Inverse cascades and resonant triads in rotating and stratified turbulence
Kraichnan's seminal ideas on inverse cascades yielded new tools to study common phenomena in geophysical turbulent flows. In the atmosphere and the oceans, rotation and stratification result in a flow that can be approximated as two-dimensional at very large scales but which requires considerin...
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2017
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| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_10706631_v29_n11_p_Oks http://hdl.handle.net/20.500.12110/paper_10706631_v29_n11_p_Oks |
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paper:paper_10706631_v29_n11_p_Oks2023-06-08T16:04:35Z Inverse cascades and resonant triads in rotating and stratified turbulence Astrophysics Horizontal pressure Inertia gravity waves Non-linear phenomena Quasi-geostrophic Spatio-temporal spectrum Stratified turbulence Three dimensional effect Turbulent transport process Rotation Kraichnan's seminal ideas on inverse cascades yielded new tools to study common phenomena in geophysical turbulent flows. In the atmosphere and the oceans, rotation and stratification result in a flow that can be approximated as two-dimensional at very large scales but which requires considering three-dimensional effects to fully describe turbulent transport processes and non-linear phenomena. Motions can thus be classified into two classes: fast modes consisting of inertia-gravity waves and slow quasi-geostrophic modes for which the Coriolis force and horizontal pressure gradients are close to balance. In this paper, we review previous results on the strength of the inverse cascade in rotating and stratified flows and then present new results on the effect of varying the strength of rotation and stratification (measured by the inverse Prandtl ratio N/f, of the Coriolis frequency to the Brunt- Väisäla frequency) on the amplitude of the waves and on the flow quasi-geostrophic behavior. We show that the inverse cascade is more efficient in the range of N/f for which resonant triads do not exist, 1/2 ≤ N/f ≤ 2.We then use the spatio-temporal spectrum to show that in this range slow modes dominate the dynamics, while the strength of the waves (and their relevance in the flow dynamics) is weaker. 2017 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_10706631_v29_n11_p_Oks http://hdl.handle.net/20.500.12110/paper_10706631_v29_n11_p_Oks |
| institution |
Universidad de Buenos Aires |
| institution_str |
I-28 |
| repository_str |
R-134 |
| collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
| topic |
Astrophysics Horizontal pressure Inertia gravity waves Non-linear phenomena Quasi-geostrophic Spatio-temporal spectrum Stratified turbulence Three dimensional effect Turbulent transport process Rotation |
| spellingShingle |
Astrophysics Horizontal pressure Inertia gravity waves Non-linear phenomena Quasi-geostrophic Spatio-temporal spectrum Stratified turbulence Three dimensional effect Turbulent transport process Rotation Inverse cascades and resonant triads in rotating and stratified turbulence |
| topic_facet |
Astrophysics Horizontal pressure Inertia gravity waves Non-linear phenomena Quasi-geostrophic Spatio-temporal spectrum Stratified turbulence Three dimensional effect Turbulent transport process Rotation |
| description |
Kraichnan's seminal ideas on inverse cascades yielded new tools to study common phenomena in geophysical turbulent flows. In the atmosphere and the oceans, rotation and stratification result in a flow that can be approximated as two-dimensional at very large scales but which requires considering three-dimensional effects to fully describe turbulent transport processes and non-linear phenomena. Motions can thus be classified into two classes: fast modes consisting of inertia-gravity waves and slow quasi-geostrophic modes for which the Coriolis force and horizontal pressure gradients are close to balance. In this paper, we review previous results on the strength of the inverse cascade in rotating and stratified flows and then present new results on the effect of varying the strength of rotation and stratification (measured by the inverse Prandtl ratio N/f, of the Coriolis frequency to the Brunt- Väisäla frequency) on the amplitude of the waves and on the flow quasi-geostrophic behavior. We show that the inverse cascade is more efficient in the range of N/f for which resonant triads do not exist, 1/2 ≤ N/f ≤ 2.We then use the spatio-temporal spectrum to show that in this range slow modes dominate the dynamics, while the strength of the waves (and their relevance in the flow dynamics) is weaker. |
| title |
Inverse cascades and resonant triads in rotating and stratified turbulence |
| title_short |
Inverse cascades and resonant triads in rotating and stratified turbulence |
| title_full |
Inverse cascades and resonant triads in rotating and stratified turbulence |
| title_fullStr |
Inverse cascades and resonant triads in rotating and stratified turbulence |
| title_full_unstemmed |
Inverse cascades and resonant triads in rotating and stratified turbulence |
| title_sort |
inverse cascades and resonant triads in rotating and stratified turbulence |
| publishDate |
2017 |
| url |
https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_10706631_v29_n11_p_Oks http://hdl.handle.net/20.500.12110/paper_10706631_v29_n11_p_Oks |
| _version_ |
1768543622728253440 |