Fine Structure of Solar Radio Bursts

2011
ISBN: 978-3-642-20014-4
Verlag: Springer

Buch, Englisch, 284 Seiten, Format (B × H): 160 mm x 241 mm, Gewicht: 617 g

Reihe: Astrophysics and Space Science Library

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.

Zielgruppe

Research

Autoren/Hrsg.

Chernov, Gennady P.

Fachgebiete

• Naturwissenschaften Astronomie Astronomische Beobachtung: Observatorien, Instrumente, Methoden
• Naturwissenschaften Astronomie Sonnensystem: Sonne und Planeten
• Naturwissenschaften Physik Angewandte Physik Astrophysik
• Naturwissenschaften Physik Thermodynamik Plasmaphysik
• Naturwissenschaften Astronomie Astrophysik

Inhaltsverzeichnis

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.

Über Autor(innen)

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.