Rising motion of a behind-the-limb flare at 35 GHz

Details Rising motion of a behind-the-limb flare at 35 GHz Rising motion of a behind-the-limb flare at 35 GHz

May 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982soph...78..137k&link_type=abstract

Solar Physics, vol. 78, May 1982, p. 137-140. Ministry of Education, Science, and Culture

Physics

Microwave Emission, Solar Corona, Solar Flares, Solar Limb, Solar Radio Bursts, Diffraction Patterns, H Alpha Line, Radial Distribution, Radiant Flux Density, Radio Interferometers, Temporal Distribution, Velocity Distribution

Scientific paper

An observation of a behind-the-limb solar flare occurring on Sept. 7, 1977, using the 35 GHz solar interferometer at Nagoya, is described. The radio source lies in the coronal region higher than 7000 km above the photosphere and rises gradually at 25-35 km/s velocity. The fan-beam location of the radio source was measured by referring to the fringe patterns due to the quiet solar disk, and the height above the optical limb was determined by assuming that the latitude of the radio source was the same as that of the optical flare. The time profiles of the flux densities of the radio burst and the radial distance of the radio source from the center of the solar disk are shown.

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