Anisotropic turbulence and zonal jets in rotating flows with a ?-effect

Numerical studies of small-scale forced, two-dimensional turbulent flows on the surface of a rotating sphere have revealed strong large-scale anisotropization that culminates in the emergence of quasi-steady sets of alternating zonal jets, or zonation. The kinetic energy spectrum of such flows also...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Nonlinear processes in geophysics 2006-04, Vol.13 (1), p.83-98
Hauptverfasser: Galperin, B., Sukoriansky, S., Dikovskaya, N., Read, P. L., Yamazaki, Y. H., Wordsworth, R.
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page 98
container_issue 1
container_start_page 83
container_title Nonlinear processes in geophysics
container_volume 13
creator Galperin, B.
Sukoriansky, S.
Dikovskaya, N.
Read, P. L.
Yamazaki, Y. H.
Wordsworth, R.
description Numerical studies of small-scale forced, two-dimensional turbulent flows on the surface of a rotating sphere have revealed strong large-scale anisotropization that culminates in the emergence of quasi-steady sets of alternating zonal jets, or zonation. The kinetic energy spectrum of such flows also becomes strongly anisotropic. For the zonal modes, a steep spectral distribution, E(n)=CZ (?/R)2 n-5, is established, where CZ=O(1) is a non-dimensional coefficient, ? is the angular velocity, and R is the radius of the sphere, respectively. For other, non-zonal modes, the classical, Kolmogorov-Batchelor-Kraichnan, spectral law is preserved. This flow regime, referred to as a zonostrophic regime, appears to have wide applicability to large-scale planetary and terrestrial circulations as long as those are characterized by strong rotation, vertically stable stratification and small Burger numbers. The well-known manifestations of this regime are the banded disks of the outer planets of our Solar System. Relatively less known examples are systems of narrow, subsurface, alternating zonal jets throughout all major oceans discovered in state-of-the-art, eddy-permitting simulations of the general oceanic circulation. Furthermore, laboratory experiments recently conducted using the Coriolis turntable have basically confirmed that the lateral gradient of ''planetary vorticity'' (emulated via the topographic ?-effect) is the primary cause of the zonation and that the latter is entwined with the development of the strongly anisotropic kinetic energy spectrum that tends to attain the same zonal and non-zonal distributions, ?5 and , respectively, in both the slope and the magnitude, as the corresponding spectra in other environmental conditions. The non-dimensional coefficient CZ in the ?5 spectral law appears to be invariant, , in a variety of simulated and natural flows. This paper provides a brief review of the zonostrophic regime. The review includes the discussion of the physical nature, basic mechanisms, scaling laws and universality of this regime. A parameter range conducive to its establishment is identified, and collation of laboratory and naturally occurring flows is presented through which the zonostrophic regime manifests itself in the real world.
format Article
fullrecord <record><control><sourceid>hal</sourceid><recordid>TN_cdi_hal_primary_oai_HAL_hal_00302701v1</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>oai_HAL_hal_00302701v1</sourcerecordid><originalsourceid>FETCH-hal_primary_oai_HAL_hal_00302701v13</originalsourceid><addsrcrecordid>eNqViksKwjAUAIMoWD93eFsXhZd-7UqK-Fm4dF9iTWxKTEqSWvT0KngBVzMMMyIBzTAP8yLJxh_HKA7TNRZTMnOuRaRJmkUBOZRaOuOt6WQNvreXXnFdc2D6Ci-jmYKWewdSgzWeealvIJQZHAzSN8BgE3IheO0XZCKYcnz545ys9rvz9hg2TFWdlXdmn5VhsjqWp-rbEGOMcqQPGv_zvgH9dkCH</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Anisotropic turbulence and zonal jets in rotating flows with a ?-effect</title><source>DOAJ Directory of Open Access Journals</source><source>EZB-FREE-00999 freely available EZB journals</source><creator>Galperin, B. ; Sukoriansky, S. ; Dikovskaya, N. ; Read, P. L. ; Yamazaki, Y. H. ; Wordsworth, R.</creator><creatorcontrib>Galperin, B. ; Sukoriansky, S. ; Dikovskaya, N. ; Read, P. L. ; Yamazaki, Y. H. ; Wordsworth, R.</creatorcontrib><description>Numerical studies of small-scale forced, two-dimensional turbulent flows on the surface of a rotating sphere have revealed strong large-scale anisotropization that culminates in the emergence of quasi-steady sets of alternating zonal jets, or zonation. The kinetic energy spectrum of such flows also becomes strongly anisotropic. For the zonal modes, a steep spectral distribution, E(n)=CZ (?/R)2 n-5, is established, where CZ=O(1) is a non-dimensional coefficient, ? is the angular velocity, and R is the radius of the sphere, respectively. For other, non-zonal modes, the classical, Kolmogorov-Batchelor-Kraichnan, spectral law is preserved. This flow regime, referred to as a zonostrophic regime, appears to have wide applicability to large-scale planetary and terrestrial circulations as long as those are characterized by strong rotation, vertically stable stratification and small Burger numbers. The well-known manifestations of this regime are the banded disks of the outer planets of our Solar System. Relatively less known examples are systems of narrow, subsurface, alternating zonal jets throughout all major oceans discovered in state-of-the-art, eddy-permitting simulations of the general oceanic circulation. Furthermore, laboratory experiments recently conducted using the Coriolis turntable have basically confirmed that the lateral gradient of ''planetary vorticity'' (emulated via the topographic ?-effect) is the primary cause of the zonation and that the latter is entwined with the development of the strongly anisotropic kinetic energy spectrum that tends to attain the same zonal and non-zonal distributions, ?5 and , respectively, in both the slope and the magnitude, as the corresponding spectra in other environmental conditions. The non-dimensional coefficient CZ in the ?5 spectral law appears to be invariant, , in a variety of simulated and natural flows. This paper provides a brief review of the zonostrophic regime. The review includes the discussion of the physical nature, basic mechanisms, scaling laws and universality of this regime. A parameter range conducive to its establishment is identified, and collation of laboratory and naturally occurring flows is presented through which the zonostrophic regime manifests itself in the real world.</description><identifier>ISSN: 1023-5809</identifier><identifier>EISSN: 1607-7946</identifier><language>eng</language><publisher>European Geosciences Union (EGU)</publisher><subject>Astrophysics ; Cosmology and Extra-Galactic Astrophysics ; Earth Sciences ; Physics ; Sciences of the Universe</subject><ispartof>Nonlinear processes in geophysics, 2006-04, Vol.13 (1), p.83-98</ispartof><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,780,784,885</link.rule.ids><backlink>$$Uhttps://hal.science/hal-00302701$$DView record in HAL$$Hfree_for_read</backlink></links><search><creatorcontrib>Galperin, B.</creatorcontrib><creatorcontrib>Sukoriansky, S.</creatorcontrib><creatorcontrib>Dikovskaya, N.</creatorcontrib><creatorcontrib>Read, P. L.</creatorcontrib><creatorcontrib>Yamazaki, Y. H.</creatorcontrib><creatorcontrib>Wordsworth, R.</creatorcontrib><title>Anisotropic turbulence and zonal jets in rotating flows with a ?-effect</title><title>Nonlinear processes in geophysics</title><description>Numerical studies of small-scale forced, two-dimensional turbulent flows on the surface of a rotating sphere have revealed strong large-scale anisotropization that culminates in the emergence of quasi-steady sets of alternating zonal jets, or zonation. The kinetic energy spectrum of such flows also becomes strongly anisotropic. For the zonal modes, a steep spectral distribution, E(n)=CZ (?/R)2 n-5, is established, where CZ=O(1) is a non-dimensional coefficient, ? is the angular velocity, and R is the radius of the sphere, respectively. For other, non-zonal modes, the classical, Kolmogorov-Batchelor-Kraichnan, spectral law is preserved. This flow regime, referred to as a zonostrophic regime, appears to have wide applicability to large-scale planetary and terrestrial circulations as long as those are characterized by strong rotation, vertically stable stratification and small Burger numbers. The well-known manifestations of this regime are the banded disks of the outer planets of our Solar System. Relatively less known examples are systems of narrow, subsurface, alternating zonal jets throughout all major oceans discovered in state-of-the-art, eddy-permitting simulations of the general oceanic circulation. Furthermore, laboratory experiments recently conducted using the Coriolis turntable have basically confirmed that the lateral gradient of ''planetary vorticity'' (emulated via the topographic ?-effect) is the primary cause of the zonation and that the latter is entwined with the development of the strongly anisotropic kinetic energy spectrum that tends to attain the same zonal and non-zonal distributions, ?5 and , respectively, in both the slope and the magnitude, as the corresponding spectra in other environmental conditions. The non-dimensional coefficient CZ in the ?5 spectral law appears to be invariant, , in a variety of simulated and natural flows. This paper provides a brief review of the zonostrophic regime. The review includes the discussion of the physical nature, basic mechanisms, scaling laws and universality of this regime. A parameter range conducive to its establishment is identified, and collation of laboratory and naturally occurring flows is presented through which the zonostrophic regime manifests itself in the real world.</description><subject>Astrophysics</subject><subject>Cosmology and Extra-Galactic Astrophysics</subject><subject>Earth Sciences</subject><subject>Physics</subject><subject>Sciences of the Universe</subject><issn>1023-5809</issn><issn>1607-7946</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2006</creationdate><recordtype>article</recordtype><recordid>eNqViksKwjAUAIMoWD93eFsXhZd-7UqK-Fm4dF9iTWxKTEqSWvT0KngBVzMMMyIBzTAP8yLJxh_HKA7TNRZTMnOuRaRJmkUBOZRaOuOt6WQNvreXXnFdc2D6Ci-jmYKWewdSgzWeealvIJQZHAzSN8BgE3IheO0XZCKYcnz545ys9rvz9hg2TFWdlXdmn5VhsjqWp-rbEGOMcqQPGv_zvgH9dkCH</recordid><startdate>20060404</startdate><enddate>20060404</enddate><creator>Galperin, B.</creator><creator>Sukoriansky, S.</creator><creator>Dikovskaya, N.</creator><creator>Read, P. L.</creator><creator>Yamazaki, Y. H.</creator><creator>Wordsworth, R.</creator><general>European Geosciences Union (EGU)</general><scope>1XC</scope><scope>VOOES</scope></search><sort><creationdate>20060404</creationdate><title>Anisotropic turbulence and zonal jets in rotating flows with a ?-effect</title><author>Galperin, B. ; Sukoriansky, S. ; Dikovskaya, N. ; Read, P. L. ; Yamazaki, Y. H. ; Wordsworth, R.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-hal_primary_oai_HAL_hal_00302701v13</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2006</creationdate><topic>Astrophysics</topic><topic>Cosmology and Extra-Galactic Astrophysics</topic><topic>Earth Sciences</topic><topic>Physics</topic><topic>Sciences of the Universe</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Galperin, B.</creatorcontrib><creatorcontrib>Sukoriansky, S.</creatorcontrib><creatorcontrib>Dikovskaya, N.</creatorcontrib><creatorcontrib>Read, P. L.</creatorcontrib><creatorcontrib>Yamazaki, Y. H.</creatorcontrib><creatorcontrib>Wordsworth, R.</creatorcontrib><collection>Hyper Article en Ligne (HAL)</collection><collection>Hyper Article en Ligne (HAL) (Open Access)</collection><jtitle>Nonlinear processes in geophysics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Galperin, B.</au><au>Sukoriansky, S.</au><au>Dikovskaya, N.</au><au>Read, P. L.</au><au>Yamazaki, Y. H.</au><au>Wordsworth, R.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Anisotropic turbulence and zonal jets in rotating flows with a ?-effect</atitle><jtitle>Nonlinear processes in geophysics</jtitle><date>2006-04-04</date><risdate>2006</risdate><volume>13</volume><issue>1</issue><spage>83</spage><epage>98</epage><pages>83-98</pages><issn>1023-5809</issn><eissn>1607-7946</eissn><abstract>Numerical studies of small-scale forced, two-dimensional turbulent flows on the surface of a rotating sphere have revealed strong large-scale anisotropization that culminates in the emergence of quasi-steady sets of alternating zonal jets, or zonation. The kinetic energy spectrum of such flows also becomes strongly anisotropic. For the zonal modes, a steep spectral distribution, E(n)=CZ (?/R)2 n-5, is established, where CZ=O(1) is a non-dimensional coefficient, ? is the angular velocity, and R is the radius of the sphere, respectively. For other, non-zonal modes, the classical, Kolmogorov-Batchelor-Kraichnan, spectral law is preserved. This flow regime, referred to as a zonostrophic regime, appears to have wide applicability to large-scale planetary and terrestrial circulations as long as those are characterized by strong rotation, vertically stable stratification and small Burger numbers. The well-known manifestations of this regime are the banded disks of the outer planets of our Solar System. Relatively less known examples are systems of narrow, subsurface, alternating zonal jets throughout all major oceans discovered in state-of-the-art, eddy-permitting simulations of the general oceanic circulation. Furthermore, laboratory experiments recently conducted using the Coriolis turntable have basically confirmed that the lateral gradient of ''planetary vorticity'' (emulated via the topographic ?-effect) is the primary cause of the zonation and that the latter is entwined with the development of the strongly anisotropic kinetic energy spectrum that tends to attain the same zonal and non-zonal distributions, ?5 and , respectively, in both the slope and the magnitude, as the corresponding spectra in other environmental conditions. The non-dimensional coefficient CZ in the ?5 spectral law appears to be invariant, , in a variety of simulated and natural flows. This paper provides a brief review of the zonostrophic regime. The review includes the discussion of the physical nature, basic mechanisms, scaling laws and universality of this regime. A parameter range conducive to its establishment is identified, and collation of laboratory and naturally occurring flows is presented through which the zonostrophic regime manifests itself in the real world.</abstract><pub>European Geosciences Union (EGU)</pub><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier ISSN: 1023-5809
ispartof Nonlinear processes in geophysics, 2006-04, Vol.13 (1), p.83-98
issn 1023-5809
1607-7946
language eng
recordid cdi_hal_primary_oai_HAL_hal_00302701v1
source DOAJ Directory of Open Access Journals; EZB-FREE-00999 freely available EZB journals
subjects Astrophysics
Cosmology and Extra-Galactic Astrophysics
Earth Sciences
Physics
Sciences of the Universe
title Anisotropic turbulence and zonal jets in rotating flows with a ?-effect
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-01T02%3A44%3A41IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-hal&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Anisotropic%20turbulence%20and%20zonal%20jets%20in%20rotating%20flows%20with%20a%20?-effect&rft.jtitle=Nonlinear%20processes%20in%20geophysics&rft.au=Galperin,%20B.&rft.date=2006-04-04&rft.volume=13&rft.issue=1&rft.spage=83&rft.epage=98&rft.pages=83-98&rft.issn=1023-5809&rft.eissn=1607-7946&rft_id=info:doi/&rft_dat=%3Chal%3Eoai_HAL_hal_00302701v1%3C/hal%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true