Closed jessemapel closed 11 months ago
This algorithm is well documented but involves several non-trivial steps. Implementing this will require familiarity with IDL and how its built in methods work (mostly how IDL's built in interpolation and filtering works).
There are three steps in the process:
The first step also has two options. For images with sufficient dark background, you can use the line-by-line background average. For other images, you can use the overclock pixels. The overclock pixels is sufficiently simpler because the line-by-line-average requires thresholding and filtering out stars prior to computing the averages. I would recommend starting with just the overclocked pixels approach.
The filtering step leverages the built in IDL Savitzky-Golay smoothing filter. I doubt ISIS has code to do this already; most of its filtering is for image, not signals. It's not a terribly complex filter but emulating how IDL does this or finding a library that does will be timeconsuming. The filtering step also has a check for discontinuities in the signal which adds additional computations.
Generating and subtracting the 2d image is straight-forward.
Given the complexity of this process, this could take significant work. I'd estimate a full team for at least a week. Each step can be worked on independently and verified.
This will also require a documentation update, because the current documentation says this step is explicitly excluded.
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Description
This issue is a continuation of #2677. Back since cisscal was ported to ISIS3, 2-hz noise filtering was not included even though CICLOPS's version has it.
We should add this as a calibration step to better match the calibration from the instrument team. We should match the CISSCAL v 4.0 algorithm, even if #3491 is not completed yet.
Example
The ISIS cisscal output should match the CICLOPS CISSCAL output with 2-hz noise filtering enabled and anti-bloom correction disabled. If #3491 is not complete, these should still match for non-TABLE images.