Second harmonic emission during solar flares

Type III (type U) radio bursts are signatures of energetic electrons generated during solar flares, traveling along open (closed) magnetic coronal field lines. The burst photons correspond to the second harmonic of the plasma frequency and are generated by the coalescence of two Langmuir waves excit...

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Guardado en:
Detalles Bibliográficos
Publicado: 2002
Materias:
Sun: flares
Sun: radio radiation
Turbulence
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v564_n2I_p1035_Vasquez
http://hdl.handle.net/20.500.12110/paper_0004637X_v564_n2I_p1035_Vasquez
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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