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- W1497803963 abstract "Our proposed project is to study the basic plasma processes associated with magnetic reconnection in the Earth's magnetosphere. The three-dimensional (3-D) reconnection process are emphasized in the present study. To explain the satellite observations of flux transfer events (FTEs), we have proposed a multiple X line reconnection (MXR) model for the dayside magnetopause. The same reconnection process may also explain the occurrence of geomagnetic substorms. The multiple X line reconnection is intrinsically a time- dependent process, featuring impulsive and intermittent magnetic reconnection. The study of driven magnetic reconnection process was further extended in the past year by our 3-D MHD simulations that magnetic reconnections may take place along the multiple X lines, resulting in the formulation of helical magnetic flux tubes. The simulation results confirm our earlier theoretical model of multiple X line reconnection in the real 3-D environment. The geometry of the reconnected field lines revealed in the 3-D simulations is found to be more complicated than anticipated. Strong plasma flows along the flux tubes is another feature observed in the simulations. The results suggested that the 3-D reconnections differ significantly from the 2-D reconnections." @default.
- W1497803963 created "2016-06-24" @default.
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- W1497803963 date "1993-01-01" @default.
- W1497803963 modified "2023-09-27" @default.
- W1497803963 title "[A study of the magnetic field annihilation process in the magnetosphere and some geotechnical applications]" @default.
- W1497803963 doi "https://doi.org/10.2172/6610443" @default.
- W1497803963 hasPublicationYear "1993" @default.
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