| 射电脉冲星的偏振特性与逆康普顿散射（ICS）模型 |
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| 引用本文： | 徐仁新,乔国俊,韩金林.射电脉冲星的偏振特性与逆康普顿散射（ICS）模型[J].天文学进展,2001,19(2):267-270. |
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| 作者姓名： | 徐仁新 乔国俊 韩金林 |
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| 作者单位： | 1. 北京大学天文学系,
2. 科学院北京天文台, |
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| 摘 要： | 大量射电脉冲星的偏振观测－包括红偏振和圆偏振，个别脉冲的生直偏振模式，累积脉冲的消偏振现象等－为辐射区的物理状态和辐射提供了非常确切的观测事实，但现有理论对大从观测事实尚无法给出完整的说明，综述了脉冲星的偏振观测特征，并利用逆康谱顿散射模型对这些特性进行了解释。
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| 关 键 词： | 射电射冲星 偏振 辐射机制 逆康顿散射模型 |
| 修稿时间： | 2001年2月28日 |
Polarization Properties of Radio Pulsars in the Inverse Compton Scattering(ICS)
Model |
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| Xu Renxin, Qian Guojun, Han Jinlin.Polarization Properties of Radio Pulsars in the Inverse Compton Scattering(ICS)
Model[J].Progress In Astronomy,2001,19(2):267-270. |
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| Authors: | Xu Renxin Qian Guojun Han Jinlin |
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| Abstract: | Polarization observations of radio pulsars, such as linear and circular polarization, polarization position angle jumps of individual and integrated pulses, can be used to get abundant information, which is very important to understanding the physical processes in the emission regions. In this paper, some basic properties of polarization observations of radio pulsars and their theoretical explanation in the inverse Compton Scattering (ICS) model are briefly reviewed. |
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| Keywords: | Pulsars-Polarization-Radiation mechanism |
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