This page (revision-5) was last changed on 07-Dec-2016 14:14 by PeterYoung

This page was created on 01-Jun-2010 14:15 by ViggoHanst

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Version Date Modified Size Author Changes ... Change note
5 07-Dec-2016 14:14 3 KB PeterYoung to previous
4 01-Jun-2010 15:11 3 KB ViggoHanst to previous | to last
3 01-Jun-2010 14:38 3 KB ViggoHanst to previous | to last
2 01-Jun-2010 14:35 3 KB ViggoHanst to previous | to last
1 01-Jun-2010 14:15 302 bytes ViggoHanst to last

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At line 1 added 2 lines
[{ALLOW edit EISMainUsers}]
[{ALLOW view Anonymous}]
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*Compare EIS/Chianti spectra: This is used to compare an average EIS spectrum calculated from the raster with a Chianti spectrum of the same wavelength region. An intermediate window pops up where the user must select the proper emission measure for the Chianti spectrum. The Chianti spectra have been pre-calculated for the EIS wavelength regions and the most relevant emssion measure regimes. The Chianti psectra are stored in proper files and distributed as a part of the EIS QL package.
*Compare EIS/Chianti spectra: This is used to compare an average EIS spectrum calculated from the raster with a Chianti spectrum of the same wavelength region. An intermediate window pops up where the user must select the proper emission measure for the Chianti spectrum. The Chianti spectra have been pre-calculated for the EIS wavelength regions and the most relevant emssion measure regimes. The Chianti spectra are stored in proper files and distributed as a part of the EIS QL package.
This page (revision-5) was last changed on 07-Dec-2016 14:14 by PeterYoungTop