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Coronal Magnetic Field Structure Derived from Two-Frequency Radioheliograph Observations

Published online by Cambridge University Press:  25 May 2016

K. Kai  and
K. V. Sheridan
K. Kai
Affiliation:
Division of Radiophysics, CSIRO, Sydney, Australia
K. V. Sheridan
Affiliation:
Division of Radiophysics, CSIRO, Sydney, Australia

Abstract

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(Solar Phys.). An exceptional variety of positions and polarizations was found for two type I storms and numerous sporadic bursts observed during 15 consecutive days with the Culgoora radio-heliograph at 80 and 160 MHz.

Type
Part I Magnetic Structure Responsible for Coronal Disturbances
Information
Symposium - International Astronomical Union , Volume 57: Coronal Disturbances , 1974 , pp. 97 - 101
Copyright
Copyright © Reidel 1974