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Heliospheric Current Sheet Distortions from Adjacent Outflowing Transients: Multi-spacecraft Observations

机译:来自相邻的流出瞬变的螺旋体电流薄膜畸变:多航天器观测

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The heliospheric current sheet (HCS) is a permanent solar wind feature, with well predicted Earth passages, but it can be structured and its main orientation can be highly distorted. We report new observations from 2 spacecraft in the solar wind (supported by observations from 3 spacecraft in the nightside magnetosheath), showing an evolution across the Sun-Earth line of large field reversals adjacent to the HCS. Contrary to a previously reported multi-spacecraft event, this case shows that the field inversion structure cannot be assumed to be well preserved and close to planar on the scale of the magnetospheric cross-section. However, both cases indicate the presence of field reversals in an away sector that is connected to the southern solar magnetic hemisphere but lies unexpectedly above a toward sector. Following the interpretation of the reversals as transient outflowing loops, associated initial flow deviations can be envisaged to account for the HCS deformations.
机译:Heliospheric Curtent Shore(HCS)是一个永久的太阳风特征,具有良好的地球通道,但它可以结构化,其主要方向可以高度扭曲。我们从太阳风中的2个航天器报告了新的观察(通过从夜间磁性钻井的3个航天器的观察结果支持),显示出与HCS相邻的大型场逆转的太阳地线的演变。与先前报道的多空间事件相反,这种情况表明,在磁磁横截面的规模上,不能假设现场反转结构保持良好并靠近平面。然而,这两种情况都表明,在南部太阳能半球的外部扇区中存在现场逆转,但在朝向部门出乎意料地呈现出来。在解释逆转作为瞬态外流环之后,可以设想相关的初始流偏差以考虑HCS变形。

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