This page (revision-13) was last changed on 07-Dec-2016 14:14 by Peter Young

This page was created on 06-Jul-2007 13:51 by Harry Warren

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Version Date Modified Size Author Changes ... Change note
13 07-Dec-2016 14:14 6 KB Peter Young to previous
12 07-Apr-2011 16:27 6 KB PeterYoung to previous | to last
11 08-Jul-2010 21:01 5 KB PeterYoung to previous | to last
10 06-Nov-2008 16:34 4 KB PeterYoung to previous | to last
9 09-Jul-2007 12:53 3 KB Louise Harra to previous | to last
8 09-Jul-2007 12:12 3 KB Louise Harra to previous | to last Comment by Louise Harra
7 07-Jul-2007 12:51 3 KB David Pérez-Suárez to previous | to last
6 07-Jul-2007 12:49 3 KB David Pérez-Suárez to previous | to last
5 06-Jul-2007 14:04 2 KB Harry Warren to previous | to last
4 06-Jul-2007 14:03 2 KB Harry Warren to previous | to last
3 06-Jul-2007 14:02 1 KB Harry Warren to previous | to last
2 06-Jul-2007 13:55 1 KB Harry Warren to previous | to last
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Page References

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EISGetWindata
EISGetWindata

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At line 1 added 2 lines
[{ALLOW edit EISMainUsers}]
[{ALLOW view Anonymous}]
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There are a number of routines available for performing operations on WINDATA structures.
There are a number of routines available for performing operations on WINDATA structures. The full set are listed in [EIS Software Note #21|ftp://sohoftp.nascom.nasa.gov/solarsoft/hinode/eis/doc/eis_notes/21_WINDATA/eis_swnote_21.pdf].
At line 138 added 11 lines
!Trimming the wavelength range of a windata structure (EIS_TRIM_WINDATA)
This routine is intended for WINDATA structures with a large wavelength coverage; most commonly this will be full CCD data. An example use is when EIS_AUTO_FIT is to be run on just a single emission line within a full CCD spectrum. By trimming the wavelength coverage of WINDATA to just including the wavelength region around the line of interest, the spectrum becomes easier to fit. The usage is as follows for the case where Fe XII 195.12 is to be studied:
{{{
IDL> wd=eis_getwindata(l1name, 195.12, /refill)
IDL> wd195=eis_trim_windata(wd,[194.12,196.12])
}}}
Here a +/- 1 angstrom band around the line of interest is extracted.
This page (revision-13) was last changed on 07-Dec-2016 14:14 by Peter YoungTop