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Fine Structure of Solar Radio Bursts
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 pro...
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Lenguaje: | eng |
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Springer
2011
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Acceso en línea: | https://dx.doi.org/10.1007/978-3-642-20015-1 http://cds.cern.ch/record/1383397 |