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contributor authorChew, Frank
contributor authorBushnell, Mark H.
date accessioned2017-06-09T14:49:38Z
date available2017-06-09T14:49:38Z
date copyright1990/07/01
date issued1990
identifier issn0022-3670
identifier otherams-27662.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4164692
description abstractWe address the problem of the oscillatory periods of two observed phenomena in the instability zone in the eastern equatorial Pacific. The first case concerns two high-speed anticyclonic flow with periods of approximately 12 and 15 mean solar days. The second concerns the long waves with an average period of about 25 days. The problem is that, in terms of their respective mean latitudes, these periods are about twice as large as those of the inertial period of one-half pendulum day. As a solution we offer the hypothesis of the half-inertial flow with its period of one pendulum day. The inertial flow is governed by KV = ?f, where K is the path curvature, V the speed of the flow, and f the Coriolis parameter. In contrast, the half-inertial flow is governed by KV = ?f/2 with a speed that is the maximum for a given curvature and latitude and approaches twice that of the geostrophic speed. In terms of the half-inertial flow, the average lone-wave period of 25 days would correspond to a plausible mean latitude of 2.3°N. Efficient at extracting horizontal shear energy, the half inertial flow could also play an important role in the near-surface heat balance.
publisherAmerican Meteorological Society
titleThe Half-Inertial Flow in the Eastern Equatorial Pacific: A Case Study
typeJournal Paper
journal volume20
journal issue7
journal titleJournal of Physical Oceanography
identifier doi10.1175/1520-0485(1990)020<1124:THIFIT>2.0.CO;2
journal fristpage1124
journal lastpage1133
treeJournal of Physical Oceanography:;1990:;Volume( 020 ):;issue: 007
contenttypeFulltext


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