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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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Detalles Bibliográficos
Autor principal: Chernov, Gennady P
Lenguaje:eng
Publicado: Springer 2011
Materias:
Acceso en línea:https://dx.doi.org/10.1007/978-3-642-20015-1
http://cds.cern.ch/record/1383397