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SUMMARY:Recent Progress in Understanding Solar Flare Magnetism using Data-
 Driven Simulations and Statistical Analysis of Vector Magnetic Fields
DTSTART;VALUE=DATE-TIME:20230510T073000Z
DTEND;VALUE=DATE-TIME:20230510T075500Z
DTSTAMP;VALUE=DATE-TIME:20240704T115654Z
UID:indico-contribution-361@meetings.aip.de
DESCRIPTION:Speakers: Maria Kazachenko (University of Colorado - Boulder /
  National Solar Observatory)\n​Continuous vector magnetic-field measurem
 ents by the Helioseismic and Magnetic Imager (HMI) onboard the Solar Dynam
 ics Observatory (SDO) allowed us to run  data-driven simulations of solar 
 eruptions and perform statistical studies of magnetic-fields for many flar
 es. In this talk I will review new aspects of flare magnetism discovered u
 sing SDO data\, including progress in data-driven simulations and statisti
 cal studies of magnetic-reconnection fluxes\, their rates\, magnetic fluxe
 s of flare dimmings\, and magnetic-field changes during flares. I will sum
 marize 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\, I will highlight future directions t
 o improve the current state of understanding of solar-flare magnetism usin
 g observations and simulations.\n\nhttps://meetings.aip.de/event/24/contri
 butions/361/
LOCATION:Haus H\, Telegrafenberg
URL:https://meetings.aip.de/event/24/contributions/361/
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