Description of the issue
Due to incorrect normalization of the response function, the densities reported by the L3 code are consistently too high compared to other spacecraft. Additionally, the spin phase variation is not handled correctly by the current algorithm.
Steps to reproduce the issue
Compare SWAPI L3 moments to moments from another spacecraft side-by-side, and the difference is obvious.
Expected vs Actual behavior
There should be a reasonable level of agreement.
Code Snippet (If applicable)
Additional notes, affected areas, and suggested fixes
We (the SWAPI team) are close to completing a new fitting algorithm that fixes these problems, for which I intend to open a pull request soon.
Description of the issue
Due to incorrect normalization of the response function, the densities reported by the L3 code are consistently too high compared to other spacecraft. Additionally, the spin phase variation is not handled correctly by the current algorithm.
Steps to reproduce the issue
Compare SWAPI L3 moments to moments from another spacecraft side-by-side, and the difference is obvious.
Expected vs Actual behavior
There should be a reasonable level of agreement.
Code Snippet (If applicable)
CodeAdditional notes, affected areas, and suggested fixes
We (the SWAPI team) are close to completing a new fitting algorithm that fixes these problems, for which I intend to open a pull request soon.