Hostname: page-component-cd9895bd7-jkksz Total loading time: 0 Render date: 2024-12-24T01:39:10.487Z Has data issue: false hasContentIssue false

The Spatial Structure of Solar Microwave Bursts

Published online by Cambridge University Press:  14 August 2015

K. A. Marsh
Affiliation:
California Institute of Technology
G. J. Hurford
Affiliation:
California Institute of Technology
H. Zirin
Affiliation:
California Institute of Technology

Extract

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.

Observations of five impulsive microwave bursts were made during July 15–18, 1978 using the VLA at 4.9 GHz with temporal and spatial resolutions of 10 s and up to 1″ respectively. A series of 2-dimensional snapshot synthesis maps was made as a function of time, and compared with Hα photographs and magnetograms. Each flare was characterized by a single source of constant size, located on the magnetic neutral line between the Hα kernels.

Type
Session III - Solar Bursts - cm Wavelengths
Copyright
Copyright © Reidel 1980