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木星大红斑上方高层大气的加热。

Heating of Jupiter's upper atmosphere above the Great Red Spot.

出版信息

Nature. 2016 Aug 11;536(7615):190-2. doi: 10.1038/nature18940. Epub 2016 Jul 27.

DOI:10.1038/nature18940
PMID:27462811
Abstract

The temperatures of giant-planet upper atmospheres at mid- to low latitudes are measured to be hundreds of degrees warmer than simulations based on solar heating alone can explain. Modelling studies that focus on additional sources of heating have been unable to resolve this major discrepancy. Equatorward transport of energy from the hot auroral regions was expected to heat the low latitudes, but models have demonstrated that auroral energy is trapped at high latitudes, a consequence of the strong Coriolis forces on rapidly rotating planets. Wave heating, driven from below, represents another potential source of upper-atmospheric heating, though initial calculations have proven inconclusive for Jupiter, largely owing to a lack of observational constraints on wave parameters. Here we report that the upper atmosphere above Jupiter's Great Red Spot--the largest storm in the Solar System--is hundreds of degrees hotter than anywhere else on the planet. This hotspot, by process of elimination, must be heated from below, and this detection is therefore strong evidence for coupling between Jupiter's lower and upper atmospheres, probably the result of upwardly propagating acoustic or gravity waves.

摘要

巨行星中低纬度的高层大气温度比单纯基于太阳加热的模拟温度高出数百摄氏度。关注额外加热源的建模研究未能解决这一重大差异。人们曾预计,从热极光区向赤道方向输送能量会加热低纬度地区,但模型表明,由于快速旋转行星上的强科里奥利力,极光能量被困在高纬度地区。从下方驱动的波加热是另一种潜在的高层大气加热源,但最初的计算结果对木星来说并不确定,主要是因为缺乏对波参数的观测限制。在这里,我们报告说,木星大红斑(太阳系中最大的风暴)上方的高层大气比行星上任何其他地方都要热数百摄氏度。通过排除法,这个热点必然是从下方加热的,因此这一发现有力地证明了木星的低层和高层大气之间存在耦合,这可能是向上传播的声波或重力波的结果。

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Temperature changes and energy inputs in giant planet atmospheres: what we are learning from H3+.巨行星大气中的温度变化和能量输入:我们从 H3+中学到了什么。
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Why is the H hot spot above Jupiter's Great Red Spot so hot?为何木星大红斑上方的H热点如此之热?
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H3+: the driver of giant planet atmospheres.H3+:巨行星大气层的驱动因素
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