Sofia Tynelius

ORCID: 0000-0001-7793-5646
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About
Contact & Profiles
Research Areas
  • Solar and Space Plasma Dynamics
  • Solar Radiation and Photovoltaics
  • Ionosphere and magnetosphere dynamics

ETH Zurich
2022

Context. We present an analysis of a GOES M1.8 flare with excellent observational coverage in UV, EUV, and X-ray, including observations from the instruments IRIS, SDO AIA, Hinode/EIS, Hinode/XRT, Solar Orbiter Spectrometer/Telescope for Imaging X-rays (STIX). Hard X-ray emission is often observed at footpoints loops occasionally corona. In this flare, four nonthermal hard sources are seen. Aim. Our aim to understand why we can observe individual how characterize physical properties these...

10.1051/0004-6361/202245044 article EN cc-by Astronomy and Astrophysics 2022-12-20
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