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- W2017651405 abstract "This paper describes the quasi-periodic fine structures (FS) in a solar radio burst which was observed with time resolution of 10ms at 3.2cm wavelength on 23 May 1990. The radio burst was associated with a M8.7/1B flare occurred in the active region AR 6063. The average period of these fine structures is about 1.5s and the amplitude modulation range from 2% to 5%. A preliminary analysis shows that there is a linear relation between the mean flux S of the radio burst and the repetition rate R of the quasiperiodic fine structures at 3.2cm wavelength. This relation is similar to that obtained by Kaufmann et al. in millimeter wavelength region. We suggest that these quasi-periodic fine structures probably reflect the modulated gyro-synchrotron emission due to MHD waves oscillating along magnetic field lines." @default.
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- W2017651405 date "1992-01-01" @default.
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- W2017651405 title "The quasi-periodic fine structures in a solar radio burst at 3.2 cm wavelength on 23 May 1990" @default.
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- W2017651405 doi "https://doi.org/10.1016/0275-1062(92)90012-z" @default.
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