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Steve to provide all computed demodulation matrices for the different emission lines over the mission in order to examine their variation with sky conditions, time-of-day, seasonally, over mission. Th…
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The center finding should happen between the dark and flat application.
Note: don't forget to make sure the correct flips happen during the temporary distortion correction.
At least for now unt…
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The corona moves over the day under the occulter. This is clear when you look at daily movies. Align the coronal structures between the Level 1 images in order to stabilize the images over the day. Ca…
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There are a couple potential solutions for this issue:
- [x] Manually mark all the 706 nm science files for the day as "do not process" in the epoch file.
- [ ] Move the publish `publish_l1` and `…
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The new criteria adopted to estimate the rest wavelength do not work when the line center is more in the blue filter than in the center one.
Let's reverse back to what we are currently doing for th…
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Compute the rest wavelength for CoMP the same way we did for UCoMP, i.e., compute the rest wavelength for each median file, plot and fit, and then create a model that we apply for rest wavelengths.
…
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Only occulter mask visible in frames on the web:
Dates Times
20220202 195044
20220310 195208, 200822 (both doppler)
20220311 193315
20220313 194616, in doppler 200551…
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When creating an average:
- cluster available files in program using 30 minute gaps
- take the first cluster
#### Questions
- [ ] What is the averaging criteria for waves files?
#### Task…
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The file to check is `20220901.182014.02.ucomp.1074.l0.fts`.
- Do the run with intermediate products and interpolating flats.
- Produce difference images.
- Produce % difference images.
Verify…
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Some examples:
- [ ] create a simple notebook to read and display level 1 and level 2 files
- [ ] use template from #166 to create a notebook that displays UCoMP and AIA images together
#### Qu…