Metric and Decimetric Observations of the Quiet Solar Corona

Details Metric and Decimetric Observations of the Quiet Solar Corona Metric and Decimetric Observations of the Quiet Solar Corona

Oct 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999esasp.446..483m&link_type=abstract

8th SOHO Workshop: Plasma Dynamics and Diagnostics in the Solar Transition Region and Corona. Proceedings of the Conference hel

Astronomy and Astrophysics

Astrophysics

4

Scientific paper

We describe a multi-wavelength analysis of the solar corona in the metric and decimetric range for a period in May 1992. The four radio wavelengths, available with the Nancay Radioheliograph provide a 3-dimensional view of the corona from about 1.05 to 1.2 solar radius. Some of the radio features are relative to the large scale structure of the corona (coronal plateau, coronal holes) and to medium scale structures (streamers) we can follow during their transit on the disk. We also observe thermal emission associated to active regions and we compare locations of radio emissions with structures of the X-ray loops.

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