The three-dimensional MHD simulation studies of the structure and dynamics at the leading part of a reconnection jet

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7519 Flares, 7835 Magnetic Reconnection (2723, 7526), 7836 Mhd Waves And Instabilities (2149, 2752, 6050)

Scientific paper

Magnetic reconnection is the one of the most essential phenomenon in magnetospheric physics, solar physics and laboratory experiments. It is well-known that fast plasma flows are generated in the reconnection process, so called the reconnection jet. We focused on the three-dimensionality of the structure and dynamics at the leading part of the reconnection jet and performed three-dimensional MHD simulations. We found that the leading part of the jet is likely to be unstable to two types of the interchange instability, specifically the Rayleigh-Taylor instability and ballooning instability. These two instabilities do not seem to compete with each other and the jet-front instability arises via complimentary effects of the two instabilities. We will discuss the detail of the dynamics at the leading part of the reconnection jet, and, additionally, a possible application of the process to a phenomenon observed in the solar flares will be discussed.

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