The influence of out‐of‐plane shear flow on Hall magnetic reconnection and FTE generation. Issue 7 (23rd July 2013)

• Record Type: Journal Article
• Authors: Chen, Yangao; Xiao, Chijie; Wang, Xiaogang; Wang, Jiaqi; Zhang, Hui; Pu, Zuyin; Ma, Zhiwei; Guo, Zhibin
• Is Part Of: Journal of geophysical research. Volume 118:Issue 7(2013:Jul.)
• Page Start: 4279
• Page End: 4288
• Publication Date: 2013-07-23
• Subjects: Hall magnetic reconnection -- FTE -- Shear flow -- Magnetospheric Interactions with the Solar Wind; Magnetospheric physics -- Periodicals; Space environment -- Periodicals; Cosmic physics -- Periodicals; Planets -- Atmospheres -- Periodicals; Heliosphere (Astrophysics) -- Periodicals; Geophysics -- Periodicals; 523.01
• DOI: 10.1002/jgra.50417
• Languages: English
• ISSNs: 2169-9380

Abstract

Abstract : [1] Magnetic reconnection driven by an out‐of‐plane shear flow is carried out based on the three‐dimensional Hall magnetohydrodynamics (MHD) code. The simulation results indicate that an out‐of‐plane shear flow can drive a secondary tearing instability to quickly form a magnetic island without a guide field or a flux rope with a guide field. It is found that the size of the flux rope within ~240 Alfven time reaches about 20 a ( a is the initial current sheet thickness) that is roughly one Earth radius, the typical scale of Flux Transfer Event (FTE) observed at the dayside magnetopause. From a special simulation case based on the THEMIS data, it is found that an observed FTE is well reproduced by the Hall MHD simulation, which may give some clues on the generation mechanism of FTE. Key Points: FTE generation due to out‐of‐plane shear flow and Hall effect An X‐line splits into two X‐line Both simulation results and in‐situ measurements are analyzed