#include <hextra.h>
◆ t_hextra()
◆ chName()
const char * t_hextra::chName |
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const |
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inlinevirtual |
◆ comment()
◆ zero()
void t_hextra::zero |
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void | | ) |
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virtual |
◆ background_density
realnum t_hextra::background_density |
default cosmic ray background density and rate
Referenced by t_hextra().
◆ background_rate
◆ cr_energydensity
double t_hextra::cr_energydensity |
cosmic ray energy density erg cm-3
◆ crpowr
◆ CrsSecNeutron
double t_hextra::CrsSecNeutron |
cross section for stopping relativistic neutrons
◆ crtemp
◆ cryden
◆ cryden_ov_background
realnum t_hextra::cryden_ov_background |
current cosmic ray density divided by default galactic background
◆ effneu
◆ frcneu
frcneu is fraction of total luminosity in neutrons, dimensionless
◆ HextraScaleDensity
realnum t_hextra::HextraScaleDensity |
◆ HextraSS_M
double t_hextra::HextraSS_M |
mass of the black hole in grams
◆ HextraSSalpha
the parameter alpha of alpha model, dimensionless
◆ HextraSSradius
◆ lg_CR_B_equipartition
bool t_hextra::lg_CR_B_equipartition |
true for cosmic rays in equipartition with magnetic field
◆ lgHextraDensity
bool t_hextra::lgHextraDensity |
options for extra heating the depends on density, as set with hextra command
◆ lgHextraDepth
bool t_hextra::lgHextraDepth |
options for heating to depth on depth, true is depth occurs on hextra command
◆ lgHextraSS
bool t_hextra::lgHextraSS |
options for extra heating is from SS model, as set with hextra command
◆ lgNeutrnHeatOn
bool t_hextra::lgNeutrnHeatOn |
flag lgNeutrnHeatOn says heating due to neutrons is enabled
◆ lgTurbHeatVaryTime
bool t_hextra::lgTurbHeatVaryTime |
set true if extra heat varies with time in time dependent sims
◆ totneu
totneu is neutron energy flux, erg cm-2 s-1
◆ turback
the scale radius from the back of the cloud
◆ TurbHeat
extra heating set with hextra command, first the heating rate
◆ TurbHeatSave
save the initial value in case TurbHeat varies with time
◆ turrad
the scale radius for the heating
The documentation for this struct was generated from the following files: