Juno-Derived Electron Density Profiles of the High-Latitude Jovian Ionosphere

IF 2.6 2区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS
Drew A. Coffin, Paul Withers, Omakshi Agiwal, Dustin Buccino, Marzia Parisi, Ryan S. Caruso, Andrea Caruso, Luis Gomez Casajus, Edoardo Gramigna, Paolo Tortora, Marco Zannoni, Jack Hunter Waite, Paul Steffes, Sushil Atreya, Scott Bolton
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Abstract

The magnetosphere of Jupiter is an excellent natural laboratory for plasma dynamics due to its strength and internal plasma source. However, a complication in understanding the flow of energy through the system is the closure of the driving current systems within the chaotic high-latitude ionosphere of Jupiter, a region that has been poorly surveyed. The polar orbit of the Juno spacecraft permits for the first time multiple observations of the high- and mid-latitude ionosphere through the radio occultation technique. This paper presents derived electron density profiles from four such occultations. Seven profiles, four ingress and three egress, all sample the dawn limb but at a range of magnetic latitudes, including an ingress profile within 5 o ${5}^{o}$ of the main oval that is consistent with a response to high-energy electron influx. These profiles demonstrate variability in peak densities, peak altitude, and even the number of layers present. This high level of variability in Jupiter's high-latitude ionosphere suggests a complex network of current closure with high temporal variability.

朱诺衍生的高纬度木星电离层电子密度剖面
由于木星磁层的强度和内部等离子体源,它是一个极好的等离子体动力学天然实验室。然而,理解通过系统的能量流的一个复杂问题是,在木星混乱的高纬度电离层内,驱动电流系统的关闭,这是一个调查很少的区域。朱诺号航天器的极地轨道允许首次通过无线电掩星技术对高纬度和中纬度电离层进行多次观测。本文给出了四个掩星的电子密度分布图。7个剖面,4个入口和3个出口,都是在黎明边缘取样,但在磁纬度范围内,包括在主椭圆的5 0 ${5}^{o}$范围内的入口剖面,这与高能电子流入的响应一致。这些剖面显示了峰密度、峰高度甚至存在层数的可变性。木星高纬度电离层的这种高变异性表明,当前闭合的复杂网络具有高时间变异性。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Journal of Geophysical Research: Space Physics
Journal of Geophysical Research: Space Physics Earth and Planetary Sciences-Geophysics
CiteScore
5.30
自引率
35.70%
发文量
570
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