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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

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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