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Abstract: 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 (AGU25)

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

Momchil Molnar, Southwest Research Institute Boulder, Solar and Heliospheric Physics, Boulder, CO, United States, Joseph Plowman, Southwest Research Institute Boulder, Boulder, United States, Dr. Ritesh Patel, Southwest Research Institute, Boulder, CO, United States, Don Hassler, Southwest Research Institute, Boulder, United States, Ryan French, Laboratory for Atmospheric and Space Physics, Boulder, United States, Lakshmi Pradeep Chitta, Max Planck Institute for Solar System Research, Göttingen, Germany, Arpit Kumar Shrivastav, Southwest Research Institute Boulder, Boulder, CO, United States and Tania Varesano, University of Colorado Boulder, Boulder, United States
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