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Accretion Disk Flares in Energetic Radiation Fields

Published online by Cambridge University Press:  19 July 2016

R.F. Van Oss ,
G.H.J. Van Den Oord  and
M. Kuperus
R.F. Van Oss
Affiliation:
Sterrekundig Instituut, P.O. Box 80000, 3508 TA Utrecht, The Netherlands
G.H.J. Van Den Oord
Affiliation:
Sterrekundig Instituut, P.O. Box 80000, 3508 TA Utrecht, The Netherlands
M. Kuperus
Affiliation:
Sterrekundig Instituut, P.O. Box 80000, 3508 TA Utrecht, The Netherlands

Abstract

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We consider the physics of magnetic flares in the energetic radiation field of an accretion disk corona (ADC). The X-ray emission from these flares is thought to be responsable for the observed hard powerlaw component in the X-ray spectra of galactic black hole candidates in their ‘high’ spectral state. During the flare event (inverse Compton) scattering of soft photons from the underlying disk into hard photons occurs on accelerated electrons in current sheets. The electrons are decelerated by the radiation drag force that results from the up-scattering. This friction-like effect of the intense background radiation field on the motion of the electrons in the sheet can be considered as a form of resistivity in the magnetohydrodynamical picture of the current sheet: Compton resistivity. A spectrum is derived for the up-scattered radiation from current sheets in the ADC and it is found that this spectrum mimics a powerlaw above a critical photon energy.

Keywords

accretion disksparticle accelerationmagnetic fieldsinverse Compton scattering
Type
5. Magnetic Field Generation in Accretion Disks
Information
Symposium - International Astronomical Union , Volume 157: The Cosmic Dynamo , 1993 , pp. 217 - 218
Copyright
Copyright © Kluwer 1993 

References

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