Hostname: page-component-cd9895bd7-8ctnn Total loading time: 0 Render date: 2024-12-13T00:08:10.373Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

(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