SUBROUTINE RATES1(IMOR) C ====================== C C Evaluation of radiative rates C C Output (transferred by COMMON blocks): C RRU(IT,ID) - upward radiative rate in transition IT and C depth ID C RRD(IT,ID) - analogously the downward rate; more precisely C the exact downward rate is given by: C lines : RRD * stat.weight(lower)/stat.weight(upper) C continua: RRD * n(elec) * Saha-Boltzmann factor C INCLUDE 'IMPLIC.FOR' INCLUDE 'BASICS.FOR' INCLUDE 'ATOMIC.FOR' INCLUDE 'MODELQ.FOR' INCLUDE 'ODFPAR.FOR' INCLUDE 'ALIPAR.FOR' INCLUDE 'ITERAT.FOR' DIMENSION RBNE(MDEPTH) C DIMENSION EHKL(MFREQL) C C zero the rates C DO ID=1,ND PRADT(ID)=0. PRADA(ID)=0. FLRD(ID)=0. DO ITR=1,NTRANS RRU(ITR,ID)=0. RRD(ITR,ID)=0. END DO DO ITRP=1,NTRPRD PJBAR(ITRP,ID)=0. END DO END DO PRD0=0. C LROSS=NDRE.LE.0.AND.ITER.EQ.1.OR.LFIN IF(HMIX0.GT.0.) LROSS=.TRUE. IF(LROSS) THEN DO ID=1,ND ABROSD(ID)=0. SUMDPL(ID)=0. END DO END IF C DO 100 IJ=1,NFREQ IF(IJX(IJ).EQ.-1) GOTO 100 FR=FREQ(IJ) W0=W0E(IJ) WW=W(IJ) CALL OPACF1(IJ) IF(IMOR.EQ.0) THEN CALL RTEFR1(IJ) ELSE RAD1(ID)=RAD(IJ,ID) END IF IF(LROSS) CALL ROSSTD(IJ) FLRD(1)=FLRD(1)+WW*FH(IJ)*RAD1(1)-WW*HEXTRD(IJ) DO ID=2,ND DT=UN/(ABSOT(ID)+ABSOT(ID-1))/DELDMZ(ID-1) FL=(RAD1(ID)*FAK1(ID)-RAD1(ID-1)*FAK1(ID-1))*DT FLRD(ID)=FLRD(ID)+WW*FL END DO if(ioptab.lt.0) go to 100 C C --------------------- C Continuum transitions C --------------------- C DO ID=1,ND RBNE(ID)=(RAD1(ID)+BNUE(IJ))*EXP(-HKT1(ID)*FR) DO 10 IBFT=1,NTRANC ITR=ITRBF(IBFT) SG=CROSS(IBFT,IJ) IF(SG.LE.0.) GO TO 10 II=ILOW(ITR) JJ=IUP(ITR) IF(IPZERO(II,ID).NE.0.OR.IPZERO(JJ,ID).NE.0) GO TO 10 JC=ITRA(JJ,II) IF(IFWOP(II).GE.0) THEN ICDW=MCDW(ITR) IF(ICDW.GE.1) SG=SG*DWF1(ICDW,ID) ELSE IMER=IMRG(II) SG=SGMG(IMER,ID) ENDIF SGW0=SG*W0 RRU(ITR,ID)=RRU(ITR,ID)+SGW0*RAD1(ID) RRD(ITR,ID)=RRD(ITR,ID)+SGW0*RBNE(ID) 10 CONTINUE END DO C C ---------------- C Line transitions C ---------------- C IF(IJLIN(IJ).GT.0) THEN C C the "primary" line at the given frequency C ITR=IJLIN(IJ) II=ILOW(ITR) JJ=IUP(ITR) DO 50 ID=1,ND IF(IPZERO(II,ID).NE.0.OR.IPZERO(JJ,ID).NE.0) GO TO 50 SGW=PRFLIN(ID,IJ)*W0 RRU(ITR,ID)=RRU(ITR,ID)+SGW*RAD1(ID) RRD(ITR,ID)=RRD(ITR,ID)+SGW*RBNE(ID) 50 CONTINUE c itrprd=iprd(itr) if(itrprd.gt.0) then s=un/(0.02654*osc0(itr)) do id=1,nd sg=prflin(id,ij)*s pjbar(itrprd,id)=pjbar(itrprd,id)+sg*w(ij)*rad1(id) end do end if c ENDIF IF(NLINES(IJ).LE.0) GO TO 100 C C the "overlapping" lines at the given frequency C DO 90 ILINT=1,NLINES(IJ) ITR=ITRLIN(ILINT,IJ) if(linexp(itr)) goto 90 IJ0=IFR0(ITR) II=ILOW(ITR) JJ=IUP(ITR) DO IJT=IJ0,IFR1(ITR) IF(FREQ(IJT).LE.FR) THEN IJ0=IJT GO TO 70 END IF END DO 70 IJ1=IJ0-1 A1=(FR-FREQ(IJ0))/(FREQ(IJ1)-FREQ(IJ0))*W0 A2=W0-A1 DO 80 ID=1,ND IF(IPZERO(II,ID).NE.0.OR.IPZERO(JJ,ID).NE.0) GO TO 80 SGW=A1*PRFLIN(ID,IJ1)+A2*PRFLIN(ID,IJ0) RRU(ITR,ID)=RRU(ITR,ID)+SGW*RAD1(ID) RRD(ITR,ID)=RRD(ITR,ID)+SGW*RBNE(ID) 80 CONTINUE c itrprd=iprd(itr) if(itrprd.gt.0) then s=un/(0.02654*osc0(itr)) do id=1,nd SG=(A1*PRFLIN(ID,IJ1)+A2*PRFLIN(ID,IJ0))*s pjbar(itrprd,id)=pjbar(itrprd,id)+sg*w(ij)*rad1(id) end do end if c 90 CONTINUE 100 CONTINUE C DO ID=1,ND IF(CRSW(ID).NE.UN) THEN DO ITR=1,NTRANS RRU(ITR,ID)=RRU(ITR,ID)*CRSW(ID) RRD(ITR,ID)=RRD(ITR,ID)*CRSW(ID) END DO END IF END DO C C radiation pressure C DO ID=1,ND PRADT(ID)=PRADT(ID)*PCK PRADA(ID)=PRADA(ID)*PCK END DO PRD0=PRD0/DENS1(1)*DM(1)*PCK C C Rosseland mean opacity C IF(LROSS) THEN DO ID=1,ND ABROSD(ID)=SUMDPL(ID)/(ABROSD(ID)*DENS(ID)) END DO END IF c RETURN END