Fine Structure of Solar Radio Bursts [electronic resource] /
Chernov, Gennady P.author.
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.
Description based upon print version of record.
Includes bibliographical references and index.
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.
Space sciences.
Observations, Astronomical.
Astronomy—Observations.
Astrophysics.
Plasma (Ionized gases).
Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics).
Astronomy, Observations and Techniques.
Astrophysics and Astroparticles.
Plasma Physics.
Astrophysics and space science library