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Ryan French
Laboratory for Atmospheric and Space PhysicsMeeting roles in:
Chromospheric spectral variability during the impulsive phase of a solar flare observed at high spatial resolution with DKIST
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
Dual Origins of Rapid Flare Ribbon Downflows in an X9-class Solar Flare
Unprecedented Fine Structures in Coronal Flare Ribbons Revealed by Solar Orbiter’s High-Resolution Imager
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