A mechanism for the quasiperiodic decameter pulsations of the quiet sun

The intensity fluctuations observed in the decameter-wavelength emission of the quiet sun can be interpreted by a plasma mechanism rather than by bremsstrahlung. The fluctuations would develop as the propagation of acoustic wave trains through the corona modulates the optical depth of the radio sour...

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Veröffentlicht in:	Soviet astronomy letters 1983-07, Vol.9, p.258-260
Hauptverfasser:	Levin, B N, SNEGIREV, S D
Format:	Artikel
Sprache:	eng
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description	The intensity fluctuations observed in the decameter-wavelength emission of the quiet sun can be interpreted by a plasma mechanism rather than by bremsstrahlung. The fluctuations would develop as the propagation of acoustic wave trains through the corona modulates the optical depth of the radio source.
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identifier	ISSN: 0360-0327
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issn	0360-0327
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source	EZB-FREE-00999 freely available EZB journals; Alma/SFX Local Collection
title	A mechanism for the quasiperiodic decameter pulsations of the quiet sun
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