EIT Software Listings

 

anal
obsolete
response
util

 

Previous Routine
Next Routine

 

Listing of $SSW/soho/eit/idl/anal/eit_temp_resp.pro

 


function eit_temp_resp,wave,pressure=pressure,temp=temp
;
; +
; NAME:
;  eit_temp_resp
; PURPOSE
;  Compute EIT temperature response (EM=1.e26 cm^-5) for each filter
;  Useful on its own as well an example of calling EIT_FLUX 
; CALLING SEQUENCE:
;  response = eit_temp_resp(wavelngth,pressure=pressure,temp=temp)
; INPUT:
;   wavelength
;   pressure (used only for level population calculations - not
;                    sensitive to this)
; OUTPUT:
;   response
;   temperature array
; HISTORY
;   created 8-Dec-1997 J. Newmark
;   1999-May-11 J. Newmark New data file
; -

defsysv,'!xuvtop',exist=yes_chianti
if not yes_chianti then ssw_packages,/chianti,/prepend

if n_elements(pressure) eq 0 then pressure = 1.e15

;specs = [1e8,5e8,1e9,5e9,1e10,5e10,1e11]
;spec_choice = where(specs eq eldens)
restore,concat_dir(getenv('SSW_EIT_RESPONSE'),'chianti_spec.save')
;stat = execute("inspec = "+ 'spec'+strtrim(spec_choice(0),2)) 

response = eit_flux(wave,temp,pressure=pressure,dem_name='unit',inspec=spec0,$
   inwave=waves)

return,response
end




Web curator: Frédéric Auchère
Responsible NASA official: Joseph B. Gurman, Facility Scientist, Solar Data Analysis Center
joseph.b.gurman@gsfc.nasa.gov
+1 301 286-4767
NASA Goddard Space Flight Center
Solar Physics Branch / Code 682

Last revised: - Wed May 9 21:45:04 2007- F. Auchère