#include "cddefines.h"#include "taulines.h"#include "opacity.h"#include "hydrogenic.h"#include "conv.h"#include "iso.h"#include "wind.h"#include "magnetic.h"#include "phycon.h"#include "thermal.h"#include "h2.h"#include "dense.h"#include "dynamics.h"#include "trace.h"#include "rt.h"#include "pressure.h"#include "radius.h"#include "rfield.h"#include "doppvel.h"#include "rt_escprob.h"
Functions | |
| void | PresTotCurrent () |
Function Documentation
◆ PresTotCurrent()
| void PresTotCurrent | ( | void | ) |
PressureTotal determine the gas and line radiation pressures for current conditions, this sets the variable pressure.PresTotlCurr
- Todo
- 2 this is the total binding energy of the molecules, and is negative, the energy need to get back to free atoms never set and only appears in print statements
- Todo
- 0 add this press term due to cosmic rays - hextra.cr_energydensity
- Todo
- 0 code has variable magnetic energydensity and pressure, which are equal, as they must be - del one or the other
References ASSERT, broken(), cdEXIT, chLineLbl(), conv, dBaseSpecies, dBaseTrans, DEBUG_ENTRY, dense, diatoms, DoppVel, DynaFlux(), dynamics, EXIT_FAILURE, fixit, fnzone, fprintf(), GetDopplerWidth(), t_ADfA::getEthresh(), Heavy, HFLines, hydro, Singleton< t_ADfA >::Inst(), ioQQQ, ipH1s, ipH2p, ipH_LIKE, ipHE_LIKE, ipHYDROGEN, iso_ctrl, iso_sp, iteration, lgElemsConserved(), LIMELM, magnetic, Magnetic_evaluate(), MAX2, MIN2, NISO, nSpecies, nWindLine, nzone, opac, phycon, POW2, pressure, PressureRadiationLine(), radius, rfield, RT_line_driving(), RT_LineWidth(), SDIV(), ShowMe(), SMALLFLOAT, SumDensities(), TauLine2, TempChange(), TorF(), trace, and wind.
Referenced by ConvBase(), ConvInitSolution(), ConvPresTempEdenIoniz(), ConvTempEdenIoniz(), CoolHeatError(), IterStart(), map_do(), and PressureChange().
