Titlebook: Radio Continua During Solar Flares; Selected Contributio Arnold O. Benz Book 1986 Springer Science+Business Media Dordrecht 1986 Corona.Pla

Scintillations

EXPEL

On Fast Pulsations in Flare Continuaed, simultaneously or in time succession. Pulsations occur both in classical type IV events and in short-lasting continuum events. The power spectrum shows no large variation during one or two hours. Some implications of fast pulsations for the generation mechanism are discussed.

滲入

Exponential Decay and Exciter Profile of Fast Pulses in Type IV Eventsfficiently isolated from the adjacent pulsating activity, appear to have an exponential decay phase similar to that of fast type III bursts..A computational procedure, based on Fourier transform techniques, has been applied; it allows the computation, for every observed point in the time profile, of

syring

The Polarization of Decimetric Pulsationslarized, the other half showed a mild polarization of 15–55%. The polarization is constant in time and frequency for the strongly polarized group. All the mildly polarized bursts originate from near the limb; the lower degree of circular polarization is likely to be caused by depolarization due to p

發(fā)牢騷

Overthrow

FUSC

Millisecond Radio Spikesre fascinated by their high brightness temperature of up to 10. K, their association with hard X-ray bursts, and a possibly very intimate relation to electron acceleration. This review is intended to bridge the gap that presently seems to separate theory and observations. The wide range of spike obs

Abrade

淘氣

Wernickes-area

Hollow Beam Distribution of Energetic Electrons and Higher Harmonics of Electron Cyclotron Maserelectrons with a parameter ξ = ω./Ω. are presented in this paper. The results show that the second harmonic of ECM in .-mode dominates the instability if ξ < 1, and if 1.2 ? ξ ? 2 or 2.2 ? ξ ? 3 the third or fourth harmonic will dominate. The second and third harmonics of .-mode waves grow faster on