HR: 0830h
AN: SH31A-1097 [PDF]
TI: Microphysics of Magnetic Reconnection: Experiments on RSX and Simulation
AU: * Intrator, T P
EM: intrator@lanl.gov
AF: Los Alamos National Laboratory, P-24 Plasma Physics, Los Alamos, NM 87545 United States
AU: Furno, I G
EM: furno@lanl.gov
AF: Los Alamos National Laboratory, P-24 Plasma Physics, Los Alamos, NM 87545 United States
AU: Hsu, S C
EM: scotthsu@lanl.gov
AF: Los Alamos National Laboratory, P-24 Plasma Physics, Los Alamos, NM 87545 United States
AU: Lapenta, G
EM: lapenta@lanl.gov
AF: Los Alamos National Laboratory, T-15 Plasma Theory, Los Alamos, NM 87545 United States
AU: Ricci, P
EM: ricci@lanl.gov
AF: Los Alamos National Laboratory, T-15 Plasma Theory, Los Alamos, NM 87545 United States
AB:
Using a unique LANL laboratory facility, the Reconnection Scaling Experiment (RSX), and a state-of-the-art LANL numerical
code, CELESTE3D, we are beginning an experimental and numerical study of the microphysics of 2D and 3D "fast magnetic
reconnection". RSX at Los Alamos National Laboratory is already operational and producing research plasmas. In RSX, the
radial boundaries and thus the reconnection geometry are not constrained to two dimensions. It is capable of investigating 3D
magnetic reconnection occurring in a free-boundary 3D linear geometry during the coalescence of two parallel current plasma
channels, which are produced by using plasma gun technology. RSX can also scale the guide field (ion gyroradius)
independently of other reconnection parameters. Frontier reconnection research invokes (1) `anomalous'
microinstability-induced resistivity, which enhances dissipation rates inside the reconnection layer and (2) terms of the
two-fluid generalized Ohm's law which introduce whistler and kinetic Alfv‚n wave dynamics. The two-fluid approach predicts
(a) a two-spatial-scale spatial structure of the reconnection layer, with outer (inner) thickness equal to the ion (electron)
skin depth and (b) Hall currents in the reconnection plane and out-of-plane magnetic field on the electron scale. We will
show spatially resolved RSX experimental measurements of the dynamics of the reconnection layer, and take advantage of our
scaling capabilities to address the applicability of the two-fluid approach.
UR: http://wsx.lanl.gov/
DE: 2740 Magnetospheric configuration and dynamics
DE: 2744 Magnetotail
DE: 7835 Magnetic reconnection
SC: SPA - Solar and Heliospheric Physics [SH]
MN: 2003 Fall Meeting