2006 APS April Meeting
Saturday–Tuesday, April 22–25, 2006;
Dallas, TX
Session E3: Laboratory Astrophysics: Magnetic Reconnection
3:30 PM–5:18 PM,
Saturday, April 22, 2006
Hyatt Regency Dallas
Room: Landmark C
Sponsoring
Units:
DPP DAP GPAP
Chair: Vincent Chan, General Atomics
Abstract ID: BAPS.2006.APR.E3.3
Abstract: E3.00003 : Magnetic Reconnection in the DIII-D Tokamak*
4:42 PM–5:18 PM
Preview Abstract
Abstract
Author:
E.J. Strait
(General Atomics)
Magnetic reconnection is an important feature of
tokamak plasmas, with the resulting changes in magnetic topology
often
leading to redistribution of the plasma's thermal and magnetic
energy.
Improved experimental diagnostics, including direct measurements
of the
internal magnetic field, and large nonlinear 3D numerical
simulations have
begun to offer new views of tokamak magnetohydrodynamic (MHD)
instabilities.
The full potential of these tools for investigation of
reconnection physics
and quantitative comparison of theory and experiment has yet to be
exploited. This talk summarizes several areas of research related to
reconnection in the DIII-D tokamak. The sawtooth is a periodic
reconnection
with poloidal and toroidal mode numbers m=1, n=1 that occurs in
the core of
a tokamak plasma. DIII-D results demonstrate a wide range of
sawtooth
behavior in different plasma regimes, ranging from fast, complete
reconnection of the core region (similar to the classic Kadomtsev
model) to
a quasi-interchange-like instability with slower reconnection.
Reconnection
often leads to tearing modes and magnetic islands at flux
surfaces with
rational safety factors q=m/n$>$1. At low plasma pressure, the
onset and
growth of tearing modes in DIII-D are in good agreement with the
classic
stability index $\Delta $'. At higher pressure the evolution and
saturation
of ``neoclassical tearing modes'' agrees well with the Rutherford
equation,
modified to include the pressure-driven bootstrap current. Forced
reconnection is also important in tokamak plasmas. Tearing modes
may be
driven by external magnetic field errors or by other MHD events.
However,
plasma rotation at the resonant surface can shield the driving
perturbation
and inhibit reconnection, leading to nonlinear threshold behavior as
observed in DIII-D and other experiments. The shielding becomes
stronger as
the Lundquist number increases, a possibly favorable result for
larger,
hotter, stronger-field fusion devices of the future.
*Work supported by US DOE under DE-FC02-04ER54698
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2006.APR.E3.3