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This repository has been archived by the owner on Mar 22, 2023. It is now read-only.
Saha-Boltzmann may be a good starting point. This should be temperature and density sensitive. We can then test it against NIST.
CHIANTI and fiasco have functions for this, but for diffuse, high-temperature plasmas (e.g. solar corona), where LTE doesn't hold. We may be able to call those for certain non-LTE distributions, but we should implement our own more general methods to cover wider range of plasmas.
The text was updated successfully, but these errors were encountered:
See this discussion in PlasmaPy.
Saha-Boltzmann may be a good starting point. This should be temperature and density sensitive. We can then test it against NIST.
CHIANTI and fiasco have functions for this, but for diffuse, high-temperature plasmas (e.g. solar corona), where LTE doesn't hold. We may be able to call those for certain non-LTE distributions, but we should implement our own more general methods to cover wider range of plasmas.
The text was updated successfully, but these errors were encountered: