Astronomy and Astrophysics – Astrophysics
Scientific paper
2003-12-15
Astronomy and Astrophysics
Astrophysics
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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