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JUPITERS IONOSPHERE - RESULTS FROM THE FIRST GALILEO RADIO OCCULTATION EXPERIMENT

机译:JUPITERS电离层-伽利略无线电波第一次实验的结果

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The Galileo spacecraft passed behind Jupiter on December 8, 1995, allowing the first radio occultation measurements of its ionospheric structure in 16 years. At ingress (24 degrees S, 68 degrees W), the principal peak of electron density is located at an altitude of 900 km above the 1-bar pressure level, with a peak density of 10(5) cm(-3) and a thickness of similar to 200 km. At egress (43 degrees S, 28 degrees W), the main peak is centered near 2000 km altitude, with a peak density of 2x10(4) cm(-3) and a thickness of similar to 1000 km. Two thin layers, possibly forced by upwardly propagating gravity waves, appear at lower altitudes in the ingress profile. This is the first in a two-year series of observations that should help to resolve long-standing questions about Jupiter's ionosphere. [References: 24]
机译:伽利略号航天器于1995年12月8日经过木星,这是16年以来首次对其电离层结构进行无线电掩星测量。在入口处(南纬24度,西经68度),电子密度的主峰位于1-bar压力水平以上900 km的高度,峰密度为10(5)cm(-3),并且厚度约200公里。在出口处(南纬43度,西纬28度),主峰的中心位于2000 km高度附近,峰密度为2x10(4)cm(-3),厚度类似于1000 km。在入口轮廓的较低高度处出现了两个可能由向上传播的重力波推动的薄层。这是两年观察系列的第一部分,这将有助于解决关于木星电离层的长期问题。 [参考:24]

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