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Magnetic Fields in the Lower Corona Associated with the Expanding Limb Burst On March 30th 1969 Inferred from the Microwave High-Resolution Observations

Published online by Cambridge University Press:  14 August 2015

Shinzo Énomé  and
Haruo Tanaka
Shinzo Énomé
Affiliation:
The Research Institute of Atmospherics, Nagoya University, Japan
Haruo Tanaka
Affiliation:
The Research Institute of Atmospherics, Nagoya University, Japan

Abstract

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An expansion of the source of a great solar microwave burst was observed a little beyond the west limb on March 30, 1969. This expansion is interpreted in terms of diffusion of energetic electrons in a turbulent magnetic field in the flare region. The height of the source is estimated to have been 104 km.

Type
Part IV: Observations of Magnetic Fields Associated with Flares and Other Transitory Phenomena
Information
Symposium - International Astronomical Union , Volume 43: Solar Magnetic Fields , 1971 , pp. 413 - 416
Copyright
Copyright © Reidel 1971 

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