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Detailed Reference Information
Karimabadi et al. 2004
Karimabadi, H., Daughton, W. and Quest, K.B. (2004). Role of electron temperature anisotropy in the onset of magnetic reconnection. Geophysical Research Letters 31: doi: 10.1029/2004GL020791. issn: 0094-8276.

Predictions of tearing saturation in a neutral sheet range from minute amplitude to explosive growth. It is shown that in 2D, single island tearing saturates at very small amplitudes due to preferential electron heating in the parallel direction. However, the presence of multiple unstable modes allows the system to get past the stabilization and grow to ion scales. In 3D there are two current aligned instabilities that can affect the tearing mode. One is the Weibel instability driven by electron anisotropy T$perp$e/T$parallel$e 1 within the current layer. In this limit, the parallel Weibel instability merges with tearing to give rise to anisotropic tearing, which becomes the dominant electron anisotropy driven mode with a broad angular spectrum. The level of electron anisotropy generated by the LHDI can significantly enhance the tearing growth rate and extend the spectrum to very short wavelength which expedites the transition to large scale reconnection. Thus LHDI's main contribution to reconnection onset is not through anomalous resistivity but through its effect on tearing mode.

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Abstract

Keywords
Space Plasma Physics, Magnetic reconnection, Space Plasma Physics, Numerical simulation studies, Space Plasma Physics, Waves and instabilities
Journal
Geophysical Research Letters
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Publisher
American Geophysical Union
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