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Topographic Rossby waves in a polar basin

Published online by Cambridge University Press:  15 July 2020

Andrew P. Bassom*
Affiliation:
School of Natural Sciences, University of Tasmania, Hobart, TAS7001, Australia
Andrew J. Willmott
Affiliation:
School of Mathematics, Statistics and Physics, Newcastle University, Herschel Building, Newcastle upon TyneNE1 7RU, UK
*
Email address for correspondence: [email protected]

Abstract

Approximate analytical expressions for the eigenfrequencies of freely propagating, divergent, barotropic topographic Rossby waves over a step shelf are derived. The amplitude equation, that incorporates axisymmetric topography while retaining full spherical geometry, is analysed by standard asymptotic methods based on the limited latitudinal extent of the polar basin as the natural small parameter. The magnitude of the planetary potential vorticity field, $\Pi _P$, increases poleward in the deep basin and over the shelf. However, everywhere over the shelf $\Pi _P$ exceeds its deep-basin value. Consequently, the polar basin waveguide supports two families of vorticity waves; here, our concern is restricted to the study of topographic Rossby (shelf) waves. The leading-order eigenfrequencies and cross-basin eigenfunctions of these modes are derived. Moreover, the spherical geometry allows an infinite number of azimuthally propagating modes. We also discuss the corrections to these leading-order eigenfrequencies. It is noted that these corrections can be associated with planetary waves that can propagate in the opposite direction to the shelf waves. For parameter values typical of the Arctic Ocean, planetary wave modes have periods of tens of days, significantly longer than the shelf wave periods of one to five days. We suggest that observations of vorticity waves in the Beaufort Gyre with periods of tens of days reported in the refereed literature could be associated with planetary, rather than topographic, Rossby waves.

Type
JFM Papers
Copyright
© The Author(s), 2020. Published by Cambridge University Press

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References

REFERENCES

Bassom, A. P. & Willmott, A. J. 2019 Accurate approximations for planetary and gravity waves in a polar basin. Tellus A 71, 1618133.CrossRefGoogle Scholar
Bokhove, O. & Johnson, E. R. 1999 Hybrid coastal and interior modes for two-dimensional homogeneous flow in a cylindrical ocean. J. Phys. Oceanogr. 29, 93118.2.0.CO;2>CrossRefGoogle Scholar
LeBlond, P. H. 1964 Planetary waves in a symmetrical polar basin. Tellus A 15, 503512.Google Scholar
LeBlond, P. H. & Mysak, L. A. 1978 Waves in the Ocean. Elsevier.Google Scholar
Nøst, O. A. & Isachsen, P. E. 2003 The large-scale time-mean ocean circulation in the Nordic Seas and Arctic Ocean estimated from simplified dynamics. J. Mar. Res. 61, 175210.CrossRefGoogle Scholar
Rhines, P. B. 1970 Edge-, bottom-, and Rossby waves in a rotating stratified fluid. Geophys. Fluid Dyn. 1, 273302.CrossRefGoogle Scholar
Timmermans, M.-L., Rainville, L., Thomas, L. & Proshutinsky, A. 2010 Moored observations of bottom-intensified motions in the deep Canada Basin, Arctic Ocean. J. Mar. Res. 68, 625641.CrossRefGoogle Scholar
Zhao, B. & Timmermans, M.-L. 2018 Topographic Rossby waves in the Arctic Ocean's Beaufort Gyre. J. Geophys. Res. 123, 65216530.CrossRefGoogle Scholar