Evolution of small-scale turbulence at large Richardson numbers
<p>The theory of stratified turbulent flow developed earlier by the authors is applied to data from different areas of the ocean. It is shown that turbulence can be amplified and supported even at large gradient Richardson numbers. The cause of that is the exchange between kinetic and potent...
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Format: | Article |
Language: | English |
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Copernicus Publications
2024-04-01
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Series: | Nonlinear Processes in Geophysics |
Online Access: | https://npg.copernicus.org/articles/31/219/2024/npg-31-219-2024.pdf |
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author | L. Ostrovsky I. Soustova Y. Troitskaya D. Gladskikh D. Gladskikh D. Gladskikh |
author_facet | L. Ostrovsky I. Soustova Y. Troitskaya D. Gladskikh D. Gladskikh D. Gladskikh |
author_sort | L. Ostrovsky |
collection | DOAJ |
description | <p>The theory of stratified turbulent flow developed earlier by the authors is applied to data from different areas of the ocean. It is shown that turbulence can be amplified and supported even at large gradient Richardson numbers. The cause of that is the exchange between kinetic and potential energies of turbulence. Using the profiles of Brunt–Väisälä frequency and vertical current shear given in <span class="cit" id="xref_text.1"><a href="#bib1.bibx4">Forryan et al.</a> (<a href="#bib1.bibx4">2013</a>)</span>, the profiles of the kinetic energy dissipation rate are calculated. The results are in reasonable agreement with the experimental data.</p> |
first_indexed | 2024-04-24T05:53:58Z |
format | Article |
id | doaj.art-e82e0f127f3b44c99ad8fb4dc80a1322 |
institution | Directory Open Access Journal |
issn | 1023-5809 1607-7946 |
language | English |
last_indexed | 2024-04-24T05:53:58Z |
publishDate | 2024-04-01 |
publisher | Copernicus Publications |
record_format | Article |
series | Nonlinear Processes in Geophysics |
spelling | doaj.art-e82e0f127f3b44c99ad8fb4dc80a13222024-04-23T09:41:11ZengCopernicus PublicationsNonlinear Processes in Geophysics1023-58091607-79462024-04-013121922710.5194/npg-31-219-2024Evolution of small-scale turbulence at large Richardson numbersL. Ostrovsky0I. Soustova1Y. Troitskaya2D. Gladskikh3D. Gladskikh4D. Gladskikh5Dept. of Applied Mathematics, University of Colorado, Boulder, CO 80309, USAInstitute of Applied Physics, Russian Academy of Sciences, 603950 Nizhny Novgorod, RussiaInstitute of Applied Physics, Russian Academy of Sciences, 603950 Nizhny Novgorod, RussiaInstitute of Applied Physics, Russian Academy of Sciences, 603950 Nizhny Novgorod, RussiaMoscow Center for Fundamental and Applied Mathematics, 119991 Moscow, RussiaResearch Computing Center, Moscow State University, 119991 Moscow, Russia<p>The theory of stratified turbulent flow developed earlier by the authors is applied to data from different areas of the ocean. It is shown that turbulence can be amplified and supported even at large gradient Richardson numbers. The cause of that is the exchange between kinetic and potential energies of turbulence. Using the profiles of Brunt–Väisälä frequency and vertical current shear given in <span class="cit" id="xref_text.1"><a href="#bib1.bibx4">Forryan et al.</a> (<a href="#bib1.bibx4">2013</a>)</span>, the profiles of the kinetic energy dissipation rate are calculated. The results are in reasonable agreement with the experimental data.</p>https://npg.copernicus.org/articles/31/219/2024/npg-31-219-2024.pdf |
spellingShingle | L. Ostrovsky I. Soustova Y. Troitskaya D. Gladskikh D. Gladskikh D. Gladskikh Evolution of small-scale turbulence at large Richardson numbers Nonlinear Processes in Geophysics |
title | Evolution of small-scale turbulence at large Richardson numbers |
title_full | Evolution of small-scale turbulence at large Richardson numbers |
title_fullStr | Evolution of small-scale turbulence at large Richardson numbers |
title_full_unstemmed | Evolution of small-scale turbulence at large Richardson numbers |
title_short | Evolution of small-scale turbulence at large Richardson numbers |
title_sort | evolution of small scale turbulence at large richardson numbers |
url | https://npg.copernicus.org/articles/31/219/2024/npg-31-219-2024.pdf |
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