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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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 13 changed one line
*The detector display shows full CCD images (see the [Xdetector|Quicklookdetector] section below), i.e. count rates as a function of wavelength (abscissa) and slit position (ordinate). The ordinate translates into Solar-Y position.
*The detector display shows full CCD images (see the [Xdetector|QuicklookDetector] section below), i.e. count rates as a function of wavelength (abscissa) and slit position (ordinate). The ordinate translates into Solar-Y position.
This page (revision-5) was last changed on 07-Dec-2016 14:14 by PeterYoungTop