Equatorial kelvin wave: Difference between revisions
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<div class="definition"><div class="short_definition">An eastward propagating [[wave]] centered about the [[equator]] with [[zonal]] but no [[meridional]] velocity.</div><br/> <div class="paragraph">The zonal velocity has a Gaussian meridional structure centered about the equator with [[standard deviation]] equal to the equatorial [[Rossby radius of deformation]]. In the [[shallow water approximation]] the waves are nondispersive with [[frequency]] <div class="display-formula"><blockquote>[[File:ams2001glos-Ee47.gif|link=|center|ams2001glos-Ee47]]</blockquote></div> in which ''k'' is the along-boundary [[wavenumber]], and the [[phase speed]] <div class="display-formula"><blockquote>[[File:ams2001glos-Ee48.gif|link=|center|ams2001glos-Ee48]]</blockquote></div> with ''g'' the [[acceleration of gravity]] and ''H'' the mean fluid depth. The equatorial Rossby radius of deformation in this case is <div class="display-formula"><blockquote>[[File:ams2001glos-Ee49.gif|link=|center|ams2001glos-Ee49]]</blockquote></div> in which β is the meridional gradient of the [[Coriolis parameter]] at the equator. A [[Kelvin wave]] propagating equatorward along the western boundary of an ocean basin can generate an equatorial Kelvin wave when reaching the equator. Upon reaching the eastern boundary of an ocean basin, an equatorial Kelvin wave can generate a coastal Kelvin wave propagating poleward along the eastern boundary of the ocean basin.</div><br/> </div> | <div class="definition"><div class="short_definition">An eastward propagating [[wave]] centered about the [[equator]] with [[zonal]] but no [[meridional]] velocity.</div><br/> <div class="paragraph">The zonal velocity has a Gaussian meridional structure centered about the equator with [[standard deviation|standard deviation]] equal to the equatorial [[Rossby radius of deformation]]. In the [[shallow water approximation]] the waves are nondispersive with [[frequency]] <div class="display-formula"><blockquote>[[File:ams2001glos-Ee47.gif|link=|center|ams2001glos-Ee47]]</blockquote></div> in which ''k'' is the along-boundary [[wavenumber]], and the [[phase speed]] <div class="display-formula"><blockquote>[[File:ams2001glos-Ee48.gif|link=|center|ams2001glos-Ee48]]</blockquote></div> with ''g'' the [[acceleration of gravity]] and ''H'' the mean fluid depth. The equatorial Rossby radius of deformation in this case is <div class="display-formula"><blockquote>[[File:ams2001glos-Ee49.gif|link=|center|ams2001glos-Ee49]]</blockquote></div> in which β is the meridional gradient of the [[Coriolis parameter]] at the equator. A [[Kelvin wave]] propagating equatorward along the western boundary of an ocean basin can generate an equatorial Kelvin wave when reaching the equator. Upon reaching the eastern boundary of an ocean basin, an equatorial Kelvin wave can generate a coastal Kelvin wave propagating poleward along the eastern boundary of the ocean basin.</div><br/> </div> | ||
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Latest revision as of 15:55, 25 April 2012
equatorial Kelvin wave
The zonal velocity has a Gaussian meridional structure centered about the equator with standard deviation equal to the equatorial Rossby radius of deformation. In the shallow water approximation the waves are nondispersive with frequency in which k is the along-boundary wavenumber, and the phase speed with g the acceleration of gravity and H the mean fluid depth. The equatorial Rossby radius of deformation in this case is in which β is the meridional gradient of the Coriolis parameter at the equator. A Kelvin wave propagating equatorward along the western boundary of an ocean basin can generate an equatorial Kelvin wave when reaching the equator. Upon reaching the eastern boundary of an ocean basin, an equatorial Kelvin wave can generate a coastal Kelvin wave propagating poleward along the eastern boundary of the ocean basin.