Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3840
Title: Radio emission by parallel acceleration mechanism
Authors: Krishan, V
Sivaram, C
Keywords: Electron Beams;Harmonic Generations;Magnetohydrodynamic Stability;Particle Acceleration;Solar Magnetic Field;Type 3 Bursts;Beam Interactions;Emission Spectra;Particle Trajectories;Plasma Interactions
Issue Date: Apr-1983
Publisher: Springer
Citation: Solar Physics, Vol. 84, No. 1 - 2, pp. 125 - 130
Abstract: The equations describing the linear-acceleration mechanism of radiation emission are generalized and applied to type III and IIIb solar radio bursts. A general expression for the power emitted by an electron in a spatially and temporally periodic electromagnetic/electrostatic field parallel to the ambient magnetic field is derived, allowing for harmonic generation and relaxing the dipole approximation used in previous quantifications of the mechanism. The general expression is used to calculate the radiation due to the electric field generated by saturation-phase beam-plasma instability in the proposed linear-acceleration model of III/IIIb-type solar radio bursts.
Description: Open Access
URI: http://hdl.handle.net/2248/3840
ISSN: 0038-0938
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http://adsabs.harvard.edu/abs/1983SoPh...84..125K
Appears in Collections:IIAP Publications

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