Quiet Sun and slowly varying component at meter and decameter wavelengths |
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| Authors: | P Lantos C E Alissandrakis T Gergely M R Kundu |
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| Institution: | (1) Observatoire de Meudon, 92195 Heudon, France;(2) Laboratory of Astrophysics, National University of Athens, 15771 Athens, Greece;(3) Astronomy Program, University of Maryland, 20742 College Park, MD, U.S.A. |
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| Abstract: | Comparison of maps of the Sun obtained over the period June 29 to July 8, 1982 at 169 MHz with the Nançay Radioheliograph and at 73.8, 50, and 30.9 MHz with the Clark Lake Radioheliograph shows that the slowly varying component at meter and decameter wavelengths is not always thermal emission. During the period under study weak noise storm continua were the most frequent sources of slowly varying component at 169 and 73.8 MHz. Most filaments show no radio counterpart on the disk. A streamer has been detected on the disk from 169 to 30.9 MHz with an optimum observability at 50 MHz. The brightest source of the slowly varying component from 73.8 to 30.9 MHz for most of the period was located above an extended coronal hole in a region where a depression was observed at 169 MHz. In favorable cases, electron densities can be derived from the positions of noise storms and radio streamers; these are in agreement with previous K-corona eclipse observations. |
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