Inertia-Gravity Waves Emitted from Balanced Flow: Observations, Properties, and Consequences
Inertia-Gravity Waves Emitted from Balanced Flow: Observations, Properties, and Consequences
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DOI:
10.1175/2008jas2480.1
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发表时间:
2008-11-01
影响因子:
3.1
通讯作者:
Read, Peter L.
中科院分区:
文献类型:
--
作者:
Williams, Paul D.;Haine, Thomas W. N.;Read, Peter L.
This paper describes laboratory observations of inertia-gravity waves emitted from balanced fluid flow. In a rotating two-layer annulus experiment, the wavelength of the inertia-gravity waves is very close to the deformation radius. Their amplitude varies linearly with Rossby number in the range 0.05-0.14, at constant Burger number (or rotational Froude number). This linear scaling challenges the notion, suggested by several dynamical theories, that inertia-gravity waves generated by balanced motion will be exponentially small. It is estimated that the balanced flow leaks roughly 1% of its energy each rotation period into the inertia-gravity waves at the peak of their generation.The findings of this study imply an inevitable emission of inertia-gravity waves at Rossby numbers similar to those of the large-scale atmospheric and oceanic flow. Extrapolation of the results suggests that inertia gravity waves might make a significant contribution to the energy budgets of the atmosphere and ocean. In particular, emission of inertia-gravity waves from mesoscale eddies may be an important source of energy for deep interior mixing in the ocean.