This page (revision-828) was last changed on 03-Feb-2017 10:35 by Denver

This page was created on 04-Feb-2009 11:25 by David R Williams

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Version Date Modified Size Author Changes ... Change note
828 03-Feb-2017 10:35 18 KB Denver to previous The line's engaged cena anafranilu Minter is now trying his hand at headhunting

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At line 67 added 7 lines
* Effects on-orbit
** From Dec 2006 to Jan 2007, don't trust the header information: it's ''all'' Al_Poly.
** absorption layer is decreasing response ({{make_xrt_wave_resp}}). This is a time-dependent absorption function. So it's a fairly sticky bit of correction. There was a hope of coming up with a photometric correction. There's nothing in the software
** spot-like contamination -- can remove this with {{xrt_tup_comtam}}. This does a simple averaging. Another to be released soon does gradient fits iteratively. The attenuation isn't 100%, though, so you can recover the contrast in those areas in many cases, with AR signal levels.
** cross-calibration with EIS, etc. May be a bone of contention?
** Co-alignment
** ...
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TWo lists can be joined:
xrt_science -- discussion of science
xrt_users -- for end-users to provide support for one another.
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KPD: one of the things I'd like to have are movies or time-sequences from a single filter or single exposure times. Can you make them with {{XRT_CAT}}?
KK: There's no standard
EDL: XRT_CAT, WHERE on filter wheel.
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*XBPs
''missed this part due to editor's prerogative''
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*Sheared field in ARs through morphology.
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*DEM intro:
Need 6 or 7 different filters to do this. Reeves broke the DEM up into images into different temperatures.
Can EIS be used to check some of this data. Helen and Kathy might wish to work onthis. Could we somehow make a filter respons for EIS.
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*Flare shrinking loops through morphology
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*Sigmoid structures