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Fine Structure of Solar Radio Bursts [electronic resource] / by Gennady P. Chernov.

By: Chernov, Gennady P [author.].
Contributor(s): SpringerLink (Online service).
Material type: materialTypeLabelBookSeries: Astrophysics and Space Science Library: 375Publisher: Berlin, Heidelberg : Springer Berlin Heidelberg : Imprint: Springer, 2011Description: XVI, 284 p. online resource.Content type: text Media type: computer Carrier type: online resourceISBN: 9783642200151.Subject(s): Physics | Astrophysics | Physics | Extraterrestrial Physics, Space Sciences | Astronomy, Observations and Techniques | Astrophysics and Astroparticles | Plasma PhysicsDDC classification: 520 | 500.5 Online resources: Click here to access online
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.
In: Springer eBooksSummary: 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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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.

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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