Physics – Optics
Scientific paper
Oct 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989azh....66.1061i&link_type=abstract
Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 66, Sept.-Oct. 1989, p. 1061-1068. In Russian.
Physics
Optics
1
Radio Transmission, Solar Corona, Type 3 Bursts, Differential Equations, Electron Flux Density, Geometrical Optics, Radio Echoes, Solar Limb
Scientific paper
Geometrical optics is used to perform a ray-tracing analysis of radio waves in the solar corona in the presence of large-scale ducts. It is shown that some of the characteristic features of type III bursts can be explained by taking into account the effects of radio-wave propagation in the inhomomgenous coronal plasma. In particular, it is possible to explain the fact that the radial coordinates of the point of radio-wave emergence from the corona exceed the level of the fundamental plasma frequency, and the fact that the bursts of decametric storms are observed at the fundamental frequency near the central meridian and at the second harmonic near the solar limb.
Itkina M. A.
Yashnov V. A.
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