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Baroclinic, Kelvin and inertia-gravity waves in the barostrat instability experiment
- Source :
- Geophysical and Astrophysical Fluid Dynamics, Geophysical and Astrophysical Fluid Dynamics, Taylor & Francis, 2018, Geophysical and Astrophysical Fluid Dynamics, 2018
- Publication Year :
- 2018
- Publisher :
- HAL CCSD, 2018.
-
Abstract
- International audience; The differentially heated rotating annulus is a laboratory experiment historically designed for modelling large-scale features of the mid-latitude atmosphere. In the present study, we investigate a modified version of the classic baroclinic experiment in which a juxtaposition of convective and motionless stratified layers is created by introducing a vertical salt stratification. The thermal convective motions are suppressed in a central region at mid-depth of the rotating tank, therefore double-diffusive convection rolls can develop only in thin layers located at top and bottom, where the salt stratification is weakest. For high enough rotation rates, the baroclinic instability destabilises the flow in the top and the bottom shallow convective layers, generating cyclonic and anticyclonic eddies separated by the stable stratified layer. Thanks to this alternation of layers resembling the convective and radiative layers of stars, the planetary's atmospheric troposphere and stratosphere or turbulent layers at the sea surface above stratified waters, this new laboratory setup is of interest for both astrophysics and geophysical sciences. More specifically, it allows to study the exchange of momentum and energy between the layers, primarly by the propagation of internal gravity waves (IGW). PIV velocity maps are used to describe the wavy flow pattern at different heights. Using a co-rotating laser and camera, the wave field is well resolved and different wave types can be found: baroclinic waves, Kelvin, and Poincaré type waves. The signature of small-scale IGW can also be observed attached to the baroclinic jet. The baroclinic waves occur at the thin convectively active layer at the surface and the bottom of the tank, though decoupled they show different manifestation of nonlinear interactions. The inertial Kelvin and Poincaré waves seem to be mechanically forced. The small-scale wave trains attached to the meandering jet point to an imbalance of the large-scale flow. For the first time, the simultaneous occurrence of differentwave types is reported in detail for a differentially heated rotating annulus experiment.
- Subjects :
- [PHYS.PHYS.PHYS-FLU-DYN]Physics [physics]/Physics [physics]/Fluid Dynamics [physics.flu-dyn]
010504 meteorology & atmospheric sciences
Baroclinic instability
media_common.quotation_subject
Baroclinity
Computational Mechanics
Inertia
01 natural sciences
Instability
010305 fluids & plasmas
Physics::Fluid Dynamics
inertia-gravity waves
Geochemistry and Petrology
waves in rotating and stratified 31 fluids
0103 physical sciences
Annulus (firestop)
Astrophysics::Solar and Stellar Astrophysics
Astrophysics::Galaxy Astrophysics
Physics::Atmospheric and Oceanic Physics
0105 earth and related environmental sciences
media_common
Gravitational wave
Astronomy and Astrophysics
[PHYS.PHYS.PHYS-FLU-DYN] Physics [physics]/Physics [physics]/Fluid Dynamics [physics.flu-dyn]
Mechanics
Geophysics
13. Climate action
Mechanics of Materials
differentially heated rotating annulus
Astrophysics::Earth and Planetary Astrophysics
Laboratory experiment
Geology
Subjects
Details
- Language :
- English
- ISSN :
- 03091929 and 10290419
- Database :
- OpenAIRE
- Journal :
- Geophysical and Astrophysical Fluid Dynamics, Geophysical and Astrophysical Fluid Dynamics, Taylor & Francis, 2018, Geophysical and Astrophysical Fluid Dynamics, 2018
- Accession number :
- edsair.doi.dedup.....c800702adcec9228e2f07d1cb7dbabc5