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Generation of highly energetic electrons at reconnection outflow shocks during solar flares - MaRDI portal

Generation of highly energetic electrons at reconnection outflow shocks during solar flares

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Publication:3618889

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DOI10.1051/0004-6361:200810099zbMATH Open1160.85309OpenAlexW2127141930WikidataQ68675039 ScholiaQ68675039MaRDI QIDQ3618889

Author name not available (Why is that?)

Publication date: 3 April 2009

Published in: Astronomy & Astrophysics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1051/0004-6361:200810099

zbMATH Keywords

shock waves gamma rays acceleration of particles Sun: flares Sun: radio radiation Sun: x-rays

Mathematics Subject Classification ID

Galactic and stellar structure (85A15) Radiative transfer in astronomy and astrophysics (85A25)

Related Items (2)

Title not available (Why is that?) ⋮ Electron acceleration in solar flares: theory of spectral evolution

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