© 2011

Fine Structure of Solar Radio Bursts

  • Provides up-to-date review of the field of Fine Structure of Solar Radio Bursts

  • Discusses latest theoretical models in view of a large diversity of experimental data

  • Author has fourty years of research experience in the field


Part of the Astrophysics and Space Science Library book series (ASSL, volume 375)

Table of contents

  1. Front Matter
    Pages i-xv
  2. G. P. Chernov
    Pages 1-6
  3. G. P. Chernov
    Pages 7-18
  4. G. P. Chernov
    Pages 19-65
  5. G. P. Chernov
    Pages 67-192
  6. Back Matter
    Pages 271-282

About this book


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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Authors and affiliations

  1. 1., Russian Academy of SciencesIZMIRANTroitskRussian Federation

About the authors

The author, Dr. Gennady Pavlovich Chernov, is Leading scientist of IZMIRAN (Russian Academy of Sciences). He has 40-years of experience in the study of spectral fine structures.

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