Please use this identifier to cite or link to this item: http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/7688
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dc.contributor.authorRaghav, Mukesh Singh-
dc.contributor.authorJose, Sharath-
dc.contributor.authorAPTE, AMIT-
dc.contributor.authorGovindarajan, Rama-
dc.date.accessioned2023-04-03T06:37:47Z-
dc.date.available2023-04-03T06:37:47Z-
dc.date.issued2022-12-
dc.identifier.citationDynamics of Atmospheres and Oceans, 100, 101331.en_US
dc.identifier.issn1872-6879-
dc.identifier.issn0377-0265-
dc.identifier.urihttps://doi.org/10.1016/j.dynatmoce.2022.101331en_US
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/7688-
dc.description.abstractLinear modal stability analysis of a mean zonal shear flow is carried out in the framework of rotating shallow water equations (RSWE), both under the -plane approximation and in the full spherical coordinate system. Two base flows – equatorial easterly (EE) and westerly (EW) – with Gaussian profiles highly confined to small latitudes are analysed. At low Froude number, mixed Rossby-gravity (MRG) and Rossby waves are found to be particularly affected by shear, with prominent changes at higher wavenumbers. These waves become practically non-dispersive at large wavenumbers in EE. The perturbations are found to be more confined equatorially in EE than in EW with the degree of confinement being more pronounced in the -plane system compared to the full spherical system. At high Froude number, the phase speeds are significantly larger in the -plane system for all families of waves. Under the -plane approximation, exponentially unstable modes can be excited, having negative (positive) phase speed in EE (EW). Strikingly, this flow is always neutrally stable with the full spherical system. This speaks for the importance of studying the whole spherical system even for equatorially confined shear.en_US
dc.language.isoenen_US
dc.publisherElsevier B.V.en_US
dc.subjectData Scienceen_US
dc.subject2023-MAR-WEEK4en_US
dc.subjectTOC-MAR-2023en_US
dc.subject2022en_US
dc.titleEffects of equatorially-confined shear flow on MRG and Rossby wavesen_US
dc.typeArticleen_US
dc.contributor.departmentDept. of Data Scienceen_US
dc.identifier.sourcetitleDynamics of Atmospheres and Oceansen_US
dc.publication.originofpublisherForeignen_US
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