49th Annual Meeting of the Division of Plasma Physics
Volume 52, Number 11
Monday–Friday, November 12–16, 2007;
Orlando, Florida
Session DI2: Reconnection, Gamma-Ray Bursts, and Angular Momentum Transport
3:00 PM–5:00 PM,
Monday, November 12, 2007
Rosen Centre Hotel
Room: Salon 3/4
Chair: David Newman, University of Colorado
Abstract ID: BAPS.2007.DPP.DI2.2
Abstract: DI2.00002 : Three-dimensional magnetic reconnection in Earth's magnetosphere
3:30 PM–4:00 PM
Preview Abstract
Abstract
Author:
John Dorelli
(Space Science Center, University of New Hampshire)
Magnetic reconnection is thought to be the primary mode by which
the solar wind couples to the terrestrial magnetosphere, driving
phenomena such as magnetic storms and aurorae. While the theory
of two-dimensional reconnection is well developed, and has been
applied with great success to axisymmetric and toroidal systems
such as laboratory plasma experiments and fusion devices, it is
difficult to justify the application of two-dimensional theory to
nontoroidal plasma systems such as Earth's magnetosphere.
Unfortunately, the theory of three-dimensional magnetic
reconnection is much less well developed, and even defining
magnetic reconnection has turned out to be problematic. In this
talk, we review recent progress in the use of MHD to address the
physics of three-dimensional reconnection in Earth's
magnetosphere. The talk consists of two parts. In the first
part, we review the various definitions of three-dimensional
reconnection which have appeared in the literature in the last
twenty years. Our goal here is to map these definitions to sets
of physical phenomena which have been identified as
``reconnection'' in various three-dimensional contexts. In the
second part of the talk, we present our latest magnetosphere MHD
simulation results and indentify two qualitatively distinct types
of reconnection phenomena (organized by the orientation of the
Interplanetary Magnetic Field): 1) steady separator reconnection
under generic northward IMF conditions, involving plasma flow
across magnetic separatrix boundaries, and 2) time-dependent
reconnection under generic southward IMF conditions, involving a
global change in the topology of the magnetic field. While
neither of these types of reconnection is well described by
two-dimensional theory (indeed, we argue that attempts to apply
two-dimensional ideas to the magnetopause have resulted in more
confusion than clarification), both can be easily categorized
according to existing definitions of three-dimensional reconnection.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2007.DPP.DI2.2