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 researchers in this field.
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