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Stellar Flares and Coronal Structure

Published online by Cambridge University Press:  26 May 2016

Manuel Güdel
Manuel Güdel*
Affiliation:
Paul Scherrer Institut, 5232 Villigen PSI, Switzerland

Abstract

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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.

Type
Part 4: High Energy Phenomena in Sun and Stars
Information
Symposium - International Astronomical Union , Volume 219: Stars as Suns : Activity, Evolution and Planets , 2004 , pp. 159 - 170
Copyright
Copyright © Astronomical Society of the Pacific 2004 

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