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A laboratory study of baroclinic waves and turbulence in an internally heated rotating fluid annulus with sloping endwalls
Abstract
New laboratory experiments have been performed in a rotating fluid annulus, subject to internal heating and sidewall cooling, in which a radial depth gradient has been created by the inclusion of oppositely sloping boundaries. Endwall configurations that cause the fluid depth ( D ) to increase with radius (∂ D /∂ r >0) and to decrease with radius (∂ D /∂ r <0) have been studied, as the former is applicable to the terrestrial atmosphere and oceans, while the latter may be relevant to deep atmospheres such as those of the giant planets. Even with the steepest boundary slopes, isolated or periodic chains of stable coherent eddies are observed with both endwall configurations, and these regular eddy modes are seen to drift relative to the walls of the convection chamber concordant with simple Rossby wave ideas. When the boundary slope (δ) is small, no difference is observed in the range of azimuthal wavenumbers seen in the regular wave regimes of the two endwall configurations. At larger values of δ, however, this symmetry is lost, since regular modes m =2 to 8 are observed with ∂ D /∂ r >0 endwalls, while only a large vertically trapped anticyclonic gyre is seen with ∂ D /∂ r <0 endwalls. The other effects of the radial depth gradient are the observed reduction in both the lateral and vertical scale of the eddy features, and the formation of two independent trains of eddies within the gap width at sufficiently high rotation rates in the ∂ D /∂ r >0 endwall experiments. The zonal mean flow is also found to develop a significant barotropic component, superimposed on the vertically and horizontally sheared zonal jets generated by the non-monotonic thermal gradient of the experiment. This barotropic component is predominantly prograde (retrograde) in the ∂ D /∂ r >0 (∂ D /∂ r <0) endwall experiments, and confined close to the outer (inner) wall where the fluid depth is greatest. There is evidence of the formation of increased numbers of zonal jets in the ∂ D /∂ r >0 endwall experiments above that expected from the form of the thermal forcing. These multiple zonal jets are highly localized in the vertical, and are trapped close to the top boundary. Their radial scale is, nevertheless, close to that given by the Rhines argument. No comparable increase in the radial wavenumber of the mean flow is observed in the ∂ D /∂ r <0 endwall experiments in the present system.
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Previous studies have shown that baroclinic instabilities can equilibrate into meanders in such profiles.
“Previous studies have also shown how baroclinic instabilities can equilibrate into meanders in such pro fi les ( Koschmieder & White 1981; Bastin & Read 1997; Sutyrin et al. 2001 ) .”
From MEANDERING SHALLOW ATMOSPHERIC JET AS A MODEL OF SATURNʼS NORTH-POLAR HEXAGON (2015) · cites this paper as Bastin & Read 1997
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A laboratory model of Saturn's North Polar hexagon
Barbosa Aguiar, A. C., Read, P. L., Wordsworth, R. D., Salter, T., & Hiro Yamazaki, Y. (2010) · Icarus · doi:10.1016/j.icarus.2009.10.022 · Cited by 95
Self-citationMEANDERING SHALLOW ATMOSPHERIC JET AS A MODEL OF SATURNʼS NORTH-POLAR HEXAGON
Morales-Juberías, R., Sayanagi, K. M., Simon, A. A., Fletcher, L. N., & Cosentino, R. G. (2015) · The Astrophysical Journal · doi:10.1088/2041-8205/806/1/l18 · Cited by 35
Zonal jets at the laboratory scale: hysteresis and Rossby waves resonance
Lemasquerier, D., Favier, B., & Le Bars, M. (2021) · Journal of Fluid Mechanics · doi:10.1017/jfm.2020.1000 · Cited by 30
“…thanks to natural instabilities such as barotropic (Condie & Rhines 1994; Gillet et al. 2007; Read et al. 2015) or baroclinic thermal convection, in the differentially heated rotating annulus configuration (Hide & Mason 1975; Bastin & Read 1997, 1998; Wordsworth et al. 2008; Smith et al. 2014).”
Background
Metadata
- Authors
- BASTIN, M. E., & READ, P. L.
- Affiliations
- University of Oxford (GB)
- Venue
- Journal of Fluid Mechanics
- Publisher
- Cambridge University Press (CUP)
- Published
- 1997-05-25
- Volume
- 339
- Pages
- 173-198
- ISSN
- 0022-1120 (ISSN-L)
- 1469-7645
- OpenAlex
- W1964253424
- Cited by
- 27
- References
- 0
- Citations by year
- 2025: 1 · 2024: 1 · 2022: 2 · 2021: 3 · 2017: 1 · 2016: 1 · 2015: 1 · 2014: 4 · 2012: 1
- FWCI
- 2.95
- Type
- journal article
- Language
- en
- Open access
- closed
- Locations
- Journal of Fluid Mechanics (publishedVersion)
- Topics
- Physical Sciences › Engineering › Computational Mechanics › Fluid Dynamics and Turbulent Flows
- Physical Sciences › Earth and Planetary Sciences › Oceanography › Oceanographic and Atmospheric Processes
- Physical Sciences › Earth and Planetary Sciences › Atmospheric Science › Meteorological Phenomena and Simulations
- Keywords
- baroclinic waves, internal heating, Rossby waves, zonal jets, Rhines scale, anticyclonic gyre, turbulent flow, giant planet atmospheres, azimuthal wavenumber
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