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pared_multiple.f
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pared_multiple.f
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c---- viene de pared_ramiro pero calcula para varios valores
c---- de tdp, con polvo (amin,amax,p,filesil) fijo
program pared
integer ncdsx,i,j,kk,escribir,nwlirs,nwl,est00,jpaola
parameter (ncdsx=100)
parameter(ntdpt=15)
character*100 wlfile,fileimagen,filespectro,filestar
character*24 d_and_t
real*4 step,nu,tauext,tau00,gg,mui,integra
real*4 dummy(10)
real*4 cs,Rd,mu,seni,sent,altura,delta,alt
real*4 Rstar,Mstar,Tstar,mmu,xlbb,xnu
real*4 X(0:ncdsx)
real*4 Y(-ncdsx:ncdsx)
real*4 Z
real*4 iYup,sYup,sYdown
real*4 Iterm(0:ncdsx,-ncdsx:ncdsx),Itotp(0:ncdsx,-ncdsx:ncdsx)
real*4 Iscat(0:ncdsx,-ncdsx:ncdsx),Itot(0:ncdsx,-ncdsx:ncdsx)
real*4 W,Bdel,Bscat
real*4 Msol,Rsol,G,au,mh
parameter (Msol=1.989e33,Rsol=6.95508e10,
1 G=6.67e-8,au=1.495979e13,mh=1.67e-24)
real*4 h,k,c,Pi
parameter (h=6.6260755e-27, k=1.380658e-16, c=2.99792458e10,
1 Pi=3.14159)
parameter(nwl0=4000,ntaumaxx=5000,nflll=nwl0,nmax=nwl0)
character*120 filesil,filetroi,fileice1,fileice2
common/dustfiles/filesil,filetroi,fileice1,fileice2
c almacena los datos necesarios para calcular la I y el
c flujo en el principal
common/tdpvarios/tdpt(ntdpt),tkt(ntaumaxx,ntdpt),rdt(ntdpt),
. alturat(ntdpt),xkdt(ntdpt),ntdp
c almacena las opacidades individuales para sumarlas despues
c con las tsub de acuerdo con las tk
common/opacidadesvarias/polsil(nmax),police(nmax),
. poltroi(nmax),polorg(nmax),albesil(nmax),albeice(nmax),
. albetroi(nmax),albeorg(nmax)
c. sale de pared_arbitraria:
dimension taud(ntaumaxx),tk(ntaumaxx)
dimension wl(nwl0),alb(nwl0),xk(nwl0),xls(nwl0),dusto(nwl0)
dimension xlbb(nwl0)
c rd en R_*, altura desde el plano medio en R_*
common/salida/rd,altura,xkd,taud,tk,xk,xls,ntaumax
c. entra a pared_arbitraria:
c. amin y amax en micras (tipico: 0.005 y 0.25), p=3.5
common/sizes/amin,amax,p
c. rstar y mstar en unidades de radio estelares en pared_arbitraria_iso
common/estrella/Rstar,Mstar
common/otros/xmu,alt,mmu,wlfile,filestar
common/masotros/tdp,xmp,alfa
common/alt1/fz0nada,scalenada,rdcmnada,deltar
common/salva/dusto,alb
common/ww/wl,nwl
common/lambdas/nwlirs
common/tstar1/tstar
real*4 fluu(nflll,ntdpt)
real*8 flujo(nflll),faprox(nflll),area,angsol
external fscat, plank, integra
data torg,ttroi,tice/425.,680,1./
read(5,*)ntdp
read(*,*)(tdpt(i),i=1,ntdp)
write(6,*)(tdpt(i),i=1,ntdp)
read(*,*)xmp,alfa,ntaumax
c en unidades solares
read(*,*)Mstar, Tstar, Rstar
rstarori=rstar
read(*,*)distancia
c definimos cosas para la subtrutina pared arbitraria
read(*,*)mui
xmu=mui
mmu=2.36
c. en unidades de la escala de altura a teff. Poner = 1, el flujo escala
read(*,*)alt
alt0=alt
c para que lambdas queremos
read(*,'(a)')wlfile
c---- propiedades del polvo
read(*,*)amin,amax,p
write(17,*)amin,amax,p
read(*,'(a)')filesil
read(*,'(a)')filetroi
read(*,'(a)')fileice1
read(*,'(a)')fileice2
c estrella
c read(*,'(a)')filestar
c Se escribe el archivo del mapa ? 1=si
c 'Estrella en la imagen (si=1, extingida=2)?'
read(*,*)est00
write(6,*)'est00',est00
if(est00.eq.2) then
write(*,*)'tau?'
read(*,*)tauext
endif
c call and print time to screen
c call fdate(d_and_t)
c write(*,*)'TIME calling tyopas: ', d_and_t(12:19)
c write(*,*)'TIME calling tyopas: '
cCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCC
c write(*,*)'begin with tyopas'
call tyopas
c write(*,*)'done with tyopas'
ccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccc
c call and print time to screen
c call fdate(d_and_t)
c write(*,*)'TIME done with tyopas:',d_and_t(12:19)
c write(*,*)'TIME done with tyopas'
c stop
c pasamos a cm lo que sale de pared_arbitraria
c for input to propio3
write(20,*)(rdt(itdp)*rstar*rsol/au,itdp=1,ntdp)
do itdp=1,ntdp
rstar=rstarori
c-------------------------
c llena los arreglos correspondientes
tdp=tdpt(itdp)
rd=rdt(itdp)
altura=alturat(itdp)
xkd=xkdt(itdp)
do itau=1,ntaumax
tk(itau)=tkt(itau,itdp)
enddo
c-------opacidades, kappa, alb monocromaticos
do il=1,nwlirs
dustsil1=polsil(il)
xksil1=(1.-albesil(il))*dustsil1
if (tdp.lt.torg) then
dustorg1=polorg(il)
xkorg1=(1.-albeorg(il))*dustorg1
else
dustorg1=0.
xkorg1=0.
endif
if (tdp.lt.tice) then
dustice1=police(il)
xkice1=(1.-albeice(il))*dustice1
else
dustice1=0.
xkice1=0.
endif
if (tdp.lt.ttroi) then
dusttroi1=poltroi(il)
xktroi1=(1.-albetroi(il))*dusttroi1
else
dusttroi1=0.
xktroi1=0.
endif
dusto(il)=dustsil1+dustice1+dustorg1+dusttroi1
xk(il)=xksil1+xkice1+xkorg1+xktroi1
alb(il)=(dusto(il)-xk(il))/dusto(il)
c de il
enddo
c-------------------------
rd0=rd
write(*,*)'rd=',rd0
rdau=rd0*rstar*rsol/au
write(6,*)'rstar,rd',rstar,rd
Rstar=rstar*rsol
Rd=rd*Rstar
write(6,*)'rd,rstar,altura',rd,rstar,altura
altura=altura*Rstar
write(6,*)'altura',altura
seni=sqrt(1-mui**2)
delta=(altura/Rd)*(seni/mui)
step=Rd/float(ncdsx)
area=step**2
write(6,*)'seni,delta,step,area,altura'
write(6,*)seni,delta,step,area,altura
c calculamos el factor de dilucion de una vez para 'Rd' dado
dummy(1)=Rstar/Rd
W=0.5*(1-sqrt(1-(dummy(1))**2))
angsol=area/(distancia*206265.*au)/(distancia*206265.*au)
fac=(rd/(distancia*206265.*au))**2
if(delta.gt.1.) then
angsolp=pi*fac*mui
else
angsolp=2.*fac*mui*
* (delta*sqrt(1.-delta**2)+asin(delta))
endif
c write(6,*)'w,angsol,fac,angsolp',w,angsol,fac,angsolp
c. OJO: esta version no calcula el factor de asimetria consistentemente !!
gg=0.24
c tau del pixel central
tau00=0.
cCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCC
c Aqui empieza el bucle para las diferentes lambdas
c call and print time to screen
c call fdate(d_and_t)
c write(*,*)'TIME begin pared do loop:',d_and_t(12:19)
c write(*,*)'TIME begin pared loop:'
do kk=1,nwlirs
c lambda en micras
nu=c/(wl(kk)*1e-4)
c Bscat=plank(nu,Tstar)
c if (kk.eq.1) then
c call fdate(d_and_t)
c write(*,*)'TIME begin Bscat:',d_and_t(12:19)
c end if
Bscat=bnu(tstar,wl(kk))
c if (kk.eq.1) then
c call fdate(d_and_t)
c write(*,*)'TIME end Bscat:',d_and_t(12:19)
c end if
c ahora calculamos para todos los puntos y escribimos
flujo(kk)=0.
do i=0,ncdsx
X(i)=step*float(i)
do j=-ncdsx,ncdsx
c if((kk/100)*100.eq.kk)write(6,*)itdp,kk,i,j
Y(j)=step*float(j)
Z=Y(j)*mui/seni - sqrt(Rd**2-X(i)**2)/seni
c el seno del angulo theta (azimutal) en las coordenadas del
c disco
sent=(Y(j)*mui-Z*seni)/Rd
mu=seni*sent
c write(6,*)'sent',sent
dummy(2)=dusto(kk)/xkd/mu
c write(6,*)'dusto(kk),xkd,mu',dusto(kk),xkd,mu
c primero por los casos posibles en delta
sYup= mui*sqrt(1-(X(i)/Rd)**2)*Rd+altura*seni
iYup=-mui*sqrt(1-(X(i)/Rd)**2)*Rd+altura*seni
sYdown= mui*sqrt(1-(X(i)/Rd)**2)*Rd-altura*seni
c en este bloque preguntamos si el punto esta dentro de la zona
c visible y evaluamos si no I=0
if (delta.gt.1.0) then
c toda la elipse de arriba
if ((Y(j).gt.iYup).and.(Y(j).lt.sYup)) then
c call and print time to screen
c call fdate(d_and_t)
c write(*,*)'TIME begin integra:',d_and_t(12:19)
Iterm(i,j)=
. integra(dummy(2),nu,taud,tk,ntaumaxx,ntaumax)
c call and print time to screen
c call fdate(d_and_t)
c write(*,*)'TIME end integra:',d_and_t(12:19)
Iscat(i,j)=W*Bscat*alb(kk)*fscat(gg,mu)/(1.+mu)
Itot(i,j)=Iterm(i,j)+Iscat(i,j)
else
Itot(i,j)=0.
end if
else
c ya se ve el hueco y preguntamos
if(sent.lt.delta) then
if ((Y(j).gt.iYup).and.(Y(j).lt.sYup)) then
c call and print time to screen
c call fdate(d_and_t)
c write(*,*)'TIME begin integra:',d_and_t(12:19)
Iterm(i,j)=
. integra(dummy(2),nu,taud,tk,ntaumaxx,ntaumax)
c call and print time to screen
c call fdate(d_and_t)
c write(*,*)'TIME end integra:',d_and_t(12:19)
Iscat(i,j)=W*Bscat*alb(kk)*fscat(gg,mu)/(1.+mu)
Itot(i,j)=Iterm(i,j)+Iscat(i,j)
c. prueba
c Itot(i,j)=1.
else
Itot(i,j)=0.
end if
else
if ((Y(j).gt.sYdown).and.(Y(j).lt.sYup)) then
c call and print time to screen
c call fdate(d_and_t)
c write(*,*)'TIME begin integra:',d_and_t(12:19)
Iterm(i,j)=
. integra(dummy(2),nu,taud,tk,ntaumaxx,ntaumax)
c call and print time to screen
c call fdate(d_and_t)
c write(*,*)'TIME end integra:',d_and_t(12:19)
Iscat(i,j)=W*Bscat*alb(kk)*fscat(gg,mu)/(1.+mu)
Itot(i,j)=Iterm(i,j)+Iscat(i,j)
c. prueba
c Itot(i,j)=1.
else
Itot(i,j)=0.
end if
c if(i.lt.65)then
c write(6,*)'i,j,kk,wl(kk),Bscat,Iterm(i,j),Iscat(i,j),Itot(i,j)'
c write(6,*)i,j,kk,wl(kk),Bscat,Iterm(i,j),Iscat(i,j),Itot(i,j)
c endif
c if(i.lt.65)then
c write(6,*)'i,Iterm(i,j)'
c write(6,*)i,Iterm(i,j)
c endif
end if
end if
cccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccc
c aqui extinguimos la intesidad de la PARED y la ESTRELLA
c si es que se pide. 1.085.. es 2.5log(e)
if(est00.eq.2) then
Itot(i,j)=Itot(i,j)*exp(-1.08573*tauext)
Bscat=Bscat*exp(-1.08573*tauext)
endif
ccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccccc
if((i.eq.0).and.(j.eq.0)) then
xfactor=Pi*rstar**2/(step**2)
Itotp(i,j)=Itot(i,j)+Bscat*xfactor
else
Itotp(i,j)=Itot(i,j)
end if
flujo(kk)=flujo(kk)+2*Itot(i,j)*angsol
end do
end do
fluu(kk,itdp)=flujo(kk)
c if(itdp.eq.2)write(6,*)wl(kk),flujo(kk),fluu(kk,itdp)
end do
c termino el ciclo de las lambdas
c call fdate(d_and_t)
c write(*,*)'TIME end pared do loop:',d_and_t(12:19)
c write(*,*)'TIME finish pared loop:'
write(6,*)'itdp',itdp
c de itdp
enddo
c write(*,*)'writing output'
write(17,*)ntdp
write(17,*)'Tdp'
write(17,200)(tdpt(itdp),itdp=1,ntdp)
200 format(10(1pe10.2))
c write(17,201)(rdt(itdp)*rstar*rsol/au,itdp=1,ntdp)
write(17,*)'Rd(AU)'
write(17,200)(rdt(itdp)*rstarori*rsol/au,itdp=1,ntdp)
write(17,*)'zwall(AU)(1 H)'
write(17,200)(alturat(itdp)*rstarori*rsol/au,itdp=1,ntdp)
write(17,*)'wl(mic),log(nuFnu)'
do i=1,nwlirs
xnu=c/(wl(i)*1e-4);
write(17,202)wl(i),(alog10(xnu*fluu(i,itdp)),itdp=1,ntdp)
202 format(15(0pf8.3))
end do
close(17)
end program pared