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About shape of the interplanetary shock front

机译:关于行星际震动前线的形状

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The method of the interplanetary shock front shape determination has been developed. Weak large-scale asymmetry of the front has been revealed for two sets of the vector-normal to front components obtained from data of ACE experiment during from 1998 to 2003 years (199 measurements) and from 1998 to 2008 years (257 measurements). Axial symmetric shape of the front has been determined. It agrees in general with one calculated in the magneto-hydrodynamic approximation for conditions of the solar wind. Statistical method of the determination of a surface shape using set of the vector-normal to surface has been established.
机译:已经开发了行星冲击前形状确定的方法。对于从1998年至2003年(199次测量)和1998年至2008年的ACE实验数据,从ACE实验数据和2008年(257次测量)从ACE实验数据中获得的两组载体正常的前部组件揭示了前部的弱大规模不对称。已经确定了前部的轴对称形状。它一般都与在太阳风的条件下计算的磁力 - 流体动力学近似。已经建立了使用一组向量到表面测定表面形状的统计方法。

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