Stellar Flares and Coronal Structure

Astronomy and Astrophysics – Astrophysics

Scientific paper

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to appear in proceedings of IAU Symposium 219, Stars as Suns: Activity, Evolution, Planets; preprint also at http://www.astr

Scientific paper

Coronal 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.

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