Non-LTE Calculations of the Mg i 12.32 μm Line in a Flaring Atmosphere
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4357/ab9c21/pdf
Reference35 articles.
1. Dynamic Models of Optical Emission in Impulsive Solar Flares
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1. Forward modeling of the Mg I 12.32 μm line from a 3D magnetohydrodynamic model of an enhanced network;Astronomy & Astrophysics;2024-06
2. Design and Realization of High-Speed Acquisition System for Two Dimensional Fourier Transform Solar Spectrometer;SPECTROSC SPECT ANAL;2022
3. Infrared diagnostics of the solar magnetic field with Mg I 12 μm lines: forward-model results;Astronomy & Astrophysics;2021-02
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