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首页> 外文期刊>Journal of Geophysical Research. Biogeosciences >Ammonia abundance in Jupiter's atmosphere derived from the attenuation of the Galileo probe's radio signal
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Ammonia abundance in Jupiter's atmosphere derived from the attenuation of the Galileo probe's radio signal

机译:木星大气中的氨含量来自伽利略探测器无线电信号的衰减

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The radio signal from the Galileo probe to the orbiter experienced attenuation due to ammonia in Jupiter's atmosphere during the probe descent. A profile of the ammonia content as a function of depth in the atmosphere has been derived from the measurements of the attenuation. The derived ammonia abundance rises to a molar fraction of 700 +/- 100 parts per million for pressures greater than 7 bars, about 4 times that expected based on the solar abundance of nitrogen. [References: 27]
机译:由于木星大气层中的氨在探测器下降期间从伽利略探测器到轨道器的无线电信号经历了衰减。从衰减的测量中得出了氨含量随大气深度变化的曲线。对于大于7 bar的压力,所得到的氨的丰度提高到700 +/- 100百万分之一的摩尔分数,是基于氮的太阳丰度的预期值的约4倍。 [参考:27]

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