Cloudy
Spectral Synthesis Code for Astrophysics
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#include <thermal.h>
Public Attributes | |
double | HeatNet |
double | HeatLowEnr |
double | HeatHiEnr |
double t_phoHeat::HeatHiEnr |
this is the part of the heating that does secondaries, but without efficiency
Referenced by diatomics::CalcPhotoionizationRate(), GammaBn(), GammaK(), highen(), ion_photo(), and iso_photo().
double t_phoHeat::HeatLowEnr |
this is the part of the heating that cannot do secondary ionizations
Referenced by diatomics::CalcPhotoionizationRate(), GammaBn(), GammaK(), highen(), ion_photo(), and iso_photo().
double t_phoHeat::HeatNet |
HeatNet is heating due to individual species
Referenced by GammaBn(), GammaK(), ion_photo(), iso_photo(), and mole_h_reactions().