Physics
Scientific paper
Dec 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agufmsm31b1723l&link_type=abstract
American Geophysical Union, Fall Meeting 2008, abstract #SM31B-1723
Physics
2723 Magnetic Reconnection (7526, 7835), 2753 Numerical Modeling, 7829 Kinetic Waves And Instabilities, 7833 Mathematical And Numerical Techniques (0500, 3200), 7845 Particle Acceleration
Scientific paper
A novel gyrokinetic electron and fully kinetic ion (GKe/FKi) particle simulation model has been developed [Lin et al., PPCF, 2005] for the purpose of investigation of magnetic reconnection in collisionless plasmas. In this model, the rapid electron cyclotron motion is removed, while retaining the finite electron Larmor radii, wave-particle interaction, and off-diagonal components of the electron pressure tensor. This treatment results in a larger time step and allows one to treat the realistic ion-to-electron mass ratio mi/me in a large-scale system. The model is particularly suitable for ω < Ωe and k∥/ k⊥<1, and for problems in which the wave modes ranging from Alfven waves to lower-hybrid/whistler waves need to be handled on an equal footing. In this talk, we introduce the GKe/FKi model and present our simulation of instabilities of Harris sheet under a broad range of finite guide field BG and with a realistic mi/me using the linearized δ f GKe/FKi code [Wang et al., PoP, 2008]. The simulation is carried out in the 2-D plane containing the guide field in the y direction and the current sheet normal along z. For a finite BG/Bx0<1, where Bx0 is the asymptotic anti-parallel field component, quasi-electrostatic modified two-stream instability/whistler mode are found on the edge of current sheet. In addition, a new mode is found to be confined in the sheet center and carry a compressional δ By along the direction of electron drift, and may contribute directly to the electron anomalous resistivity in reconnection. For BG/Bx0≫1, the wave modes evolve to a globally propagating instability. The presence of finite BG is found to modify the physics of current sheet significantly.
Chen Leon L.
Lin Yangtin
Lin Zhangda
Wang Xinhua
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