Stellar Flares and Coronal Structure
天体物理学
2007-05-23 v1
摘要
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.
引用
@article{arxiv.astro-ph/0312378,
title = {Stellar Flares and Coronal Structure},
author = {M. Guedel},
journal= {arXiv preprint arXiv:astro-ph/0312378},
year = {2007}
}
备注
to 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