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NONLINEAR PARAMETRIC-INSTABILITY AND MILLISECOND SOLAR RADIO SPIKES
WANG, DY ; LI, DY
1991
Source PublicationSOLAR PHYSICS
ISSN0038-0938
Volume135Issue:2Pages:393-405
AbstractA model of nonlinear parametric instability (NLPI) modulation is suggested to explain the millisecond spikes in solar decimetric radio emission. The radio emission energy will periodically transfer to two other waves, and the intensity of the radio emission will be modified by NLPI processes in the corona, when the matching conditions of three-wave coupling are satisfied. This model can simultaneously explain the duration of spikes, why the millisecond spikes have not been observed in other solar radio emission, and the relation between the duration of the spikes and the intensity and the frequency of the radio emission as well.
Subject Area天文和天体物理
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/8558
Collection期刊(老文献)
Recommended Citation
GB/T 7714
WANG, DY,LI, DY. NONLINEAR PARAMETRIC-INSTABILITY AND MILLISECOND SOLAR RADIO SPIKES[J]. SOLAR PHYSICS,1991,135(2):393-405.
APA WANG, DY,&LI, DY.(1991).NONLINEAR PARAMETRIC-INSTABILITY AND MILLISECOND SOLAR RADIO SPIKES.SOLAR PHYSICS,135(2),393-405.
MLA WANG, DY,et al."NONLINEAR PARAMETRIC-INSTABILITY AND MILLISECOND SOLAR RADIO SPIKES".SOLAR PHYSICS 135.2(1991):393-405.
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