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contributor authorGent, Peter R.
date accessioned2017-06-09T14:45:08Z
date available2017-06-09T14:45:08Z
date copyright1979/07/01
date issued1979
identifier issn0022-3670
identifier otherams-25943.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4162782
description abstractA new type of standing equatorial wave mode is described that exists in the semi-infinite ocean 0 ? x ? L, ?∞ ? y ? ∞. It consists of a finite sum of the meridionally trapped equatorial waves in an infinite x domain. The new mode is thus itself equatorially trapped and requires no energy sources or sinks at |y| = ∞. However, it exists only for a discrete, countable set of pairs of values of the frequency ? and the ocean zonal width L. Previously described standing modes exist for any ocean width, but are infinite sums of trapped equatorial waves and require a continuous energy source in the west at |y| = ∞ to balance the continuous energy sink in the east at |y| = ∞. Several examples of the new type of standing mode are given, and it is shown that as the standing mode period becomes very long, so the zonal scale becomes very short. The effect on the standing modes of bounding the basin meridionally is also described; energy is recycled round the basin by boundary-trapped Kelvin waves along the zonal walls. The amount of energy recycled in the new type of standing mode, however, is exponentially small compared to that recycled in the previously described standing modes.
publisherAmerican Meteorological Society
titleStanding Equatorial Wave Modes in Bounded Ocean Basins
typeJournal Paper
journal volume9
journal issue4
journal titleJournal of Physical Oceanography
identifier doi10.1175/1520-0485(1979)009<0653:SEWMIB>2.0.CO;2
journal fristpage653
journal lastpage662
treeJournal of Physical Oceanography:;1979:;Volume( 009 ):;issue: 004
contenttypeFulltext


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