热与机械形貌:旋转斜压环的实验研究

IF 1.1 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS Geophysical and Astrophysical Fluid Dynamics Pub Date : 2020-02-03 DOI:10.1080/03091929.2019.1697875
S. D. Marshall, P. Read
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引用次数: 3

摘要

我们提出了一系列的实验研究,其中微分加热环空被用来研究地形对旋转,分层流动的影响。特别是,我们通过方位变化的差热来研究阻塞效应,并将它们与先前利用部分机械屏障的实验进行比较。所使用的热地形包括覆盖一小块基地方位角范围的加热元件的平坦斑块,形成相当于部分屏障,以研究阻塞和未阻塞流动之间的差异。这些方位变化的加热实验产生的结果与我们之前的机械屏障实验有很多相似之处,尽管没有物理障碍或形成底部困波。特别是在低泰勒数时,漂流流与地形的相互作用表现为“干涉”型,而在高泰勒数时形成不规则的“不规则”型,形成独特的流动结构。这表明阻塞可能是由热或机械不均匀性中的一种或两种引起的。在这两种实验中都注意到相干/持久共振波三联的证据,尽管发现三联波的分量波数及其对流动的影响取决于所讨论的地形。
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Thermal versus mechanical topography: an experimental investigation in a rotating baroclinic annulus
We present a series of experimental investigations in which a differentially-heated annulus was used to investigate the effects of topography on rotating, stratified flows. In particular, we investigate blocking effects via azimuthally varying differential-heating and compare them to previous experiments utilising partial mechanical barriers. The thermal topography used consisted of a flat patch of heating elements covering a small azimuthal extent of the base, forming an equivalent of a partial barrier, to study the difference between blocked and unblocked flow. These azimuthally-varying heating experiments produced results with many similarities to our previous experiments with a mechanical barrier, despite the lack of a physical obstacle or formation of bottom-trapped waves. In particular, a unique flow structure was found when the drifting flow and the topography interacted in the form of an “interference” regime at low Taylor number, but forming an erratic “irregular” regime at higher Taylor number. This suggests that blocking may be induced by either or both of a thermal or mechanical inhomogeneity. Evidence of coherent/persistent resonant wave triads was noted in both kinds of experiment, though the component wavenumbers of the wave-triads and their impact on the flow was found to depend on the topography in question.
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来源期刊
Geophysical and Astrophysical Fluid Dynamics
Geophysical and Astrophysical Fluid Dynamics 地学天文-地球化学与地球物理
CiteScore
3.10
自引率
0.00%
发文量
14
审稿时长
>12 weeks
期刊介绍: Geophysical and Astrophysical Fluid Dynamics exists for the publication of original research papers and short communications, occasional survey articles and conference reports on the fluid mechanics of the earth and planets, including oceans, atmospheres and interiors, and the fluid mechanics of the sun, stars and other astrophysical objects. In addition, their magnetohydrodynamic behaviours are investigated. Experimental, theoretical and numerical studies of rotating, stratified and convecting fluids of general interest to geophysicists and astrophysicists appear. Properly interpreted observational results are also published.
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