Gyoto
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Blob of plasma following a Star orbit, emitting synchrotron, with Gaussian time-evolving density and temperature. More...
#include <GyotoBlob.h>
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. More... | |
Public Member Functions | |
virtual Property const * | getProperties () const |
Get list of properties. More... | |
Blob () | |
Default constructor. More... | |
Blob (const Blob &orig) | |
Copy constructor. | |
virtual Blob * | clone () const |
Cloner. More... | |
virtual | ~Blob () |
Destructor. | |
virtual std::string | className () const |
"Blob" More... | |
virtual std::string | className_l () const |
"inflate_star" More... | |
double | numberDensity () const |
double | numberDensity (std::string const &unit) const |
void | numberDensity (double ne) |
void | numberDensity (double dens, std::string const &unit) |
double | temperature () const |
void | temperature (double tt) |
double | timeRef () const |
double | timeRef (std::string const &unit) const |
void | timeRef (double tt) |
void | timeRef (double tt, std::string const &unit) |
double | timeSigma () const |
double | timeSigma (std::string const &unit) const |
void | timeSigma (double tt) |
void | timeSigma (double tt, std::string const &unit) |
void | magnetizationParameter (double rr) |
double | magnetizationParameter () const |
double | kappaIndex () const |
void | kappaIndex (double) |
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 More... | |
virtual void | metric (SmartPointer< Metric::Generic >) |
Set the Metric gg_. More... | |
virtual SmartPointer< Metric::Generic > | metric () const |
Get the Metric gg_. More... | |
virtual double | getMass () const |
Return 1. More... | |
virtual double | rMax () |
Get maximal distance from center of coordinate system. More... | |
virtual double | rMax () const |
Get maximal distance from center of coordinate system. | |
virtual double | rMax (std::string const &unit) |
Get rmax_ is specified unit. More... | |
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. More... | |
virtual void | rMax (double val, std::string const &unit) |
Set maximal distance from center of coordinate system. More... | |
virtual void | setInitialCondition (double const coord[8]) |
Same as Worldline::setInitialCondition(gg, coord, sys,1) More... | |
void | setInitialCondition (SmartPointer< Metric::Generic > gg, const double coord[8], const int dir, double const Ephi[4], double const Etheta[4]) |
Set or re-set the initial condition prior to integration. More... | |
void | setInitialCondition (SmartPointer< Metric::Generic > gg, const double coord[8], const int dir) |
Set or re-set the initial condition prior to integration. More... | |
virtual int | setParameter (std::string name, std::string content, std::string unit) |
Set parameter by name. More... | |
virtual void | setParameter (Gyoto::Property const &p, std::string const &name, std::string const &content, std::string const &unit) |
Set parameter by Property (and name) More... | |
virtual void | setParameters (FactoryMessenger *fmp) |
Main loop in Subcontractor_t function. More... | |
virtual void | fillProperty (Gyoto::FactoryMessenger *fmp, Property const &p) const |
Output a single Property to XML. More... | |
virtual 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) |
Get the 6 Cartesian coordinates for specific dates. More... | |
virtual void | getVelocity (double const pos[4], double vel[4]) |
Yield velocity of the center of the sphere. More... | |
virtual void | spectrum (SmartPointer< Spectrum::Generic >) |
Set spectrum_. | |
virtual SmartPointer< Spectrum::Generic > | spectrum () const |
Get spectrum_. | |
virtual void | opacity (SmartPointer< Spectrum::Generic >) |
Set opacity_. | |
virtual SmartPointer< Spectrum::Generic > | opacity () const |
Get opacity_. | |
double | radius () const |
Get radius_ in geometrical units. | |
virtual void | radius (double) |
Set radius_ in geometrical units. More... | |
double | radius (std::string const &) const |
Get radius_ in specified unit. | |
virtual void | radius (double, std::string const &) |
Set radius_ in specified unit. More... | |
double | deltaMaxOverRadius () const |
Get dltmor_. | |
virtual void | deltaMaxOverRadius (double f) |
Set dltmor_. | |
double | deltaMaxOverDistance () const |
Get dltmod_. | |
virtual void | deltaMaxOverDistance (double f) |
Set dltmod_. | |
bool | isotropic () const |
void | isotropic (bool) |
double | alpha () const |
void | alpha (double) |
virtual double | operator() (double const coord[4]) |
Square distance to the center of the sphere. More... | |
virtual double | operator() (double const data[])=0 |
The actual function. More... | |
virtual double | deltaMax (double *coord) |
virtual double | deltaMax (double coord[8]) |
Get max step constraint for adaptive integration. More... | |
double | deltaMax () const |
Get delta_max_. | |
virtual double | deltaMax (double const pos[8], double delta_max_external) const |
void | deltaMax (double h1) |
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 Iν for several values of νem More... | |
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 double | integrateEmission (double nu1, double nu2, double dsem, state_t const &c_ph, double const c_obj[8]=NULL) const |
∫ν1ν2 Iν dν (or jν) More... | |
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, state_t const &cph, double const *co) const |
∫ν1ν2 Iν dν (or jν) More... | |
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( αν * dsem ) More... | |
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. | |
virtual void | safetyValue (double val) |
Set Standard::safety_value_. | |
virtual double | safetyValue () const |
Get Standard::safety_value_. | |
double | deltaInObj () const |
Get Generic::delta_inobj_. More... | |
void | deltaInObj (double val) |
Set Generic::delta_inobj_. | |
virtual int | Impact (Gyoto::Photon *ph, size_t index, Astrobj::Properties *data=NULL) |
Does a photon at these coordinates impact the object? More... | |
virtual double | giveDelta (double coord[8]) |
Maximum δ inside object. More... | |
const std::string | kind () const |
Get the kind of the Astrobj (e.g. "Star") | |
GYOTO_OBJECT_ACCESSORS_UNIT (deltaMaxInsideRMax) | |
void | opticallyThin (bool flag) |
Set whether the object is optically thin. More... | |
bool | opticallyThin () const |
Query whether object is optically thin. More... | |
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. More... | |
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. More... | |
virtual void | processHitQuantities (Photon *ph, double *coord_ph_hit, double *coord_obj_hit, double dt, Astrobj::Properties *data) const =delete |
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, double *alphaInu, double *alphaQnu, double *alphaUnu, double *alphaVnu, double *rQnu, double *rUnu, double *rVnu, double const *nuem, size_t nbnu, double dsem, state_t const &cph, double const *co) 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. More... | |
void | set (Property const &p, Value val) |
Set Value of a Property. | |
void | set (Property const &p, Value val, std::string const &unit) |
Set Value (expressed in unit) of a Property. | |
void | set (std::string const &pname, Value val) |
Set Value of a Property. | |
void | set (std::string const &pname, Value val, std::string const &unit) |
Set Value (expressed in unit) of a Property. | |
Value | get (Property const &p) const |
Get Value of a Property. | |
Value | get (std::string const &pname) const |
Get Value of a Property. | |
Value | get (Property const &p, std::string const &unit) const |
Get Value of a Property, converted to unit. | |
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. More... | |
virtual void | fillElement (Gyoto::FactoryMessenger *fmp) const |
Fill the XML element for this Object. More... | |
std::string | describeProperty (Gyoto::Property const &p) const |
Format desrciption for a property. More... | |
void | help () const |
Print (to stdout) some help on this class. More... | |
size_t | getImin () const |
Get imin_. | |
size_t | getImax () const |
Get imax_. | |
size_t | getI0 () const |
Get i0_. | |
void | initCoord (std::vector< double > const &) |
std::vector< double > | initCoord () const |
virtual void | setInitCoord (const double coord[8], int dir, double const Ephi[4], double const Etheta[4]) |
Set Initial coordinate. More... | |
virtual void | setInitCoord (const double coord[8], int dir=0) |
Set Initial coordinate. More... | |
virtual void | setInitCoord (double const pos[4], double const vel[3], int dir=0) |
Set initial coordinate. More... | |
virtual void | setPosition (double const pos[4]) |
Set initial 4-position. | |
virtual void | setVelocity (double const vel[3]) |
Set initial 3-velocity. | |
void | reset () |
Forget integration, keeping initial contition. | |
void | reInit () |
Reset and recompute particle properties. | |
void | integrator (std::string const &type) |
Set the integrator. More... | |
std::string | integrator () const |
Describe the integrator used by state_. | |
double | deltaMin () const |
Get delta_min_. | |
void | deltaMin (double h1) |
Set delta_min_. | |
void | absTol (double) |
Set abstol_. | |
double | absTol () const |
Get abstol_. | |
void | relTol (double) |
Set reltol_. | |
double | relTol () const |
Get reltol_. | |
double | deltaMaxOverR () const |
Get delta_max_over_r_. | |
void | deltaMaxOverR (double t) |
Set delta_max_over_r_. | |
void | delta (const double delta) |
Expand memory slots for polarization vectors. More... | |
void | delta (double, const std::string &unit) |
Set delta_ in specified units. | |
double | delta () const |
Get delta_. | |
double | delta (const std::string &unit) const |
Get delta_ in specified units. | |
double | tMin () const |
Get tmin_. | |
double | tMin (const std::string &unit) const |
Get tmin_ in specified unit. | |
void | tMin (double tlim) |
Set tmin_. | |
void | tMin (double, const std::string &unit) |
Set tmin_ in specified unit. | |
void | adaptive (bool mode) |
Set adaptive_. | |
bool | adaptive () const |
Get adaptive_. | |
void | secondary (bool sec) |
Set secondary_. | |
bool | secondary () const |
Get secondary_. | |
void | parallelTransport (bool pt) |
Set parallel_transport_. | |
bool | parallelTransport () const |
Get parallel_transport_. | |
void | maxiter (size_t miter) |
Set maxiter_. | |
size_t | maxiter () const |
Get maxiter_. | |
double const * | getCst () const |
Returns the worldline's cst of motion (if any) More... | |
void | setCst (double const *cst, size_t const ncsts) |
Set Metric-specific constants of motion. More... | |
void | getInitialCoord (std::vector< double > &dest) const |
Get initial coordinates + base vectors. More... | |
void | getCoord (size_t index, Gyoto::state_t &dest) const |
Get coordinates+base vectors corresponding to index. More... | |
void | getCoord (size_t index, Gyoto::state_t &dest) |
Get coordinates+base vectors corresponding to index. More... | |
void | getCoord (double date, Gyoto::state_t &dest, bool proper=false) |
Get coordinates+base vectors corresponding to date dest[0]. More... | |
void | getCoord (double const *const dates, size_t const n_dates, double *const x1dest, double *const x2dest, double *const x3dest, double *const x0dot=NULL, double *const x1dot=NULL, double *const x2dot=NULL, double *const x3dot=NULL, double *ep0=NULL, double *ep1=NULL, double *ep2=NULL, double *ep3=NULL, double *et0=NULL, double *et1=NULL, double *et2=NULL, double *et3=NULL, double *otime=NULL, bool proper=false) |
Get 8-coordinates for specific dates. More... | |
void | getCoord (double *x0, double *x1, double *x2, double *x3) const |
Get all computed positions. More... | |
void | getCartesianPos (size_t index, double dest[4]) const |
Get Cartesian expression of 4-position at index. | |
virtual void | xStore (size_t ind, state_t const &coord, double tau) |
Store coord at index ind. More... | |
virtual void | xStore (size_t ind, state_t const &coord)=delete |
Obsolete, update your code. | |
virtual void | xStore (size_t ind, double const coord[8])=delete |
Obsolete, update your code. | |
virtual void | xFill (double tlim, bool proper=false) |
Fill x0, x1... by integrating the Worldline from previously set inittial condition to time tlim. | |
size_t | get_nelements () const |
Get number of computed dates. | |
void | get_t (double *dest) const |
Get computed dates. | |
void | get_tau (double *dest) const |
Get computed proper times or values of the affine parameter. | |
void | get_xyz (double *x, double *y, double *z) const |
Get 3-position in cartesian coordinates for computed dates. | |
void | checkPhiTheta (double coord[8]) const |
Bring θ in [0,Π] and φ in [0,2Π]. More... | |
void | getSkyPos (SmartPointer< Screen > screen, double *dalpha, double *ddellta, double *dD) const |
Get computed positions in sky coordinates. | |
void | get_dot (double *x0dot, double *x1dot, double *x2dot, double *x3dot) const |
Get computed 4-velocities. | |
void | get_prime (double *x1prime, double *x2prime, double *x3prime) const |
Get computed 3-velocities. | |
void | save_txyz (char *fichierxyz) const |
Save in a file. | |
void | save_txyz (char *const filename, double const t1, double const mass_sun, double const distance_kpc, std::string const unit, SmartPointer< Screen > sc=NULL) |
Save, converted. | |
Public Attributes | |
GYOTO_WORLDLINE | |
int | stopcond |
Whether and why integration is finished. | |
Static Public Attributes | |
static GYOTO_OBJECT Property const | properties [] |
Protected Member Functions | |
virtual double | emission (double nu_em, double dsem, state_t const &cp, double const co[8]=NULL) const |
Emission is determined by spectrum_ and opacity_. More... | |
virtual double | integrateEmission (double nu1, double nu2, double dsem, state_t const &c_ph, double const *c_obj=NULL) const |
virtual double | transmission (double nuem, double dsem, state_t const &, double const *) const |
Transmission is determined by opacity_. | |
virtual void | xAllocate () |
Allocate x0, x1 etc. with default size. More... | |
virtual void | xAllocate (size_t size) |
Allocate x0, x1 etc. with a specified size. More... | |
virtual size_t | xExpand (int dir) |
Expand x0, x1 etc... to hold more elements. More... | |
virtual void | xExpand (double *&x, int dir) |
Expand one array to hold more elements. More... | |
virtual void | eAllocate () |
Allocate ep0_ ... et3_. More... | |
virtual void | eDeallocate () |
Deallocate ep0_ ... et3_. More... | |
virtual void | eExpand (int dir) |
virtual void | tell (Gyoto::Hook::Teller *) |
This is how a Teller tells. More... | |
Protected Attributes | |
double | radius_ |
sphere radius [geometrical units] | |
bool | isotropic_ |
if 1, then emission just returns 1 | |
SmartPointer< Spectrum::Generic > | spectrum_ |
sphere emission law | |
SmartPointer< Spectrum::Generic > | opacity_ |
if optically thin, opacity law | |
double | dltmor_ |
see deltaMax(double*) | |
double | dltmod_ |
see deltaMax(double*) | |
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]. More... | |
double | deltamaxinsidermax_ |
Maximum Photon integration step inside rmax_ [geometrical units]. More... | |
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. More... | |
std::vector< std::string > | plugins_ |
The plug-ins that needs to be loaded to access this instance's class. More... | |
SmartPointer< Gyoto::Metric::Generic > | metric_ |
The Gyoto::Metric in this part of the universe. | |
double * | tau_ |
proper time or affine parameter | |
double * | x0_ |
t or T | |
double * | x1_ |
r or x | |
double * | x2_ |
θ or y | |
double * | x3_ |
φ or z | |
double * | x0dot_ |
tdot or Tdot | |
double * | x1dot_ |
rdot or xdot | |
double * | x2dot_ |
θdot or ydot | |
double * | x3dot_ |
φdot or zdot | |
double * | ep0_ |
double * | ep1_ |
Coordinate of first base vector to parallel transport. | |
double * | ep2_ |
Coordinate of first base vector to parallel transport. | |
double * | ep3_ |
Coordinate of first base vector to parallel transport. | |
double * | et0_ |
Coordinate of first base vector to parallel transport. | |
double * | et1_ |
Coordinate of Second base vector to parallel transport. | |
double * | et2_ |
Coordinate of Second base vector to parallel transport. | |
double * | et3_ |
Coordinate of Second base vector to parallel transport. | |
size_t | x_size_ |
Coordinate of Second base vector to parallel transport. More... | |
size_t | imin_ |
Minimum index for which x0_, x1_... have been computed. | |
size_t | i0_ |
Index of initial condition in array. | |
size_t | imax_ |
Maximum index for which x0_, x1_... have been computed. | |
bool | adaptive_ |
Whether integration should use adaptive delta. | |
bool | secondary_ |
Experimental: choose 0 to compute only primary image. More... | |
bool | parallel_transport_ |
Whether to parallel transport a local triad. More... | |
double | delta_ |
Initial integrating step. More... | |
double | tmin_ |
Time limit for the integration (geometrical units) More... | |
double * | cst_ |
Worldline's csts of motion (if any) | |
size_t | cst_n_ |
Number of constants of motion. | |
int | wait_pos_ |
Hack in setParameters() | |
double * | init_vel_ |
Hack in setParameters() | |
size_t | maxiter_ |
Maximum number of iterations when integrating. | |
double | delta_min_ |
Minimum integration step for the adaptive integrator. More... | |
double | delta_max_ |
Maximum integration step for the adaptive integrator. More... | |
double | delta_max_over_r_ |
Numerical tuning parameter. More... | |
double | abstol_ |
Absolute tolerance of the integrator. More... | |
double | reltol_ |
Absolute tolerance of the integrator. More... | |
SmartPointer< Worldline::IntegState::Generic > | state_ |
An object to hold the integration state. | |
Private Attributes | |
double | numberDensity_cgs_ |
cgs-unit number density of hotspot | |
double | temperature_ |
temperature of hotspot | |
double | timeRef_M_ |
M-unit reference time for Gaussian hotspot evolution. | |
double | timeSigma_M_ |
M-unit temporal sigma for Gaussian hotspot evolution. | |
double | magnetizationParameter_ |
magnetization parameter | |
double | kappaIndex_ |
hotspot synchrotron kappa-distribution index | |
SmartPointer< Spectrum::KappaDistributionSynchrotron > | spectrumKappaSynch_ |
int | __defaultfeatures |
Whether some virtual methods are implemented. More... | |
int | refCount |
Reference counter. | |
pthread_mutex_t | mutex_ |
A mutex. More... | |
Friends | |
class | Gyoto::SmartPointer< Gyoto::Astrobj::Blob > |
Blob of plasma following a Star orbit, emitting synchrotron, with Gaussian time-evolving density and temperature.
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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().
Gyoto::Astrobj::Blob::Blob | ( | ) |
Default constructor.
Create Blob object with undefined initial conditions. One needs to set the coordinate system, the metric, and the initial position and velocity before integrating the orbit. setInititialCondition() can be used for that.
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inherited |
Bring θ in [0,Π] and φ in [0,2Π].
checkPhiTheta() Modifies coord if the corrdinates are spherical-like so that coord[2]=theta is in [0,pi] and coord[3]=phi is in [0,2pi]. Important to use in all astrobj in spherical coordinates to prevent "z-axis problems".
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virtual |
"Blob"
Reimplemented from Gyoto::Astrobj::Star.
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virtual |
"inflate_star"
Reimplemented from Gyoto::Astrobj::Star.
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virtual |
Cloner.
This method must be implemented by the various Astrobj::Generic subclasses in order to support cloning:
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:
Reimplemented from Gyoto::Astrobj::Star.
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inherited |
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inherited |
Get Generic::delta_inobj_.
Get the constant integration step inside the astrobj
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virtualinherited |
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virtualinherited |
Get delta max at a given position
[in] | pos | 4-position |
[in] | delta_max_external | external constraint on delta_max |
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virtualinherited |
Get max step constraint for adaptive integration.
[in] | coord | position |
Reimplemented in Gyoto::Astrobj::Complex.
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inherited |
Set delta_max_
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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.
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protectedvirtualinherited |
Allocate ep0_ ... et3_.
Allocate memory for polarization vectors
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protectedvirtualinherited |
Deallocate ep0_ ... et3_.
Deallocate memory for polarization vectors
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protectedvirtualinherited |
Call xExpand(double * &x, int dir) on #ep0_, ep1_ etc.
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virtualinherited |
Specific intensity Iν for several values of νem
Called by the default implementation for processHitQuantities().
emission() computes the intensity Iν 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.
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 |
Reimplemented in Gyoto::Astrobj::Python::Standard, and Gyoto::Astrobj::Python::ThinDisk.
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protectedvirtualinherited |
Emission is determined by spectrum_ and opacity_.
Reimplemented from Gyoto::Astrobj::Generic.
Reimplemented in Gyoto::Astrobj::InflateStar.
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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::Spectrometer::Complex, and Gyoto::Scenery.
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virtualinherited |
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:
Reimplemented from Gyoto::Object.
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virtualinherited |
Get the 6 Cartesian coordinates for specific dates.
This method is present in both the API of UniformSphere and Worldline. It is pure virtual in UniformSphere. The Star reimplementation is a trivial wrapper around Worldline::getCartesian().
Implements Gyoto::Astrobj::UniformSphere.
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inherited |
Get all computed positions.
Get all the pre-computed 8 coordinates (e.g. thanks to a prior call to xFill()) of this worldline.
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inherited |
Get 8-coordinates for specific dates.
The coordinates will be computed using the integrator, so they will be as accurate as possible. Some heuristics are used to speed up the process and it is presumably faster to call this routine with a sorted list of dates. The line will be integrated further as required. An error will be thrown if it is not possible to reach a certain date.
[in] | dates | the list of dates for which the coordinates are to be computed in proper time or affine parameter if #proper is true or in coordinate time if #proper is false (default); |
[in] | n_dates | the number of dates to compute ; |
[out] | x1dest,x2dest,x3dest,x0dot,x1dot,x2dot,x3dot | arrays in which to store the result. These pointer may be set to NULL to retrieve only part of the information. They must be pre-allocated. |
[out] | ephi0,ephi1,ephi2,ephi3,etheta0,etheta1,etheta2,etheta3 | arrays in which to store the ephi and etheta (parallel transport case). These pointer may be set to NULL to retrieve only part of the information. They must be pre-allocated. |
[out] | otime | array in which to store the other time: coordinate time if #proper, else proper time or affine parameter. |
[in] | proper | bool: whether #dates is proper time (or affine parameter) or coordinate time. |
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inherited |
Get coordinates+base vectors corresponding to date dest[0].
Depending on the value of parallel_transport_, get position (xi_), velocity (xidot_) and possibly other triad vectors (epi_ and eti_). coord is resized to the right number of elements.
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inherited |
Get coordinates+base vectors corresponding to index.
We need this non-const implementation to allow the const, size_t and the non-const, double implementations to coexist.
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inherited |
Get coordinates+base vectors corresponding to index.
Depending on the value of parallel_transport_, get position (xi_), velocity (xidot_) and possibly other triad vectors (epi_ and eti_). coord is resized to the right number of elements.
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inherited |
Returns the worldline's cst of motion (if any)
Return pointer to array holding the previously set Metric-specific constants of motion
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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.
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inherited |
Get initial coordinates + base vectors.
Depending on the size of dest and on the value of parallel_transport_, get position (xi_), velocity (xidot_) and possibly other triad vectors (epi_ and eti_).
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virtualinherited |
Return 1.
The mass of a Star is always 1. Stars do not perturb the metric. The only relevant point is that Stars are massive particules, their exact mass is of no importance.
Implements Gyoto::Worldline.
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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::Star.
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virtualinherited |
Yield velocity of the center of the sphere.
Implements Gyoto::Astrobj::UniformSphere.
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virtualinherited |
Maximum δ inside object.
Gives the requested integration step δt (in coordinate time t) between two neighbooring points along a portion of geodesic inside an astrobj; the current implementation only considers a constant delta, equal to Standard::deltaInobj()
coord | input coordinate at which δt is given |
Reimplemented in Gyoto::Astrobj::Python::Standard.
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inherited |
Print (to stdout) some help on this class.
Describe all properties that this instance supports.
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virtualinherited |
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.
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. |
Implements Gyoto::Astrobj::Generic.
Reimplemented in Gyoto::Astrobj::InflateStar, and Gyoto::Astrobj::PolishDoughnut.
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virtualinherited |
∫ν1ν2 Iν dν (or jν)
Like double integrateEmission(double nu1, double nu2, double dsem, double c_ph[8], double c_obj[8]) const for each Spectrometer channel.
Reimplemented in Gyoto::Astrobj::PolishDoughnut, Gyoto::Astrobj::Python::Standard, and Gyoto::Astrobj::Python::ThinDisk.
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virtualinherited |
∫ν1ν2 Iν dν (or jν)
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.
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inherited |
Set the integrator.
Initialize state_ to use the required integrator.
[in] | type | Either "Legacy" or (if GYOTO_HAVE_BOOST_INTEGRATORS) one of "runge_kutta_cash_karp54", "runge_kutta_fehlberg78", "runge_kutta_dopri5", "runge_kutta_cash_karp54_classic" |
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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.
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virtualinherited |
Reimplemented from Gyoto::Astrobj::Generic.
Reimplemented in Gyoto::Astrobj::StarTrace.
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virtualinherited |
Reimplemented from Gyoto::Astrobj::Generic.
Reimplemented in Gyoto::Astrobj::StarTrace, and Gyoto::Astrobj::StarTrace.
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virtualinherited |
Square distance to the center of the sphere.
Ensure integration does not miss the object
Implements Gyoto::Astrobj::Standard.
Reimplemented in Gyoto::Astrobj::StarTrace.
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pure virtualinherited |
The actual function.
Implemented in Gyoto::Astrobj::ThinDisk.
|
inherited |
Query whether object is optically thin.
|
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.
flag | 1 if optically thin, 0 if optically thick. |
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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, and Gyoto::Astrobj::DynamicalDiskBolometric.
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inherited |
|
virtual |
emission and transmission together
Reimplemented from Gyoto::Astrobj::Generic.
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virtualinherited |
Set radius_ in geometrical units.
Reimplemented in Gyoto::Astrobj::FixedStar, and Gyoto::Astrobj::FixedStar.
|
virtualinherited |
Set radius_ in specified unit.
Reimplemented in Gyoto::Astrobj::FixedStar.
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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().
Reimplemented from Gyoto::Astrobj::Generic.
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virtualinherited |
|
virtualinherited |
Set maximal distance from center of coordinate system.
Call Generic::rMax(double val) after converting val from unit to geometrical units.
val | rmax_ expressed in unit "unit"; |
unit | string... |
|
virtualinherited |
Get rmax_ is specified unit.
Call rMax() and convert result to unit.
unit | string |
|
inherited |
Set Metric-specific constants of motion.
The will (re)allocate Worldline::cst_, copy cst into it, and set Worldline::cst_n_.
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virtualinherited |
Set Initial coordinate.
Set imin_=imax_=i0_, and x[i0]=coord[].
If dir==1, i0_ is set to 0. If dir==-1, i0_ is set to x_size_-1.
If dir==0 and the Worldine has never been computed (i0_==0, imin_==1 and imax_==0), then dir defaults to 1 for a massive particle and -1 for a massless particle.
If dir==0 and the Worldine has already been computed, i0_ is not changed.
coord | new initial coordinates |
dir | direction of integration. 1 for forward integration, -1 for backards integration, 0 for unknown or both |
Ephi | initial value of base vector to parallel-transport. Ignored if parallel_transport_ is false. |
Etheta | initial value of base vector to parallel-transport. Ignored if parallel_transport_ is false. |
|
virtualinherited |
Set Initial coordinate.
Set imin_=imax_=i0_, and x[i0]=coord[].
If dir==1, i0_ is set to 0. If dir==-1, i0_ is set to x_size_-1.
If dir==0 and the Worldine has never been computed (i0_==0, imin_==1 and imax_==0), then dir defaults to 1 for a massive particle and -1 for a massless particle.
If dir==0 and the Worldine has already been computed, i0_ is not changed.
coord | new initial coordinates |
dir | direction of integration. 1 for forward integration, -1 for backards integration, 0 for unknown or both |
Reimplemented in Gyoto::Astrobj::StarTrace.
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virtualinherited |
Set initial coordinate.
pos | initial 4-position |
vel | initial 3-velocity |
dir | direction of integration |
|
virtualinherited |
Same as Worldline::setInitialCondition(gg, coord, sys,1)
Reimplemented in Gyoto::Astrobj::StarTrace, and Gyoto::Astrobj::StarTrace.
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inherited |
Set or re-set the initial condition prior to integration.
gg | Gyoto::SmartPointer to the Gyoto::Metric in this universe; |
coord | 8 element array containing the initial condition, i.e. the 4-position and the 4-velocity of the Photon at the receiving end; |
dir | direction: 1 for future, -1 for past. |
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inherited |
Set or re-set the initial condition prior to integration.
gg | Gyoto::SmartPointer to the Gyoto::Metric in this universe; |
coord | 8 element array containing the initial condition, i.e. the 4-position and the 4-velocity of the Photon at the receiving end; |
dir | direction: 1 for future, -1 for past. |
Ephi | initial value of base vector to parallel-transport. Ignored if parallel_transport_ is false. |
Etheta | initial value of base vector to parallel-transport. Ignored if parallel_transport_ is false. |
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virtualinherited |
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:
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 in Gyoto::Astrobj::PolishDoughnut.
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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:
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 |
Reimplemented from Gyoto::Object.
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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>):
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::Astrobj::Generic.
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protectedvirtualinherited |
This is how a Teller tells.
A teller will basically call listener->tell(this).
msg | Teller* the Teller who is telling... Useful if the Listener listens to several Tellers. |
Reimplemented from Gyoto::Hook::Listener.
|
virtualinherited |
Transmission: exp( αν * dsem )
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.
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.
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protectedvirtualinherited |
Allocate x0, x1 etc. with default size.
The default size is GYOTO_DEFAULT_X_SIZE
|
protectedvirtualinherited |
Allocate x0, x1 etc. with a specified size.
size | : number of cells in each array x0, x1 etc. |
Reimplemented in Gyoto::Astrobj::StarTrace.
|
protectedvirtualinherited |
Expand one array to hold more elements.
If you need to expand more arrays than x0_ ... x3_ and the dots, call this on your array before calling xExpand(int dir).
[in,out] | x | array to expand |
[in] | dir |
|
protectedvirtualinherited |
Expand x0, x1 etc... to hold more elements.
Double the size of arrays x0, x1 etc. and copy old version of the array in the first half if dir =1 and in the second half if dir =-1.
dir | : 1 to expand after last element, -1 to expand before first element |
Reimplemented in Gyoto::Astrobj::StarTrace.
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virtualinherited |
Store coord at index ind.
Reimplemented in Gyoto::Astrobj::StarTrace.
|
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.
|
protectedinherited |
Absolute tolerance of the integrator.
Used by the adaptive integrators implemented in IntegState::Boost. Refer to the boost::numeric::odeint documentation for more details.
|
protectedinherited |
Initial integrating step.
Default: GYOTO_DEFAULT_DELTA
|
protectedinherited |
Maximum integration step for the adaptive integrator.
The default (GYOTO_DEFAULT_DELTA_MAX) is usually fine.
For IntegState::Legacy, set it in the Metric instead!
|
protectedinherited |
Numerical tuning parameter.
For IntegState::Legacy, set it in the Metric instead!
Ensure that delta (the numerical integration step) is never larger than a fraction of the distance between the current location and the center of the coordinate system.
The default (GYOTO_DEFAULT_DELTA_MAX_OVER_R) is usually fine.
|
protectedinherited |
Minimum integration step for the adaptive integrator.
The default (GYOTO_DEFAULT_DELTA_MIN) is usually fine.
For IntegState::Legacy, set it in the Metric instead!
|
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.
|
protectedinherited |
The "kind" that is output in the XML entity.
E.g. for an Astrobj, fillElement() will ensure
is written.
|
privateinherited |
A mutex.
When compiled with libpthread
|
protectedinherited |
Whether to parallel transport a local triad.
Typically used to trace the base in which the Stokes parameters are expressed in the context of polarization.
|
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.
|
protectedinherited |
Absolute tolerance of the integrator.
Used by the adaptive integrators implemented in IntegState::Boost. Refer to the boost::numeric::odeint documentation for more details.
|
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.
|
protectedinherited |
Experimental: choose 0 to compute only primary image.
This feature is in development.
|
protectedinherited |
Time limit for the integration (geometrical units)
Computation does not go back before tmin_. Default is -DBL_MAX. tmin_ is always expressed in geometrical units, it is essentially a tuning parameter for the ray-tracing process. tmin_ should be chosen to always be longer than the distance between the screen and the object.
|
protectedinherited |