Stellar Flares and Coronal Structure

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dc.creatorGuedel, M.
dc.date2003-12-15
dc.date.accessioned2026-07-07T02:11:35Z
dc.date.available2026-07-07T02:11:35Z
dc.descriptionCoronal structure and coronal heating are intimately related in magnetically active stars. Coronal structure is commonly inferred from radio interferometry and from eclipse and rotational modulation studies. We discuss to what extent flares may be responsible for coronal structure and global observable properties in magnetically active stars.
dc.descriptionto appear in proceedings of IAU Symposium 219, Stars as Suns: Activity, Evolution, Planets; preprint also at http://www.astro.phys.ethz.ch/papers/guedel/guedel_p_nf.html
dc.identifierhttps://arxiv.org/abs/astro-ph/0312378
dc.identifierhttp://arxiv.org/abs/astro-ph/0312378
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7142
dc.subjectAstrophysics
dc.titleStellar Flares and Coronal Structure
dc.typetext

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