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Primary Computational Subroutines

xstar:
Main program.

dsec:
calculate thermal equilibrium and charge neutrality using secant method

ener:
set up energy grid

func:
calculate all ion fractions, level populations, heating, cooling, emissivities and opacities.

func1:
calculate rates affecting ion fractions

func2:
calculate rates affecting level populations

func2a:
calculate rates affecting level populations due to Auger and inner shell photoionization

func2i:
calculate number of bound levels for an ion

func3:
calculate heating-cooling rates, opacities and emissivities.

init:
initialization. Zeroes most variables

heatt:
total heating and cooling rate calculation, and calculation of radiation fields (i.e. radiative transfer solution).

msolvelucy:
Level population calculation

ioneqm:
calculation ion fractions (for first pass).

istruc:
calculate ion abundances (for first pass)

invert:
used to prepare for next iteration of global calculation

step:
calculates spatial step size

stpcut:
update important quantities after each spatial step.

trnfrc:
calculates local continuum flux

trnfrn:
calculates transfer of diffusely emitted radiation.


next up previous contents
Next: Rate Calculation Subroutines Up: List of Subroutines Previous: List of Subroutines   Contents
Tim Kallman 2014-06-30