Radio observations of the quiet solar corona

Details Radio observations of the quiet solar corona Radio observations of the quiet solar corona

Apr 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994adspr..14...81a&link_type=abstract

Advances in Space Research, vol. 14, no. 4, p. (4)81-(4)91

Physics

4

Coronal Holes, Current Sheets, Electron Energy, Radio Emission, Satellite Observation, Solar Corona, Solar Prominences, Heliosphere, Plasma Diagnostics, Refraction, Solar Cycles, Solar Limb, Solar Wind, Spatial Resolution

Scientific paper

Observations of radio emission from the quiet solar atmosphere and the associate emission mechanisms are discussed. Long wavelength observations, with a spatial resolution of approximately 1 arc min are ideal for the study of the large scale structure of the corona, including coronal holes, arches, streamers and the base of the heliospheric current sheet. These structures are observed both beyond the limb and on the solar disk, with little line of sight integration. We also discuss diagnostics of electron temperature and density, as well as the interpretation problems arising from the inhomogeneity of the corona and refraction effects.

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