Relations between solar radio millisecond spike-type III bursts in metric waves and acceleration processes of coronal electrons
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[1] M. Kundu,et al. Non-radial magnetic field structures in the solar corona , 1994 .
[2] G. Chernov. Whistlers in the solar corona and their relevance to fine structures of type IV radio emission , 1990 .
[3] J. Kurths,et al. On a sequence of remarkable fine structures in the type IV burst of 24 April, 1985 , 1987 .
[4] H. Urbarz. Occurrence of solar decimetric spike bursts over a period of 4 years during the 21st cycle , 1986 .
[5] M. Perrenoud,et al. Millisecond structures in solar radio emission close to 264 MHz , 1984 .
[6] O. P. Sveen,et al. Drifting spikes—a new species of solar radio bursts , 1979, Nature.