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Radio Observations of High Energy Solar Flares

Published online by Cambridge University Press:  30 March 2016

Mukul R. Kundu
Mukul R. Kundu*
Affiliation:
Department of Astronomy, University of Maryland, College Park, MD 20742, USA

Abstract

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In this paper we discuss some recent observations of radio emission produced by high energy electrons resulting from solar flares. We discuss the spatial structure of simple weak spiky burst emissions observed simultaneously, at 17 and 34 GHz with the Nobeyama Radio Heliograph (NoRH). Using simultaneous imaging observations obtained by Yohkoh/HXT and SXT along with NoRH17 & 34 GHz observations, we attempt to model a relatively stronger and longer flare using gyrosynchrotron mechanism for the flaring radio emission.

Type
II. Joint Discussions
Information
Highlights of Astronomy , Volume 12: Highlights of Astronomy. As presented at the XXIVth General Assembly of the IAU, 2000 , 2002 , pp. 379 - 383
Copyright
Copyright © Astronomical Society of Pacific 2002

References

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