Hostname: page-component-cd9895bd7-fscjk Total loading time: 0 Render date: 2024-12-23T19:52:40.509Z Has data issue: false hasContentIssue false
  • English
  • Français

Flaring Processes in Stellar Atmospheres: The Importance of Electromagnetic Coupling

Published online by Cambridge University Press:  12 April 2016

D.S. Spicer
D.S. Spicer*
Affiliation:
ETH Zentrum, Institute of Astronomy, Zurich, Switzerland

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Linsky: We do not know all of the energy released in the course of a dMe star flare. What we actually measure however is often 104 to 105 times larger than what is seen in large solar flares. I have two questions. Why do you think flares in dMe stars are so much more energetic than in the solar case? Secondly, why are solar flares so much less energetic than those in dMe stars?

Type
Session IV: Theoretical Aspects
Information
International Astronomical Union Colloquium , Volume 71: Activity in Red-Dwarf Stars , 1983 , pp. 559 - 560
Copyright
Copyright © Reidel 1983