This page (revision-7) was last changed on 07-Dec-2016 14:14 by Terje Fredvik

This page was created on 14-Jun-2010 15:59 by PeterYoung

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HKmethod
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At line 9 added 8 lines
The following three examples demonstrate how the new wavelength correction can be obtained. The example data-set is specified through
{{{
IDL> paths = '~/hinodedata/eis/mission/2007/12/11/eis_l0_20071211_162413.fits.gz'
}}}
(please modify the path to the location where your Hinode data are stored) and the data-file can be obtained [here|http://tinyurl.com/wavecorr-example].
At line 14 removed one line
IDL> paths = '~/hinodedata/eis/mission/2007/12/11/eis_l0_20071211_162413.fits.gz' ; This file can be downloaded here
At line 23 changed one line
* wvl_cube: If set to a named variable, wvl_cube will return a 3 dimensional wavelength cube in the format used by mk_analysis.pro of the Component Fitting System for IDL (cfit) package.
* wvl_cube: If set to a named variable, wvl_cube will return a 3 dimensional wavelength cube in the format used by [mk_analysis.pro|http://www.astro.washington.edu/docs/idl/cgi-bin/getpro/library32.html?MK_ANALYSIS] of the [Component Fitting System for IDL (cfit)|http://solar.bnsc.rl.ac.uk/swnotes/cds_swnote_47.pdf] package.
This page (revision-7) was last changed on 07-Dec-2016 14:14 by Terje FredvikTop