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Bifurcation of the tail current sheet in Jovian magnetosphere

机译:木星磁层尾电流片的分叉

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Multiple crossings of the magnetotail current sheet by a single spaceraft give possibility to distinguish between two types of electric current density distribution: single-peaked (Harris type current layer) and double-peaked (bifurcated current sheet). Magnetic field measurements in Jovian magnetic tail by Voyager-2 and Galileo reveal the bifurcation of tail current sheet. Electric current density possesses minimum at the point of B_x-component reversal and two maxima at the distance where the magnetic field strength reaches 50% of its value in the tail lobe. Solution for self-consistent magnetic field in the geomagnetic tail is obtained in a simple model. We arrive at the conclusion that the bifurcated current sheet with two maxima of the electric current density is an equilibrium state of the geomagnetic tail when ion pressure is anisotropic in the plane perpendicular to the magnetic field.
机译:单个航天器多次穿过磁尾电流片,从而有可能区分两种电流密度分布:单峰(哈里斯型电流层)和双峰(分叉电流片)。 Voyager-2和Galileo对木星的磁性尾巴进行的磁场测量揭示了尾流片的分叉。电流密度在B_x分量反转点处最小,在磁场强度在尾瓣中达到其值的50%的距离处具有两个最大值。在一个简单的模型中获得了地磁尾部中自洽磁场的解。我们得出的结论是,当离子压力在垂直于磁场的平面中各向异性时,具有两个最大电流密度的分叉电流片是地磁尾部的平衡状态。

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