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GIS – an update Dr Lucie Green Mullard Space Science Laboratory UCL
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To get Good recent spectra Webpages to go through Giulio’s plot which show ghosted regions Ghost information file
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GIS – New Web Pages www.mssl.ucl.ac.uk/www_solar/gis
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GIS – Users Guide
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GIS – ghost information file The ghostbuster software generates an information file SPECTRAL ATLAS 4 / GIS Meridian Study 2004-10-03T23:24:52.538, s31134r17.fits GSET: 66 ; Slit no/size: 2 / 4"x4" ; Pointing: [0,968] ------------------------------------------------------------------- --GIS Detector 1 - Likely Ghosting Regions-- ------------------------------------------------------------------- 154.544-162.676 173.922-182.495 192.073-199.780 210.414-214.423 Fe XI 180.2 A line ghosts to 160 A, 1434 counts (15%) recovered Fe X 177.1 A line ghosts to 157 A, 5791 counts (18%) recovered Fe X 174.0 A line ghosts to 154 A, 6293 counts (16%) recovered Fe XII 193.4 A line ghosts into 175 A --- Blend / unrecovered Fe XII 192. A line ghosts into 174.0 A --- Blend / unrecovered Wavelengths affected by ghosting Locations of recovered counts Blended lines
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GIS - Studies
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GIS – Data Archive Synoptic observations run since the start of the mission. For example, quiet sun obs: -SPECT_1 Slit: 2x2" Raster area: 30x30" Exposure time: 30s -GIMCP Slit: 2x2" Raster area: 2x2" Exposure time: 100s Search the archive! IDL> headcat, cat96, year=1996 Search though cat96.SCI_OBJ to look for coronal holes, active region loops etc…
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GIS – Line Intensities LTGD decreases line intensity and broadens lines Uncorrected intensities give an idea of detector evolution
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SPECT_1 study Spectral line counts
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GIS – LTGD methods Filament dumps GIS1 in 2001 GIMCPS1 study – line by line analysis 197 A 171A
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GIS – Long-term Gain Depression Flat fields available Strong lines
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bla
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GIS – Line Profiles
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No LTGD cor. Line widths with LTGD cor.
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Summary Request observations Request data GIS is working well Revision of calibration is underway Comments on User Guide are welcome
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