PRO dustem_write_isrf_release,file,st,help=help

;+
; NAME:
;    dustem_write_isrf_release
;
; PURPOSE:
;    Writes file ISRF.DAT used by DustemWrap
;
; CATEGORY:
;    DustEMWrap, Distributed, Low-level, Fortran
;
; CALLING SEQUENCE:
;    dustem_write_isrf_release,file,st[,/help]
;
; INPUTS:
;    file : file name 
;    st   : input structure containing ISRF information (will be modified)
;
; OPTIONAL INPUT PARAMETERS:
;    None
;
; OUTPUTS:
;    None
;
; OPTIONAL OUTPUT PARAMETERS:
;    None
;
; ACCEPTED KEY-WORDS:
;    help      = If set print this help
;
; COMMON BLOCKS: 
;    None
;
; SIDE EFFECTS:
;    Writes a file
;
; RESTRICTIONS:
;    The DustEM fortran code must be installed
;    The DustEMWrap IDL code must be installed
;
; PROCEDURE AND SUBROUTINES
;    
; EXAMPLES
;    
; MODIFICATION HISTORY:
;    Written by Ilyes Choubani 2022
;    Evolution details on the DustEMWrap gitlab.
;    See http://dustemwrap.irap.omp.eu/ for FAQ and help.  
;-

IF keyword_set(help) THEN BEGIN
  doc_library,'dustem_write_isrf_release'
  goto,the_end
ENDIF

;LOCATING THE ISRF PLUGINS

;IF PLUGINS AREN'T SET. WRITE THE DEFAULT DUSTEM ISRF.DAT FILE
scopes = strarr(n_tags(*!dustem_plugin))
IF (tag_names(*!dustem_plugin))[0] EQ 'NONE' then goto, the_after

;IF PLUGINS ARE SET, LOOP OVER THEIR SCOPES.
;Getting the actual scopes 
FOR i=0L, n_tags(*!dustem_plugin)-1 DO BEGIN
    if isa((*!dustem_plugin).(i).scope) THEN BEGIN
        scopes[i] = (*(*!dustem_plugin).(i).scope)
    ENDIF ELSE goto, the_after
ENDFOR

;TESTING FOR THE TWO CURRENT ISRF PLUGINS
tstpop = where(scopes EQ 'STELLAR_POPULATION',ctpop)
tstusrisrf = where(scopes EQ 'USER_ISRF',ctusrisrf)

IF ctpop NE 0 or ctusrisrf NE 0 THEN BEGIN

    ;NB: Since we're using G0_mathis=1 by default now. We will test on the !dustem_params sysvar instead of the parameter description vectors
    
    G0_mathis = 1. ;Default value
    
    IF ((*!dustem_params).g0) NE 1. then G0_mathis = ((*!dustem_params).g0) 
    IF ((*!dustem_params).gas.g0) NE 1. then G0_mathis = float((*!dustem_params).gas.g0)
       
    ;Getting the ISRF default wavelengths
    ;using this structure
    st=((*!dustem_params).isrf)
    final_isrf = fltarr(n_elements(st)) ;Initializing the ISRF vector
    Ncomments=3 ;default number of comments in the .DAT file (minus the ISRF used)
    c=strarr(Ncomments)
    c(0)='# DUSTEM_WRAP: exciting radiation field featuring'
    ;stop
    IF ctpop NE 0. THEN final_isrf=final_isrf+(*(*!dustem_plugin).(tstpop).spec)
    IF ctusrisrf NE 0. THEN final_isrf=final_isrf+(*(*!dustem_plugin).(tstusrisrf).spec)
    
    IF ctpop NE 0. and ctusrisrf EQ 0. THEN c(1) = '# Stellar population ISRF'
    IF ctpop EQ 0. and ctusrisrf NE 0. THEN  c(1) = '# User-defined ISRF'
    
    IF ctpop NE 0. and ctusrisrf NE 0. THEN BEGIN
        Ncomments+=1
        c=strarr(Ncomments)
        c(0)='# DUSTEM_WRAP: exciting radiation field featuring'  
        c(1) = '# Stellar population ISRF'
        c(2) = '# User-defined ISRF'
    ENDIF
    
    ;WHEN G0 IS USED (MATHIS FIELD ON)
    IF G0_mathis GT 1E-10 THEN BEGIN  ;discussed with JP
        ;This is reading the mathis isrf from the fortran release
        ;Let's hope they keep releasing it otherwise we'll have to include it ourselves
        ma_isrf_dir=!dustem_soft_dir+'data/ISRF_MATHIS.DAT'
        ma_isrf=dustem_read_isrf(ma_isrf_dir)
        final_isrf=final_isrf/G0_mathis+ma_isrf.isrf ;[0]
        Ncomments=4
        c=strarr(Ncomments)
        c(0)='# DUSTEM_WRAP: exciting radiation field featuring'
        
        IF ctpop NE 0 and ctusrisrf EQ 0 THEN c(1) = '# Stellar population ISRF'
        IF ctpop EQ 0 and ctusrisrf NE 0 THEN c(1) = '# User-Defined ISRF'
        
        IF ctpop NE 0 and ctusrisrf NE 0 THEN BEGIN
            Ncomments+=2
            c=strarr(Ncomments)
            c(0)='# DUSTEM_WRAP: exciting radiation field featuring'  
            c(1) = '# Stellar population ISRF'
            c(2) ='# User-defined ISRF'
            c(3) = '# Mathis ISRF'
        ENDIF ELSE c(Ncomments-3) = '# Mathis ISRF'
        
    ENDIF ELSE final_isrf = final_isrf/G0_mathis ;WHEN G0 ISN'T USED (MATHIS FIELD OFF) ie: lower values than 1.0E-10.
    
    st.isrf = final_isrf  

    ;Last .DAT header comments lines
    c(Ncomments-2)='# Nbr of points'
    c(Ncomments-1)='# wave (microns), 4*pi*Inu (erg/cm2/s/Hz)'

    ;Computing the 'G0' of the new ISRF (integral(ISRF)/integral(MATHIS_ISRF))
;         un=uniq(ma_isrf.isrf) ;because of the zeros
;         
;         int_mathis=INT_TABULATED((ma_isrf.lambisrf)[un],(ma_isrf.isrf)[un])
;         
;         
;         ;integrating the composite isrf
;         int_isrf=INT_TABULATED((ma_isrf.lambisrf)[un],(st.isrf)[un])
;         print, 'G0_stellar_population='
;         print, int_isrf/(int_mathis)
    

;WRITING THE NEW ISRF
    
    file=!dustem_dat+'data/ISRF.DAT'  
    openw,unit,file,/get_lun
        
    FOR i=0,Ncomments-1 DO BEGIN
        printf,unit,c(i)
    ENDFOR

    n_waves=n_elements(st)
    printf,unit,n_waves

    FOR i=0L,n_waves-1 DO BEGIN
        printf,unit,st(i).lambisrf,st(i).isrf
    ENDFOR

    close,unit
    free_lun,unit 

    goto, the_end
ENDIF



the_after: ;Defaut ISRF writing (MATHIS)

;This was changed because 6 comments aren't needed
;Ncomments=6
Ncomments=4
c=strarr(Ncomments)

;First lines of the ISRF.DAT file
c(0)='# DUSTEM_WRAP: exciting radiation field featuring'
c(1)='# Mathis ISRF'
;c(2)='# Blackbody with     T=   0.0000E+00'
;c(3)='# dilution factor wdil=   1.0000E+00'
c(2)='# Nbr of points'
c(3)='# wave (microns), 4*pi*Inu (erg/cm2/s/Hz)'

openw,unit,file,/get_lun

FOR i=0,Ncomments-1 DO BEGIN
    printf,unit,c(i)
ENDFOR

n_waves=n_elements(st)
printf,unit,n_waves

FOR i=0L,n_waves-1 DO BEGIN
    printf,unit,st(i).lambisrf,st(i).isrf
ENDFOR

close,unit
free_lun,unit

the_end:


END