globalchange  > 气候减缓与适应
DOI: 10.1002/2014GL061434
论文题名:
Tide-driven shear instability in planetary liquid cores
作者: Sauret A.; Le Bars M.; Le Gal P.
刊名: Geophysical Research Letters
ISSN: 0094-9806
EISSN: 1944-9537
出版年: 2014
卷: 41, 期:17
起始页码: 6078
结束页码: 6083
语种: 英语
Scopus关键词: Astronomy ; Stability ; Velocity measurement ; Axisymmetric jet ; Deformable spheres ; Particle image velocimetry measurement ; Planetary system ; Resonant forcing ; Self-interactions ; Semi-empirical ; Shear instability ; Liquids ; ellipse ; experimental study ; measurement method ; nonlinearity ; numerical model ; threshold ; tidal cycle ; turbulence
英文摘要: We present an experimental study on the shear instability driven by tidal forcing in a model planetary liquid core. The experimental setup consists of a water-filled deformable sphere rotating around its axis and subjected to an elliptical forcing. At resonant forcing frequencies, the nonlinear self-interaction of the excited inertial mode drives an intense and localized axisymmetric jet. The jet becomes unstable at low Ekman number because of a shear instability. Using particle image velocimetry measurements, we derive a semiempirical scaling law that captures the instability threshold of the shear instability. This mechanism is fully relevant to planetary systems, where it constitutes a new route to generate turbulence in their liquid cores. © 2014. American Geophysical Union.
URL: https://www.scopus.com/inward/record.uri?eid=2-s2.0-84906800454&doi=10.1002%2f2014GL061434&partnerID=40&md5=1bd78bc8fad5d5d2b8d85ba81f8cc5b8
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资源类型: 期刊论文
标识符: http://119.78.100.158/handle/2HF3EXSE/7070
Appears in Collections:气候减缓与适应

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作者单位: Aix Marseille Université, CNRS, Centrale Marseill, Marseille, France

Recommended Citation:
Sauret A.,Le Bars M.,Le Gal P.. Tide-driven shear instability in planetary liquid cores[J]. Geophysical Research Letters,2014-01-01,41(17).
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