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首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >Reconstruction of steady, three‐dimensional, magnetohydrostatic field and plasma structures in space: Theory and benchmarking
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Reconstruction of steady, three‐dimensional, magnetohydrostatic field and plasma structures in space: Theory and benchmarking

机译:稳定的重建,三维的,应承担的magnetohydrostatic场和等离子体结构空间:理论和基准测试

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摘要

A first attempt is made to reconstruct magnetic field and pressure distributions in steady, three‐dimensional (3D), magnetohydrostatic structures, using field and plasma data taken by two proximate spacecraft as they traverse such structures in space. The reconstruction is based on integration of the four scalar magnetohydrostatic equations for the field components and the pressure in a narrow region surrounding the spacecraft paths. The equations have been adapted for use in such reconstruction and a numerical code based on them has been written. The code has been benchmarked by use of synthetic data taken at points along straight lines through an exact, spheromak‐type, axially symmetric, solution of the equations. The results demonstrate that reasonably accurate reconstruction of time‐independent, 3D magnetohydrostatic structures is in principle possible.
机译:第一次尝试重建磁场和压力分布稳定,三维(3 d)应承担magnetohydrostatic结构,使用领域和等离子体数据了两个直接遍历等航天器在空间结构。在集成的四个标量magnetohydrostatic方程组件和压力在一个狭窄的地区宇宙飞船周围的路径。已用于在这种重建根据他们已经和一个数字代码写的。沿着笔直的合成数据点线通过一个精确,spheromak列车类型、轴向对称的,方程的解。证明合理准确三维重建的时间量独立原则上magnetohydrostatic结构可能的。

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