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SUMMARY:Flare-accelerated electrons and the evolution of the associated ac
 tive region
DTSTART;VALUE=DATE-TIME:20230510T102500Z
DTEND;VALUE=DATE-TIME:20230510T104000Z
DTSTAMP;VALUE=DATE-TIME:20240704T115654Z
UID:indico-contribution-333@meetings.aip.de
DESCRIPTION:Speakers: Malte Bröse (AIP)\nA multi-wavelength analysis is c
 onducted to study flare signatures both in the\nlow and higher corona. LOF
 AR\, STIX/Rhessi\, and AIA data provide an extensive\npicture about differ
 ent aspects of flare characteristics. The active region and\nits thermal e
 volution are studied through Differential Emission Measure (DEM)\nreconstr
 uctions from AIA data. Flare-accelerated electrons and their radio\ntraces
  are observed with STIX and LOFAR\, respectively. These are in principal\n
 all  associated with the energy release during the flare process. We focus
  on\nfluctuations of the radio sources and the thermal evolution of the ac
 tive\nregion\, and their possible relations. Solar magnetic fields are a b
 inding\nelement between low and high corona\, accelerated electrons\, and 
 heated flare\nloops. They are included in the analysis via a Potential Fie
 ld Source Surface\n(PFSS) model.\n\nhttps://meetings.aip.de/event/24/contr
 ibutions/333/
LOCATION:Haus H\, Telegrafenberg
URL:https://meetings.aip.de/event/24/contributions/333/
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