PMO OpenIR  > 太阳活动的多波段观测研究团组
Birefringence effect as a tool for astrophysical plasma study
Fleishman, GD ; Fu, QJ ; Wang, M ; Huang, GL ; Melnikov, VF
2002
Source PublicationPHYSICAL REVIEW LETTERS
ISSN0031-9007
Volume88Issue:25Pages:251101
AbstractGroup delay between two magnetoionic modes is discovered and spectrally, confirmed (Deltat(g) proportional to f(-3)) for the first time for quasiperiodic narrow band millisecond solar radio pulsations. Analysis of cross delays and autodelays proves that both X and O modes originate at the same source, so the radiation is weakly polarized originally. This finding allows one to specify the emission mechanism of the pulsations to be a nonlinear plasma mechanism operating at the second harmonics. Physical parameters of the solar corona are determined by the use of the theory of the nonlinear plasma mechanism; they agree well with independent observations of solar millisecond pulsations.
KeywordRadio
Subject AreaPhysics
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/7904
Collection太阳活动的多波段观测研究团组
Recommended Citation
GB/T 7714
Fleishman, GD,Fu, QJ,Wang, M,et al. Birefringence effect as a tool for astrophysical plasma study[J]. PHYSICAL REVIEW LETTERS,2002,88(25):251101.
APA Fleishman, GD,Fu, QJ,Wang, M,Huang, GL,&Melnikov, VF.(2002).Birefringence effect as a tool for astrophysical plasma study.PHYSICAL REVIEW LETTERS,88(25),251101.
MLA Fleishman, GD,et al."Birefringence effect as a tool for astrophysical plasma study".PHYSICAL REVIEW LETTERS 88.25(2002):251101.
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