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Introduction.

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Title: Introduction.
Authors: Favier, Benjamin1 (AUTHOR), Le Bars, Michael1 (AUTHOR), Le Dizès, Stéphane1 (AUTHOR), Le Gal, Patrice1 (AUTHOR), Meunier, Patrice1 (AUTHOR)
Source: Geophysical & Astrophysical Fluid Dynamics. Jun2021, Vol. 115 Issue 3, p231-233. 3p.
Subjects: Astrophysical fluid dynamics, Geophysical fluid dynamics, Gravitational interactions, Taylor vortices, Earth sciences
Abstract: In the work of G. Meletti I et al. i , numerical simulations are complemented by laboratory experiments on the Strato-Rotational Instability (SRI) making the rotating shear flow unstable in regions where - without stratification - it would be stable. Inversely, the present results allow to use the Velikhov-Chandrasekhar criterion of the MRI to predict the elasto-rotational instability (ERI) observed in their experiment. Graph This special issue includes some of the many contributions and lectures given at the "Waves, Instabilities and Turbulence in Geophysical and Astrophysical Flows (WITGAF)" summer school and workshop held at the Institut d'Etudes Scientifiques de Cargèse (Corsica, France) from 8 to 19 of July 2019 (https://witgaf2019.sciencesconf.org/). [Extracted from the article]
Copyright of Geophysical & Astrophysical Fluid Dynamics is the property of Taylor & Francis Ltd and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)
Database: Engineering Source
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  Data: In the work of G. Meletti I et al. i , numerical simulations are complemented by laboratory experiments on the Strato-Rotational Instability (SRI) making the rotating shear flow unstable in regions where - without stratification - it would be stable. Inversely, the present results allow to use the Velikhov-Chandrasekhar criterion of the MRI to predict the elasto-rotational instability (ERI) observed in their experiment. Graph This special issue includes some of the many contributions and lectures given at the "Waves, Instabilities and Turbulence in Geophysical and Astrophysical Flows (WITGAF)" summer school and workshop held at the Institut d'Etudes Scientifiques de Cargèse (Corsica, France) from 8 to 19 of July 2019 (https://witgaf2019.sciencesconf.org/). [Extracted from the article]
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  Data: <i>Copyright of Geophysical & Astrophysical Fluid Dynamics is the property of Taylor & Francis Ltd and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.)
PLink https://search.ebscohost.com/login.aspx?direct=true&site=eds-live&db=egs&AN=150677586
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        Value: 10.1080/03091929.2021.1910458
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      – Code: eng
        Text: English
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        PageCount: 3
        StartPage: 231
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      – SubjectFull: Astrophysical fluid dynamics
        Type: general
      – SubjectFull: Geophysical fluid dynamics
        Type: general
      – SubjectFull: Gravitational interactions
        Type: general
      – SubjectFull: Taylor vortices
        Type: general
      – SubjectFull: Earth sciences
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      – TitleFull: Introduction.
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              M: 06
              Text: Jun2021
              Type: published
              Y: 2021
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