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Abstract: Chromospheric spectral variability during the impulsive phase of a solar flare observed at high spatial resolution with DKIST (AGU25)

Chromospheric spectral variability during the impulsive phase of a solar flare observed at high spatial resolution with DKIST

Cole Aiken Tamburri1, Adam F Kowalski2, Maria Kazachenko3, Graham Kerr4, Gianna Cauzzi5, Ryan French6, Jiong Qiu7, Marcel Corchado-Albelo8 and Rahul Yadav1, (1)National Solar Observatory, Boulder, United States, (2)National Solar Observatory, University of Colorado, and Laboratory for Atmospheric and Space Physics, Boulder, United States, (3)University of Colorado at Boulder, NSO, LASP, Boulder, CO, United States, (4)Catholic University of America, Washington, DC, United States, (5)National Solar Observatory, Tucson, United States, (6)Laboratory for Atmospheric and Space Physics, Boulder, United States, (7)Montana State University, Department of Physics, Bozeman, MT, United States, (8)University of Colorado at Boulder, NSO, Astrophysical and Planetary Sciences, Boulder, United States
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