EOVSA and STIX: jointly observed flares in 2021

Jul 8, 2021, 5:05 PM


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Working Group 2: Particle acceleration Working Group 2: Particle acceleration


Sam Krucker


Radio and hard X-ray diagnostics provide very strong complementary tools to probe electron acceleration in solar flares. With the Expanded Owens Valley Solar Array (EOVSA) and the Spectrometer/Telescope for Imaging X-rays (STIX) we have currently two solar dedicated observatories jointly observing on a daily basis. To date, we already have more than 10 jointly observed flares ranging from small microflares up to M-class flares. We will present initial results in the hope of sparking discussions, and finding interest for future collaborations.

Email krucker@berkeley.edu

Primary author

Sam Krucker

Presentation materials