Hostname: page-component-7bb8b95d7b-495rp Total loading time: 0 Render date: 2024-09-22T10:25:41.819Z Has data issue: false hasContentIssue false
  • English
  • Français

Multiple Magnetic-Loop Structure of a Type IV Solar Radio Outburst

Published online by Cambridge University Press:  25 April 2016

R. T. Stewart  and
K. V. Sheridan
R. T. Stewart
Affiliation:
Division of Radiophysics, CSIRO, Sydney
K. V. Sheridan
Affiliation:
Division of Radiophysics, CSIRO, Sydney
Get access Rights & Permissions [Opens in a new window]

Extract

In this paper we discuss 80 MHz heliograph observations of the multiple source structure and polarization of a type IV solar radio outburst on 1970 November 16. At times during the event six sources were present. Three of these were highly circularly polarized in a L.H. sense and two in a R.H. sense. The sixth source was extended and had oppositely polarized edges. From the source behaviour we conclude that the radio emission came from two expanding and one stationary magnetic arch.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 2 , Issue 1 , July 1971 , pp. 60 - 62
Copyright
Copyright © Astronomical Society of Australia 1971

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

1 Wild, J. P., Solar Phys., 9, 260 (1969).Google Scholar
2 Solar Geophysical Data, No. 317, Pt. I, U.S. Dept. Commerce (January 1971).Google Scholar
3 Altschuler, M. D. and Newkirk, G. Jr., Solar Phys., 9, 131 (1969).Google Scholar