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Radio echo and sporadic radiation scattering in the solar corona

โœ Scribed by E. P. Abranin; L. L. Bazelyan; V. V. Zaitsev; V. O. Rapoport; Ya. G. Tsybko


Publisher
Springer
Year
1982
Tongue
English
Weight
377 KB
Volume
78
Category
Article
ISSN
0038-0938

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โœฆ Synopsis


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 = 2Re has been also found during the burst lifetime.


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