Magnetic Reconnection in Three Dimensions – Spine, Fan and Separator Solutions

被引:0
|
作者
J. Heerikhuisen
I.J.D. Craig
机构
[1] University of California,Institute of Geophysics and Planetary Physics
[2] University of Waikato,Department of Mathematics
来源
Solar Physics | 2004年 / 222卷
关键词
Dynamic Simulation; Spatial Dimension; Localize Current; Accurate Description; Magnetic Reconnection;
D O I
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学科分类号
摘要
Magnetic reconnection in three spatial dimensions can occur in three distinct ways. In the case of reconnection at a neutral point, localized currents can accumulate either in the form of a quasi one-dimensional `fan' current, or as a cylindrical `spine' current aligned to the exhaust axis of the flow. A third possibility, which does not involve a null of the field, is separator reconnection, where reconnection occurs in two dimensions with a uniform guide field. In this paper we employ steady-state and time-dependent analytic models to predict resistive scaling laws associated with null point and separator reconnection. These predictions are then tested computationally by exploring dynamic simulations in 3D periodic geometries. We find that the simple, steady-state models provide an accurate description of a time-dependent, reconnecting current layer.
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页码:95 / 114
页数:19
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