Physics – Plasma Physics
Scientific paper
Dec 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009agufmsm21a1567t&link_type=abstract
American Geophysical Union, Fall Meeting 2009, abstract #SM21A-1567
Physics
Plasma Physics
[7526] Solar Physics, Astrophysics, And Astronomy / Magnetic Reconnection, [7833] Space Plasma Physics / Mathematical And Numerical Techniques, [7835] Space Plasma Physics / Magnetic Reconnection, [7846] Space Plasma Physics / Plasma Energization
Scientific paper
How to trigger magnetic reconnection is one of the most interesting and important problems in space plasma physics. Recently, electron pressure anisotropy (aeo=Pe,perp/Pe,para) at the center of a current sheet and non-local effect of the lower-hybrid drift instability (LHDI) that develops at the current sheet edges have attracted attention in this context. In addition to these effects, here we also study the effects of ion pressure anisotropy (aio=Pi,perp/Pi,para). Electron anisotropy effects are known to be helpless in a current sheet whose thickness is of ion-scale. In this range of current sheet thickness, the LHDI effects are shown to weaken substantially with a small increase in thickness and the obtained saturation level is too low for a large-scale reconnection to be achieved. Then we investigate whether introduction of electron and ion pressure anisotropies in the initial stage would couple with the LHDI effects to revive quick triggering of large-scale reconnection in a super-ion-scale current sheet. The results are as follows. (1) The initial electron pressure anisotropy is consumed very quickly when a number of minuscule magnetic islands (each lateral length is 1.5~3 times the ion inertial length) form. These minuscule islands do not coalesce into a large-scale island to enable large-scale reconnection. (2) The subsequent LHDI effects disturb the current sheet filled with the small islands. This makes the triggering time scale to be accelerated substantially but does not enhance the saturation level of reconnected flux. (3) When the ion pressure anisotropy is added, it survives through the small island formation stage and makes even quicker triggering to happen when the LHDI effects set-in. Furthermore the saturation level is seen to be elevated by a factor of ~2 and large-scale reconnection is achieved only in this case. Comparison with two-dimensional simulations that exclude the LHDI effects confirms that the saturation level enhancement is due to the ion anisotropy effects, while the LHDI effects shorten the overall time scale significantly. Anatomy of the ion anisotropy reveals that that explosive reconnection process is subject to the spatial difference of the ion gas pressure parallel to the initial magnetic field (i.e. the difference between the pressure at the X- and O-line). The results imply that re-distribution of the ion pressure tensors is one of the key properties that enable large-scale magnetic reconnection to develop in a super-ion-scale current sheet.
Fujimoto Minoru
Shinohara Iku
Tanaka Kenny G.
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