rt_continuum_shield_fcn.cpp

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/* This file is part of Cloudy and is copyright (C)1978-2013 by Gary J. Ferland and
 * others.  For conditions of distribution and use see copyright notice in license.txt */
/*rt_continuum_shield_fcn computing continuum shielding due to single line */
/*conpmp local continuum pumping rate radiative transfer for all lines */
 
#include "cddefines.h"
#include "rt.h"
#include "transition.h"
#include "thirdparty.h"
 
/*conpmp local continuum pumping rate radiative transfer for all lines */
STATIC double conpmp(const TransitionProxy& t);
STATIC inline double FITTED( double t );
 
namespace {
        class my_Integrand
        {
        public:
        double PumpDamp, PumpTau;
 
        double operator() (double x)
        {
                realnum v, rx = realnum(x);
                VoigtH(realnum(PumpDamp),&rx,&v,1);
                double opfun_v = sexp(PumpTau*v)*v;
                return opfun_v;
        }
};
}
 
 
/*rt_continuum_shield_fcn computing continuum shielding due to single line */
double RT_continuum_shield_fcn( const TransitionProxy& t )
{
        double value;
 
        DEBUG_ENTRY( "rt_continuum_shield_fcn()" );
 
        value = -1.;
 
        ASSERT( t.Emis().damp() > 0. );
 
        if( rt.nLineContShield == LINE_CONT_SHIELD_PESC )
        {
                /* set continuum shielding pesc - shieding based on escape probability */
                if( t.Emis().iRedisFun() == ipPRD )
                {
                        value =  esc_PRD_1side(t.Emis().TauCon(),t.Emis().damp());
                }
                else if( t.Emis().iRedisFun() == ipCRD )
                {
                        value =  esca0k2(t.Emis().TauCon());
                }
                else if( t.Emis().iRedisFun() == ipCRDW )
                {
                        value =  esc_CRDwing_1side(t.Emis().TauCon(),t.Emis().damp());
                }
                else if( t.Emis().iRedisFun() == ipLY_A )
                {
                        value = esc_PRD_1side(t.Emis().TauCon(),t.Emis().damp());
                }
                else
                        TotalInsanity();
        }
        else if( rt.nLineContShield == LINE_CONT_SHIELD_FEDERMAN )
        {
                /* set continuum shielding Federman - this is the default */
                double core, wings;
 
                /* these expressions implement the appendix of
                 * >>refer      line    shielding       Federman, S.R., Glassgold, A.E., & 
                 * >>refercon   Kwan, J. 1979, ApJ, 227, 466 */
                /* doppler core - equation A8 */
                if( t.Emis().TauCon() < 2. )
                {
                        core = sexp( t.Emis().TauCon() * 0.66666 );
                }
                else if( t.Emis().TauCon() < 10. )
                {
                        core = 0.638 * pow(t.Emis().TauCon(),(realnum)-1.25f );
                }
                else if( t.Emis().TauCon() < 100. )
                {
                        core = 0.505 * pow(t.Emis().TauCon(),(realnum)-1.15f );
                }
                else
                {
                        core = 0.344 * pow(t.Emis().TauCon(),(realnum)-1.0667f );
                }
 
                /* do we add damping wings? */
                wings = 0.;
                if( t.Emis().TauCon() > 1.f && t.Emis().damp()>0. )
                {
                        /* equation A6 */
                        double t1 = 3.02*pow(t.Emis().damp()*1e3,-0.064 );
                        double u1 = sqrt(t.Emis().TauCon()*t.Emis().damp() )/SDIV(t1);
                        wings = t.Emis().damp()/SDIV(t1)/sqrt( 0.78540 + POW2(u1) );
                        /* add very large optical depth tail to converge this with respect
                         * to escape probabilities - if this function falls off more slowly
                         * than escape probability then upper level will become overpopulated.
                         * original paper was not intended for this regime */
                        if( t.Emis().TauCon()>1e7 )
                                wings *= pow( t.Emis().TauCon()/1e7,-1.1 );
                }
                value = core + wings;
                /* some x-ray lines have vastly large damping constants, greater than 1.
                 * in these cases the previous wings value does not work - approximation
                 * is for small damping constant - do not let pump efficiency exceed unity
                 * in this case */
                if( t.Emis().TauCon()>0. )
                        value = MIN2(1., value );
        }
        else if( rt.nLineContShield == LINE_CONT_SHIELD_FERLAND )
        {
                /* set continuum shielding ferland */
                value = conpmp( t );
        }
        else if( rt.nLineContShield == 0 )
        {
                /* set continuum shielding none */
                value = 1.;
        }
        else
        {
                TotalInsanity();
        }
 
        /* the returned pump shield function must be greater than zero,
         * and less than 1 if a maser did not occur */
        ASSERT( value>=0 && (value<=1.||t.Emis().TauCon()<0.) );
 
        return value;
}
 
static const double BREAK = 3.;
/* fit to results for tau less than 10 */
STATIC inline double FITTED( double t )
{
        return (0.98925439 + 0.084594094*t)/(1. + t*(0.64794212 + t*0.44743976));
}
 
/*conpmp local continuum pumping rate radiative transfer for all lines */
STATIC double conpmp(const TransitionProxy& t)
{
        double a0, 
          conpmp_v, 
          tau, 
          yinc1, 
          yinc2;
 
        DEBUG_ENTRY( "conpmp()" );
 
        /* tau used will be optical depth in center of next zone
         * >>chng 96 july 6, had been ipLnTauIn, did not work when sphere static set */
        tau = t.Emis().TauCon();
        /* compute pumping probability */
        if( tau <= 10. )
        {
                /* for tau<10 a does not matter, and one fit for all */
                conpmp_v = FITTED(tau);
        }
        else if( tau > 1e6 )
        {
                /* this far in winds line opacity well below electron scattering
                        * so ignore for this problem */
                conpmp_v = 0.;
        }
        else
        {
                my_Integrand func;
                func.PumpDamp = t.Emis().damp();
                func.PumpTau = tau;
                Integrator<my_Integrand,Gaussian32> opfun;
 
                yinc1 = opfun.sum( 0., BREAK, func );
                yinc2 = opfun.sum( BREAK, 100., func );
 
                a0 = 0.886227*(1. + func.PumpDamp);
                conpmp_v = (yinc1 + yinc2)/a0;
        }
 
        /* EscProb is escape probability, will not allow conpmp to be greater than it
         * on second iteration with thick lines, pump prob=1 and esc=0.5
         * conpmp = MIN( conpmp , t.t(ipLnEscP) )
         * */
        return conpmp_v;
}