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Modeling of the ionosphere dynamics during a magnetic storm requires knowledge of parameter variations in the disturbed thermosphere during the storm. A method to estimate height distributions of temperature and thermosphere composition from satellite density measurements in the upper thermosphere has been proposed. The method description employs data of the SWARM-C satellite measurements during the 17 March 2015 magnetic storm.
A. V. Tashchilin andL. A. Leonovich
"Estimation of variations in the thermosphere parameters during a magnetic storm from satellite measurements of thermospheric density", Proc. SPIE 11916, 27th International Symposium on Atmospheric and Ocean Optics, Atmospheric Physics, 119167S (15 December 2021); https://doi.org/10.1117/12.2603309
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A. V. Tashchilin, L. A. Leonovich, "Estimation of variations in the thermosphere parameters during a magnetic storm from satellite measurements of thermospheric density," Proc. SPIE 11916, 27th International Symposium on Atmospheric and Ocean Optics, Atmospheric Physics, 119167S (15 December 2021); https://doi.org/10.1117/12.2603309