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Invited Review: Short-term Variability with the Observations from the Helioseismic and Magnetic Imager (HMI) Onboard the Solar Dynamics Observatory (SDO): Insights into Flare Magnetism View all abstracts by submitter

Maria D Kazachenko   Submitted: 2022-05-19 09:31

Continuous vector magnetic-field measurements by the Helioseismic and Magnetic Imager (HMI) onboard the Solar Dynamics Observatory (SDO) allow us to study magnetic-field properties of many flares. Here, we review new observational aspects of flare magnetism described using SDO data, including statistical properties of magnetic-reconnection fluxes and their rates, magnetic fluxes of flare dimmings, and magnetic-field changes during flares. We summarize how these results, along with statistical studies of coronal mass ejections (CMEs), have improved our understanding of flares and the flare/CME feedback relationship. Finally, we highlight future directions to improve the current state of understanding of solar-flare magnetism using observations.

Authors: Maria D. Kazachenko, Marcel F. Corchado-Albelo, Cole A. Tamburri, Brian T. Welsch
Projects: SDO-AIA,SDO-HMI,SDO-EVE

Publication Status: Published in Solar Physics
Last Modified: 2022-05-19 09:38
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