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The Spatial Structure of Solar Microwave Bursts
Published online by Cambridge University Press: 14 August 2015
Extract
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
- Information
- Symposium - International Astronomical Union , Volume 86: Radio Physics of the Sun , 1980 , pp. 191 - 194
- Copyright
- Copyright © Reidel 1980
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