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  • Presentation | SH51E: Solar Orbiter: Solar-Heliospheric Connections and First Out-of-the-Ecliptic Observations III Poster
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  • SH51E-1212: Coronal Abundance Evolution During the M7.6 Flare on September 30, 2024 with SolO/SPICE, Hinode EIS, and Chandrayaan-2 XSM: A disharmonious picture between the cool and hot plasma components
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Author(s):
Momchil Molnar, Southwest Research Institute Boulder (First Author, Presenting Author)
Joseph Plowman, Southwest Research Institute Boulder
Ritesh Patel, Southwest Research Institute
Don Hassler, Southwest Research Institute
Ryan French, Laboratory for Atmospheric and Space Physics
Lakshmi Pradeep Chitta, Max Planck Institute for Solar System Research
Arpit Kumar Shrivastav, Southwest Research Institute Boulder
Tania Varesano, University of Colorado Boulder


The chemical composition of solar plasma during flares changes rapidly by a process not well yet understood. In this study, we show that the chemical abundance composition of solar plasma at different temperatures evolve in different ways, which complicates the matter even more. We report for the first time a comparison between the cool plasma chemical evolution compared to the hotter plasma which has been previously observed extensively.



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