Fine Structure of Solar Radio Bursts

This book 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.

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.

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 Includes supplementary material: sn.pub/extras

Auteur
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.

Contenu

Preface.- Acknowledgments.- 1 Introduction.- 2 Pulsations.- 3 Spike bursts.- 4 Zebra pattern and fiber bursts.- 5 Recent results of zebra patterns in solar radio bursts.- References.- Subject Index.