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The level 0 data have the following comment for `OBSSWID`:
OBSSWID = '1.0.6' / TODO calculate software id.
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For consistency with UCoMP, we will save the FWHM in the level2 and quick invert. We need to check thresholds to make sure we are consistent in the units we use in the code.
- [x] initialize `fwhm_…
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Steve's implementation is in `UCoMP_GBU` and the current conditions are:
1 spar guider control loop is not locked
2 spar guider intensity below threshhold
4 background > gbu_…
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The current LOS color table blue-white-red does an excellent job of drawing the eye to locations in the image where the velocity flips from positive to negative. However, our zero-point uncertainty …
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#### Tasks
- [x] compute demodulation matrix for 20240409 for each wave region
- [x] compare to temperature dependent fit from existing demodulation matrices in pipeline
- [x] use `UCoMP_Pol_Cal_…
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If the gaussian fit doesn't converge for a pixel, set all level 2 dynamics products to NaN for that pixel.
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We need to update the user guide in light of changes for 1.0.11.
#### Changes
- [ ] different averaging with different filenames, i.e., "daily" synoptic files, for #208
- [ ] update header tab…
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The geometric mask adds 3 pixels to occulter radius. For weak signal lines like 637, this obscures a noticeable amount of pixels with coronal signal. Example is shown below.
Suggest we reduce this to…
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A crude filtering algorithm was implemented in the ucomp code to prevent the lyot filter from reacting to noise in the temperature readings, slow the reaction to temperature change, and better match t…
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The new wavelength positions for the 5 and 7 points are not equally spaced.
The code needs to handle it when it computes the `d_lambda` for the analytical gaussian fit and we need to implement a le…