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DiscussionAn issue opened for, or undergoing discussion.An issue opened for, or undergoing discussion.Effort MediumRequires a moderate time investment.Requires a moderate time investment.Feature RequestNew feature wanted.New feature wanted.Solar Physics KnowledgeThis requires some understanding of solar physics.This requires some understanding of solar physics.TestsAffects tests in some measure.Affects tests in some measure.background info neededmore background information neededmore background information needed
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For the thermal plasma emission function, we currently rely on IDL .sav files generated externally.
I hope this issue starts a conversation around generating the data in Python.
I made a github gist which shows how to save out all of the emission lines on a temperature grid. This uses the Fiasco package made by @wtbarnes. Those lines can get binned into an (E, T) matrix much like the IDL version, and summed with the continuum. This is one part of the problem.
I stopped working on this after the lines, so I haven't touched the continuum.
Things that need to happen:
- make a continuum emission function analogous to the lines one
- figure out how to integrate the two
- decide how we want to bin things
- ... ?
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DiscussionAn issue opened for, or undergoing discussion.An issue opened for, or undergoing discussion.Effort MediumRequires a moderate time investment.Requires a moderate time investment.Feature RequestNew feature wanted.New feature wanted.Solar Physics KnowledgeThis requires some understanding of solar physics.This requires some understanding of solar physics.TestsAffects tests in some measure.Affects tests in some measure.background info neededmore background information neededmore background information needed