Low Frequency Observations of the Quiet Sun: a Review

Physics

Scientific paper

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Scientific paper

We present a review of the results obtained on the quiet sun at long decimeter, meter and decameter wavelengths with radioheliographs. Similarities and differences of the radio corona with the corona seen at other wavelengths are analysed. Large-scale structures including coronal holes, the coronal plateau (the radio counterpart of the coronal plasma sheet) and the background quiet sun are considered. The sources of the slowly varying component are identified and described. The importance of low frequency observations of the sun, in addition to X-ray and EUV observations, is pointed out for a better understanding of coronal and solar-terrestrial physics.

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