c*********************************************************************** c mztf.f c*********************************************************************** subroutine mztud ( ig,cf,cfup,cfdw,vc,taugr, ib,isot, @ iirw,iimu,itauout,icfout,itableout ) c program for calculating atmospheric transmittances c to be used in the calculation of curtis matrix coefficients c i*out = 1 output of data c i*out = 0 no output c itableout = 30 output de toda la C.M. y el VC y las poblaciones de los c estados 626(020), esta opcion nueva se aƱade porque c itableout=1 saca o bien solamente de 5 en 5 capas c o bien los elementos de C.M. desde una cierta capa c (consultese elimin_mz1d.f que es quien lo hace); lo c de las poblaciones (020) lo hace mztf_correcion.f c jul 2011 malv+fgg Adapted to LMD-MGCM c jan 07 malv Add new vertical fine grid zy, similar to zx c sep-oct 01 malv update for fluxes for hb and fb, adapt to Linux c nov 98 mavl allow for overlaping in the lorentz line c jan 98 malv version for mz1d. based on curtis/mztf.for c 17-jul-96 mlp&crs change the calculation of mr. c evitar: divide por cero. anhadiendo: ff c oct-92 malv correct s(t) dependence for all histogr bands c june-92 malv proper lower levels for laser bands c may-92 malv new temperature dependence for laser bands c @ 991 malv boxing for the averaged absorber amount and t c ? malv extension up to 200 km altitude in mars c 13-nov-86 mlp include the temperature weighted to match c the eqw in the strong doppler limit. c*********************************************************************** implicit none include 'nltedefs.h' include 'nlte_atm.h' include 'nlte_data.h' include 'nlte_curtis.h' include 'tcr_15um.h' include 'nlte_results.h' c arguments integer ig !ADDED FOR TRACEBACK real*8 cf(nl,nl), cfup(nl,nl), cfdw(nl,nl) ! o real*8 vc(nl), taugr(nl) ! o integer ib ! i integer isot ! i integer iirw ! i integer iimu ! i integer itauout ! i integer icfout ! i integer itableout ! i c local variables and constants integer i, in, ir, im, k,j integer nmu parameter (nmu = 8) real*8 tau(nl,nl) real*8 tauinf(nl) real*8 con(nzy), coninf real*8 c1, c2 real*8 t1, t2 real*8 p1, p2 real*8 mr1, mr2 real*8 st1, st2 real*8 c1box(70), c2box(70) real*8 ff ! to avoid too small numbers real*8 tvtbs(nzy) real*8 st, beta, ts, eqwmu real*8 mu(nmu), amu(nmu) real*8 zld(nl), zyd(nzy) real*8 correc real deltanux ! width of vib-rot band (cm-1) character isotcode*2 integer idummy real*8 Desp,wsL c formats 111 format(a1) 112 format(a2) 101 format(i1) 202 format(i2) 180 format(a80) 181 format(a80) c*********************************************************************** c some needed values ! rl=sqrt(log(2.d0)) ! pi2 = 3.14159265358989d0 beta = 1.8d0 ! beta = 1.0d0 idummy = 0 Desp = 0.0d0 wsL = 0.0d0 !write (*,*) ' MZTUD/ iirw = ', iirw c esto es para que las subroutines de mztfsub calculen we c de la forma apropiada para mztf, no para fot icls=icls_mztf c codigos para filenames ! if (isot .eq. 1) isotcode = '26' ! if (isot .eq. 2) isotcode = '28' ! if (isot .eq. 3) isotcode = '36' ! if (isot .eq. 4) isotcode = '27' ! if (isot .eq. 5) isotcode = '62' ! if(ib.eq.1.or.ib.eq.2.or.ib.eq.3.or.ib.eq.4.or.ib.eq.5 ! @ .or.ib.eq.6.or.ib.eq.7.or.ib.eq.8.or.ib.eq.9) then ! write (ibcode1,101) ib ! else ! write (ibcode2,202) ib ! endif ! write (*,'( 30h calculating curtis matrix : ,2x, ! @ 8h band = ,i2,2x, 11h isotope = ,i2)') ib, isot c integration in angle !!!!!!!!!!!!!!!!!!!! c------- diffusivity approx. if (iimu.eq.1) then ! write (*,*) ' diffusivity approx. beta = ',beta mu(1) = 1.0d0 amu(1)= 1.0d0 c-------data for 8 points integration elseif (iimu.eq.4) then write (*,*)' 4 points for the gauss-legendre angle quadrature.' mu(1)=(1.0d0+0.339981043584856)/2.0d0 mu(2)=(1.0d0-0.339981043584856)/2.0d0 mu(3)=(1.0d0+0.861136311594053)/2.0d0 mu(4)=(1.0d0-0.861136311594053)/2.0d0 amu(1)=0.652145154862546 amu(2)=amu(1) amu(3)=0.347854845137454 amu(4)=amu(3) beta=1.0d0 c-------data for 8 points integration elseif(iimu.eq.8) then write (*,*)' 8 points for the gauss-legendre angle quadrature.' mu(1)=(1.0d0+0.183434642495650)/2.0d0 mu(2)=(1.0d0-0.183434642495650)/2.0d0 mu(3)=(1.0d0+0.525532409916329)/2.0d0 mu(4)=(1.0d0-0.525532409916329)/2.0d0 mu(5)=(1.0d0+0.796666477413627)/2.0d0 mu(6)=(1.0d0-0.796666477413627)/2.0d0 mu(7)=(1.0d0+0.960289856497536)/2.0d0 mu(8)=(1.0d0-0.960289856497536)/2.0d0 amu(1)=0.362683783378362 amu(2)=amu(1) amu(3)=0.313706645877887 amu(4)=amu(3) amu(5)=0.222381034453374 amu(6)=amu(5) amu(7)=0.101228536290376 amu(8)=amu(7) beta=1.0d0 end if c!!!!!!!!!!!!!!!!!!!!!!! ccc ccc determine abundances included in the absorber amount ccc c first, set up the grid ready for interpolation. do i=1,nzy zyd(i) = dble(zy(i)) enddo do i=1,nl zld(i) = dble(zl(i)) enddo c vibr. temp of the bending mode : if (isot.eq.1) call interdp ( tvtbs,zyd,nzy, v626t1,zld,nl, 1 ) if (isot.eq.2) call interdp ( tvtbs,zyd,nzy, v628t1,zld,nl, 1 ) if (isot.eq.3) call interdp ( tvtbs,zyd,nzy, v636t1,zld,nl, 1 ) if (isot.eq.4) call interdp ( tvtbs,zyd,nzy, v627t1,zld,nl, 1 ) !if (isot.eq.5) call interdp ( tvtbs,zxd,nz, vcot1,zld,nl, 1 ) c 2nd: correccion a la n10(i) (cantidad de absorbente en el lower state) c por similitud a la que se hace en cza.for ; esto solo se hace para CO2 !write (*,*) 'imr(isot) = ', isot, imr(isot) do i=1,nzy if (isot.eq.5) then con(i) = dble( coy(i) * imrco ) else con(i) = dble( co2y(i) * imr(isot) ) correc = 2.d0 * dexp( dble(-ee*elow(isot,2))/tvtbs(i) ) con(i) = con(i) * ( 1.d0 - correc ) ! write (*,*) ' iz, correc, co2y(i), con(i) =', ! @ i,correc,co2y(i),con(i) endif !----------------------------------------------------------------- ! mlp & cristina. 17 july 1996 change the calculation of mr. ! it is used for calculating partial press ! alpha = alpha(self,co2)*pp +alpha(n2)*(pt-pp) ! for an isotope, if mr is obtained by ! co2*imr(iso)/nt ! we are considerin collisions with other co2 isotopes ! (including the major one, 626) as if they were with n2. ! assuming mr as co2/nt, we consider collisions ! of type 628-626 as of 626-626 instead of as 626-n2. ! mrx(i)=con(i)/ntx(i) ! old malv ! mrx(i)= dble(co2x(i)/ntx(i)) ! mlp & crs ! jan 98: ! esta modif de mlp implica anular el correc (deberia revisar esto) mr(i) = dble(co2y(i)/nty(i)) ! malv, jan 98 !----------------------------------------------------------------- end do ! como beta y 1.d5 son comunes a todas las weighted absorber amounts, ! los simplificamos: ! coninf = beta * 1.d5 * dble( con(n) / log( con(n-1) / con(n) ) ) !write (*,*) ' con(nz), con(nz-1) =', con(nz), con(nz-1) coninf = dble( con(nzy) / log( con(nzy-1) / con(nzy) ) ) ! if(ig.eq.1682)write(*,*)'mztud/218',coninf,con(nzy), ! 1 con(nzy-1),log(con(nzy-1)/con(nzy)),co2y(nzy),co2y(nzy-1) !write (*,*) ' coninf =', coninf ccc ccc temp dependence of the band strength and ccc nlte correction factor for the absorber amount ccc call mztf_correccion ( coninf, con, ib, isot, itableout ) ! if(ig.eq.1682)write(*,*)'mztud/227',coninf ccc ccc reads histogrammed spectral data (strength for lte and vmr=1) ccc !hfile1 = dirspec//'hi'//dn !Ya no hacemos distincion d/n en esto ! hfile1 = dirspec//'hid' !(see why in his.for) ! hfile1='hid' !! if (ib.eq.13 .or. ib.eq.14 ) hfile1 = dirspec//'his' ! if (ib.eq.13 .or. ib.eq.14 ) hfile1 = 'his' ! if(ib.eq.1.or.ib.eq.2.or.ib.eq.3.or.ib.eq.4.or.ib.eq.5 ! @ .or.ib.eq.6.or.ib.eq.7.or.ib.eq.8.or.ib.eq.9) then ! if (isot.eq.1) hisfile = hfile1//'26-'//ibcode1//'.dat' ! if (isot.eq.2) hisfile = hfile1//'28-'//ibcode1//'.dat' ! if (isot.eq.3) hisfile = hfile1//'36-'//ibcode1//'.dat' ! if (isot.eq.4) hisfile = hfile1//'27-'//ibcode1//'.dat' ! if (isot.eq.5) hisfile = hfile1//'62-'//ibcode1//'.dat' ! else ! if (isot.eq.1) hisfile = hfile1//'26-'//ibcode2//'.dat' ! if (isot.eq.2) hisfile = hfile1//'28-'//ibcode2//'.dat' ! if (isot.eq.3) hisfile = hfile1//'36-'//ibcode2//'.dat' ! if (isot.eq.4) hisfile = hfile1//'27-'//ibcode2//'.dat' ! if (isot.eq.5) hisfile = hfile1//'62-'//ibcode2//'.dat' ! endif if(ib.eq.1) then if(isot.eq.1) then !Case 1 mm=mm_c1 nbox=nbox_c1 tmin=tmin_c1 tmax=tmax_c1 do i=1,nbox_max no(i)=no_c1(i) dist(i)=dist_c1(i) do j=1,nhist sk1(j,i)=sk1_c1(j,i) xls1(j,i)=xls1_c1(j,i) xln1(j,i)=xln1_c1(j,i) xld1(j,i)=xld1_c1(j,i) enddo enddo do j=1,nhist thist(j)=thist_c1(j) enddo else if(isot.eq.2) then !Case 2 mm=mm_c2 nbox=nbox_c2 tmin=tmin_c2 tmax=tmax_c2 do i=1,nbox_max no(i)=no_c2(i) dist(i)=dist_c2(i) do j=1,nhist sk1(j,i)=sk1_c2(j,i) xls1(j,i)=xls1_c2(j,i) xln1(j,i)=xln1_c2(j,i) xld1(j,i)=xld1_c2(j,i) enddo enddo do j=1,nhist thist(j)=thist_c2(j) enddo else if(isot.eq.3) then !Case 3 mm=mm_c3 nbox=nbox_c3 tmin=tmin_c3 tmax=tmax_c3 do i=1,nbox_max no(i)=no_c3(i) dist(i)=dist_c3(i) do j=1,nhist sk1(j,i)=sk1_c3(j,i) xls1(j,i)=xls1_c3(j,i) xln1(j,i)=xln1_c3(j,i) xld1(j,i)=xld1_c3(j,i) enddo enddo do j=1,nhist thist(j)=thist_c3(j) enddo else if(isot.eq.4) then !Case 4 mm=mm_c4 nbox=nbox_c4 tmin=tmin_c4 tmax=tmax_c4 do i=1,nbox_max no(i)=no_c4(i) dist(i)=dist_c4(i) do j=1,nhist sk1(j,i)=sk1_c4(j,i) xls1(j,i)=xls1_c4(j,i) xln1(j,i)=xln1_c4(j,i) xld1(j,i)=xld1_c4(j,i) enddo enddo do j=1,nhist thist(j)=thist_c4(j) enddo else write(*,*)'isot must be 2,3 or 4 for ib=1!!' write(*,*)'stop at mztud/324' stop endif else if (ib.eq.2) then if(isot.eq.1) then !Case 5 mm=mm_c5 nbox=nbox_c5 tmin=tmin_c5 tmax=tmax_c5 do i=1,nbox_max no(i)=no_c5(i) dist(i)=dist_c5(i) do j=1,nhist sk1(j,i)=sk1_c5(j,i) xls1(j,i)=xls1_c5(j,i) xln1(j,i)=xln1_c5(j,i) xld1(j,i)=xld1_c5(j,i) enddo enddo do j=1,nhist thist(j)=thist_c5(j) enddo else write(*,*)'isot must be 1 for ib=2!!' write(*,*)'stop at mztud/348' stop endif else if (ib.eq.3) then if(isot.eq.1) then !Case 6 mm=mm_c6 nbox=nbox_c6 tmin=tmin_c6 tmax=tmax_c6 do i=1,nbox_max no(i)=no_c6(i) dist(i)=dist_c6(i) do j=1,nhist sk1(j,i)=sk1_c6(j,i) xls1(j,i)=xls1_c6(j,i) xln1(j,i)=xln1_c6(j,i) xld1(j,i)=xld1_c6(j,i) enddo enddo do j=1,nhist thist(j)=thist_c6(j) enddo else write(*,*)'isot must be 1 for ib=3!!' write(*,*)'stop at mztud/372' stop endif else if (ib.eq.4) then if(isot.eq.1) then !Case 7 mm=mm_c7 nbox=nbox_c7 tmin=tmin_c7 tmax=tmax_c7 do i=1,nbox_max no(i)=no_c7(i) dist(i)=dist_c7(i) do j=1,nhist sk1(j,i)=sk1_c7(j,i) xls1(j,i)=xls1_c7(j,i) xln1(j,i)=xln1_c7(j,i) xld1(j,i)=xld1_c7(j,i) enddo enddo do j=1,nhist thist(j)=thist_c7(j) enddo else write(*,*)'isot must be 1 for ib=4!!' write(*,*)'stop at mztud/396' stop endif else write(*,*)'ib must be 1,2,3 or 4!!' write(*,*)'stop at mztud/401' endif ! write (*,*) 'hisfile: ', hisfile ! the argument to rhist is to make this compatible with mztf_comp.f, ! which is a useful modification of mztf.f (to change strengths of bands ! call rhist (1.0) if (isot.ne.5) deltanux = deltanu(isot,ib) if (isot.eq.5) deltanux = deltanuco c****** c****** calculation of tauinf(nl) c****** call initial ff=1.0e10 do i=nl,1,-1 if(i.eq.nl)then call intz (zl(i),c2,p2,mr2,t2, con) do kr=1,nbox ta(kr)=t2 end do ! write (*,*) ' i, t2 =', i, t2 call interstrength (st2,t2,ka,ta) aa = p2 * coninf * mr2 * (st2 * ff) bb = p2 * coninf * st2 cc = coninf * st2 dd = t2 * coninf * st2 do kr=1,nbox ccbox(kr) = coninf * ka(kr) ! if(i.eq.nl.and.ig.eq.1682)write(*,*)'mztud/435', ! 1 ccbox(kr),coninf,ka(kr),kr ddbox(kr) = t2 * ccbox(kr) ! c2box(kr) = c2 * ka(kr) * beta * dble(deltaz) * 1.d5 c2box(kr) = c2 * ka(kr) * dble(deltaz) end do ! c2 = c2 * st2 * beta * dble(deltaz) * 1.d5 c2 = c2 * st2 * dble(deltaz) else call intz (zl(i),c1,p1,mr1,t1, con) do kr=1,nbox ta(kr)=t1 end do ! write (*,*) ' i, t1 =', i, t1 call interstrength (st1,t1,ka,ta) do kr=1,nbox ! c1box(kr) = c1 * ka(kr) * beta * dble(deltaz) * 1.d5 c1box(kr) = c1 * ka(kr) * dble(deltaz) end do ! c1 = c1 * st1 * beta * dble(deltaz) * 1.d5 c1 = c1 * st1 * dble(deltaz) aa = aa + ( p1*mr1*(c1*ff) + p2*mr2*(c2*ff)) / 2.d0 bb = bb + ( p1*c1 + p2*c2 ) / 2.d0 cc = cc + ( c1 + c2 ) / 2.d0 dd = dd + ( t1*c1 + t2*c2 ) / 2.d0 do kr=1,nbox ccbox(kr) = ccbox(kr) + @ ( c1box(kr) + c2box(kr) )/2.d0 ! if(i.eq.nl.and.ig.eq.1682)write(*,*)'mztud/464', ! 1 ccbox(kr),c1box(kr),c2box(kr),kr ddbox(kr) = ddbox(kr) + @ ( t1*c1box(kr)+t2*c2box(kr) )/2.d0 end do mr2 = mr1 c2=c1 do kr=1,nbox c2box(kr) = c1box(kr) end do t2=t1 p2=p1 end if pt = bb / cc pp = aa / (cc*ff) ! ta=dd/cc ! tdop = ta ts = dd/cc do kr=1,nbox ta(kr) = ddbox(kr) / ccbox(kr) end do ! write (*,*) ' i, ts =', i, ts call interstrength(st,ts,ka,ta) ! call intershape(alsa,alna,alda,tdop) call intershape(alsa,alna,alda,ta) * ua = cc/st c next loop calculates the eqw for an especified path uapp,pt,ta eqwmu = 0.0d0 do im = 1,iimu eqw=0.0d0 do kr=1,nbox ua(kr) = ccbox(kr) / ka(kr) * beta * 1.0d5 / mu(im) if(ua(kr).lt.0.)write(*,*)'mztud/504',ua(kr),ccbox(kr), $ ka(kr),beta,mu(im),kr,im,i,nl call findw(ig,iirw, idummy,c1,p1,Desp,wsL) if ( i_supersat .eq. 0 ) then eqw=eqw+no(kr)*w else eqw = w + (no(kr)-1) * ( asat_box*dist(kr) ) endif end do eqwmu = eqwmu + eqw * mu(im)*amu(im) end do tauinf(i) = exp( - eqwmu / dble(deltanux) ) end do ! i continue ! if ( isot.eq.1 .and. ib.eq.2 ) then ! write (*,*) ' tauinf(nl) = ', tauinf(nl) ! write (*,*) ' tauinf(1) = ', tauinf(1) ! endif c****** c****** calculation of tau(in,ir) for n<=r c****** do 1 in=1,nl-1 call initial call intz (zl(in), c1,p1,mr1,t1, con) do kr=1,nbox ta(kr) = t1 end do call interstrength (st1,t1,ka,ta) do kr=1,nbox ! c1box(kr) = c1 * ka(kr) * beta * dble(deltaz) * 1.d5 c1box(kr) = c1 * ka(kr) * dble(deltaz) end do ! c1 = c1 * st1 * beta * dble(deltaz) * 1.d5 c1 = c1 * st1 * dble(deltaz) do 2 ir=in,nl-1 if (ir.eq.in) then tau(in,ir) = 1.d0 goto 2 end if call intz (zl(ir), c2,p2,mr2,t2, con) do kr=1,nbox ta(kr) = t2 end do call interstrength (st2,t2,ka,ta) do kr=1,nbox ! c2box(kr) = c2 * ka(kr) * beta * dble(deltaz) * 1.d5 c2box(kr) = c2 * ka(kr) * dble(deltaz) end do ! c2 = c2 * st2 * beta * dble(deltaz) * 1.e5 c2 = c2 * st2 * dble(deltaz) c aa = aa + ( p1*mr1*c1 + p2*mr2*c2 ) / 2.d0 aa = aa + ( p1*mr1*(c1*ff) + p2*mr2*(c2*ff)) / 2.d0 bb = bb + ( p1*c1 + p2*c2 ) / 2.d0 cc = cc + ( c1 + c2 ) / 2.d0 dd = dd + ( t1*c1 + t2*c2 ) / 2.d0 do kr=1,nbox ccbox(kr) = ccbox(kr) + ( c1box(kr) + c2box(kr) ) /2.d0 ddbox(kr) = ddbox(kr) + ( t1*c1box(kr) + t2*c2box(kr) ) /2.d0 end do mr1=mr2 t1=t2 c1=c2 p1=p2 do kr=1,nbox c1box(kr) = c2box(kr) end do pt = bb / cc pp = aa / (cc * ff) * ta=dd/cc * tdop = ta ts = dd/cc do kr=1,nbox ta(kr) = ddbox(kr) / ccbox(kr) end do call interstrength(st,ts,ka,ta) call intershape(alsa,alna,alda,ta) * ua = cc/st c next loop calculates the eqw for an especified path ua,pp,pt,ta eqwmu = 0.0d0 do im = 1,iimu eqw=0.0d0 do kr=1,nbox ua(kr) = ccbox(kr) / ka(kr) * beta * 1.0d5 / mu(im) if(ua(kr).lt.0.)write(*,*)'mztud/599',ua(kr),ccbox(kr), $ ka(kr),beta,mu(im),kr,im,i,nl call findw(ig,iirw, idummy,c1,p1,Desp,wsL) if ( i_supersat .eq. 0 ) then eqw=eqw+no(kr)*w else eqw = w + (no(kr)-1) * ( asat_box*dist(kr) ) endif end do eqwmu = eqwmu + eqw * mu(im)*amu(im) end do tau(in,ir) = exp( - eqwmu / dble(deltanux) ) 2 continue 1 continue ! if ( isot.eq.1 .and. ib.eq.2 ) then ! write (*,*) ' tau(1,*) , *=1,20 ' ! write (*,*) ( sngl(tau(1,k)), k=1,20 ) ! endif c********** c********** calculation of tau(in,ir) for n>r c********** in=nl call initial call intz (zl(in), c1,p1,mr1,t1, con) do kr=1,nbox ta(kr) = t1 end do call interstrength (st1,t1,ka,ta) do kr=1,nbox ! c1box(kr) = c1 * ka(kr) * beta * dble(deltaz) * 1.d5 c1box(kr) = c1 * ka(kr) * dble(deltaz) end do ! c1 = c1 * st1 * beta * dble(deltaz) * 1.d5 c1 = c1 * st1 * dble(deltaz) do 4 ir=in-1,1,-1 call intz (zl(ir), c2,p2,mr2,t2, con) do kr=1,nbox ta(kr) = t2 end do call interstrength (st2,t2,ka,ta) do kr=1,nbox ! c2box(kr) = c2 * ka(kr) * beta * dble(deltaz) * 1.d5 c2box(kr) = c2 * ka(kr) * dble(deltaz) end do ! c2 = c2 * st2 * beta * dble(deltaz) * 1.d5 c2 = c2 * st2 * dble(deltaz) aa = aa + ( p1*mr1*(c1*ff) + p2*mr2*(c2*ff)) / 2.d0 bb = bb + ( p1*c1 + p2*c2 ) / 2.d0 cc = cc + ( c1 + c2 ) / 2.d0 dd = dd + ( t1*c1 + t2*c2 ) / 2.d0 do kr=1,nbox ccbox(kr) = ccbox(kr) + ( c1box(kr) + c2box(kr) ) /2.d0 ddbox(kr) = ddbox(kr) + ( t1*c1box(kr) + t2*c2box(kr) ) /2.d0 end do mr1=mr2 c1=c2 t1=t2 p1=p2 do kr=1,nbox c1box(kr) = c2box(kr) end do pt = bb / cc pp = aa / (cc * ff) ts = dd / cc do kr=1,nbox ta(kr) = ddbox(kr) / ccbox(kr) end do call interstrength (st,ts,ka,ta) call intershape (alsa,alna,alda,ta) * ua = cc/st c next loop calculates the eqw for an especified path ua,pp,pt,ta eqwmu = 0.0d0 do im = 1,iimu eqw=0.0d0 do kr=1,nbox ua(kr) = ccbox(kr) / ka(kr) * beta * 1.0d5 / mu(im) if(ua(kr).lt.0.)write(*,*)'mztud/691',ua(kr),ccbox(kr), $ ka(kr),beta,mu(im),kr,im,i,nl call findw(ig,iirw, idummy,c1,p1,Desp,wsL) if ( i_supersat .eq. 0 ) then eqw=eqw+no(kr)*w else eqw = w + (no(kr)-1) * ( asat_box*dist(kr) ) endif end do eqwmu = eqwmu + eqw * mu(im)*amu(im) end do tau(in,ir) = exp( - eqwmu / dble(deltanux) ) 4 continue c c due to the simmetry of the transmittances c do in=nl-1,2,-1 do ir=in-1,1,-1 tau(in,ir) = tau(ir,in) end do end do ccc ccc writing out transmittances ccc if (itauout.eq.1) then ! if(ib.eq.1.or.ib.eq.2.or.ib.eq.3.or.ib.eq.4.or.ib.eq.5 ! @ .or.ib.eq.6.or.ib.eq.7.or.ib.eq.8.or.ib.eq.9) then ! open( 1, file= ! @ dircurtis//'taul'//isotcode//dn//ibcode1//'.dat', ! @ access='sequential', form='unformatted' ) ! else ! open( 1, file= ! @ dircurtis//'taul'//isotcode//dn//ibcode2//'.dat', ! @ access='sequential', form='unformatted' ) ! endif ! write(1) dummy ! write(1)' format: (tauinf(n),(tau(n,r),r=1,nl),n=1,nl)' ! do in=1,nl ! write (1) tauinf(in), ( tau(in,ir), ir=1,nl ) ! end do ! close(unit=1) elseif (itauout.eq.2) then ! if(ib.eq.1.or.ib.eq.2.or.ib.eq.3.or.ib.eq.4.or.ib.eq.5 ! @ .or.ib.eq.6.or.ib.eq.7.or.ib.eq.8.or.ib.eq.9) then ! open( 1, file= ! @ dircurtis//'taul'//isotcode//dn//ibcode1//'.dat') ! else ! open( 1, file= ! @ dircurtis//'taul'//isotcode//dn//ibcode2//'.dat') ! endif ! !write(1,*) dummy ! !write(1,*) 'tij for curtis matrix calculations ' ! !write(1,*)' cira mars model atmosphere ' ! !write(1,*)' beta= ',beta,'deltanu= ',deltanux ! write(1,*) nl ! write(1,*) ! @ ' format: (tauinf(in),(tau(in,ir),ir=1,nl),in=1,nl)' ! do in=1,nl ! write (1,*) tauinf(in) ! write (1,*) (tau(in,ir), ir=1,nl) ! end do ! close(unit=1) ! if(ib.eq.1.or.ib.eq.2.or.ib.eq.3.or.ib.eq.4.or.ib.eq.5 ! @ .or.ib.eq.6.or.ib.eq.7.or.ib.eq.8.or.ib.eq.9) then ! write (*,'(1x, 31htransmitances written out in: ,a22)') ! @ 'taul'//isotcode//dn//ibcode1 ! else ! write (*,'(1x, 31htransmitances written out in: ,a22)') ! @ 'taul'//isotcode//dn//ibcode2 ! endif end if c cleaning of transmittances ! call elimin_tau(tau,tauinf,nl,nan,itableout,nw,dummy, ! @ isotcode,dn,ibcode2) c construction of the curtis matrix call mzcud ( tauinf,tau, cf,cfup,cfdw, vc,taugr, @ ib,isot,icfout,itableout ) c end return end