Radio echo and sporadic radiation scattering in the solar corona |
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Authors: | E P Abranin L L Bazelyan V V Zaitsev V O Rapoport Ya G Tsybko |
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Institution: | (1) Institute of Radiophysics and Electronics AN UkSSR, Khar'kov, U.S.S.R.;(2) Applied Physics Institute, AN USSR, Gorky, U.S.S.R.;(3) Radiophysical Research Institute, Gorky, U.S.S.R. |
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Abstract: | Some properties of solar radio bursts observed at the Earth are mainly due to propagation effects in the corona. A radio echo of short-time narrow-band bursts is observed by a decameter radioheliograph on the basis of UTR-2 antenna. Propagation effects are manifested in the marked regular change of the burst intensity-time profile at 25 MHz during a half-rotation of the Sun. A displacement of limb diffuse bursts deep into the solar atmosphere of 1.5 - 2R
has been also found during the burst lifetime. |
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