Results 241 to 250 of about 106,724 (293)
Reading signatures of supermassive binary black holes in pulsar timing array observations. [PDF]
Goncharov B +12 more
europepmc +1 more source
A Faint Progenitor System for the Faint Supernova 2024vjm
Zimmerman E +69 more
europepmc +1 more source
Some of the next articles are maybe not open access.
Related searches:
Related searches:
RADIO EMISSION FROM SOLAR FLARES
Annual Review of Astronomy and Astrophysics, 1998▪ 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, D. E. Gary
openaire +3 more sources
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
openaire +1 more source
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
openaire +1 more source
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
openaire +1 more source
2023
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.
openaire +1 more source
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.
openaire +1 more source
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
openaire +2 more sources

