Demonstrates the effectiveness of a Python library in simulating solar plasma behavior, suggesting improved understanding of solar radiative processes.
Non-LTE radiative transfer numerical simulation is the key to understand the physics behind the non-linearly coupled system consisting of the solar radiation and the plasma in solar atmosphere. A highly flexible library (hereafter, SPECTRA for short) for Non-LTE radiative transfer numerical simulation was developed in Python programming language, for the purpose of solving problems scaling from statistical equilibrium, cloud model to non- LTE radiative transfer. This library is also focusing on interactively interpreting the observed spectroscopy data of the Sun and experimental plasma.
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Huang et al. (2023) studied this question.
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