基于IGS提供的TEC数据,研究了2003年10月大磁暴期间的暴时密度增强(Storm EnhancedDensity,SED)现象;利用GPS观测数据,计算出ROTI(Standard deviations of ROT)指数,分析了SED边界附近电离层小尺度不均匀体结构的时间和空间演变.研究表...基于IGS提供的TEC数据,研究了2003年10月大磁暴期间的暴时密度增强(Storm EnhancedDensity,SED)现象;利用GPS观测数据,计算出ROTI(Standard deviations of ROT)指数,分析了SED边界附近电离层小尺度不均匀体结构的时间和空间演变.研究表明,在磁暴主相期间SED边界附近不均匀体随着磁暴的发展逐渐增多;在主相的中后期不均匀体的分布密集度达到最大;在恢复相期间,不均匀体分布很少;随着磁暴的发展,不均匀体开始主要集中在40°～45°N范围内,随后向高纬漂移,主要集中在45°～55°N范围内.展开更多
Electrostatic solitary waves （ESWs） are observed in the vicinity of the magnetic null of the widely studied magnetic reconnection taking place at the near-earth tail when current sheet becomes dramatic thinning duri...Electrostatic solitary waves （ESWs） are observed in the vicinity of the magnetic null of the widely studied magnetic reconnection taking place at the near-earth tail when current sheet becomes dramatic thinning during substorm time on 1 October 2001. We use the Imada method for the 2-D reconnection model and study the characteristics of ESWs near the X-line region and the magnetic null points. The result shows that the amplitude of the observed ESWs in the vicinity of X-line region ranges from 0.1mV/m to 5mV/m, and the amplitude is larger near the magnetic null points. The generation mechanism and the role of ESWs associated with magnetic reconnection are also discussed.展开更多
文摘基于IGS提供的TEC数据,研究了2003年10月大磁暴期间的暴时密度增强(Storm EnhancedDensity,SED)现象;利用GPS观测数据,计算出ROTI(Standard deviations of ROT)指数,分析了SED边界附近电离层小尺度不均匀体结构的时间和空间演变.研究表明,在磁暴主相期间SED边界附近不均匀体随着磁暴的发展逐渐增多;在主相的中后期不均匀体的分布密集度达到最大;在恢复相期间,不均匀体分布很少;随着磁暴的发展,不均匀体开始主要集中在40°～45°N范围内,随后向高纬漂移,主要集中在45°～55°N范围内.
基金Supported by the National Natural Science Foundation of China under Grant Nos 40890163, 40574073, 40574074, 40640420563 and 40325012, and the Key Project of the Ministry of Education of China under Grant No 307019.
文摘Electrostatic solitary waves （ESWs） are observed in the vicinity of the magnetic null of the widely studied magnetic reconnection taking place at the near-earth tail when current sheet becomes dramatic thinning during substorm time on 1 October 2001. We use the Imada method for the 2-D reconnection model and study the characteristics of ESWs near the X-line region and the magnetic null points. The result shows that the amplitude of the observed ESWs in the vicinity of X-line region ranges from 0.1mV/m to 5mV/m, and the amplitude is larger near the magnetic null points. The generation mechanism and the role of ESWs associated with magnetic reconnection are also discussed.
