Abstract
Magnetic null points and flux ropes play important roles in the three-dimensional process of magnetic reconnection. In this study, a cluster of null points are reconstructed in the reconnection region in the magnetotail by applying a fitting-reconstruction method to measurements from the Cluster mission. The number of reconstructed null points varies rapidly, presenting a turbulent-like evolution of the magnetic structure. The electron density and the flux of the accelerated electrons were enhanced in this turbulent-like region. During this unstable reconnection process, a B–A s –B null structure was formed, showing flux rope features and resembling a secondary island in the observation.
摘要
磁零点和小尺度磁通量绳在三维磁重联过程中起着重要作用。本文根据Cluster星簇测量数据重构得到磁重联区的三维磁场结构,并在磁重联区内发现了一簇磁零点。这些磁零点在快速地运动,移入或移出重构区域,并不断地成对消失和产生,导致磁零点的数目不停地断变化。磁零点簇的这种急促的演变过程使得磁场呈现出类似湍动的性质,同时伴随着电子密度及被加速电子通量的升高。在磁零点簇的演化过程中,产生了B-A s -B磁零点构型形成的小尺度磁通量绳结构,并在二维投影上呈现出次级磁岛的特征。
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Acknowledgments
This work was supported by the National Natural Science Foundations of China (41274167, 41374166, 41474139 and 41404117) and PKU/UCLA Joint Research Institute in Science and Engineering, partly by the European Space Agency 2013–2014 Guest Investigator Program, and a working group sponsored by ISSI, Bern. We acknowledge the Cluster Plasma Electron And Current Experiment, Cluster Ion Spectrometry, Fluxgate Magnetometer, Spatio-Temporal Analysis of field Fluctuations, and Electric Field and Waves instrument teams for providing the data and the Cluster Cluster Science Archive for providing access to the data. M Dunlop and Y V Bogdanova are supported by Science & Technology Facilities Council in-house research grants. We thank the International Space Science Institute in Bern, Switzerland, and its staff and directors for partial support through the International Space Science Institute Team (from Cluster to Magnetospheric Multiscale).
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Guo, R., Pu, Z., Fu, S. et al. Evolution of clustered magnetic nulls in a turbulent-like reconnection region in the magnetotail. Sci. Bull. 61, 1145–1150 (2016). https://doi.org/10.1007/s11434-016-1121-z
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DOI: https://doi.org/10.1007/s11434-016-1121-z