Overview

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.

Full Product Details

Author:   Gennady P. Chernov
Publisher:   Springer-Verlag Berlin and Heidelberg GmbH & Co. KG
Imprint:   Springer-Verlag Berlin and Heidelberg GmbH & Co. K
Edition:   2011 ed.
Volume:   375
Dimensions:   Width: 15.50cm , Height: 2.30cm , Length: 23.50cm
Weight:   0.617kg
ISBN:  

9783642200144

ISBN 10:   3642200141
Pages:   284
Publication Date:   30 June 2011
Audience:   College/higher education ,  Postgraduate, Research & Scholarly
Format:   Hardback
Publisher's Status:   Active
Availability:   Out of stock  
The supplier is temporarily out of stock of this item. It will be ordered for you on backorder and shipped when it becomes available.

Table of Contents

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.

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Author Information

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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