Comparison of the solar corona and the coronae above accretion disks surrounding black holes

Details Comparison of the solar corona and the coronae above accretion disks surrounding black holes Comparison of the solar corona and the coronae above accretion disks surrounding black holes

Nov 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..801..188c&link_type=abstract

ASTROPHYSICAL SOURCES OF HIGH ENERGY PARTICLES AND RADIATION. AIP Conference Proceedings, Volume 801, pp. 188-191 (2005).

Astronomy and Astrophysics

Astrophysics

1

Solar Corona, Accretion Disks, Black Holes, Black Holes

Scientific paper

We develope a model of an accretion disk corona motivated by the observed solar corona. Such a model consists of many unresolved magnetic loops coexisting above the disk surface. We compare the predicted energy-dependent fractional variability amplitude with the observed one, both for standard rms(E) and point-to-point rms(E). Finally, we compare the parameters of a single large flare seen in the lightcurve of MCG -6-15-30 with large solar flares.

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