Abstract
Two-dimensional maps of circularly polarized emission from the Sun at 7.8 GHz, with a resolution of 4.4 arc minutes, show polarization of local sources of up to 15% and variations as small as 2% in flux density and 0.2% in polarization, as functions of time. Both flux density and polarization in McMath plage 11002 showed substantial increases thirty minutes or more before a flare on October 24, 1970. It is suggested that flares may be triggered when both of these quantities surpass critical values.
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RICHARDS, D., STRAKA, R. Mapping of Solar Polarization at 7.8 GHz. Nature Physical Science 233, 92–94 (1971). https://doi.org/10.1038/physci233092a0
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DOI: https://doi.org/10.1038/physci233092a0
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