Hostname: page-component-586b7cd67f-gb8f7 Total loading time: 0 Render date: 2024-11-26T12:50:19.435Z Has data issue: false hasContentIssue false
  • English
  • Français

Evolution of a Jet-like Structure in the Late Phase of a Complex Solar Outburst

Published online by Cambridge University Press:  25 April 2016

A. C. Riddle  and
K. V. Sheridan
A. C. Riddle
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

A new feature in the form of a jet formed by close juxtaposition of a number of highly polarized, separately resolved 80 MHz sources was observed as the late phase of a very complex outburst on 1971 January 25. We present here a source model which, we think, can explain the observed source properties. The early phase, also complex and involving numerous moving sources, will be described first.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 2 , Issue 1 , July 1971 , pp. 62 - 65
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 Solar Geophys. Data, No. 318 Part I, U.S. Dept. Commerce, (February 1971)Google Scholar
2 Wild, J. P. (ed.), ‘The Culgoora Radioheliograph’, Proc. IREE Aust., 28, No. 9 (1967).Google Scholar
3 Wild, J. P., Solar Phys., 9, 260 (1969).CrossRefGoogle Scholar
4 Kai, K., Solar Phys., 11, 310 (1970).CrossRefGoogle Scholar
5 Wild, J. P., Proc. ASA, 1, 365 (1970).Google Scholar
6 Dulk, G. A., Aust. J. Phys., 24, 177 (1971).Google Scholar
7 Dulk, G. A., Proc. ASA, 1, 372 (1970).Google Scholar