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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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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.
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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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Polarization of Solar Radio-frequency Emissions
Nature, 1946THE recent experimental proof1 that the sun emits energy on radio frequencies was followed by evidence2 that the amount of such energy can increase markedly during the passage of important sunspots across the solar disk. Such sunspots are invariably associated with strong magnetic fields, the influence of which almost certainly extends into the upper ...
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Radio cyclotron emission from extra-solar planets
Proceedings of the International Astronomical Union, 2008AbstractWe present results from an attempt to detect radio emission from the interaction between a transiting extra-solar planet and its host star. We determine a new upper limit of 47 mJy on the radio flux density from HD 189733b, in the frequency range 327–347 MHz.
Alexis Smith +5 more
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Microwave Bursts of Solar Radio Emission
Publications of the Astronomical Society of Japan, 1960Abstract Wide-band compound dynamic spectra of solar radio outbursts have been studied in the frequency range from 9500 Mc to 67 Mc. The range of 9500–1000 Mc has been covered by the records at several fixed frequencies, and both the swept frequency records and fixed frequency records have been used on the frequencies below 1000 Mc.
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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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Pulsating radio emissions from the solar corona
Solar Physics, 1970Three solar outbursts which show pulsating radio emissions at metric waves (239 MHz) are examined. The behaviour of the single frequency, high-time resolution records and the spectral diagrams seem to indicate that such phenomena are peculiar phases of type IV radiation, perhaps connected with absorptions in the solar corona.
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Directivity of Radio Emission from Solar Flares
Publications of the Astronomical Society of Japan, 1985Abstract The center-limb variation of the solar microwave burst intensity is investigated statistically with a sufficient number of events (~ 1000) at 17 GHz far above the mean turnover frequency of the microwave burst spectrum. The intensity of bursts (except that of GRF bursts) is independent of the disk longitude, which is slightly ...
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Sporadic solar radio emission at decameter wavelengths
2005Results of observations of the solar sporadic radio emission in decameter range are presented. These observations were carried out at UTR-2 radio telescope with 60-channel spectrometer and DSP (Digital Spectral Polarimeter) last years. Particular attention is devoted to such components of sporadic radio emission as Type III bursts, Type II bursts ...
Melnik, Valentin N. +7 more
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