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Radio and X-ray diagnostics of electrons accelerated in solar flares

Published online by Cambridge University Press:  01 August 2006

Miroslav Bárta  and
Marian Karlický
Miroslav Bárta
Affiliation:
Astronomical Institute of the Academy of Sciences of the Czech Republic, CZ-25165 Ondřejov, Czech Republic email: barta@asu.cas.cz, karlicky@asu.cas.cz
Marian Karlický
Affiliation:
Astronomical Institute of the Academy of Sciences of the Czech Republic, CZ-25165 Ondřejov, Czech Republic email: barta@asu.cas.cz, karlicky@asu.cas.cz
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Abstract

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Starting from 2.5D MHD modelling of solar flares on a global scale we calculate (using the PIC and test-particle simulations) the radio and X-ray emissions generated in solar flare reconnection. Our results – the radio and X-ray spectra and brightness distributions, and their dynamics – are directly comparable with observations providing thus a test of particle acceleration models as well as of the ‘standard’ global flare scenario.

Keywords

Solar flaresacceleration of particlesradio and X-ray emissions
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Highlights of Astronomy 14: Highlights of Astronomy , August 2006 , pp. 88
Copyright
Copyright © International Astronomical Union 2007

References

Karlický, M., & Bárta, M. 2006, ApJ, 647, 1472Google Scholar
Karlický, M., & Kosugi, T. 2004, A&A, 419, 1159Google Scholar
Karlický, M., Bárta, M., Meszárosová, H., & Zlobec, P. 2005, A&A, 432, 705Google Scholar
Kliem, B., Karlický, M., & Benz, A.O. 2000, A&A, 360, 715Google Scholar