From solar nanoflares to stellar giant flares: Scaling laws and non-implications for coronal heating

Author:

Aschwanden Markus J.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Aerospace Engineering,General Earth and Planetary Sciences,Atmospheric Science,Geophysics,Astronomy and Astrophysics

Reference38 articles.

1. Evaporative cooling of flare plasma;Antiochos;ApJ,1978

2. Solar flare spectral diagnosis: present and future;Antonucci;SoPh,1989

3. Are coronae of magnetically active stars heated by flares? III. Analytical distribution of superimposed flares;Arzner;ApJ,2004

4. Flare plasma cooling from 30MK down to 1MK modeled from Yohkoh, GOES, and TRACE observations during the Bastille-Day Event (2000 July 14);Aschwanden;SoPh,2001

5. Aschwanden, M.J., Aschwanden, P.D. The fractal dimension of solar flares. ApJ, submitted for publication.

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