The new features of spikes received at 2545 and 2645 MHz frequencies.

Details The new features of spikes received at 2545 and 2645 MHz frequencies. The new features of spikes received at 2545 and 2645 MHz frequencies.

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993pbeio..21....6j&link_type=abstract

Publications of the Beijing Astronomical Observatory, No. 21, p. 6 - 13

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Solar Microwave Bursts: Fine Structure

Scientific paper

In this paper, some new features of spike radiations and other fast fine structures of microwave bursts at 2545 and 2645 MHz frequencies, such as the narrow bandwidth, the rapid frequency drift, the quasi-oscillation and the quick reversion of the polarization senses are introduced and discussed. These features may be closely related to the electro-cyclotron instability, the wave beam resonance condition, the movement of the MHD wave and the nonthermal beam in the solar corona source region.

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