A new explanation of solar radio millisecond 'spikes'

Details A new explanation of solar radio millisecond 'spikes' A new explanation of solar radio millisecond 'spikes'

Apr 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993apj...407..380w&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 407, no. 1, p. 380-384.

Physics

7

Electron Beams, Electron Scattering, Solar Electrons, Solar Physics, Solar Radio Emission, Electrostatic Waves, Solar Magnetic Field

Scientific paper

The study proposes an explanation for solar radio spikes that involves an electromagnetic instability in fast electrons at a frequency of greater than 2 Omega (Omega = cyclotron frequency), so that the radiation can escape, and in which the unstable anisotropy is easily regenerated. The instability occurs after scattering of an electron beam by Langmuir waves. The radiation grows best along surfaces of constant magnetic field strength and has very narrow intrinsic bandwidth.

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