu, double rVnu, double sin2Chi, double cos2Chi, double dsem) const

Eigen::Vector4d	rotateJs (double jInu, double jQnu, double jUnu, double jVnu, double sin2Chi, double cos2Chi) const

Eigen::Vector4d	rotateJs (double jInu, double jQnu, double jUnu, double jVnu, double Chi) const

double	getChi (double const fourvect[4], state_t const &cph, double const vel[4], bool elec=false) const

void	getSinCos2Chi (double const fourvect[4], state_t const &cph, double const vel[4], double sin2Chi, double cos2Chi, bool elec=false) const

void	computeB4vect (double B4vect[4], std::string const magneticConfig, double const co[8], state_t const &cph) const

void	computeB4vect_ipole (double B4vect[4], std::string const magneticConfig, double const co[8], state_t const &cph, double spin) const

double	interpolate (int const N, double const array, double const Xq, double *const X, int const X_params, std::string const *cond_limits) const

double	interpolate (int const N, double const array, double const Xq, double *const X_params, std::string const cond_limits) const

void	incRefCount ()
	Increment the reference counter. Warning: Don't mess with the counter.

int	decRefCount ()
	Decrement the reference counter and return current value. Warning: Don't mess with the counter.

int	getRefCount ()
	Get the current number of references.

virtual bool	isThreadSafe () const
	Whether this class is thread-safe.

virtual void	set (Property const &p, Value val)
	Set Value of a Property.

virtual void	set (Property const &p, Value val, std::string const &unit)
	Set Value (expressed in unit) of a Property.

virtual void	set (std::string const &pname, Value val)
	Set Value of a Property.

virtual void	set (std::string const &pname, Value val, std::string const &unit)
	Set Value (expressed in unit) of a Property.

virtual Value	get (Property const &p) const
	Get Value of a Property.

virtual Value	get (std::string const &pname) const
	Get Value of a Property.

virtual Value	get (Property const &p, std::string const &unit) const
	Get Value of a Property, converted to unit.

virtual Value	get (std::string const &pname, std::string const &unit) const
	Get Value of a Property, converted to unit.

Property const *	property (std::string const pname) const
	Find property by name.

virtual void	fillElement (Gyoto::FactoryMessenger *fmp) const
	Fill the XML element for this Object.

virtual int	setParameter (std::string name, std::string content, std::string unit)
	Set parameter by name.

std::string	describeProperty (Gyoto::Property const &p) const
	Format desrciption for a property.

void	help () const
	Print (to stdout) some help on this class.

virtual std::string	kind () const
	Get kind_.

Public Attributes
	GYOTO_OBJECT_THREAD_SAFETY

Static Public Attributes
static GYOTO_OBJECT Property const	properties []

Protected Member Functions
virtual void	tell (Gyoto::Hook::Teller *msg)
	Update PolishDoughnut::aa_.

virtual void	getVelocity (double const pos[4], double vel[4])
	Fluid velocity field.

virtual void	integrateEmission (double I, double const boundaries, size_t const chaninds, size_t nbnu, double dsem, state_t const &cph, double const co) const
	∫_ν₁^ν₂ I_ν dν (or j_ν)

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
	emission and transmission together

virtual void	kind (const std::string)
	Set kind_.

Protected Attributes
SmartPointer< Spectrum::ThermalBremsstrahlung >	spectrumBrems_

SmartPointer< Spectrum::ThermalSynchrotron >	spectrumSynch_

SmartPointer< Spectrum::PowerLawSynchrotron >	spectrumPLSynch_

double	l0_
	Angular momentum. Tied to PolishDoughnut::lambda_.

double	lambda_
	Adimentionned angular momentum.

double	W_surface_
	Potential surface value. Tied to PolishDoughnut::lambda_.

double	W_centre_
	Potential central value. Tied to PolishDoughnut::lambda_.

double	r_cusp_
	Cusp radius in geometrical units. Tied to PolishDoughnut::lambda_.

double	r_centre_
	Central radius in geometrical units. Tied to PolishDoughnut::lambda_.

double	r_torusouter_
	Torus outer coordinate radius. Tied to PolishDoughnut::lambda_.

double	DeltaWm1_
	1./(W_centre_ - W_surface_);

double	central_enthalpy_cgs_
	Central enthalpy per unit volume in erg/cm3.

double	central_temperature_
	T_center in K.

double	beta_
	P_gas/P_magn (careful not standard)

double	magnetizationParameter_
	P_magn/(n_e m_p c²) (careful, very different from above)

double	aa_
	PolishDoughnut::gg_ spin, cached when setting PolishDoughnut::lambda_.

double	aa2_
	aa_²

size_t	spectral_oversampling_
	Oversampling used in integrateEmission()

bool	angle_averaged_
	1 if Komissarov model should be angle averaged

bool	bremsstrahlung_
	1 if Komissarov model should compute Brems radiation

double	deltaPL_
	fraction of thermal energy in non-thermal electrons

bool	adaf_
	true to switch to an ADAF model rather tha Polish doughnut

double	ADAFtemperature_
	ADAF central temperature.

double	ADAFdensity_
	ADAF central density.

bool	changecusp_
	true to apply the fishy rcusp_ change (to be changed)

bool	rochelobefilling_
	true if torus filling its Roche lobe

bool	defangmomrinner_
	true if torus defined from l0 and rin

double	rintorus_
	Inner radius of the doughnut.

double	critical_value_
	See operator()(double const coord[4])

double	safety_value_
	See operator()(double const coord[4])

double	delta_inobj_
	Constant value of the integration step inside object, in units of the compact object's mass M.

SmartPointer< Gyoto::Metric::Generic >	gg_
	The Metric in this end of the Universe.

double	rmax_
	Maximum distance to the center of the coordinate system [geometrical units].

double	deltamaxinsidermax_
	Maximum Photon integration step inside rmax_ [geometrical units].

bool	flag_radtransf_
	1 if radiative transfer inside Astrobj, else 0

int	shadow_
	1 to highlight the shadow region in the image

int	noredshift_
	1 to impose redshift factor g = 1

std::string	kind_
	The "kind" that is output in the XML entity.

std::vector< std::string >	plugins_
	The plug-ins that needs to be loaded to access this instance's class.

Private Member Functions
double	potential (double r, double theta) const
	Potential defining shape, used by operator()()

double	interp1d (double const x, double const y0, double const y1) const

double	interpNd (int const N, double const Xq, double const X, double const Y, std::string const *cond_limit) const

int	getIndice (double &xq, std::string const cond_limit, double const X_params[3], double *const X=NULL) const

Private Attributes
intersection_t	intersection
	double intersection(double) Functor

int	__defaultfeatures
	Whether some virtual methods are implemented.

int	refCount
	Reference counter.

pthread_mutex_t	mutex_
	A mutex.

Friends
class	Gyoto::SmartPointer< Gyoto::Astrobj::PolishDoughnut >

class	intersection_t

Detailed Description

A toroidal accretion structure.

Latest reference: Vincent, F. H.; Yan, W.; Straub, O.; Zdziarski, A. A.; Abramowicz, M. A. 2015, A magnetized torus for modeling Sagittarius A* millimeter images and spectra, A&A 574:A48.

Reference: Straub, O.; Vincent, F. H.; Abramowicz, M. A.; Gourgoulhon, E.; & Paumard, T. 2012, Modelling the black hole silhouette in Sagittarius A* with ion tori, A&A 543:83.

Member Typedef Documentation

◆ Subcontractor_t

typedef Gyoto::SmartPointer< Gyoto::SmartPointee > Gyoto::SmartPointee::Subcontractor_t(Gyoto::FactoryMessenger *, std::vector< std::string > const &)

inherited

A subcontractor builds an object upon order from the Factory.

Various classes need to provide a subcontractor to be able to instantiate themselves upon order from the Factory. A subcontractor is a function (often a static member function) which accepts a pointer to a FactoryMessenger as unique parameter, communicates with the Factory using this messenger to read an XML description of the object to build, and returns this objet. SmartPointee::Subcontractor_t* is just generic enough a typedef to cast to and from other subcontractor types: Astrobj::Subcontractor_t, Metric::Subcontractor_t, Spectrum::Subcontractor_t. A subcontractor needs to be registered using the relevant Register() function: Astrobj::Register(), Metric::Register(), Spectrum::Register().

Member Function Documentation

◆ clone()

virtual PolishDoughnut * Gyoto::Astrobj::PolishDoughnut::clone ( ) const

virtual

Cloner.

This method must be implemented by the various Astrobj::Generic subclasses in order to support cloning:

SmartPointer<Astrobj> deep_copy = original->clone();

Gyoto::SmartPointer

Pointers performing reference counting.

Definition GyotoSmartPointer.h:135

Cloning is necessary for multi-threading, recommended for interaction with the Yorick plug-in etc.

Implementing it is very straightforward, as long as the copy constructor Generic(const Generic& ) has been implemented:

MyAstrobj* MyAstrobj::clone() const { return new MyAstrobj(*this); }

Implements Gyoto::Astrobj::Generic.

◆ computeB4vect()

void Gyoto::Astrobj::Generic::computeB4vect	(	double	B4vect[4],
		std::string const	magneticConfig,
		double const	co[8],
		state_t const &	cph
	)		const

inherited

Compute the magnetic field 4-vector at a given position and a given configuration

Parameters

B4vect	the output 4-vector magnetic field
magneticConfig	string which determine the wanted configuration ('Radial', 'Azimuthal', 'Vertical')
co	coordinate of the object which also contain its velocity
cph	coordinate of the photon

◆ deltaInObj()

double Gyoto::Astrobj::Standard::deltaInObj ( ) const

inherited

Get Generic::delta_inobj_.

Get the constant integration step inside the astrobj

Returns: delta_inobj_ in geometrical units

◆ deltaMax()

virtual double Gyoto::Astrobj::Generic::deltaMax ( double coord[8] )

virtualinherited

Get max step constraint for adaptive integration.

Parameters

[in] coord position

Returns: max step to find this object reliably

Reimplemented in Gyoto::Astrobj::Complex.

◆ describeProperty()

std::string Gyoto::Object::describeProperty ( Gyoto::Property const & p ) const

inherited

Format desrciption for a property.

Returns a string containing the name(s) and type of the property, as well as whether it supports unit.

◆ emission() [1/2]

virtual void Gyoto::Astrobj::Generic::emission	(	double	Inu[],
		double const	nu_em[],
		size_t	nbnu,
		double	dsem,
		state_t const &	coord_ph,
		double const	coord_obj[8] = `NULL`
	)		const

virtualinherited

Specific intensity I_ν for several values of ν_em

Called by the default implementation for processHitQuantities().

emission() computes the intensity I_ν emitted by the small volume of length dsem. It should take self-absorption along dsem into account.

Same as emission(double nu_em, double dsem, double coord_ph[8], double coord_obj[8]=NULL) const looping on several values of nu_em.

Parameters

Inu[nbnu]	Output (must be set to a previously allocated array of doubles)
nu_em[nbnu]	Frequencies at emission
nbnu	Size of Inu[] and nu_em[]
dsem	Length over which to integrate inside the object
coord_ph	Photon coordinate
coord_obj	Emitter coordinate at current photon position

Returns: I_ν or dI_ν [W m-2 sr-2]

Reimplemented in Gyoto::Astrobj::Python::Standard, and Gyoto::Astrobj::Python::ThinDisk.

◆ emission() [2/2]

virtual double Gyoto::Astrobj::Generic::emission	(	double	nu_em,
		double	dsem,
		state_t const &	coord_ph,
		double const	coord_obj[8] = `NULL`
	)		const

virtualinherited

Specific intensity I_ν

Called by the default implementation for processHitQuantities().

emission() computes the intensity I_ν emitted by the small volume of length ds_em, in the emitter's frame. It should take self-absorption along ds_em into account.

Reminder :

intensity = I_ν [J m^-2 s^-1 ster^-1 Hz^-1];
invariant intensity = I_ν/ν³, which has the same value in any frame;
emission coefficient = j_ν [J m^-3 s^-1 ster^-1 Hz^-1] , defined by dI_ν = j_ν*ds, where ds is the distance travelled by the photon inside the object;
invariant emission coef = j_ν/ν², which has the same value in any frame.

The equation used for radiative transfer (without absorption) is:

d(I_ν/ν³)/dλ = (j_ν/ν²) [*]

where λ is the integration parameter along the null geodesic.

NB: Let us consider a particular observer, with ν being the frequency measured by this observer, and ds being the proper distance (as measured by the observer) that the photon travels as it moves from λ to λ+dλ along its geodesic. Then it can be shown that:

dλ = ds/ν

This shows that Eq. [*] is homogeneous.

The default implementation returns 1. if optically thick and ds_em if optically thin. It allows for a quick implementation of your object for visualization purposes.

Parameters

nu_em	Frequency at emission [Hz]
dsem	length over which to integrate inside the object [geometrical units]
coord_ph	Photon coordinate
coord_obj	Emitter coordinate at current photon position

Reimplemented in Gyoto::Astrobj::DynamicalDiskBolometric, Gyoto::Astrobj::EquatorialHotSpot, Gyoto::Astrobj::NeutronStarAnalyticEmission, Gyoto::Astrobj::NeutronStarModelAtmosphere, Gyoto::Astrobj::XillverReflection, Gyoto::Astrobj::DirectionalDisk, Gyoto::Astrobj::DynamicalDisk, Gyoto::Astrobj::DynamicalDisk, Gyoto::Astrobj::DynamicalDisk3D, Gyoto::Astrobj::PageThorneDisk, Gyoto::Astrobj::PatternDisk, Gyoto::Astrobj::PatternDiskBB, Gyoto::Astrobj::PatternDiskBB, Gyoto::Astrobj::ThinDiskGridIntensity, Gyoto::Astrobj::ThinDiskIronLine, Gyoto::Astrobj::ThinDiskPL, Gyoto::Astrobj::ThinDiskProfile, Gyoto::Astrobj::Torus, Gyoto::Astrobj::Python::Standard, Gyoto::Astrobj::Python::ThinDisk, Gyoto::Astrobj::InflateStar, and Gyoto::Astrobj::UniformSphere.

◆ fillElement()

virtual void Gyoto::Object::fillElement ( Gyoto::FactoryMessenger * fmp ) const

virtualinherited

Fill the XML element for this Object.

The base implementation simply calls fillProperty() for each Property defined for the Object.

Derived classes should avoid overriding fillElement(). It may make sense occasionally, e.g. to make sure that the metric is output first.

To customize how a given Property is rendered, it is better to override fillProperty().

If this method is overridden, the implementation should in general call fillElement() on the direct base.

Reimplemented in Gyoto::Astrobj::Complex, Gyoto::Metric::Complex, Gyoto::Spectrometer::Complex, and Gyoto::Scenery.

◆ fillProperty()

void Gyoto::Astrobj::PolishDoughnut::fillProperty	(	Gyoto::FactoryMessenger *	fmp,
		Property const &	p
	)		const

virtual

Output a single Property to XML.

The base implementation decides what to do based on the p.type. The format matches how setParameters() an setParameter() would interpret the XML descition.

Overriding this method should be avoided, but makes sense in some cases (for instance Screen::fillProperty() selects a different unit for Distance based on its magnitude, so that stellar sizes are expressed in solar radii while smaller sizes can be expressed in meters and larger sizes in parsecs).

Overriding implementation should fall-back on calling the implementation in the direct parent class:

class A: public Object {};
class B: public A { 
 using B::setParameter;
 virtual void fillProperty(Gyoto::FactoryMessenger *fmp,
                        Property const &p) const ;
};
void B::fillProperty(Gyoto::FactoryMessenger *fmp,
                        Property const &p) const {
  if (name=="Duff") fmp->doSomething();
  else A::fillProperty(fmp, p);
}

Reimplemented from Gyoto::Object.

◆ getChi()

double Gyoto::Astrobj::Generic::getChi	(	double const	fourvect[4],
		state_t const &	cph,
		double const	vel[4],
		bool	elec = `false`
	)		const

inherited

Get Chi angle. Return the angle between the parallel transported observer polarization basis (Ephi,Etheta) and the Stokes basis in the rest frame of the emitter defined by the 4-vector magnetic/electric field.

Parameters

fourvect	4-vector magnetic/electric field depending on elec (false/true)
cph	Photon coordinate, must contain the Ephi and Etheta vectors i.e. size(cph)==16
vel	Fluid velocity at the photon coordinate

◆ getDefaultQuantities()

virtual Gyoto::Quantity_t Gyoto::Astrobj::Generic::getDefaultQuantities ( )

virtualinherited

Which quantities to compute if know was requested.

Return a Gyoto::Quantity_t suitable as input to Gyoto::Scenery::setRequestedQuantities() to set de default quantities to compute for this object. The default of these defaults GYOTO_QUANTITY_INTENSITY.

Reimplemented in Gyoto::Astrobj::PageThorneDisk.

◆ getIndice()

int Gyoto::Astrobj::Generic::getIndice	(	double &	xq,
		std::string const	cond_limit,
		double const	X_params[3],
		double *const	X = `NULL`
	)		const

privateinherited

Function that return the closest indice of the query value on an axis.

Parameters

xq	query value on the axis. Could be modified in case of periodic boundary condition.
cond_limit	boundary conditions that will be applied to the axis.
X_params[3]	array which contain the minimum value, the maximum value and the length of the axe.
X	(optional) array which contains the value of the axis points. Usefull for not linearly spaced axis.

◆ getProperties()

virtual Property const * Gyoto::Astrobj::PolishDoughnut::getProperties ( ) const

virtual

Get list of properties.

This method is declared automatically by the GYOTO_OBJECT macro and defined automatically by the GYOTO_PROPERTY_END macro.

Reimplemented from Gyoto::Astrobj::Standard.

◆ getSinCos2Chi()

void Gyoto::Astrobj::Generic::getSinCos2Chi	(	double const	fourvect[4],
		state_t const &	cph,
		double const	vel[4],
		double *	sin2Chi,
		double *	cos2Chi,
		bool	elec = `false`
	)		const

inherited

Get the cosinus and sinus of 2*Chi angle. Chi being the angle between the parallel transported observer polarization basis (Ephi,Etheta) and the Stokes basis in the rest frame of the emitter defined by the 4-vector magnetic/electric field.

Parameters

fourvect	4-vector magnetic/electric field depending on elec (false/true)
cph	Photon coordinate, must contain the Ephi and Etheta vectors i.e. size(cph)==16
vel	Fluid velocity at the photon coordinate

◆ getVelocity()

virtual void Gyoto::Astrobj::PolishDoughnut::getVelocity	(	double const	pos[4],
		double	vel[4]
	)

protectedvirtual

Fluid velocity field.

Fill vel with the 4-vector velocity of the fluid at 4-position pos.

Parameters

[in]	pos	4-position at which to compute velocity;
[out]	vel	4-velocity at pos.

Implements Gyoto::Astrobj::Standard.

◆ giveDelta()

virtual double Gyoto::Astrobj::Standard::giveDelta ( double coord[8] )

virtualinherited

Maximum δ inside object.

Gives the requested integration step δ_t (in coordinate time t) between two neighboring points along a portion of geodesic inside an astrobj; the current implementation only considers a constant delta, equal to Standard::deltaInobj()

Parameters

coord input coordinate at which δ_t is given

Reimplemented in Gyoto::Astrobj::Python::Standard.

◆ help()

void Gyoto::Object::help ( ) const

inherited

Print (to stdout) some help on this class.

Describe all properties that this instance supports.

◆ Impact()

int Gyoto::Astrobj::PolishDoughnut::Impact	(	Photon *	ph,
		size_t	index,
		Astrobj::Properties *	data
	)

virtual

Does a photon at these coordinates impact the object?

Impact() checks whether a Photon impacts the object between two integration steps of the photon's trajectory (those two steps are photon->getCoord(index, coord1) and photon->getCoord(index+1, coord2)). Impact returns 1 if the photon impacts the object between these two steps, else 0. In many cases of geometrically thick obects, the implementation Astrobj::Standard::Impact() will be fine.

Impact will call Generic::processHitQuantities() (which is virtual and may be re-implemented) to compute observable properties on demand: if the data pointer is non-NULL, the object will look in it for pointers to properties which apply to its kind. If a pointer to a property known to this object is present, then the property is computed and store at the pointed-to address. For instance, all objects know the "intensity" property. If data->intensity != NULL, the instensity is computed and stored in *data->intensity.

If data is non-NULL and only in this case, processHitQuantities() will also call ph->transmit() to update the transmissions of the Photon (see Photon::transmit(size_t, double)). This must not be done if data is NULL (see Astrobj::Complex::Impact() for an explanation).

Impact() may not extend the ph Worldline. The only two dates that are guaranteed to be defined are at indices index and index+1.

Parameters

ph	Gyoto::Photon aimed at the object;
index	Index of the last photon step;
data	Pointer to a structure to hold the observables at impact.

Returns: 1 if impact, 0 if not.

Reimplemented from Gyoto::Astrobj::Standard.

◆ integrateEmission() [1/2]

virtual void Gyoto::Astrobj::PolishDoughnut::integrateEmission	(	double *	I,
		double const *	boundaries,
		size_t const *	chaninds,
		size_t	nbnu,
		double	dsem,
		state_t const &	cph,
		double const *	co
	)		const

protectedvirtual

∫_ν₁^ν₂ I_ν dν (or j_ν)

PolishDought::emission() is slow. Integrating it is very slow. This implementation simply oversamples the spectrum by PolishDoughnut::spectral_oversampling_ and sums the trapezoids.

For general documentation, see Astrobj::Generic::integrateEmission(double * I, double const * boundaries, size_t const * chaninds, size_t nbnu, double dsem, double *cph, double *co) const .

Reimplemented from Gyoto::Astrobj::Generic.

◆ integrateEmission() [2/2]

virtual double Gyoto::Astrobj::Generic::integrateEmission	(	double	nu1,
		double	nu2,
		double	dsem,
		state_t const &	c_ph,
		double const	c_obj[8] = `NULL`
	)		const

virtualinherited

∫_ν₁^ν₂ I_ν dν (or j_ν)

Compute the integral of emission() from ν₁ to ν₂. The default implementation is a numerical integrator which works well enough and is reasonably fast if emission() is a smooth function (i.e. no emission or absorption lines). If possible, it is wise to implement an analytical solution. It is used by processHitQuantities to compute the "BinSpectrum" quantity which is the most physical: it is the only quantity that can be actually measured directly by a real-life instrument.

Reimplemented in Gyoto::Astrobj::Torus, Gyoto::Astrobj::Python::Standard, and Gyoto::Astrobj::Python::ThinDisk.

◆ interp1d()

double Gyoto::Astrobj::Generic::interp1d	(	double const	x,
		double const	y0,
		double const	y1
	)		const

privateinherited

Function which returns the 1D linear interpolation.

Parameters

x	the x query position along the linear function [0,1].
y0	the value of the array to be interpolated at the low position.
y1	the value of the array to be interpolated at the high position.

◆ interpNd()

double Gyoto::Astrobj::Generic::interpNd	(	int const	N,
		double *const	Xq,
		double **const	X,
		double *const	Y,
		std::string const *	cond_limit
	)		const

privateinherited

Function which returns the N- dimension interpolation on an N-dimensional cube

Parameters

N	number of dimensions
Xq	query position at which the interpolation should be done. 1D array with N elements.
X[2**N][N]	2D array that contains for the 2**N points of the N dimensional cube the associated axes values.
Y[2**N]	1D array that contain the value of the array to be interpolated at each points of the N-dimensional cube.
cond_limit	1D array of strings that set the boundary conditions that will be applied to each axes.

◆ interpolate() [1/2]

double Gyoto::Astrobj::Generic::interpolate	(	int const	N,
		double *const	array,
		double *const	Xq,
		double **const	X,
		int *const	X_params,
		std::string const *	cond_limits
	)		const

inherited

N-dimensional linear interpolation function

Parameters

N	number of dimensions
array	array that should be interpolated. This array has to be a 1D array with the first dimension evolving the slowest
Xq	query position at which the interpolation should be done. 1D array with N elements.
X	2D array containing the range of all the axes (for example : radius, \theta, \varphi) at which the array is knwon. Should be built as a pointer of pointers.
X_params	1D array that contain the length of each axes.
cond_limits	1D array of strings that set the boundary conditions that will be applied to each axes

◆ interpolate() [2/2]

double Gyoto::Astrobj::Generic::interpolate	(	int const	N,
		double *const	array,
		double *const	Xq,
		double **const	X_params,
		std::string const *	cond_limits
	)		const

inherited

N-dimensional linear interpolation function

Parameters

N	number of dimensions
array	array that should be interpolated. This array has to be a 1D array with the first dimension evolving the slowest
Xq	query position at which the interpolation should be done. 1D array with N elements.
X_params[N][3]	2D array that contain the minimum value, the maximum value and the length of each axes. The axes will be assumed to be linearly spaced.
cond_limits	1D array of strings that set the boundary conditions that will be applied to each axes.

◆ isThreadSafe()

virtual bool Gyoto::Object::isThreadSafe ( ) const

virtualinherited

Whether this class is thread-safe.

Return True if this object is thread-safe, i.e. if an instance and its clone can be used in parallel threads (in the context of Scenery::raytrace()). Known objects which are not thread-safe include Lorene metrics and everything from the Python plug-in.

The default implementation considers that the class itself is thread safe and recurses into the declared properties to check whether they are safe too. Classes that abide to the Object/Property paradigm and are themselves thread-safe have nothing special to do.

Objects that clone children in their copy constructor that are not declared as properties must take these children into account.

Classes that are never thread-safe must declare it. It acn be easily done using GYOTO_OBJECT_THREAD_SAFETY in the class declaration and GYOTO_PROPERTY_THREAD_UNSAFE in the class definition.

◆ kind() [1/2]

virtual std::string Gyoto::Object::kind ( ) const

virtualinherited

Get kind_.

Reimplemented in Gyoto::Spectrometer::Uniform.

◆ kind() [2/2]

virtual void Gyoto::Object::kind ( const std::string )

protectedvirtualinherited

Set kind_.

kind(const std::string) is protected because, for most Objects, it should not be changed in runtime. Set kind_

◆ metric() [1/2]

virtual SmartPointer< Metric::Generic > Gyoto::Astrobj::Generic::metric ( ) const

virtualinherited

Get the Metric gg_.

Reimplemented in Gyoto::Astrobj::Complex, Gyoto::Astrobj::DeformedTorus, Gyoto::Astrobj::DirectionalDisk, Gyoto::Astrobj::DynamicalDisk3D, Gyoto::Astrobj::EquatorialHotSpot, Gyoto::Astrobj::FixedStar, Gyoto::Astrobj::FlaredDiskSynchrotron, Gyoto::Astrobj::Jet, Gyoto::Astrobj::NeutronStar, Gyoto::Astrobj::OscilTorus, Gyoto::Astrobj::Plasmoid, Gyoto::Astrobj::SphericalAccretion, Gyoto::Astrobj::Star, Gyoto::Astrobj::StarTrace, Gyoto::Astrobj::ThickDisk, Gyoto::Astrobj::ThinDiskGridIntensity, and Gyoto::Astrobj::XillverReflection.

◆ metric() [2/2]

virtual void Gyoto::Astrobj::PolishDoughnut::metric ( Gyoto::SmartPointer< Gyoto::Metric::Generic > )

virtual

Set the Metric gg_.

Reimplemented from Gyoto::Astrobj::Generic.

◆ Omatrix()

Eigen::Matrix4d Gyoto::Astrobj::Generic::Omatrix	(	double	alphanu[4],
		double	rnu[3],
		double	Chi,
		double	dsem
	)		const

inherited

Omatrix() computes the exponential of the Mueller matrix which contains the absorption and Faraday coefficients and is used in the polarized radiative transfer equation.

Parameters

Onu	output matrix (must be allocated previously)
alphanu[4]	array containing the 4 absorption coefficients in the Stokes basis (I,Q,U,V)
rnu[3]	array containing the 3 Faraday coefficients in the Stokes basis (Q,U,V)
Chi	angle of rotation between the parallel transported observer polarization basis and the Stokes basis
dsem	geometrical length in geometrical units

◆ operator()() [1/2]

virtual double Gyoto::Astrobj::PolishDoughnut::operator() ( double const coord[4] )

virtual

Function defining the object interior.

A potential, distance, or whatever function such that operator()(double const coord[4]) < Standard::critical_value_ if and only if coord is inside the object. This function is used by the default implmenetation of Impact(). If Impact() is overloaded, it is not necessary to overload operator()(double coord[4]). The default implementation throws an error.

Implements Gyoto::Astrobj::Standard.

◆ operator()() [2/2]

virtual double Gyoto::Functor::Double_constDoubleArray::operator() ( double const data[] )

pure virtualinherited

The actual function.

Implemented in Gyoto::Astrobj::ThinDisk.

◆ opticallyThin() [1/2]

bool Gyoto::Astrobj::Generic::opticallyThin ( ) const

inherited

Query whether object is optically thin.

See opticallyThin(bool flag).

◆ opticallyThin() [2/2]

void Gyoto::Astrobj::Generic::opticallyThin ( bool flag )

inherited

Set whether the object is optically thin.

Set flag indicating that radiative transfer should be integrated, i.e. the object is to be considered optically thin.

Parameters

flag	1 if optically thin, 0 if optically thick.

◆ processHitQuantities()

virtual void Gyoto::Astrobj::Generic::processHitQuantities	(	Photon *	ph,
		state_t const &	coord_ph_hit,
		double const *	coord_obj_hit,
		double	dt,
		Astrobj::Properties *	data
	)		const

virtualinherited

Fills Astrobj::Properties.

processHitQuantities fills the requested data in Impact. To use it, you need to call it in the Impact() method for your object in case of hit. It will fill Redshift, Intensity, Spectrum, BinSpectrum and update the Photon's transmission by calling Photon::transmit(), only if data==NULL.

You can overload it for your Astrobj. The generic implementation calls emission(), integrateEmission() and transmission() below.

Reimplemented in Gyoto::Astrobj::PageThorneDisk, Gyoto::Astrobj::DynamicalDiskBolometric, and Gyoto::Astrobj::ThinDiskProfile.

◆ property()

Property const * Gyoto::Object::property ( std::string const pname ) const

inherited

Find property by name.

Look into the Property list for a Property whose name (or name_false, for a boolean Property) is pname. Return a const pointer to the first such property found, or NULL if none is found.

◆ radiativeQ() [1/2]

virtual void Gyoto::Astrobj::Generic::radiativeQ	(	double *	Inu,
		double *	Qnu,
		double *	Unu,
		double *	Vnu,
		Eigen::Matrix4d *	Onu,
		double const *	nuem,
		size_t	nbnu,
		double	dsem,
		state_t const &	cph,
		double const *	co
	)		const

virtualinherited

Compute the increment of Stokes parameters and transmission matrix. Polarised version of RadiaveQ.

First function to be called for radiative quantities. If exist, i.e. implemented in an Astrobj, return the Stokes parameters emitted by the small volume of length dsem.

Warning :

The basis used to determine the Stokes coefficients is different from the observer parallel transported polarisation basis. One should use getChi function to compute the angle between these two basis.
The non polarized case must also be implemented in this function to avoid error.

See example in SimplePolarStar.C.

Parameters

Inu[nbnu]	Output increment of intensity (must be set to a previously allocated array of doubles)
Qnu[nbnu]	Output increment of Stokes parameter Q (must be set to a previously allocated array of doubles)
Unu[nbnu]	Output increment of Stokes parameter U (must be set to a previously allocated array of doubles)
Vnu[nbnu]	Output increment of Stokes parameter V (must be set to a previously allocated array of doubles)
Onu[nbnu]	Output transmission (Eigen) matrix (must be set to a previously allocated array of Matrix4d)
nu_em[nbnu]	Frequencies at emission
nbnu	Size of nu_em[], Inu[], Qnu[], Unu[], Vnu[], and Onu[]
dsem	Length over which to integrate inside the object
cph	Photon coordinate
co	Emitter coordinate at current photon position

Returns: Increment of the Stokes parameters (I,Q,U,V) and local Transmission matrix (O).

Reimplemented in Gyoto::Astrobj::EquatorialHotSpot, Gyoto::Astrobj::PageThorneDisk, Gyoto::Astrobj::Star, and Gyoto::Astrobj::ThickDisk.

◆ radiativeQ() [2/2]

virtual void Gyoto::Astrobj::PolishDoughnut::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

protectedvirtual

emission and transmission together

Reimplemented from Gyoto::Astrobj::Generic.

◆ rMax() [1/4]

virtual double Gyoto::Astrobj::Generic::rMax ( )

virtualinherited

Get maximal distance from center of coordinate system.

Get maximal distance from center of coordinate system at which a Photon may hit the object.

Child classes may use the rmax_ member to cache this value, if its current value is DBL_MAX.

It can also be set using rMax().

Returns: rmax_ in geometrical units

Reimplemented in Gyoto::Astrobj::Complex, Gyoto::Astrobj::FixedStar, Gyoto::Astrobj::Star, and Gyoto::Astrobj::Torus.

◆ rMax() [2/4]

virtual void Gyoto::Astrobj::Generic::rMax ( double val )

virtualinherited

Set maximal distance from center of coordinate system.

Set maximal distance from center of coordinate system at which a Photon may hit the object.

Parameters

val	new rmax_ in geometrical units.

◆ rMax() [3/4]

virtual void Gyoto::Astrobj::Generic::rMax	(	double	val,
		std::string const &	unit
	)

virtualinherited

Set maximal distance from center of coordinate system.

Call Generic::rMax(double val) after converting val from unit to geometrical units.

Parameters

val	rmax_ expressed in unit "unit";
unit	string...

◆ rMax() [4/4]

virtual double Gyoto::Astrobj::Generic::rMax ( std::string const & unit )

virtualinherited

Get rmax_ is specified unit.

Call rMax() and convert result to unit.

Parameters

unit string

Returns: double rmax converted to unit

◆ rotateJs()

Eigen::Vector4d Gyoto::Astrobj::Generic::rotateJs	(	double	jInu,
		double	jQnu,
		double	jUnu,
		double	jVnu,
		double	sin2Chi,
		double	cos2Chi
	)		const

inherited

Apply the rotation matrix with angle Chi to the emission Stokes vector constructed in the fonction from the individual coefficients

◆ setParameter() [1/2]

void Gyoto::Astrobj::PolishDoughnut::setParameter	(	Gyoto::Property const &	p,
		std::string const &	name,
		std::string const &	content,
		std::string const &	unit
	)

virtual

Set parameter by Property (and name)

This function is used when parsing an XML description, if Property (p) of this name is found (i.e. either p.name or p.name_false is equal to name). Implementation should fall-back on calling the direct's parent implementation:

class A: public Object {};
class B: public A { 
 using B::setParameter;
 virtual void setParameter(Gyoto::Property const &p,
                           std::string name,
                        std::string content,
                        std::string unit);
};
void B::setParameter(Gyoto::Property const &p,
                          std::string name,
                  std::string content,
                  std::string unit) {
  if (name=="Duff") doSomething(content, unit);
  else A::setParameter(p, name, content, unit);
}

Parameters

p	Property that matches name (p.name == name or p.name_false == name)
name	XML name of the parameter (XML entity)
content	string representation of the value
unit	string representation of the unit

Reimplemented from Gyoto::Object.

◆ setParameter() [2/2]

virtual int Gyoto::Object::setParameter	(	std::string	name,
		std::string	content,
		std::string	unit
	)

virtualinherited

Set parameter by name.

This function is used when parsing an XML description, if no Property of this name is found. Overriding implementation should fall-back on calling the direct's parent implementation:

class A: public Object {};
class B: public A { 
 using B::setParameter;
 virtual int setParameter(std::string name,
                    std::string content,
                    std::string unit);
};
int B::setParameter(std::string name,
                    std::string content,
                    std::string unit) {
  if (name=="Duff") doSomething(content, unit);
  else return A::setParameter(name, content, unit);
  return 0;  // name was known
}

Parameters

name	XML name of the parameter (XML entity). This may have a path component, e.g. "Astrobj::Radius", in which case a property named "Astrobj" will be sought in the current object, and setParameter will be called recusrively on this Astrobj with Radius as name.
content	string representation of the value
unit	string representation of the unit

Returns: 0 if this parameter is known, 1 if it is not.

Reimplemented in Gyoto::Astrobj::EquatorialHotSpot, Gyoto::Metric::KerrKS, Gyoto::Astrobj::Star, and Gyoto::Metric::RotStar3_1.

◆ setParameters()

virtual void Gyoto::Astrobj::Generic::setParameters ( FactoryMessenger * fmp )

virtualinherited

Main loop in Subcontractor_t function.

The Subcontractor_t function for each Astrobj kind should look somewhat like this (templated as Gyoto::Astrobj::Subcontractor<MyKind>):

SmartPointer<Astrobj::Generic>
Gyoto::Astrobj::MyKind::Subcontractor(FactoryMessenger* fmp) {
  SmartPointer<MyKind> ao = new MyKind();
  ao -> setParameters(fmp);
  return ao;
}

Each object kind should implement setParameter(string name, string content, string unit) to interpret the individual XML elements. setParameters() can be overloaded in case the specific Astrobj class needs low level access to the FactoryMessenger. See UniformSphere::setParameters().

Reimplemented from Gyoto::Object.

Reimplemented in Gyoto::Astrobj::Complex, Gyoto::Astrobj::EquatorialHotSpot, Gyoto::Astrobj::Star, and Gyoto::Astrobj::OscilTorus.

◆ tell()

virtual void Gyoto::Astrobj::PolishDoughnut::tell ( Gyoto::Hook::Teller * msg )

protectedvirtual

Update PolishDoughnut::aa_.

See Hook::Listener::tell().

Reimplemented from Gyoto::Hook::Listener.

◆ transmission()

virtual double Gyoto::Astrobj::Generic::transmission	(	double	nuem,
		double	dsem,
		state_t const &	coord_ph,
		double const	coord_obj[8]
	)		const

virtualinherited

Transmission: exp( α_ν * ds_em )

transmission() computes the transmission of this fluid element or 0 if optically thick. The default implementation returns 1. (no attenuation) if optically thin, 0. if optically thick.

Parameters

nuem	frequency in the fluid's frame
coord	Photon coordinate
dsem	geometrical length in geometrical units

Reimplemented in Gyoto::Astrobj::PatternDisk, and Gyoto::Astrobj::DynamicalDisk3D.

Member Data Documentation

◆ __defaultfeatures

int Gyoto::Astrobj::Generic::__defaultfeatures

privateinherited

Whether some virtual methods are implemented.

The default implementations of some methods call one-another. This member is used internally to avoid infinite recursion.

◆ deltamaxinsidermax_

double Gyoto::Astrobj::Generic::deltamaxinsidermax_

protectedinherited

Maximum Photon integration step inside rmax_ [geometrical units].

Maximum step for Photon integation when inside the sphere of radius rmax_.

deltamaxinsidermax_ is in geometrical units.

◆ deltaPL_

double Gyoto::Astrobj::PolishDoughnut::deltaPL_

protected

fraction of thermal energy in non-thermal electrons

Obsiously, 0 means no non-thermal electrons at all. In this case, the (trivial) non-thermal computations are skipped. Ther is thus non need for an additional "nonthermal_" flag. Fraction of electrons emitting powerlaw synchro

◆ kind_

std::string Gyoto::Object::kind_

protectedinherited

The "kind" that is output in the XML entity.

E.g. for an Astrobj, fillElement() will ensure

Gyoto::Object::kind

virtual std::string kind() const

Get kind_.

is written.

◆ mutex_

pthread_mutex_t Gyoto::SmartPointee::mutex_

privateinherited

A mutex.

When compiled with libpthread

◆ plugins_

std::vector<std::string> Gyoto::Object::plugins_

protectedinherited

The plug-ins that needs to be loaded to access this instance's class.

E.g. for an Astrobj, fillElement() will ensure

is written.

◆ rmax_

double Gyoto::Astrobj::Generic::rmax_

protectedinherited

Maximum distance to the center of the coordinate system [geometrical units].

Maximum distance from the center of the coordinate system at which a photon may hit the object. Child classes may compute a decent value for rmax_ at any time if rmax_ is DBL_MAX. External classes (Photons in particular) must use rMax() to access this information.

rmax_ is in geometrical units.

The documentation for this class was generated from the following file:

GyotoPolishDoughnut.h

Classes

Public Types

Public Member Functions

Public Attributes

Static Public Attributes

Protected Member Functions

Protected Attributes

Private Member Functions

Private Attributes

Friends

Detailed Description

Member Typedef Documentation

◆ Subcontractor_t

Member Function Documentation

◆ clone()

◆ computeB4vect()

◆ deltaInObj()

◆ deltaMax()

◆ describeProperty()

◆ emission() [1/2]

◆ emission() [2/2]

◆ fillElement()

◆ fillProperty()

◆ getChi()

◆ getDefaultQuantities()

◆ getIndice()

◆ getProperties()

◆ getSinCos2Chi()

◆ getVelocity()

◆ giveDelta()

◆ help()

◆ Impact()

◆ integrateEmission() [1/2]

◆ integrateEmission() [2/2]

◆ interp1d()

◆ interpNd()

◆ interpolate() [1/2]

◆ interpolate() [2/2]

◆ isThreadSafe()

◆ kind() [1/2]

◆ kind() [2/2]

◆ metric() [1/2]

◆ metric() [2/2]

◆ Omatrix()

◆ operator()() [1/2]

◆ operator()() [2/2]

◆ opticallyThin() [1/2]

◆ opticallyThin() [2/2]

◆ processHitQuantities()

◆ property()

◆ radiativeQ() [1/2]

◆ radiativeQ() [2/2]

◆ rMax() [1/4]

◆ rMax() [2/4]

◆ rMax() [3/4]

◆ rMax() [4/4]

◆ rotateJs()

◆ setParameter() [1/2]

◆ setParameter() [2/2]

◆ setParameters()

◆ tell()

◆ transmission()

Member Data Documentation

◆ __defaultfeatures

◆ deltamaxinsidermax_

◆ deltaPL_

◆ kind_

◆ mutex_

◆ plugins_

◆ rmax_