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Data Fields

t_hextra Struct Reference

#include <hextra.h>

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Data Fields

realnum cryden
realnum crpowr
realnum crtemp
bool lg_CR_B_equipartition
double cr_energydensity
realnum cryden_ov_background
realnum background_density
realnum background_rate
realnum TurbHeat
realnum TurbHeatSave
bool lgHextraDepth
realnum turrad
realnum turback
bool lgHextraDensity
realnum HextraScaleDensity
bool lgTurbHeatVaryTime
realnum totneu
bool lgNeutrnHeatOn
realnum frcneu
realnum effneu
double CrsSecNeutron

Detailed Description

Definition at line 12 of file hextra.h.


Field Documentation

default cosmic ray background density and rate

Definition at line 28 of file hextra.h.

Referenced by highen(), InitCoreload(), and ParseCosmicRays().

Definition at line 29 of file hextra.h.

Referenced by InitCoreload(), and ParseCosmicRays().

cosmic ray energy density erg cm-3

Definition at line 22 of file hextra.h.

Referenced by highen(), and InitDefaultsPreparse().

Definition at line 14 of file hextra.h.

Referenced by highen(), InitDefaultsPreparse(), and ParseCosmicRays().

cross section for stopping relativistic neutrons

Definition at line 64 of file hextra.h.

Referenced by highen(), radius_increment(), and zero().

Definition at line 14 of file hextra.h.

Referenced by highen(), InitDefaultsPreparse(), and ParseCosmicRays().

current cosmic ray density divided by default galactic background

Definition at line 25 of file hextra.h.

Referenced by H2_X_coll_rate_evaluate(), hmole_step(), InitDefaultsPreparse(), and ParseCosmicRays().

effneu is efficiency

Definition at line 62 of file hextra.h.

Referenced by ContSetIntensity(), ParseCommands(), and zero().

frcneu is fraction of total luminosity in neutrons, dimensionless

Definition at line 60 of file hextra.h.

Referenced by ContSetIntensity(), ParseCommands(), and zero().

the scale density

Definition at line 50 of file hextra.h.

Referenced by highen(), and ParseCommands().

true for cosmic rays in equipartition with magnetic field

Definition at line 19 of file hextra.h.

Referenced by highen(), InitDefaultsPreparse(), and ParseCosmicRays().

options for extra heating the depends on density, as set with hextra command

Definition at line 47 of file hextra.h.

Referenced by highen(), InitDefaultsPreparse(), and ParseCommands().

options for heating to depth on depth, true is depth occurs on hextra command

Definition at line 39 of file hextra.h.

Referenced by highen(), InitDefaultsPreparse(), and ParseCommands().

flag lgNeutrnHeatOn says heating due to neutrons is enabled

Definition at line 58 of file hextra.h.

Referenced by ContSetIntensity(), highen(), ParseCommands(), radius_increment(), and zero().

set true if extra heat varies with time in time dependent sims

Definition at line 53 of file hextra.h.

Referenced by DynaEndIter(), InitDefaultsPreparse(), and ParseCommands().

totneu is neutron energy flux, erg cm-2 s-1

Definition at line 56 of file hextra.h.

Referenced by ContSetIntensity(), highen(), radius_increment(), and zero().

the scale radius from the back of the cloud

Definition at line 41 of file hextra.h.

Referenced by highen(), and ParseCommands().

extra heating set with hextra command, first the heating rate

Definition at line 32 of file hextra.h.

Referenced by DynaEndIter(), highen(), InitDefaultsPreparse(), ParseCommands(), and PrtComment().

save the initial value in case TurbHeat varies with time

Definition at line 32 of file hextra.h.

Referenced by DynaEndIter(), and ParseCommands().

the scale radius for the heating

Definition at line 41 of file hextra.h.

Referenced by highen(), and ParseCommands().


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