中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
磁扰期间的三维漂移壳分离

文献类型:期刊论文

作者黄朝艳 ; 徐荣栏 ; 韩建伟
刊名空间科学学报
出版日期2008
卷号28期号:4页码:288-294
关键词引导中心法 磁力线追踪法 漂移壳分离
ISSN号0254-6124
其他题名3-Dimensional Drift Shell Splitting During the Geomagnetic Disturbance
通讯作者北京8701信箱
中文摘要基于磁层粒子动力学理论,首先对比了计算漂移壳分离的引导中心法和磁力线追踪法,计算表明两种方法的计算结果一致.然后分别采用T89c和T96磁层磁场模式,用磁力线追踪法数值计算了不同初始位置(≤9Re)、不同初始投掷角、不同Kp指数和不同太阳风压力下,带电粒子的漂移壳分离.计算结果揭示了漂移壳分离随初始位置、投掷角、Kp指数和太阳风压力的变化.其具体特征如下.(1)随着径向距离的增大,漂移壳分离效应愈加显著,由正午出发的粒子将被稳定捕获,而午夜出发的径向距离≥7Re的部分大投掷角粒子将沿磁层顶逃逸.(2)正午出发的粒子,漂移到午夜时其漂移壳随投掷角减小向外排列;午夜出发的粒子,漂移到正午时其漂移壳随投掷角增大排列;90°投掷角粒子在磁赤道面的漂移壳沿着磁场等值线排列.(3)漂移壳分离随Kp指数和太阳风压力增大变得显著,且随这两种扰动参数的变化特征和趋势是基本相似的.
英文摘要Based on the theory of magnetospheric particle dynamics, the guiding center and mag-netic field line tracing methods are used to calculate the drift shell splitting of the particle motion in the radiation belt. The results show that the two methods are the same. Therefore the 3-dimensional drift shell splitting during the geomagnetic disturbances is studied using magnetic field line tracing method. The initial location of the particles is } 9Re with different initial pitch angles. Different magnetic disturbance index KP and solar wind pressure, corresponding to T89c and T96 magnetic field model, are compared to each other. The results show that drift shell splitting varies with initial position, pitch angles, Kp index and solar wind pressure. The details are: (1) The drift shell splitting is stronger when the radius distance increases. Particles staring from noon will be trapped stably;otherwise, particles starting from night will escape .from the magnetopause, when the initial radius distance and pitch angle are large. (2) When the initial pitch angles on the magnetic equatorial plane increase, the drift shell of particles starting from noon align inward, but from night align outward. (3) Drift shell splitting becomes obvious when Kp index or solar wind pressure increase, and the basic character and trend under these two disturbance parameters are the same.
学科主题空间环境
收录类别CSCD
资助信息国家自然科学基金资助项目
语种中文
CSCD记录号CSCD:3375307
源URL[http://ir.cssar.ac.cn/handle/122/86]  
专题国家空间科学中心_保障部/保障与试验验证中心
推荐引用方式
GB/T 7714
黄朝艳,徐荣栏,韩建伟. 磁扰期间的三维漂移壳分离[J]. 空间科学学报,2008,28(4):288-294.
APA 黄朝艳,徐荣栏,&韩建伟.(2008).磁扰期间的三维漂移壳分离.空间科学学报,28(4),288-294.
MLA 黄朝艳,et al."磁扰期间的三维漂移壳分离".空间科学学报 28.4(2008):288-294.

入库方式: OAI收割

来源:国家空间科学中心

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