Radio echo and sporadic radiation scattering in the solar corona

Details Radio echo and sporadic radiation scattering in the solar corona Radio echo and sporadic radiation scattering in the solar corona

May 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982soph...78..179a&link_type=abstract

Solar Physics, vol. 78, May 1982, p. 179-186.

Physics

10

Radio Echoes, Radio Scattering, Solar Corona, Solar Radio Bursts, Decametric Waves, Spectroheliographs

Scientific paper

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 approximately 2 solar radii has also been found during the burst lifetime.

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