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木星附近的等离子体观测:旅行者1号的初步结果。

Plasma observations near jupiter: initial results from voyager 1.

作者信息

Bridge H S, Belcher J W, Lazarus A J, Sullivan J D, McNutt R L, Bagenal F, Scudder J D, Sittler E C, Siscoe G L, Vasyliunas V M, Goertz C K, Yeates C M

出版信息

Science. 1979 Jun 1;204(4396):987-91. doi: 10.1126/science.204.4396.987.

Abstract

Extensive measurements of low-energy positive ions and electrons were made throughout the Jupiter encounter of Voyager 1. The bow shock and magneto-pause were crossed several times at distances consistent with variations in the upstream solar wind pressure measured on Voyager 2. During the inbound pass, the number density increased by six orders of magnitude between the innermost magnetopause crossing at approximately 47 Jupiter radii and near closest approach at approximately 5 Jupiter radii; the plasma flow during this period was predominately in the direction of corotation. Marked increases in number density were observed twice per planetary rotation, near the magnetic equator. Jupiterward of the Io plasma torus, a cold, corotating plasma was observed and the energylcharge spectra show well-resolved, heavy-ion peaks at mass-to-charge ratios A/Z* = 8, 16, 32, and 64.

摘要

在“旅行者1号”飞越木星的整个过程中,对低能正离子和电子进行了广泛测量。弓形激波和磁层顶被多次穿越,穿越距离与“旅行者2号”测量的上游太阳风压力变化一致。在向内飞行过程中,在大约47个木星半径处最内侧的磁层顶穿越点与大约5个木星半径处的最近接近点之间,数密度增加了六个数量级;在此期间,等离子体流主要沿共转方向。在磁赤道附近,每行星自转观测到数密度有两次显著增加。在木卫一等离子体环面朝向木星的一侧,观测到了一个冷的、共转的等离子体,能量/电荷谱显示在质荷比A/Z* = 8、16、32和64处有分辨率良好的重离子峰。

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