Latest Data on the fine Structure in Solar radio Emission - Chernov, Gennady
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The study of the fine structure of the solar radio emission is a key to understanding of plasma processes in the solar corona. Over the past 10 years or so, new solar instruments have been built (radio spectrographs and radio heliographs). In addition, radio data began to be studied comprehensively with new data in other wavelength ranges, in X-ray (GOES, RHESSI) and ultraviolet (SDO), which made it possible to obtain information on the position of radio sources. Such a textbook cover wide field of the Solar Radio Physics and it will be suitable for graduate students and researchers.

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Produktbeschreibung
The study of the fine structure of the solar radio emission is a key to understanding of plasma processes in the solar corona. Over the past 10 years or so, new solar instruments have been built (radio spectrographs and radio heliographs). In addition, radio data began to be studied comprehensively with new data in other wavelength ranges, in X-ray (GOES, RHESSI) and ultraviolet (SDO), which made it possible to obtain information on the position of radio sources. Such a textbook cover wide field of the Solar Radio Physics and it will be suitable for graduate students and researchers.
Autorenporträt
Dr. Chernov Gennady Pavlovich - Head scientist in IZMIRAN (Pushkov Institute of terrestrial magnetism, ionosphere and radio wave propagation of Russian Academy of sciences), Moscow, Troitsk (http://www.izmiran.ru/~gchernov).