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Astrophysics and Space Science Library, 1977
Outside active regions the Sun produces radio emission that is due entirely to bremsstrahlung from thermal electrons — the quiet-Sun radio emission. Radiation of frequency f originates at and above the level where f = f p (= plasma frequency), i.e.
A D Fokker
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Outside active regions the Sun produces radio emission that is due entirely to bremsstrahlung from thermal electrons — the quiet-Sun radio emission. Radiation of frequency f originates at and above the level where f = f p (= plasma frequency), i.e.
A D Fokker
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Advances in Space Research, 2005
Abstract In this paper, we present a tutorial review which was presented at the first Advanced School on Space Environment (ASSE 2004). We first describe the basics of radioastronomy definitions, and discuss radiation processes relevant to solar radio emissions like plasma emission, free–free bremsstrahlung and gyromagnetic emissions.
J.-P. Raulin, A.A. Pacini
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Abstract In this paper, we present a tutorial review which was presented at the first Advanced School on Space Environment (ASSE 2004). We first describe the basics of radioastronomy definitions, and discuss radiation processes relevant to solar radio emissions like plasma emission, free–free bremsstrahlung and gyromagnetic emissions.
J.-P. Raulin, A.A. Pacini
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Solar radio emission surveillance by the Trieste Solar Radio System 2.0
2020 XXXIIIrd General Assembly and Scientific Symposium of the International Union of Radio Science, 2020In this paper we describe the Trieste Solar Radio System 2.0 (TSRS 2.0), a project for a new facility dedicated to the continuous surveillance of the solar radio emission in the range 1-19 GHz. It is presently under development at the INAF Astronomical Observatory of Trieste and will be installed at the Basovizza Observing Station.
Giovanna Jerse +7 more
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RADIO EMISSION FROM SOLAR FLARES
▪ Abstract Radio emission from solar flares offers a number of unique diagnostic tools to address long-standing questions about energy release, plasma heating, particle acceleration, and particle transport in magnetized plasmas. At millimeter and centimeter wavelengths, incoherent gyrosynchrotron emission from electrons with energies of tens of kilo ...
T S Bastian, A O Benz, Dale E Gary
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Radio evidence for solar corpuscular emission
Planetary and Space Science, 1964Abstract : This paper reviews the relation of solar radio bursts of spectral type IV to the ejection of relativistic and sub-relativistic solar particles; the relation of bursts of types II and IV to the ejection of solar plasma; and radar evidence for quiet solar streaming.
A. Maxwell, R.J. Defouw, P. Cummings
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1985
The subject of solar radio emission is quite broad and has been reviewed repeatedly in articles and books (Wild et al., 1963; Kundu, 1965; Zheleznyakov, 1970; Wild and Smerd, 1972; Rosenberg, 1976; Smerd, 1976a; Kruger, 1979; Melrose, 1980a). In addition, recent conference proceedings include issue 9 of Radiophysics and Quantum Electronics 20 (1977 ...
Martin V. Goldman, Dean F. Smith
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The subject of solar radio emission is quite broad and has been reviewed repeatedly in articles and books (Wild et al., 1963; Kundu, 1965; Zheleznyakov, 1970; Wild and Smerd, 1972; Rosenberg, 1976; Smerd, 1976a; Kruger, 1979; Melrose, 1980a). In addition, recent conference proceedings include issue 9 of Radiophysics and Quantum Electronics 20 (1977 ...
Martin V. Goldman, Dean F. Smith
openaire +1 more source

