/home66/gary/public_html/cloudy/c13_branch/source/rt_escprob.cpp

Go to the documentation of this file.

/* 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 */
/*esc_CRDwing_1side fundamental escape probability radiative transfer routine, for complete redistribution */
/*esc_PRD_1side fundamental escape probability radiative transfer routine for incomplete redistribution */
/*RTesc_lya escape prob for hydrogen atom Lya, using Hummer and Kunasz results,
 * called by hydropesc */
/*esc_PRD escape probability radiative transfer for incomplete redistribution */
/*esc_CRDwing escape probability for CRD with wings */
/*esc_CRDcore escape probability for CRD with no wings */
/*esca0k2 derive Hummer's K2 escape probability for Doppler core only */
/*RT_DestProb returns line destruction probability due to continuum opacity */
/*RT_LineWidth determine half width of any line with known optical depths */
#include "cddefines.h"
#include "physconst.h"
#include "dense.h"
#include "conv.h"
#include "rfield.h"
#include "opacity.h"
#include "lines_service.h"
#include "taulines.h"
#include "doppvel.h"
#include "pressure.h"
#include "wind.h"
#include "rt.h"
#include "iso.h"
#include "thirdparty.h"

inline double tau_from_here(double tau_tot, double tau_in)
{
        const double SCALE = 2.;
        double tt = tau_tot - tau_in;
        if (1)
        {
                /*  help convergence by not letting tau go to zero at back edge of
                 *  when there was a bad guess for the total optical depth
                 *  note that this test is seldom hit since RTMakeStat does check
                 *  for overrun */
                if( tt < 0. )
                {
                        tt = tau_in/SCALE;
                }
        }
        else
        {
                // Alternatively, allow tau_from_here to go to zero, and then
                // increase again.  This will give more or less the right
                // distribution of tau values, though with tau_out estimated to
                // be zero somewhere inside the layer rather than at the edge.
                //
                // The iteration 1 inward-only treatment is equivalent to this,
                // if the estimated tau_out is set to be zero.
                //
                //     I think you'll find, I'm playing all of the right
                //     notes... but not necessarily in the right order.
                //
                //                                     -- Eric Morecambe
                tt = fabs(tt);
        }
        return tt;
}

/*escConE2 one of the forms of the continuum escape probability */
class my_Integrand_escConE2
{
public:
        double chnukt_ContTkt, chnukt_ctau;

        double operator() (double x)
        {
                return exp(-chnukt_ContTkt*(x-1.))/x*e2(chnukt_ctau/POW3(x));
        }
};

/* a continuum escape probability */
class my_Integrand_conrec
{
public:
        double chnukt_ContTkt;

        double operator() (double x)
        {
                return exp(-chnukt_ContTkt*(x-1.))/x;
        }
};


/*escmase escape probability for negative (masing) optical depths,*/
STATIC double escmase(double tau);
/*RTesc_lya_1side fit Hummer and Kunasz escape probability for hydrogen atom Lya */
STATIC void RTesc_lya_1side(double taume, 
  double beta, 
  realnum *esc, 
  realnum *dest,
  /* position of line in frequency array on c scale */
  long ipLine );

double esc_PRD_1side(double tau, 
  double a)
{
        double atau, 
          b, 
          escinc_v;

        DEBUG_ENTRY( "esc_PRD_1side()" );
        ASSERT( a>0.0 );

        /* this is one of the three fundamental escape probability routines
         * the three are esc_CRDwing_1side, esc_PRD_1side, and RTesc_lya
         * it computes esc prob for incomplete redistribution
         * */
#       if 0
        if( strcmp(rt.chEscFunSubord,"SIMP") == 0 )
        {
                /* this set with "escape simple" command, used for debugging */
                escinc_v = 1./(1. + tau);
                return escinc_v;
        }
#       endif

        if( tau < 0. )
        {
                /* line mased */
                escinc_v = escmase(tau);
        }
        else
        {
                /* first find coefficient b(tau) */
                atau = a*tau;
                if( atau > 1. )
                {
                        b = 1.6 + (3.*pow(2.*a,-0.12))/(1. + atau);
                }
                else
                {
                        double sqrtatau = sqrt(atau);
                        b = 1.6 + (3.*pow(2.*a,-0.12))*sqrtatau/(1. + sqrtatau);
                }
                b = MIN2(6.,b);

                escinc_v = 1./(1. + b*tau);
        }
        return escinc_v;
}

// Implement equation (157) of Avrett & Loeser 1966
// 1966SAOSR.201.....A for comparison with escape probability with
// damping.  Uses transformation x -> y/(1-y) to map domain of
// integral to [0,1)
class k2DampArg
{
        realnum damp, tau;
public:
        k2DampArg(realnum damp, realnum tau) : damp(damp), tau(tau) {}

        realnum operator()(realnum y) const
                {
                        if (y >= 1.)
                                return 0;
                        realnum x = y/(1.-y);
                        realnum phi;
                        VoigtU(damp,&x,&phi,1);
                        if (phi <= 0.)
                        {
                                return 0.;
                        }
                        else
                        {
                                return phi*expn(2,phi*tau)/POW2(1.-y);
                        }
                }
};

template<class F>
double trapezium(realnum xmin, realnum xmax, const F func)
{
        double tol = 1e-6;
        vector<double> vxmin, vxmax, fxmin, fxmax, step;
        vxmin.push_back(xmin);
        vxmax.push_back(xmax);
        fxmin.push_back(func(xmin));
        fxmax.push_back(func(xmax));
        step.push_back(0.5*(xmax-xmin)*(fxmin[0]+fxmax[0]));
        for (long level = 0; level < 25; ++level)
        {
                size_t nstep = step.size();
                double current = 0.0;
                for (size_t i=0; i<nstep; ++i)
                        current += step[i];
                for (size_t i=0; i<nstep; ++i)
                {
                        if (vxmax[i] > vxmin[i])
                        {
                                if (level <= 3 || step[i] > tol*current
                                        || (i == nstep-1 && current <= 0.0) )
                                {
                                        double xbar=0.5*(vxmin[i]+vxmax[i]);
                                        vxmin.push_back(xbar);
                                        fxmin.push_back(func(xbar));
                                        vxmax.push_back(vxmax[i]);
                                        fxmax.push_back(fxmax[i]);
                                        long ilast = vxmax.size()-1;
                                        vxmax[i] = xbar;
                                        fxmax[i] = fxmin[ilast];
                                        step[i] = 0.5*(vxmax[i]-vxmin[i])*(fxmin[i]+fxmax[i]);
                                        //fprintf(ioQQQ,"%g %g\n",vxmin[ilast],fxmin[ilast],
                                        //      step[i]);
                                        step.push_back(0.5*(vxmax[ilast]-vxmin[ilast])*
                                                                                (fxmin[ilast]+fxmax[ilast]));
                                }
                        }
                }
        }
        double current = 0.0;
        for (size_t i=0; i<step.size(); ++i)
                current += step[i];
        return current;
}
                                          

/*esc_CRDwing_1side fundamental escape probability radiative transfer routine, for complete redistribution */
double esc_CRDwing_1side(double tau, 
  double a )
{
        DEBUG_ENTRY( "esc_CRDwing_1side()" );

        /* this is one of the three fundamental escape probability routines
         * the three are esc_CRDwing_1side, esc_PRD_1side, and RTesc_lya
         * it computes esc prob for complete redistribution with wings
         * computes escape prob for complete redistribution in one direction
         * */

        /* this is the only case that this routine computes,
         * and is the usual case for subordinate lines, 
         * complete redistribution with damping wings */

        if (0)
        {
                // try to compare the formulae from this function with A&L
                // exact expression
                a = 1000.;
                double taustep = 2., taumin=1e-8,taumax=1e14;
                Integrator<k2DampArg,Gaussian32> IntDamp;
                for (tau = taumin; tau < taumax; tau *= taustep)
                {
                        double esccom_v = esca0k2(tau);
                        double sqrta = sqrt(a);
                        double pwing = tau > 0.0 ? sqrta/(sqrta+0.5*3.0*sqrt(SQRTPI*tau)) : 
                                1.0;
                        double esctot = esccom_v*(1.0-pwing)+pwing;
                        double intgral = IntDamp.sum(0.,1.,k2DampArg(a,SQRTPI*tau));
                        double intgralt = trapezium(0.,1.,k2DampArg(a,SQRTPI*tau));
                        fprintf(ioQQQ,"cfesc %15.8g %15.8g %15.8g %15.8g %15.8g %15.8g\n",
                                          tau,a,esccom_v,esctot,2.0*intgral,2.0*intgralt);
                }
                exit(0);
        }
        double esccom_v = esca0k2(tau);

        // Escape probability correction for finite damping
        // Results agree to +/- 20% from a=1e-3->1e3, no change for a->0

        double sqrta = sqrt(a);
        double scal = a*(1.0+a+tau)/(POW2(1.0+a)+a*tau);
        double pwing = scal*((tau > 0.0) ? sqrta/sqrt(a+2.25*SQRTPI*tau) : 1.0);
        return esccom_v*(1.0-pwing)+pwing;
}

/*RTesc_lya escape prob for hydrogen atom Lya, using 
 >>refer        La      escp    Hummer, D.G., & Kunasz, P.B., 1980, ApJ, 236, 609
 * called by hydropesc, return value is escape probability */
double RTesc_lya(
        /* the inward escape probability */
        double *esin, 
        /* the destruction probility */
        double *dest, 
        /* abundance of the species */
        double abund, 
        const TransitionProxy& t,
        realnum DopplerWidth)
{
        double beta, 
          conopc, 
          escla_v;
         realnum dstin, 
          dstout;

        DEBUG_ENTRY( "RTesc_lya()" );

        /* 
         * this is one of the three fundamental escape probability functions
         * the three are esc_CRDwing_1side, esc_PRD_1side, and RTesc_lya
         * evaluate esc prob for LA
         * optical depth in outer direction always defined
         */

        if( t.Emis().TauTot() - t.Emis().TauIn() < 0. )
        {
                /* this is the case if we overrun the optical depth scale
                 * just leave things as they are */
                escla_v = t.Emis().Pesc();
                rt.fracin = t.Emis().FracInwd();
                *esin = rt.fracin;
                *dest = t.Emis().Pdest();
                return escla_v;
        }

        /* incomplete redistribution */
        conopc = opac.opacity_abs[ t.ipCont()-1 ];
        if( abund > 0. )
        {
                /* the continuous opacity is positive, we have a valid soln */
                beta = conopc/(abund/SQRTPI*t.Emis().opacity()/
                        DopplerWidth + conopc);
        }
        else
        {
                /* abundance is zero, set miniumum dest prob */
                beta = 1e-10;
        }

        /* find rt.wayin, the escape prob in inward direction */
        RTesc_lya_1side(
                t.Emis().TauIn(),
                beta,
                &rt.wayin,
                &dstin, 
                /* position of line in energy array on C scale */
                t.ipCont()-1);

        ASSERT( (rt.wayin <= 1.) && (rt.wayin >= 0.) && (dstin <= 1.) && (dstin >= 0.) );

        /* find rt.wayout, the escape prob in outward direction */
        RTesc_lya_1side(MAX2(t.Emis().TauTot()/100.,
                t.Emis().TauTot()-t.Emis().TauIn()),
                beta,
                &rt.wayout,
                &dstout, 
                t.ipCont()-1);

        ASSERT( (rt.wayout <= 1.) && (rt.wayout >= 0.) && (dstout <= 1.) && (dstout >= 0.) );

        /* esc prob is mean of in and out */
        escla_v = (rt.wayin + rt.wayout)/2.;
        /* the inward escaping part of the line */
        *esin = rt.wayin;

        /* dest prob is mean of in and out */
        *dest = (dstin + dstout)/2.f;
        /* >>chng 02 oct 02, sum of escape and dest prob must be less then unity,
         * for very thin models this forces dest prob to go to zero, 
         * rather than the value of DEST0, caught by Jon Slavin */
        *dest = (realnum)MIN2( *dest , 1.-escla_v );
        /* but dest prob can't be negative */
        *dest = (realnum)MAX2(0., *dest );

        /* fraction of line emitted in inward direction */
        rt.fracin = rt.wayin/(rt.wayin + rt.wayout);
        ASSERT( escla_v >=0. && *dest>=0. && *esin>=0. );
        return escla_v;
}

/*esc_PRD escape probability radiative transfer for incomplete redistribution */
double esc_PRD(double tau, 
  double tau_out, 
  double damp )
{
        double escgrd_v, 
          tt;

        DEBUG_ENTRY( "esc_PRD()" );

        ASSERT( damp > 0. );

        /* find escape prob for incomp redis, average of two 1-sided probs*/

        if( iteration > 1 )
        {
                tt = tau_from_here(tau_out, tau);

                rt.wayin = (realnum)esc_PRD_1side(tau,damp);
                rt.wayout = (realnum)esc_PRD_1side(tt,damp);
                rt.fracin = rt.wayin/(rt.wayin + rt.wayout);
                escgrd_v = 0.5*(rt.wayin + rt.wayout);
        }
        else
        {
                /*  outward optical depth not defined, dont estimate fraction out */
                rt.fracin = 0.;
                rt.wayout = 1.;
                escgrd_v = esc_PRD_1side(tau,damp);
                rt.wayin = (realnum)escgrd_v;
        }

        ASSERT( escgrd_v > 0. );
        return escgrd_v;
}

/*esc_CRDwing escape probability radiative transfer for CRDS in core only */
double esc_CRDwing(double tau_in, 
  double tau_out, 
  double damp)
{
        double escgrd_v, 
          tt;

        DEBUG_ENTRY( "esc_CRDwing()" );

        /* find escape prob for CRD with damping wings, average of two 1-sided probs*/

        /* crd with wings */
        if( iteration > 1 )
        {
                /*  outward optical depth if defined */
                /* >>chng 03 jun 07, add test for masers here */
                if( tau_out <0 || tau_in < 0. )
                {
                        /* we have a maser, use smallest optical depth to damp it out */
                        tt = MIN2( tau_out , tau_in );
                        tau_in = tt;
                }
                else
                {
                        tt = tau_from_here(tau_out, tau_in);
                }

                rt.wayin = (realnum)esc_CRDwing_1side(tau_in,damp);
                rt.wayout = (realnum)esc_CRDwing_1side(tt,damp);
                rt.fracin = rt.wayin/(rt.wayin + rt.wayout);
                escgrd_v = 0.5*(rt.wayin + rt.wayout);
        }
        else
        {
                /*  outward optical depth not defined, dont estimate fraction out */
                rt.fracin = 0.;
                rt.wayout = 1.;
                escgrd_v = esc_CRDwing_1side(tau_in,damp);
                rt.wayin = (realnum)escgrd_v;
        }

        ASSERT( escgrd_v > 0. );
        return escgrd_v;
}

/*esc_CRDwing escape probability radiative transfer for incomplete redistribution */
double esc_CRDcore(double tau_in, 
  double tau_out)
{
        double escgrd_v, 
          tt;

        DEBUG_ENTRY( "esc_CRDcore()" );

        /* find escape prob for CRD with damping wings, average of two 1-sided probs*/

        /* crd with wings */
        if( iteration > 1 )
        {
                /*  outward optical depth if defined */
                /* >>chng 03 jun 07, add test for masers here */
                if( tau_out <0 || tau_in < 0. )
                {
                        /* we have a maser, use smallest optical depth to damp it out */
                        tt = MIN2( tau_out , tau_in );
                        tau_in = tt;
                }
                else
                {
                        tt = tau_from_here(tau_out, tau_in);
                }

                rt.wayin = (realnum)esca0k2(tau_in);
                rt.wayout = (realnum)esca0k2(tt);
                rt.fracin = rt.wayin/(rt.wayin + rt.wayout);
                escgrd_v = 0.5*(rt.wayin + rt.wayout);
        }
        else
        {
                /*  outward optical depth not defined, dont estimate fraction out */
                rt.fracin = 0.;
                rt.wayout = 1.;
                escgrd_v = esca0k2(tau_in);
                rt.wayin = (realnum)escgrd_v;
        }

        ASSERT( escgrd_v > 0. );
        return escgrd_v;
}

/*esca0k2 derive Hummer's K2 escape probability for Doppler core only */
double esca0k2(double taume)
{
        double arg, 
          esca0k2_v, 
          suma, 
          sumb, 
          sumc, 
          sumd, 
          tau;
        static const double a[5]={1.00,-0.1117897,-0.1249099917,-9.136358767e-3,
          -3.370280896e-4};
        static const double b[6]={1.00,0.1566124168,9.013261660e-3,1.908481163e-4,
          -1.547417750e-7,-6.657439727e-9};
        static const double c[5]={1.000,19.15049608,100.7986843,129.5307533,-31.43372468};
        static const double d[6]={1.00,19.68910391,110.2576321,169.4911399,-16.69969409,
          -36.664480000};

        DEBUG_ENTRY( "esca0k2()" );

        /* compute Hummer's K2 escape probability function for a=0
         * using approx from 
         * >>refer      line    escp    Hummer, D.G., xxxx, JQRST, 26, 187.
         *
         * convert to David's opacity */
        tau = taume*SQRTPI;

        if( tau < 0. )
        {
                /* the line mased */
                esca0k2_v = escmase(taume);

        }
        else if( tau < 0.01 )
        {
                esca0k2_v = 1. - 2.*tau;

        }
        else if( tau <= 11. )
        {
                suma = a[0] + tau*(a[1] + tau*(a[2] + tau*(a[3] + a[4]*tau)));
                sumb = b[0] + tau*(b[1] + tau*(b[2] + tau*(b[3] + tau*(b[4] + 
                  b[5]*tau))));
                esca0k2_v = tau/2.5066283*log(tau/SQRTPI) + suma/sumb;

        }
        else
        {
                /* large optical depth limit */
                arg = 1./log(tau/SQRTPI);
                sumc = c[0] + arg*(c[1] + arg*(c[2] + arg*(c[3] + c[4]*arg)));
                sumd = d[0] + arg*(d[1] + arg*(d[2] + arg*(d[3] + arg*(d[4] + 
                  d[5]*arg))));
                esca0k2_v = (sumc/sumd)/(2.*tau*sqrt(log(tau/SQRTPI)));
        }
        return esca0k2_v;
}

/*escmase escape probability for negative (masing) optical depths */
STATIC void FindNeg( void )
{
        long int i;

        DEBUG_ENTRY( "FindNeg()" );

        /* do the level 1 lines */
        for( i=1; i <= nLevel1; i++ )
        {
                /* check if a line was a strong maser */
                if( TauLines[i].Emis().TauIn() < -1. )
                        DumpLine(TauLines[i]);
        }

        /* Generic atoms & molecules from databases 
         * added by Humeshkar Nemala*/
        for (int ipSpecies=0; ipSpecies < nSpecies; ++ipSpecies)
        {
                for( EmissionList::iterator em=dBaseTrans[ipSpecies].Emis().begin();
                          em != dBaseTrans[ipSpecies].Emis().end(); ++em)
                {
                        if((*em).TauIn() < -1. )
                                DumpLine((*em).Tran());
                }
        }

        /* now do the level 2 lines */
        for( i=0; i < nWindLine; i++ )
        {
                if( (*TauLine2[i].Hi()).IonStg() < (*TauLine2[i].Hi()).nelem()+1-NISO )
                {
                        /* check if a line was a strong maser */
                        if( TauLine2[i].Emis().TauIn() < -1. )
                                DumpLine(TauLine2[i]);
                }
        }

        /* now do the hyperfine structure lines */
        for( i=0; i < nHFLines; i++ )
        {
                /* check if a line was a strong maser */
                if( HFLines[i].Emis().TauIn() < -1. )
                        DumpLine(HFLines[i]);
        }

        return;
}

STATIC double escmase(double tau)
{
        double escmase_v;

        DEBUG_ENTRY( "escmase()" );

        /* this is the only routine that computes maser escape probabilities */
        ASSERT( tau <= 0. );

        if( tau > -0.1 )
        {
                escmase_v = 1. - tau*(0.5 + tau/6.);
        }
        else if( tau > -30. )
        {
                escmase_v = (1. - exp(-tau))/tau;
        }
        else
        {
                fprintf( ioQQQ, " DISASTER escmase called with 2big tau%10.2e\n", 
                  tau  );
                fprintf( ioQQQ, " This is zone number%4ld\n", nzone );
                FindNeg();
                ShowMe();
                cdEXIT(EXIT_FAILURE);
        }

        ASSERT( escmase_v >= 1. );
        return escmase_v;
}

/*esccon continuum escape probability */
double esccon(double tau, 
              double hnukt)
{
        double dinc, 
          escpcn_v, 
          sumesc, 
          sumrec;

        DEBUG_ENTRY( "esccon()" );

        /* computes continuum escape probabilities */
        if( tau < 0.01 )
        {
                escpcn_v = 1.;
                return escpcn_v;
        }

        else if( hnukt > 1. && tau > 100. )
        {
                escpcn_v = 1e-20;
                return escpcn_v;
        }

        my_Integrand_conrec func_conrec;
        func_conrec.chnukt_ContTkt = hnukt;
        Integrator<my_Integrand_conrec,Gaussian32> conrec;

        my_Integrand_escConE2 func_escConE2;
        func_escConE2.chnukt_ContTkt = hnukt;
        func_escConE2.chnukt_ctau = tau;
        Integrator<my_Integrand_escConE2,Gaussian32> escConE2;

        dinc = 10./hnukt;
        sumrec = conrec.sum(1.,1.+dinc,func_conrec);
        sumesc = escConE2.sum(1.,1.+dinc,func_escConE2);

        if( sumrec > 0. )
        {
                escpcn_v = sumesc/sumrec;
        }
        else
        {
                escpcn_v = 0.;
        }
        return escpcn_v;
}

/*RTesc_lya_1side fit Hummer and Kunasz escape probability for hydrogen atom Lya */
STATIC void RTesc_lya_1side(double taume, 
  double beta, 
  realnum *esc, 
  realnum *dest,
  /* position of line in frequency array on c scale */
  long ipLine )
{
        double esc0, 
          fac, 
          fac1, 
          fac2, 
          tau, 
          taucon, 
          taulog;

        /* DEST0 is the smallest destruction probability to return
         * in high metallicity models, in rt.h
        const double DEST0=1e-8;*/

        DEBUG_ENTRY( "RTesc_lya_1side()" );

        /* fits to numerical results of Hummer and Kunasz Ap.J. 80 */
        tau = taume*SQRTPI;

        /* this is the real escape probability */
        esc0 = 1./((0.6451 + tau)*(0.47 + 1.08/(1. + 7.3e-6*tau)));

        esc0 = MAX2(0.,esc0);
        esc0 = MIN2(1.,esc0);

        if( tau > 0. )
        {
                taulog = log10(MIN2(1e8,tau));
        }
        else
        {
                /* the line mased 
                 *>>chng 06 sep 08, kill xLaMase 
                hydro.xLaMase = MIN2(hydro.xLaMase,(realnum)tau);*/
                taulog = 0.;
                *dest = 0.;
                *esc = (realnum)esc0;
        }

        if( beta > 0. )
        {
                taucon = MIN2(2.,beta*tau);

                if( taucon > 1e-3 )
                {
                        fac1 = -1.25 + 0.475*taulog;
                        fac2 = -0.485 + 0.1615*taulog;
                        fac = -fac1*taucon + fac2*POW2(taucon);
                        fac = pow(10.,fac);
                        fac = MIN2(1.,fac);
                }
                else
                {
                        fac = 1.;
                }

                *esc = (realnum)(esc0*fac);
                /* MIN puts cat at 50 */
                *dest = (realnum)(beta/(0.30972 - MIN2(.28972,0.03541667*taulog)));
        }

        else
        {
                *dest = 0.;
                *esc = (realnum)esc0;
        }

        *dest = MIN2(*dest,1.f-*esc);
        *dest = MAX2(0.f,*dest);

        /* >>chng 99 apr 12, limit destruction prob in case where gas dominated by scattering.
         * in this case scattering is much more likely than absorption on this event */
        *dest = (realnum)( (1. - opac.albedo[ipLine]) * *dest + opac.albedo[ipLine]*DEST0);
        /* this is for debugging H Lya */
        {
                /*@-redef@*/
                enum {BUG=false};
                /*@+redef@*/
                if( BUG )
                {
                        fprintf(ioQQQ,"scatdest tau %.2e beta%.2e 1-al%.2e al%.2e dest%.2e \n",
                        taume,
                        beta, 
                        (1. - opac.albedo[ipLine]), 
                        opac.albedo[ipLine] ,
                        *dest 
                        );
                }
        }
        return;
}

/*RT_DestProb returns line destruction probability due to continuum opacity */
double RT_DestProb(
          /* abundance of species */
          double abund, 
          /* its line absorption cross section */
          double crsec, 
          /* pointer to energy within continuum array, to get background opacity,
           * this is on the f not c scale */
          long int ipanu, 
          /* line width */
          double widl, 
          /* escape probability */
          double escp, 
          /* type of redistribution function */
          int nCore)
{
        /* this will be the value we shall return */
        double eovrlp_v;

        double conopc, 
          beta;

        /* DEST0 is the smallest destruction probability to return
         * in high metallicity models 
         * this was set to 1e-8 until 99nov18,
         * in cooling flow model the actual Lya ots dest prob was 1e-16,
         * and this lower limit of 1e-8 caused energy balance problems,
         * since dest prob was 8 orders of magnitude too great.  
         * >>chng 99 nov 18, to 1e-20, but beware that comments indicate that
         * this will cause problems with high metallicity clouds(?) */
        /* >>chng 00 jun 04, to 0 since very feeble ionization clouds, with almost zero opacity,
         * this was a LARGE number */
        /*const double DEST0=1e-20;
        const double DEST0=0.;*/

        DEBUG_ENTRY( "RT_DestProb()" );

        /* computes "escape probability" due to continuum destruction of
         *
         * if esc prob gt 1 then line is masing - return small number for dest prob */
        /* >>>chng 99 apr 10, return min dest when scattering greater than abs */
        /* no idea of opacity whatsoever, on very first soln for this model */
        /* >>chng 05 mar 20, add test on line being above upper bound of frequency 
         * do not want to evaluate opacity in this case since off scale */
        if( escp >= 1.0 || !conv.nTotalIoniz || ipanu >= rfield.nflux )
        {
                eovrlp_v = 0.;
                return eovrlp_v;
        }

        /* find continuum opacity */
        conopc = opac.opacity_abs[ipanu-1];

        ASSERT( crsec > 0. );

        /* may be no population, cannot use above test since return 0 not DEST0 */
        if( abund <= 0. || conopc <= 0. )
        {
                /* do not set this to DEST0 since energy not then conserved */
                eovrlp_v = 0.;
                return eovrlp_v;
        }

        /* fac of 1.7 convert to Hummer convention for line opacity */
        beta = conopc/(abund*SQRTPI*crsec/widl + conopc);
        /* >>chng 04 may 10, rm * 1-pesc)
        beta = MIN2(beta,(1.-escp)); */

        if( nCore == ipDEST_INCOM )
        {
                /*  fits to 
                 *  >>>refer    la      esc     Hummer and Kunasz 1980 Ap.J. 236,609.
                 *  the max value of 1e-3 is so that we do not go too far
                 *  beyond what Hummer and Kunasz did, discussed in
                 * >>refer      rt      esc proc        Ferland, G.J., 1999, ApJ, 512, 247 */
                eovrlp_v = MIN2(1e-3,8.5*beta);
        }
        else if( nCore == ipDEST_K2 )
        {
                /*  Doppler core only; a=0., Hummer 68 
                eovrlp_v = RT_DestHummer(beta);*/
                eovrlp_v = MIN2(1e-3,8.5*beta);
        }
        else if( nCore == ipDEST_SIMPL )
        {
                /*  this for debugging only 
                eovrlp_v = 8.5*beta;*/
                /* >>chng 04 may 13, use same min function */
                eovrlp_v = MIN2(1e-3,8.5*beta);
        }
        else
        {
                fprintf( ioQQQ, " chCore of %i not understood by RT_DestProb.\n", 
                  nCore );
                cdEXIT(EXIT_FAILURE);
        }

        /* renorm to unity */
        eovrlp_v /= 1. + eovrlp_v;

        /* multiply by 1-escape prob, since no destruction when optically thin */
        eovrlp_v *= 1. - escp;

        /*check results in bounds */
        ASSERT( eovrlp_v >= 0.  );
        ASSERT( eovrlp_v <= 1.  );

        {
                /* debugging code for Lya problems */
                /*@-redef@*/
                enum {DEBUG_LOC=false};
                /*@+redef@*/
                if( DEBUG_LOC )
                {
                        if( rfield.anu[ipanu-1]>0.73 && rfield.anu[ipanu-1]<0.76 &&
                            fp_equal( abund, iso_sp[ipH_LIKE][ipHYDROGEN].trans(ipH2p,ipH1s).Emis().PopOpc() ) )
                        {
                                fprintf(ioQQQ,"%li RT_DestProb\t%g\n",
                                        nzone, eovrlp_v  );
                        }
                }
        }

        /* >>chng 04 may 10, rm min */
        /* this hack removed since no fundamental reason for it to be here,
         * this should be added to scattering escape, if included at all */
#       if 0
        /* >>chng 99 apr 12, limit destruction prob in case where gas dominated by scattering.
         * in this case scattering is much more likely than absorption on this event
        eovrlp_v = (1. - opac.albedo[ipanu-1]) * eovrlp_v + 
                opac.albedo[ipanu-1]*DEST0; */
        /* >>chng 01 aug 11, add factor of 3 for increase in mean free path, and min on 0 */
        /*eovrlp_v = MAX2(DEST0,1. - 3.*opac.albedo[ipanu-1]) * eovrlp_v + 
                opac.albedo[ipanu-1]*DEST0;*/
        eovrlp_v = POW2(1. - opac.albedo[ipanu-1]) * eovrlp_v + 
                opac.albedo[ipanu-1]*0.;
#       endif

        return eovrlp_v;
}

/*RT_LineWidth compute line width (cm/sec), using optical depth array information 
 * this is where effects of wind are done */
double RT_LineWidth(const TransitionProxy& t, realnum DopplerWidth)
{
        double RT_LineWidth_v, 
          aa, 
          atau, 
          b, 
          r, 
          vth;
        realnum tau; 

        DEBUG_ENTRY( "RT_LineWidth()" );

        /* uses line width from 
         * >>refer      esc     prob    Bonilha et al. Ap.J. (1979) 233 649
         * return value is half velocity width*(1-ESC PROB) [cm s-1]
         * this assumes incomplete redistribution, damp.tau^1/3 width */

        /* thermal width */
        vth = DopplerWidth;

        /* optical depth in outer direction is defined
         * on second and later iterations. 
         * smaller of inner and outer optical depths is chosen for esc prob */
        if( iteration > 1 )
        {
                /* optical depth to shielded face */
                realnum tauout = t.Emis().TauTot() - t.Emis().TauIn();

                /* >>chng 99 apr 22 use smaller optical depth */
                tau = MIN2( t.Emis().TauIn() , tauout );
        }
        else
        {
                tau = t.Emis().TauIn();
        }
        /* do not evaluate line width if quite optically thin - will be dominated
         * by noise in this case */
        if( tau <1e-3 )
                return 0;

        t.Emis().damp() = t.Emis().dampXvel() / DopplerWidth;
        ASSERT( t.Emis().damp() > 0. );

        double Pesc =  esc_PRD_1side( tau , t.Emis().damp());

        /* max optical depth is thermalization length */
        realnum therm = (realnum)(5.3e16/MAX2(1e-15,dense.eden));
        if( tau > therm )
        {
                /* \todo 2 this seems to create an inconsistency as it changes tau
                 * for the purposes of this routine (to return the line-width),
                 * but this leaves the actual optical depth unchanged. */
                pressure.lgPradDen = true;
                tau = therm;
        }

        /* >>chng 01 jun 23, use wind vel instead of rt since rt deleted */
        /* >>chng 04 may 13, use thermal for subsonic cases */
        if( ! wind.lgBallistic() )
        {
                /* static geometry */
                /* esc prob has noise if smaller than FLT_EPSILON, or is masing */
                if( (tau-opac.taumin)/100. < FLT_EPSILON )
                {
                        RT_LineWidth_v = 0.;
                }
                else if( tau <= 20. )
                {
                        atau = -6.907755;
                        if( tau > 1e-3 )
                                atau = log(tau);
                        aa = 4.8 + 5.2*tau + (4.*tau - 1.)*atau;
                        b = 6.5*tau - atau;
                        double escProb = Pesc + t.Emis().Pelec_esc() + t.Emis().Pdest();
                        RT_LineWidth_v = vth*0.8862*aa/b*(1. - MIN2( 1., escProb ) ); 
                        /* small number roundoff can dominate this process */
                        if( escProb >= 1. - 100. * FLT_EPSILON )
                                RT_LineWidth_v = 0.;
                }
                else
                {
                        ASSERT( t.Emis().damp()*tau >= 0.);
                        atau = log(MAX2(0.0001,tau));
                        aa = 1. + 2.*atau/pow(1. + 0.3*t.Emis().damp()*tau,0.6667) + pow(6.5*
                          t.Emis().damp()*tau,0.333);
                        b = 1.6 + 1.5/(1. + 0.20*t.Emis().damp()*tau);
                        RT_LineWidth_v = vth*0.8862*aa/b*(1. - MIN2( 1. , 
                                (Pesc+ t.Emis().Pelec_esc() + t.Emis().Pdest())) );
                }

                /* we want full width, not half width */
                RT_LineWidth_v *= 2.;

        }
        else
        {
                /* ballistic wind */
                r = t.Emis().damp()*tau/PI;
                if( r <= 1. )
                {
                        RT_LineWidth_v = vth*sqrt(log(MAX2(1.,tau))*.2821);
                }
                else
                {
                        RT_LineWidth_v = 2.*fabs(wind.windv0);
                        if( r*vth <= RT_LineWidth_v )
                        {
                                RT_LineWidth_v = vth*r*log(RT_LineWidth_v/(r*vth));
                        }
                }
        }

        ASSERT( RT_LineWidth_v >= 0. );
        return RT_LineWidth_v;
}

/*RT_DestHummer evaluate Hummer's betaF(beta) function */
double RT_DestHummer(double beta) /* beta is ratio of continuum to mean line opacity,
                                                                         * returns dest prob = beta F(beta) */
{
        double fhummr_v, 
          x;

        DEBUG_ENTRY( "RT_DestHummer()" );

        /* evaluates Hummer's F(beta) function for case where damping
         * constant is zero, are returns beta*F(beta)
         * fit to Table 1, page 80, of Hummer MNRAS 138, 73-108.
         * beta is ratio of continuum to line opacity; FUMMER is
         * product of his F() times beta; the total destruction prob
         * this beta is Hummer's normalization of the Voigt function */

        ASSERT( beta >= 0.);/* non-positive is unphysical */
        if( beta <= 0. )
        {
                fhummr_v = 0.;
        }
        else
        {
                x = log10(beta);
                if( x < -5.5 )
                {
                        fhummr_v = 3.8363 - 0.56329*x;
                }
                else if( x < -3.5 )
                {
                        fhummr_v = 2.79153 - 0.75325*x;
                }
                else if( x < -2. )
                {
                        fhummr_v = 1.8446 - 1.0238*x;
                }
                else
                {
                        fhummr_v = 0.72500 - 1.5836*x;
                }
                fhummr_v *= beta;
        }
        return fhummr_v;
}

---