dustem_compute_stokext.pro
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FUNCTION dustem_compute_stokext,p_dim,$
st=st,$
QEXT_spec=QEXT_spec,$
UEXT_spec=UEXT_spec,$
PSIEXT_spec=PSIEXT_spec,$
dustem_psi_ext=dustem_psi_ext,$
help=help
;+
; NAME:
; dustem_compute_stokext
;
; PURPOSE:
; Computes Stokes Parameters for extinction in units of optical depth for a given Dustem spectrum
;
; CATEGORY:
; Dustem
;
; CALLING SEQUENCE:
; out=dustem_compute_stokext(p_dim[,st=][,QEXT_spec=QEXT_spec][,UEXT_spec=UEXT_spec][,PSIEXT_spec=PSIEXT_spec][,dustem_psi_ext=dustem_psi_ext][,/help])
;
; INPUTS:
; p_dim = parameter values
;
; OPTIONAL INPUT PARAMETERS:
; st = Dustem structure
;
; OUTPUTS:
; out = List Containing the Stokes parameters extinction for spectrum points in !dustem_data
; out[0] = Computed Stokes Q extinction for spectrum points in !dustem_data
; out[1] = Computed Stokes U extinction for spectrum points in !dustem_data
;
; OPTIONAL OUTPUT PARAMETERS:
; st = Dustem output structure
; QEXT_spec = Dustem Stokes Q extinction
; UEXT_spec = Dustem Stokes U extinction
; PSIEXT_spec = Dustem Polarization angle output in extinction
; dustem_psi_ext = Computed Polarization angle ouput for spectrum points in !dustem_data
;
; ACCEPTED KEY-WORDS:
; help = If set, print this help
;
; COMMON BLOCKS:
; None
;
; SIDE EFFECTS:
; None
;
; RESTRICTIONS:
; The DustEM fortran code must be installed
; The DustEMWrap IDL code must be installed
;
; PROCEDURE:
; None
;
; EXAMPLES
;
; MODIFICATION HISTORY:
; Written by J.-Ph. Bernard 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_compute_stokext'
out=0.
goto,the_end
ENDIF
IF not keyword_set(st) THEN BEGIN
dustem_activate_plugins,p_dim/(*(*!dustem_fit).param_init_values),st=st
;st=dustem_run(p_dim)
ENDIF
out=0. ; no specific output is required.
If keyword_set(result) THEN result=st
degtorad = !pi/180
EXT_spec = st.ext.ext_tot * (*!dustem_HCD)/1.e21 ;This is Total extinction (for a default value of 10^20 NH/cm^2)
POLEXT_spec = st.polext.ext_tot * (*!dustem_HCD)/1.e21 ;This is Polarized extinction
;Hard-coded test to set to zero potential negative values in the polarized extinction arrays:
;so far this has been seen in absorption arrays
;This test needs to include all grain species that polarize
IF !run_pol THEN BEGIN
;THIS FALSE CORRECT IT USING POLEXT_spec
;POLEXT_spec.abs_grain[2,*]
ind_ngtv_plxt = where (POLEXT_spec LT 0, ct_ngtv_plxt)
IF ct_ngtv_plxt NE 0 THEN (POLEXT_spec)[ind_ngtv_plxt] = 0.
ENDIF
Nwaves=(size(EXT_SPEC))[1]
frac=POLEXT_spec/EXT_spec
tes=where(finite(frac) eq 0)
frac(tes)=0.
plugin_tags=(*!dustem_plugin).name
ind=where(plugin_tags NE 'NONE',Nplugins)
IF Nplugins NE 0 THEN BEGIN
FOR i=0L,Nplugins-1 DO BEGIN
IF total(strsplit((*!dustem_plugin)[i].scope,'+',/extract) EQ 'REPLACE_POLEXT') THEN BEGIN
QEXT_spec = (*(*!dustem_plugin)[i].spec)[*,1]
UEXT_spec = (*(*!dustem_plugin)[i].spec)[*,2]
ENDIF
ENDFOR
ENDIF
IF ~isa(QEXT_spec) && ~isa(UEXT_spec) THEN BEGIN
polar_ippsi2iqu,EXT_spec,QEXT_spec,UEXT_spec,frac,replicate(!dustem_psi_ext,Nwaves);PSI_spec
ENDIF
IF Nplugins NE 0 THEN BEGIN
FOR i=0L,Nplugins-1 DO BEGIN
IF total(strsplit((*!dustem_plugin)[i].scope,'+',/extract) EQ 'ADD_POLEXT') THEN BEGIN
QEXT_spec+=(*(*!dustem_plugin)[i].spec)[*,1]
UEXT_spec+=(*(*!dustem_plugin)[i].spec)[*,2]
ENDIF
ENDFOR
ENDIF
;-----------------------------------------
;Hard-coded block to avoid cases where Q=-0.0 and U=0.
testnzero = where(QEXT_spec EQ -0., ct_nzero)
if ct_nzero ne 0 then QEXT_spec[testnzero] = 0
PSIEXT_spec = 0.5*atan(UEXT_spec,QEXT_spec)/degtorad
;INITIALIZING THE STOKES SEDS
dustem_qext = (*(*!dustem_data).qext).values * 0.
dustem_uext = (*(*!dustem_data).uext).values * 0.
;Using a list because dustem_qext and dustem_uext can have different dimensions
out=list(fltarr(n_elements(dustem_qext)),fltarr(n_elements(dustem_uext)))
if not isarray(EXT_spec) THEN stop
;COLOR CORRECTION NOT PERFORMED YET. ONLY SPECTRUM DATA POINTS ARE CONSIDERED FOR NOW
;
; ;Performing color corrections on the dustem spectra and generating the SEDs at the given filters
;
; IF !dustem_do_cc NE 0 AND !dustem_never_do_cc EQ 0 THEN BEGIN
; message,'DOING color correction calculations',/info
; ENDIF ELSE BEGIN
; message,'SKIPPING color correction calculations',/info
; ENDELSE
;
; ind_qsed=where((*(*!dustem_data).qsed).filt_names NE 'SPECTRUM',count_qsed)
; ind_used=where((*(*!dustem_data).used).filt_names NE 'SPECTRUM',count_used)
;
;
; IF count_qsed NE 0 THEN BEGIN
; filter_names=((*(*!dustem_data).qsed).filt_names)(ind_qsed)
; if isa(dustem_qsed) then begin
; sqsed=dustem_cc(st.polsed.wav,Q_spec,filter_names,cc=cc)
; dustem_qsed(ind_qsed)=sqsed
; endif
; ENDIF
;
; IF count_used NE 0 THEN BEGIN
; filter_names=((*(*!dustem_data).used).filt_names)(ind_used)
; if isa(dustem_used) then begin
; sused=dustem_cc(st.polsed.wav,U_spec,filter_names,cc=cc)
; dustem_used(ind_used)=sused
; endif
; ENDIF
;For spectrum data points, interpolate in log-log
;Linear interpolation leads to wrong values, in particular where few
;wavelengths points exist in the model (long wavelengths).
ind_qspec=where((*(*!dustem_data).qext).filt_names EQ 'SPECTRUM',count_qspec)
ind_uspec=where((*(*!dustem_data).uext).filt_names EQ 'SPECTRUM',count_uspec)
IF count_qspec NE 0 THEN BEGIN
if isa(dustem_qext) then dustem_qext(ind_qspec)=interpol(QEXT_spec,st.polext.wav,(((*(*!dustem_data).qext).wav)(ind_qspec)))
ENDIF
IF count_uspec NE 0 THEN BEGIN
if isa(dustem_uext) then dustem_uext(ind_uspec)=interpol(UEXT_spec,st.polext.wav,(((*(*!dustem_data).uext).wav)(ind_uspec)))
ENDIF
out_st=st
;generating interpolates for Psi_ext
dustem_psi_ext = 0.5*atan(dustem_uext,dustem_qext)/degtorad
out[0] = dustem_qext
out[1] = dustem_uext
;clean pointers
heap_gc
the_end:
RETURN,out
END