Internal shear layers in librating spherical shells: The case of periodic characteristic paths

Internal shear layers generated by the longitudinal libration of the inner core in a spherical shell rotating at a rate are analysed asymptotically and numerically. The forcing frequency is chosen as such that the layers issued from the inner core at the critical latitude in the form of concentrated...

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Bibliographic Details
Main Authors: Favier, B. (Author), He, J. (Author), Le Dizès, S. (Author), Rieutord, M. (Author)
Format: Article
Language:English
Published: Cambridge University Press 2022
Subjects:
Online Access:View Fulltext in Publisher
LEADER 02746nam a2200349Ia 4500
001 10.1017-jfm.2022.138
008 220425s2022 CNT 000 0 und d
020 |a 00221120 (ISSN) 
245 1 0 |a Internal shear layers in librating spherical shells: The case of periodic characteristic paths 
260 0 |b Cambridge University Press  |c 2022 
856 |z View Fulltext in Publisher  |u https://doi.org/10.1017/jfm.2022.138 
520 3 |a Internal shear layers generated by the longitudinal libration of the inner core in a spherical shell rotating at a rate are analysed asymptotically and numerically. The forcing frequency is chosen as such that the layers issued from the inner core at the critical latitude in the form of concentrated conical beams draw a simple rectangular pattern in meridional cross-sections. The asymptotic structure of the internal shear layers is described by extending the self-similar solution known for open domains to closed domains where reflections on the boundaries occur. The periodic ray path ensures that the beams remain localised around it. Asymptotic solutions for both the main beam along the critical line and the weaker secondary beam perpendicular to it are obtained. The asymptotic predictions are compared with direct numerical results obtained for Ekman numbers as low as. The agreement between the asymptotic predictions and numerical results improves as the Ekman number decreases. The asymptotic scalings in and for the amplitudes of the main and secondary beams, respectively, are recovered numerically. Since the self-similar solution is singular on the axis, a new local asymptotic solution is derived close to the axis and is also validated numerically. This study demonstrates that, in the limit of vanishing Ekman numbers and for particular frequencies, the main features of the flow generated by a librating inner core are obtained by propagating through the spherical shell the self-similar solution generated by the singularity at the critical latitude on the inner core. © The Author(s), 2022. Published by Cambridge University Press. 
650 0 4 |a Asymptotic solutions 
650 0 4 |a boundary layer separation 
650 0 4 |a Boundary layers 
650 0 4 |a Boundary-layer separation 
650 0 4 |a Critical latitude 
650 0 4 |a Ekman numbers 
650 0 4 |a Inner core 
650 0 4 |a Main beams 
650 0 4 |a Self-similar solution 
650 0 4 |a Shear flow 
650 0 4 |a Shear layer 
650 0 4 |a Spheres 
650 0 4 |a Spherical shell 
650 0 4 |a waves in rotating fluids 
650 0 4 |a Waves in rotating fluids 
700 1 |a Favier, B.  |e author 
700 1 |a He, J.  |e author 
700 1 |a Le Dizès, S.  |e author 
700 1 |a Rieutord, M.  |e author 
773 |t Journal of Fluid Mechanics