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Dependence of the Characteristics of Solar Wind Discontinuities and Shocks with Heliolatitude and Radial Distance

机译:太阳风不连续性和冲击的特性与太阳高度和径向距离的关系

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The distribution of the shocks in the heliosphere and their characteristic variations are investigated using Ulysses observations. The jumps in solar wind velocity, IMF magnitude, and proton density across the shocks and discontinuities are evaluated and used to characterize them. The distribution of these discontinuities with respect to heliolatitude ± 80° and with radial distance 1 to 5 AU are analyzed during solar minimum and solar maximum to understand their global behavior. It is noticed that the jumps in solar wind parameters associated with shocks and discontinuities are more prominent during the second orbit of Ulysses, which coincided with the maximum phase of solar activity.
机译:利用尤利西斯(Ulysses)的观测资料,研究了日光层中的冲击分布及其特征变化。评估了冲击和不连续过程中太阳风速,IMF大小和质子密度的跃变,并对其进行了表征。在太阳最小和太阳最大期间,分析了这些不连续性相对于日高±80°和径向距离1至5 AU的分布,以了解它们的整体行为。值得注意的是,在尤利西斯(Elysses)的第二个轨道期间,与冲击和不连续性相关的太阳风参数的跃迁更加突出,这与太阳活动的最大阶段相吻合。

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