Matches in SemOpenAlex for { <https://semopenalex.org/work/W2804067156> ?p ?o ?g. }
- W2804067156 endingPage "221" @default.
- W2804067156 startingPage "207" @default.
- W2804067156 abstract "We conduct in-depth analysis of statistical flow properties from direct numerical simulations that reproduce gas giants macroturbulence, namely large-scale zonal winds. Our numerical model has been specifically designed to simulate a recent laboratory device that reports zonal jets in the configuration of deep turbulent planetary layers. In this framework, the so-called zonostrophic regime is achieved when large topographical variations of the fluid layer combine with rapid rotation in a well developed three-dimensional (3D) turbulent flow. At steady state, strongly energetic, zonally dominated, large-scale axisymmetric structures emerge scaling with Rhines’ theoretical scale. This model differs from the shallow-layer scenario where the flow is confined to a quasi-two-dimensional (2D) fluid shell and the anisotropic β-effect arises from latitudinal variation of the Coriolis force. Thus, we aim to reveal, in the specific framework of the deep-layer scenario, signatures of the zonostrophic regime and of a β-topography in statistical flow properties. To do so, we run two large-scale 3D direct numerical simulations in a cylindrical geometry of a highly turbulent and rapidly rotating flow. These two simulations use similar set of parameters but with and without topographical β-effect. We propose a comparative phenomenological description of the temporal and spatial statistics of the three components of the velocity field. Interestingly, we report that peculiar correlations occur between the vertical and radial flow components when a β-topography is imposed and show a feature possibly due to a zonostrophic dynamics in 3D frequency spectra. These results suggest the development of new tools to remotely investigate gas giants zonal winds by extracting statistical flow properties from direct observations. Ultimately our analysis may support the relevance of the deep models in the study of prevalent features of planetary dynamics." @default.
- W2804067156 created "2018-06-01" @default.
- W2804067156 creator A5003912444 @default.
- W2804067156 creator A5010885870 @default.
- W2804067156 creator A5071249529 @default.
- W2804067156 date "2018-05-04" @default.
- W2804067156 modified "2023-09-26" @default.
- W2804067156 title "Some statistical properties of three-dimensional zonostrophic turbulence" @default.
- W2804067156 cites W1642713960 @default.
- W2804067156 cites W1676010385 @default.
- W2804067156 cites W1791800591 @default.
- W2804067156 cites W1957969437 @default.
- W2804067156 cites W1964655082 @default.
- W2804067156 cites W1966809411 @default.
- W2804067156 cites W1970730011 @default.
- W2804067156 cites W1984695169 @default.
- W2804067156 cites W2003355718 @default.
- W2804067156 cites W2004337164 @default.
- W2804067156 cites W2014901376 @default.
- W2804067156 cites W2021982399 @default.
- W2804067156 cites W2033312637 @default.
- W2804067156 cites W2036928351 @default.
- W2804067156 cites W2037444980 @default.
- W2804067156 cites W2041450865 @default.
- W2804067156 cites W2045444659 @default.
- W2804067156 cites W2047657606 @default.
- W2804067156 cites W2049125544 @default.
- W2804067156 cites W2050962398 @default.
- W2804067156 cites W2050994161 @default.
- W2804067156 cites W2053453401 @default.
- W2804067156 cites W2073636625 @default.
- W2804067156 cites W2087943296 @default.
- W2804067156 cites W2089388484 @default.
- W2804067156 cites W2090835797 @default.
- W2804067156 cites W2093085344 @default.
- W2804067156 cites W2093642301 @default.
- W2804067156 cites W2099743374 @default.
- W2804067156 cites W2128092034 @default.
- W2804067156 cites W2136446295 @default.
- W2804067156 cites W2137902856 @default.
- W2804067156 cites W2138427209 @default.
- W2804067156 cites W2160110831 @default.
- W2804067156 cites W2217256413 @default.
- W2804067156 cites W2263731895 @default.
- W2804067156 cites W2566133122 @default.
- W2804067156 cites W2581688326 @default.
- W2804067156 cites W2963245390 @default.
- W2804067156 cites W2963979763 @default.
- W2804067156 cites W3122513843 @default.
- W2804067156 doi "https://doi.org/10.1080/03091929.2018.1467413" @default.
- W2804067156 hasPublicationYear "2018" @default.
- W2804067156 type Work @default.
- W2804067156 sameAs 2804067156 @default.
- W2804067156 citedByCount "4" @default.
- W2804067156 countsByYear W28040671562020 @default.
- W2804067156 countsByYear W28040671562021 @default.
- W2804067156 countsByYear W28040671562023 @default.
- W2804067156 crossrefType "journal-article" @default.
- W2804067156 hasAuthorship W2804067156A5003912444 @default.
- W2804067156 hasAuthorship W2804067156A5010885870 @default.
- W2804067156 hasAuthorship W2804067156A5071249529 @default.
- W2804067156 hasBestOaLocation W28040671562 @default.
- W2804067156 hasConcept C116515362 @default.
- W2804067156 hasConcept C120665830 @default.
- W2804067156 hasConcept C121332964 @default.
- W2804067156 hasConcept C121864883 @default.
- W2804067156 hasConcept C145290371 @default.
- W2804067156 hasConcept C182748727 @default.
- W2804067156 hasConcept C18533594 @default.
- W2804067156 hasConcept C196558001 @default.
- W2804067156 hasConcept C2524010 @default.
- W2804067156 hasConcept C2775909724 @default.
- W2804067156 hasConcept C2778755073 @default.
- W2804067156 hasConcept C33026886 @default.
- W2804067156 hasConcept C33923547 @default.
- W2804067156 hasConcept C38349280 @default.
- W2804067156 hasConcept C57879066 @default.
- W2804067156 hasConcept C62520636 @default.
- W2804067156 hasConcept C74650414 @default.
- W2804067156 hasConcept C82706917 @default.
- W2804067156 hasConcept C85725439 @default.
- W2804067156 hasConcept C99844830 @default.
- W2804067156 hasConceptScore W2804067156C116515362 @default.
- W2804067156 hasConceptScore W2804067156C120665830 @default.
- W2804067156 hasConceptScore W2804067156C121332964 @default.
- W2804067156 hasConceptScore W2804067156C121864883 @default.
- W2804067156 hasConceptScore W2804067156C145290371 @default.
- W2804067156 hasConceptScore W2804067156C182748727 @default.
- W2804067156 hasConceptScore W2804067156C18533594 @default.
- W2804067156 hasConceptScore W2804067156C196558001 @default.
- W2804067156 hasConceptScore W2804067156C2524010 @default.
- W2804067156 hasConceptScore W2804067156C2775909724 @default.
- W2804067156 hasConceptScore W2804067156C2778755073 @default.
- W2804067156 hasConceptScore W2804067156C33026886 @default.
- W2804067156 hasConceptScore W2804067156C33923547 @default.
- W2804067156 hasConceptScore W2804067156C38349280 @default.
- W2804067156 hasConceptScore W2804067156C57879066 @default.
- W2804067156 hasConceptScore W2804067156C62520636 @default.