Evolution of the coronal plasma sheet from cycle maximum to cycle minimum observed at meter wavelengths

Details Evolution of the coronal plasma sheet from cycle maximum to cycle minimum observed at meter wavelengths Evolution of the coronal plasma sheet from cycle maximum to cycle minimum observed at meter wavelengths

Aug 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995adspr..16..185l&link_type=abstract

Advances in Space Research (ISSN 0273-1177), vol. 16, no. 9, p. (9)185-(9)188

Computer Science

Current Sheets, Heliosphere, Mapping, Solar Corona, Solar Cycles, Sunspots, Brightness Temperature, Corotation, International Quiet Sun Year, Particle Acceleration, Solar Wind, Spectroheliographs

Scientific paper

The Nancay Radioheliograph provides maps of the quiet solar corona around 160 MHz. In addition to coronal holes, localized emission sources and quiet sun, an unresolved component can be detected on the disk. The so-called 'coronal plateau' corresponds to the K-corona dense regions observed on the limb and is thus located at the base of the interplanetary plasma sheet. Its evolution is studied from 1980 to 1986, during the declining phase of the cycle 21.

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