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The study of the fine structure of solar radio emissions is key to understanding plasma processes in the solar corona. It remains a reliable means for both diagnosing the corona and verifying the results of laboratory plasma experiments on wave-wave and wave-particle interactions. This monograph provides a comprehensive review of the fine structure of solar radio bursts. Based on the diversity of experimental data resulting from the progress made in observational techniques, the validity of various theoretical models is reexamined. The book serves as an up-to-date reference work for all...

This text reexamines the validity of theoretical models, based on a diversity of experimental data resulting from new observational techniques, to provide a comprehensive and up-to-date review of the fine structure of solar radio bursts.

We continue a comparative analysis of competing generation mechanisms of the zebra pattern (ZP) (under conditions of double plasma resonance and in the model with whistlers) based on new data. At the same time, a zebra structure was discovered in the radio emission from a pulsar in the Crab Nebula. Its analysis has already been carried out within the framework of various mechanisms, and here, we propose a new mechanism of explosive instability, more suitable for the parameters of the pulsar magnetosphere.We also show new analysis of unusual type-II bursts with cessation of the frequency...