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The possibility of a change in the intensity of the radio emission from galactic sources

โœ Scribed by V. A. Sanamyan


Publisher
Springer
Year
1966
Tongue
English
Weight
198 KB
Volume
2
Category
Article
ISSN
0571-7256

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The effects of scattering and refraction on radio waves in the solar corona are considered for several different coronal models. By considering a source near the plasma level in a spherically symmetric corona and in a streamer enhancement superimposed on a spherically symmetric corona we obtain resu