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Beschreibung
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.
Details
| Verlag | LAP LAMBERT Academic Publishing |
| Ersterscheinung | 11. April 2019 |
| Maße | 22 cm x 15 cm x 1.8 cm |
| Gewicht | 453 Gramm |
| Format | Softcover |
| ISBN-13 | 9786200001658 |
| Seiten | 292 |
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