| 脉冲星微结构的研究进展 |
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| 引用本文： | 吴鑫基,金声震.脉冲星微结构的研究进展[J].紫金山天文台台刊,1994,13(3):226-232. |
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| 作者姓名： | 吴鑫基 金声震 |
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| 作者单位： | Department of Geophysics，University of Peking，Beijing，China United Laboratory for Radio Astronomy，Chinese Academy of Sciences，Beijing Astronomical Observatory，Beijing，China，Department of Applied Mathematics Theoretical Physics，University of Cambridge，U.K. National Institute for Space Research-INPE，Brazil，Beijing Astronomical Observatory，Beijing，China |
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| 基金项目： | Supported by National Climbing Program，National Science Foundation |
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| 摘 要： | The properties of pulsar radio pulse micro structure, such as the timescale, the quasiperiodic, the frequency dependence, and the relation of intensity to width, are reviewed. Then the theoritical interpretations, the radial structure models, the angular beaming models, and the nonlinear temporal models, are introduced.
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| 关 键 词： | 脉冲星 微结构 研究进展 |
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