SWS PIPELINE

From SPD to AAR


EXTRACT_AAR:

extracts valid data from SPD and creates an AAR:

aar = extract_aar( spd [,/all] )

extract_aar extracts the valid data of a SPD, sorts them according to wavelength and puts the resulting spectrum ("flux vs. wavelength ") in an AAR:

Cal-files: none

Help text: IA auto analysis


Comment:

use the showstruct command to visualize the AAR structure:
IA3 TEST> showstruct,aar
(1)
   |----TYPE(1)
   |-HISTORY(1)
   |--HEADER(1)
   |----DATA(8000)
                |---WAVE(1)  ; wavelength [um]
                |---FLUX(1)  ; flux density [Jy] 
                |--STDEV(1)  ; standard deviation 
                |---TINT(1)  ; integration time [1/24 Hz]
                |----DET(1)  ; detector number
                |----ITK(1)  ; SWS instrument time key 
                |----UTK(1)  ; ISO universal time key
                |---RPID(2)  ; raster point id
                |--SPARE(2)  ; spare
                |---LINE(1)  ; line number
                |---SDIR(1)  ; scan direction
                |---SCNT(1)  ; scan counter
                |-STATUS(1)  ; status word
                |---FLAG(1)  ; detector flag


Warning:

currently it's recommended to use the keyword /all in general. Otherwise not only the reference scan data, but also some proper science data might not show up in the AAR.

SWS TUTORIAL / PIPELINE / SPD to AAR : ... velcor < extract_aar > tbd ...

Last update: 30-Jul-1998 by D. Kunze ( mail to: isodata@mpe.mpg.de )