On the harmonic structure of solar radio spikes

Details On the harmonic structure of solar radio spikes On the harmonic structure of solar radio spikes

Oct 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994soph..154..361f&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 154, no. 2, p. 361-369

Physics

28

Cyclotron Frequency, Frequency Stability, Harmonic Radiation, Masers, Momentum, Power Series, Relativistic Electron Beams, Solar Radio Emission, Electron Distribution, Frequency Distribution, Gyrofrequency, Wave Interaction

Scientific paper

This paper analyzes the frequency structure of the bands of electron-cyclotron maser instability. The calculations show that each term of the series describing the growth rate provides a double-peak structure, if we accept a nonthermal electron distribution with a 'two-side' loss-cone. The ratio of central frequencies is found to be non-integer in general case. We conclude that the harmonic structure of solar radio spikes observed in a number of events can be imitated by electron-cyclotron maser emission of mildly relativistic electrons with a power-law momentum distribution.

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