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The Time-Dependent Structure of the Electron Reconnection LayerCollisionless magnetic reconnection is often associated with time-dependent behavior. Specifically, current layers in the diffusion region can become unstable to tearing-type instabilities on one hand, or to instabilities with current-aligned wave vectors on the other. In the former case, the growth of tearing instabilities typically leads to the production of magnetic islands, which potentially provide feedback on the reconnection process itself, as well as on the rate of reconnection. The second class of instabilities tend to modulate the current layer along the direction of the current flow, for instance generating kink-type perturbations, or smaller-scale turbulence with the potential to broaden the current layer. All of these processes contribute to rendering magnetic reconnection time-dependent. In this presentation, we will provide a summary of these effects, and a discussion of how much they contribute to the overall magnetic reconnection rate.
Document ID
20110009904
Acquisition Source
Goddard Space Flight Center
Document Type
Abstract
Authors
Hesse, Michael
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Zenitani, Seiji
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Kuznetsova, Masha
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Klimas, Alex
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 25, 2013
Publication Date
November 2, 2009
Subject Category
Space Radiation
Meeting Information
Meeting: 51st Annual Meeting of the Division of Plasma Physics (Object 2131) of the American Physical Society (APS)
Location: Atlanta, GA
Country: United States
Start Date: November 2, 2009
End Date: November 6, 2009
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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