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

This page was created on 01-Jun-2010 15:30 by ViggoHanst

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Version Date Modified Size Author Changes ... Change note
5 07-Dec-2016 14:14 985 bytes PeterYoung to previous
4 07-Jun-2010 21:46 912 bytes PeterYoung to previous | to last
3 01-Jun-2010 15:31 915 bytes ViggoHanst to previous | to last
2 01-Jun-2010 15:30 954 bytes ViggoHanst to previous | to last
1 01-Jun-2010 15:30 955 bytes ViggoHanst to last

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QuicklookIntensity
QuicklookIntensity

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At line 1 changed one line
The intensity map mode of displaying data averages the line over the line profile. An example of artificial EIS data made by John Mariska from a TRACE image of an active region is displayed below.
[{ALLOW edit EISMainUsers}]
[{ALLOW view Anonymous}]
!!!Intensity map
At line 3 changed one line
[{Image src='ximage.png' width='' height='' align='center' }]
The intensity map mode of displaying data averages the line over the line profile. An example made using the Fe XII 195 line at the north limb is shown below.
At line 5 changed one line
If more than one line is selected in {{xcontrol}}, several such windows will show up. For a raster containing M slit positions and N exposures, the map will have N x M pixels. For a scanning raster, the N exposures (abscissa) translates into solar-X position, while for a sit-and-stare the corresponding axis dimesnion will be time. The ordinate axis translates to solar-Y.
[{Image src='ximage.png' width='700' height='' align='center' }]
At line 7 changed one line
The menus available to this mode of display are the similar as those described for the [xdetector|QuicklookDetector] display. In addition, at the bottom of the left column there is a button, __Define Line__ which will allow you to choose which portion of the line profile is to be used for making the image.
If more than one line is selected in {{xcontrol}}, several such windows will show up. For a raster containing M slit positions and N exposures, the map will have N x M pixels. For a scanning raster, the N exposures (abscissa) translates into solar-X position, while for a sit-and-stare the corresponding axis dimension will be time. The ordinate axis translates to solar-Y.
At line 9 changed one line
The menus available to this mode of display are similar to those described for the [xdetector|QuicklookDetector] display. In addition, at the bottom of the left column there is a button, __Define Line__ which will allow you to choose which portion of the line profile is to be used for making the image.
This page (revision-5) was last changed on 07-Dec-2016 14:14 by PeterYoungTop