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Solar and Interplanetary Radio Emissions
2010Recent progress on radio emissions from the Sun and in the interplanetary medium is reviewed, with particular emphases on type II and III solar radio bursts, and emissions from the Earth’s foreshock. Observations from single or multi spacecraft and ground-based instruments have provided new insights into interactions of beam-wave, wave-wave, and wave ...
Bo Li +2 more
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Pulsating Solar Radio Emission
2007A status report of current research on pulsating radio emission is given, based on working group discussions at the CESRA 2004 workshop. Quasi-periodic pulsations have been observed at all wavelength ranges of the radio band. Usually, they are associated with flare events; however since the late 90s, pulsations of the slowly-varying component of the ...
Alexander Nindos, Henry Aurass
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Phenomenology of Solar Radio Emission
1979A number of solar phenomena are observed at different radio and other wavelengths exhibiting characteristic time scales ranging from small fractions of a second to tens of years. These variations of the solar radiation are closely connected with solar activity and form a part of it.
exaly +2 more sources
Anomalous Scintillation of Solar Radio Emission
Publications of the Astronomical Society of Japan, 1961Abstract A peculiar type of scintillation of solar radio emission is discussed. From the statistical study and the simultaneous observations with two separated antennae, it is found that the scintillation does not originate in the ionosphere but in the troposhpere.
Atsushi Tsuchiya, Masaki Morimoto
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Envelope Soliton in Solar Radio Emission
Chinese Physics Letters, 2000Several envelope soliton fine structures have been observed in solar radio metric-wave emission. We present a model of longitudinal modulational instability to explain these fine structures. It is found that this instability can only occur in the condition of sound velocity being larger than Alfven velocity in corona.
Wang De-Yu, G P Chernov
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1970
All radiation processes described can take place in the solar corona, depending on different physical characters of the radiating electrons and the coronal plasma, such as electron energy, electron pitch angle and the magnitude of the ratio f-2p/f-2H of the medium in the region where the radiators reside.
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All radiation processes described can take place in the solar corona, depending on different physical characters of the radiating electrons and the coronal plasma, such as electron energy, electron pitch angle and the magnitude of the ratio f-2p/f-2H of the medium in the region where the radiators reside.
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Solar Radio Emissions and Sunspots
Nature, 1948THE ratio of the equivalent source temperatures as deduced from observations of solar electromagnetic radiation for frequencies of 80 Mc./s. and 175 Mc./s. (T80/T175) by Ryle and Vonberg1 would appear to have considerable significance to solar as well as radio physicists.
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Theory of Solar Radio Emission
1979Any theory and interpretation of solar radio waves is inevitably connected with certain parameters characterizing the physical conditions of the plasma medium of the solar atmosphere, in which the relevant processes of the wave origin and propagation take place.
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The emission mechanisms for solar radio bursts
Space Science Reviews, 1980Emission mechanisms for meter-λ solar radio bursts are reviewed with emphasis on fundamental plasma emission.
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Some results of solar radio emission observations at the Siberian Solar Radio Telescope
Astronomische Nachrichten, 1990AbstractThis paper gives the main characteristics of the Siberian Solar Radio Telescope as well as some results derived by investigating the s‐component sources and radio bursts on the Sun using the SSRT.
G. N. Zubkova +6 more
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