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contributor authorPhilander, S. G. H.
date accessioned2017-06-09T14:45:00Z
date available2017-06-09T14:45:00Z
date copyright1979/03/01
date issued1979
identifier issn0022-3670
identifier otherams-25904.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4162739
description abstractBecause of the narrow region over which it has high speeds, the Equatorial Undercurrent has little effect on long waves with large phase speeds, such as long Kelvin and equatorially trapped inertia-gravity modes with equivalent depths ?30 cm. The Rossby branch of the Rossby-gravity family, and the gravest Rossby modes, have phase velocities comparable to the maximum speed of the Undercurrent and are significantly modified by this current. Meanders of the Undercurrent that are due to superimposed neutral (non-amplifying) waves must have westward phase propagation; standing or eastward traveling meanders are possible only if the Equatorial Undercurrent is unstable.
publisherAmerican Meteorological Society
titleEquatorial Waves in the Presence of the Equatorial Undercurrent
typeJournal Paper
journal volume9
journal issue2
journal titleJournal of Physical Oceanography
identifier doi10.1175/1520-0485(1979)009<0254:EWITPO>2.0.CO;2
journal fristpage254
journal lastpage262
treeJournal of Physical Oceanography:;1979:;Volume( 009 ):;issue: 002
contenttypeFulltext


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