Active Late-Type Stellar Coronae: Hints for Flare Heating?

Details Active Late-Type Stellar Coronae: Hints for Flare Heating? Active Late-Type Stellar Coronae: Hints for Flare Heating?

May 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000iaus..195..377a&link_type=abstract

Highly Energetic Physical Processes and Mechanisms for Emission from Astrophysical Plasmas, Proceedings of IAU Symposium #195, h

Astronomy and Astrophysics

Astrophysics

Scientific paper

The Extreme Ultraviolet Explorer data archive has been used to study flare energy distributions and infer the role of flares in coronal heating. We have constructed flare number distributions as a function of observed EUV and X-ray emitted thermal energy. We find cumulative flare distributions of the form N(> E) ~E-α +1 with α ~1.5--2.6. We present results in the context of spectral type classification.

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