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木星云的组成、分层、对流及波动:来自“新视野号”的视角

Jupiter cloud composition, stratification, convection, and wave motion: a view from new horizons.

作者信息

Reuter D C, Simon-Miller A A, Lunsford A, Baines K H, Cheng A F, Jennings D E, Olkin C B, Spencer J R, Stern S A, Weaver H A, Young L A

机构信息

NASA Goddard Space Flight Center, Code 693, Greenbelt, MD 20771, USA.

出版信息

Science. 2007 Oct 12;318(5848):223-5. doi: 10.1126/science.1147618.

Abstract

Several observations of Jupiter's atmosphere made by instruments on the New Horizons spacecraft have implications for the stability and dynamics of Jupiter's weather layer. Mesoscale waves, first seen by Voyager, have been observed at a spatial resolution of 11 to 45 kilometers. These waves have a 300-kilometer wavelength and phase velocities greater than the local zonal flow by 100 meters per second, much higher than predicted by models. Additionally, infrared spectral measurements over five successive Jupiter rotations at spatial resolutions of 200 to 140 kilometers have shown the development of transient ammonia ice clouds (lifetimes of 40 hours or less) in regions of strong atmospheric upwelling. Both of these phenomena serve as probes of atmospheric dynamics below the visible cloud tops.

摘要

新视野号航天器上的仪器对木星大气层进行的几次观测,对木星气象层的稳定性和动力学有重要意义。中尺度波最早由旅行者号发现,现已在11至45公里的空间分辨率下观测到。这些波的波长为300公里,相速度比当地纬向气流快100米每秒,远高于模型预测值。此外,在200至140公里的空间分辨率下,对木星连续五次自转进行的红外光谱测量显示,在强烈大气上升流区域出现了瞬态氨冰云(寿命为40小时或更短)。这两种现象都可作为可见云层顶部以下大气动力学的探测器。

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