首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >Experimental evaluation of common spacecraft data analysis techniques for reconnection region analysis in a laboratory plasma
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Experimental evaluation of common spacecraft data analysis techniques for reconnection region analysis in a laboratory plasma

机译:常规航天器数据分析技术在实验室等离子体中重新连接区域分析的实验评估

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A laboratory plasma is utilized to assess the effectiveness of several prominent spacecraft data analysis techniques. These include minimum variance analysis on the magnetic field (MVAB) and various boundary-crossing time analyses (BCTA) such as the constant velocity approach (CVA), constant thickness approach (CTA), and minimum thickness variance (MTV). Magnetic field data from measurement points that resemble the formation of multispacecraft flying though a reconnecting current sheet is used to check MVAB and BCTA to deduce a proper normal vector. Results from each method are compared to the values measured by 2-D magnetic probe arrays. We examine discharges with a two-dimensional (2-D) X-line structure as well as cases in which a flux rope forms within the layer. All discharges are in a two-fluid regime in which electrons are magnetized but ions are not. We conclude that CVA with four sample measurement points forming a tetrahedron generates a reasonable unit normal vector n, relative velocity along the normal vector V_n, and current sheet thickness δ_(CS) for all of the tested cases. Unlike CVA, both CTA and MTV sometimes generate V_n and δ_(CS) that are different from the measured values, which indicates that CTA and MTV are sensitive to changes in the current sheet thickness. CTA is, however, successful at estimating n. MVAB, on the other hand, often fails to predict a proper normal direction. This is because the reconnecting neutral sheet fundamentally contains 2-D or 3-D structures. MVAB, however, does determine the direction along the reconnecting magnetic field that is close to the real magnetic geometry. Based on these observations, we suggest a hybrid procedure for determining a local coordinate system for data from four spacecraft passing through a reconnecting current sheet.
机译:利用实验室等离子体来评估几种重要的航天器数据分析技术的有效性。这些包括磁场的最小方差分析(MVAB)和各种跨边界时间分析(BCTA),例如等速方法(CVA),等厚度方法(CTA)和最小厚度方差(MTV)。来自测量点的磁场数据类似于通过重新连接的电流表飞行形成的多宇宙飞船的形成,用于检查MVAB和BCTA以推导适当的法向矢量。将每种方法的结果与二维磁探针阵列测量的值进行比较。我们检查具有二维(2-D)X线结构的放电,以及在该层内形成磁通绳的情况。所有放电均处于双流体状态,其中电子被磁化,而离子未被磁化。我们得出结论,对于所有测试情况,具有四个样本测量点形成四面体的CVA会生成合理的单位法向矢量n,沿法向矢量V_n的相对速度以及当前的板厚δ_(CS)。与CVA不同,CTA和MTV有时会生成与测量值不同的V_n和δ_(CS),这表明CTA和MTV对当前纸张厚度的变化敏感。但是,CTA可以成功估计n。另一方面,MVAB通常无法预测正确的法线方向。这是因为重新连接的中性板基本上包含2-D或3-D结构。但是,MVAB确实确定了沿着重新连接磁场的方向,该方向接近真实的磁几何形状。基于这些观察结果,我们建议一种混合程序,用于确定来自四个航天器的数据的局部坐标系,这些航天器经过重新连接的电流表。

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