Quick reverse of the polarization sense of the spikes and FFS radiation.

Details Quick reverse of the polarization sense of the spikes and FFS radiation. Quick reverse of the polarization sense of the spikes and FFS radiation.

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993acaps..13..270j&link_type=abstract

Acta Astrophys. Sin., Vol. 13, No. 3, p. 270 - 277

Astronomy and Astrophysics

Astrophysics

Scientific paper

The spikes and fast fine structures (FFS) superimposed on the microwave burst with the type 47GB on May 16, 1991 were introduced briefly. The polarizations of the spikes and FFS recorded at 2545 MHz and 2645 MHz were reversed quickly and alternately in 50 - 100 milliseconds time scale. This is related to the fluctuations of the plasma density and the magnetic field of the source region in a small space scale. It leads to the growth of the electron-cyclotron maser to control the radiation of the X-mode or O-mode wave, and to reverse the sense of the polarization of the spikes and FFS.

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