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- xstar:
- Main program.
- cndnse:
- condense matrix for level population calculation
- dsec:
- calculate thermal equilibrium and charge neutrality using secant
method
- ener:
- set up energy grid
- func:
- calculate all ion fractions, level populations, heating, cooling.
- 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
- init:
- initialization. Zeroes most variables
- heatt:
- total heating and cooling rate calculation
- hcor1:
- Level population calculation
- ioneqm:
- calculation ion fractions
- istruc:
- calculate ion abundances
- 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 dilution and attenuation of incident radiation
- trnfrn:
- calculates transfer of diffusely emitted radiation.
Next: Rate Calculation Subroutines
Up: List of Subroutines
Previous: List of Subroutines
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Tim Kallman
2011-05-25