Article contents
Stellar Flares and Coronal Structure
Published online by Cambridge University Press: 26 May 2016
Abstract
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
References
- 1
- Cited by