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OverviewThe 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 DetailsAuthor: Gennady P. ChernovPublisher: 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: 1.60cm , Length: 23.50cm Weight: 0.462kg ISBN: 9783642269035ISBN 10: 3642269036 Pages: 284 Publication Date: 03 August 2013 Audience: College/higher education , Postgraduate, Research & Scholarly Format: Paperback Publisher's Status: Active Availability: Manufactured on demand  We will order this item for you from a manufactured on demand supplier. Table of ContentsPreface.- 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.ReviewsAuthor InformationThe 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. Tab Content 6Author Website:Countries AvailableAll regions |
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