Physics
Scientific paper
Mar 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987soph..111..201l&link_type=abstract
(Observatoire de Paris, CNRS, CNES, et al., CESRA Workshop on Particle Acceleration and Trapping in Solar Flares, 2nd, Aubigny-s
Physics
12
Cyclotron Radiation, High Energy Electrons, Masers, Solar Radio Bursts, Stellar Radiation, Distribution Functions, Harmonic Radiation
Scientific paper
A fully relativistic electron maser is proposed for the explanation of certain nonthermal solar and stellar radio bursts. This mechanism (maser synchrotron) is based on a gyroresonant interaction between waves and electrons of high energies and uses the free energy contained in an electronic distribution function that peaks for energies around 1 MeV. By a calculation of the growth rates of the three electromagnetic modes, it is shown that the X-mode prevails for values of omega(p)/omega(c) up to 2 or 3. This result is very different from the standard cyclotron maser case where such values of omega(p)/omega(c) lead to quench the X-mode growth. Hence, the synchrotron maser instability appears to be a direct and efficient amplification process for considerably larger physical conditions than the cyclotron maser. In addition, the radiation, emitted over the second gyroharmonic, freely propagates without a strong reabsorption at the omega(c) layer. All these points can constitute major advantages of this mechanism in an astrophysical context.
Le Queau Dominique
Louarn Ph.
Roux Alain
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