"Kelvinwelle"@de . . "Las ondas Kelvin son ondas oce\u00E1nicas paralelas extremadamente largas que se propagan de oeste a este en los oc\u00E9anos, especialmente notorio en el Pac\u00EDfico, donde hace que la capa superior del mar relativamente c\u00E1lido se concentre y el nivel del mar aumente.\u200B Una onda de Kelvin, en oceanograf\u00EDa y como parte de la din\u00E1mica de fluidos, es lineal o no dispersiva; es tambi\u00E9n un modo de perturbaci\u00F3n a gran escala de un v\u00F3rtice en la din\u00E1mica de superfluidos; en t\u00E9rminos de la derivaci\u00F3n meteorol\u00F3gica u oceanogr\u00E1fica, se puede suponer que el componente de velocidad meridional desaparece, es decir, no hay flujo en la direcci\u00F3n norte-sur, lo que hace que las ecuaciones de movimiento y continuidad sean mucho m\u00E1s simples.\u200B Esta ola lleva el nombre del descubridor, Lord Kelvin (1879).\u200B"@es . "Fala Kelvina \u2013 fala w oceanie lub atmosferze powstaj\u0105ca na skutek zaburzenia ruchu wody lub powietrza przez si\u0142\u0119 Coriolisa, obserwowana w pobli\u017Cu linii brzegowej l\u0105d-ocean lub na r\u00F3wniku. Nazwa fali pochodzi od tytu\u0142u Lorda Kelvina, kt\u00F3ry w 1879 roku jako pierwszy opisa\u0142 wp\u0142yw obrotu Ziemi na fale grawitacyjne w oceanie."@pl . "Die Kelvinwelle, benannt nach Lord Kelvin (1824\u20131907), ist eine Welle, die sich im Gegensatz zur Wasserwelle und Poincar\u00E9-Welle nicht frei \u00FCber die ganze Wasseroberfl\u00E4che ausbreitet. Stattdessen kann sie sich nur in schmalen G\u00FCrteln (Wellenleitern) entlang topographischer Berandungen von rotierenden Fl\u00FCssigkeiten ausbreiten, z. B. an K\u00FCsten sowie entlang des \u00C4quators im Ozean und in der Atmosph\u00E4re. Die Gezeiten propagieren in Form von barotropen K\u00FCsten-Kelvinwellen. Auch die Bugwelle eines Schiffs setzt sich aus Kelvinwellen zusammen."@de . . . . . . . . . . "Onda Kelvin"@pt . "\u5F00\u5C14\u6587\u6CE2\uFF08Kelvin Wave\uFF09\u662F\u53D1\u751F\u5728\u5927\u6C14\u6216\u6D77\u6D0B\u4E2D\u7684\uFF0C\u8FCE\u5411\u5730\u5F62\u8FB9\u754C\uFF08\u4F8B\u5982\u6D77\u5CB8\u7EBF\uFF09\u5E73\u8861\u79D1\u6C0F\u529B\u7684\u6CE2\u52A8\u73B0\u8C61\u3002\u5F00\u5C14\u6587\u6CE2\u7684\u4E00\u4E2A\u7279\u5F81\u662F\uFF0C\u4E5F\u5C31\u662F\u8BF4\uFF0C\u6CE2\u5CF0\u7684\u76F8\u901F\u5EA6\u4E0E\u6CE2\u80FD\u7684\u7FA4\u901F\u5EA6\u5728\u6240\u6709\u9891\u7387\u65F6\u5747\u76F8\u7B49\u3002\u8FD9\u4E00\u7279\u6027\u610F\u5473\u7740\u5B83\u5728\u6CBF\u5CB8\u65B9\u5411\u59CB\u7EC8\u4FDD\u6301\u5B83\u7684\u5F62\u72B6\u3002 \u6D41\u4F53\u52A8\u529B\u5B66\u610F\u4E49\u4E0A\u7684\u5F00\u5C14\u6587\u6CE2\u662F\u8D85\u6D41\u4F53\u52A8\u529B\u5B66\u4E2D\u7684\u4E00\u79CD\u5927\u5C3A\u5EA6\u7684\u6F29\u6DA1\u7D0A\u52A8\u6A21\u5F0F\uFF1B\u5728\u6C14\u8C61\u5B66\u548C\u6D77\u6D0B\u5B66\u63A8\u5BFC\u7814\u7A76\u4E2D\uFF0C\u53EF\u4EE5\u5047\u5B9A\u7ECF\u7EBF\u65B9\u5411\u901F\u5EA6\u5206\u91CF\u4E3A\u96F6\uFF08\u4E5F\u5C31\u662F\u5047\u5B9A\u6CA1\u6709\u5357\u5317\u5411\u7684\u6D41\u52A8\uFF0C\u6545\u53EF\u7B80\u5316\u52A8\u91CF\u53CA\u8FDE\u7EED\u6027\u65B9\u7A0B\uFF09\u3002"@zh . "2020-11-24"^^ . . . . . . . . . "Une onde de Kelvin est une onde de gravit\u00E9 oc\u00E9anique de taille caract\u00E9ristique assez grande pour que la force de Coriolis se fasse ressentir et en pr\u00E9sence d'une couche limite (typiquement une c\u00F4te). Physiquement c'est une onde de gravit\u00E9 (la mar\u00E9e par exemple) qui \u00E0 cause de la force de Coriolis vient \u00AB s'\u00E9craser \u00BB contre une c\u00F4te."@fr . . "Fala Kelvina \u2013 fala w oceanie lub atmosferze powstaj\u0105ca na skutek zaburzenia ruchu wody lub powietrza przez si\u0142\u0119 Coriolisa, obserwowana w pobli\u017Cu linii brzegowej l\u0105d-ocean lub na r\u00F3wniku. Nazwa fali pochodzi od tytu\u0142u Lorda Kelvina, kt\u00F3ry w 1879 roku jako pierwszy opisa\u0142 wp\u0142yw obrotu Ziemi na fale grawitacyjne w oceanie."@pl . . . . . "\u5F00\u5C14\u6587\u6CE2\uFF08Kelvin Wave\uFF09\u662F\u53D1\u751F\u5728\u5927\u6C14\u6216\u6D77\u6D0B\u4E2D\u7684\uFF0C\u8FCE\u5411\u5730\u5F62\u8FB9\u754C\uFF08\u4F8B\u5982\u6D77\u5CB8\u7EBF\uFF09\u5E73\u8861\u79D1\u6C0F\u529B\u7684\u6CE2\u52A8\u73B0\u8C61\u3002\u5F00\u5C14\u6587\u6CE2\u7684\u4E00\u4E2A\u7279\u5F81\u662F\uFF0C\u4E5F\u5C31\u662F\u8BF4\uFF0C\u6CE2\u5CF0\u7684\u76F8\u901F\u5EA6\u4E0E\u6CE2\u80FD\u7684\u7FA4\u901F\u5EA6\u5728\u6240\u6709\u9891\u7387\u65F6\u5747\u76F8\u7B49\u3002\u8FD9\u4E00\u7279\u6027\u610F\u5473\u7740\u5B83\u5728\u6CBF\u5CB8\u65B9\u5411\u59CB\u7EC8\u4FDD\u6301\u5B83\u7684\u5F62\u72B6\u3002 \u6D41\u4F53\u52A8\u529B\u5B66\u610F\u4E49\u4E0A\u7684\u5F00\u5C14\u6587\u6CE2\u662F\u8D85\u6D41\u4F53\u52A8\u529B\u5B66\u4E2D\u7684\u4E00\u79CD\u5927\u5C3A\u5EA6\u7684\u6F29\u6DA1\u7D0A\u52A8\u6A21\u5F0F\uFF1B\u5728\u6C14\u8C61\u5B66\u548C\u6D77\u6D0B\u5B66\u63A8\u5BFC\u7814\u7A76\u4E2D\uFF0C\u53EF\u4EE5\u5047\u5B9A\u7ECF\u7EBF\u65B9\u5411\u901F\u5EA6\u5206\u91CF\u4E3A\u96F6\uFF08\u4E5F\u5C31\u662F\u5047\u5B9A\u6CA1\u6709\u5357\u5317\u5411\u7684\u6D41\u52A8\uFF0C\u6545\u53EF\u7B80\u5316\u52A8\u91CF\u53CA\u8FDE\u7EED\u6027\u65B9\u7A0B\uFF09\u3002"@zh . "A Kelvin wave is a wave in the ocean or atmosphere that balances the Earth's Coriolis force against a topographic boundary such as a coastline, or a waveguide such as the equator. A feature of a Kelvin wave is that it is non-dispersive, i.e., the phase speed of the wave crests is equal to the group speed of the wave energy for all frequencies. This means that it retains its shape as it moves in the alongshore direction over time. A Kelvin wave (fluid dynamics) is also a long scale perturbation mode of a vortex in superfluid dynamics; in terms of the meteorological or oceanographical derivation, one may assume that the meridional velocity component vanishes (i.e. there is no flow in the north\u2013south direction, thus making the momentum and continuity equations much simpler). This wave is named after the discoverer, Lord Kelvin (1879)."@en . . . . . . . . "Kelvinv\u00E5g \u00E4r en geostrofisk v\u00E5g i atmosf\u00E4ren eller havet som balanserar corioliskraften mot en topografisk gr\u00E4ns som till exempel en kustlinje. Karakt\u00E4riserande f\u00F6r en Kelvinv\u00E5g \u00E4r att den \u00E4r icke-dispersiv, det vill s\u00E4ga v\u00E5gtopparnas fashastighet sammanfaller med v\u00E5genergins grupphastighet vid samtliga frekvenser. F\u00F6reteelsen beskrevs av William Whewell 1836, men \u00E4r uppkallad efter William Thomson (fr\u00E5n 1892 Lord Kelvin) som f\u00F6rklarade den 1879. I havet fortplantar sig Kelvinv\u00E5gor norrut p\u00E5 havets \u00F6stra strand och s\u00F6derut p\u00E5 havets v\u00E4stra strand (moturs kring ett centrum kallat \"amfidromisk punkt\") p\u00E5 norra halvklotet. P\u00E5 det s\u00F6dra halvklotet g\u00E4ller det omv\u00E4nda. I atmosf\u00E4ren fortplantar de sig \u00E5t \u00F6ster p\u00E5 norra halvklotet . En ekvatoriell Kelvinv\u00E5g \u00E4r en s\u00E4rskild form av Kelvinv\u00E5g som balanserar Corioliskraften p\u00E5 norra halvklotet mot den p\u00E5 s\u00F6dra halvklotet. Denna sorts Kelvinv\u00E5g existerar allts\u00E5 endast vid ekvatorn d\u00E4r den alltid fortplantar sig \u00F6sterut. Notera att kelvinv\u00E5g (engelska: Kelvin wave) ej skall blandas samman med den \"kelvinv\u00E5g\" (engelska:Kelvin balance) som konstruerades av Lord Kelvin och som \u00E4r en typ av str\u00F6mv\u00E5g, det vill s\u00E4ga ett m\u00E4tinstrument f\u00F6r best\u00E4mning av elektrisk str\u00F6mstyrka."@sv . "Onda di Kelvin"@it . . . "\u5F00\u5C14\u6587\u6CE2"@zh . . . . "Uma onda Kelvin \u00E9 uma onda no oceano ou na atmosfera que equilibra a for\u00E7a Coriolis da Terra contra um limite topogr\u00E1fico, como uma linha costeira, ou um guia de ondas, como o equador. Uma caracter\u00EDstica de uma onda Kelvin \u00E9 que ela n\u00E3o \u00E9 dispersiva, ou seja, a velocidade de fase das cristas da onda \u00E9 igual \u00E0 velocidade do grupo da energia da onda para todas as frequ\u00EAncias. Isso significa que ele mant\u00E9m sua forma \u00E0 medida que se move na dire\u00E7\u00E3o ao longo da costa ao longo do tempo. Uma onda Kelvin (din\u00E2mica dos fluidos) tamb\u00E9m \u00E9 um modo de perturba\u00E7\u00E3o de longa escala de um v\u00F3rtice na din\u00E2mica do superfluido; em termos de deriva\u00E7\u00E3o meteorol\u00F3gica ou oceanogr\u00E1fica, pode-se supor que o componente da velocidade meridional desaparece (ou seja, n\u00E3o h\u00E1 fluxo na dire\u00E7\u00E3o norte-sul, tornando assim as equa\u00E7\u00F5es de momentum e continuidade muito mais simples). Esta onda recebeu o nome de seu descobridor, Lord Kelvin (1879)."@pt . . . . . . "1117529819"^^ . . . . . "Uma onda Kelvin \u00E9 uma onda no oceano ou na atmosfera que equilibra a for\u00E7a Coriolis da Terra contra um limite topogr\u00E1fico, como uma linha costeira, ou um guia de ondas, como o equador. Uma caracter\u00EDstica de uma onda Kelvin \u00E9 que ela n\u00E3o \u00E9 dispersiva, ou seja, a velocidade de fase das cristas da onda \u00E9 igual \u00E0 velocidade do grupo da energia da onda para todas as frequ\u00EAncias. Isso significa que ele mant\u00E9m sua forma \u00E0 medida que se move na dire\u00E7\u00E3o ao longo da costa ao longo do tempo."@pt . . . "Die Kelvinwelle, benannt nach Lord Kelvin (1824\u20131907), ist eine Welle, die sich im Gegensatz zur Wasserwelle und Poincar\u00E9-Welle nicht frei \u00FCber die ganze Wasseroberfl\u00E4che ausbreitet. Stattdessen kann sie sich nur in schmalen G\u00FCrteln (Wellenleitern) entlang topographischer Berandungen von rotierenden Fl\u00FCssigkeiten ausbreiten, z. B. an K\u00FCsten sowie entlang des \u00C4quators im Ozean und in der Atmosph\u00E4re. Die Gezeiten propagieren in Form von barotropen K\u00FCsten-Kelvinwellen. Auch die Bugwelle eines Schiffs setzt sich aus Kelvinwellen zusammen."@de . . "\u30B1\u30EB\u30D3\u30F3\u6CE2"@ja . "Une onde de Kelvin est une onde de gravit\u00E9 oc\u00E9anique de taille caract\u00E9ristique assez grande pour que la force de Coriolis se fasse ressentir et en pr\u00E9sence d'une couche limite (typiquement une c\u00F4te). Physiquement c'est une onde de gravit\u00E9 (la mar\u00E9e par exemple) qui \u00E0 cause de la force de Coriolis vient \u00AB s'\u00E9craser \u00BB contre une c\u00F4te."@fr . . . "A Kelvin wave is a wave in the ocean or atmosphere that balances the Earth's Coriolis force against a topographic boundary such as a coastline, or a waveguide such as the equator. A feature of a Kelvin wave is that it is non-dispersive, i.e., the phase speed of the wave crests is equal to the group speed of the wave energy for all frequencies. This means that it retains its shape as it moves in the alongshore direction over time."@en . . . . . . . "L\u2019onda di Kelvin \u00E8 un'onda dell'oceano o dell'atmosfera che bilancia la forza di Coriolis terrestre rispetto a un bordo topografico come una linea di costa o una guida d'onda come l'equatore. Una caratteristica \u00E8 l'essere non-dispersiva, cio\u00E8 la velocit\u00E0 di fase delle creste d'onda \u00E8 uguale alla velocit\u00E0 di gruppo dell'energia del moto ondoso a tutte le frequenze e questo implica che essa mantiene la sua forma nel tempo mentre si muove lungo la direzione della costa."@it . . "Onde de Kelvin"@fr . . . "Kelvinv\u00E5g"@sv . . . . "\u30B1\u30EB\u30D3\u30F3\u6CE2\uFF08\u82F1\u8A9E: Kelvin wave\uFF09\u306F\u3001\u6D77\u6D0B\u6CE2\u52D5\u306E1\u3064\u3067\u3042\u308B\u3002"@ja . . "L\u2019onda di Kelvin \u00E8 un'onda dell'oceano o dell'atmosfera che bilancia la forza di Coriolis terrestre rispetto a un bordo topografico come una linea di costa o una guida d'onda come l'equatore. Una caratteristica \u00E8 l'essere non-dispersiva, cio\u00E8 la velocit\u00E0 di fase delle creste d'onda \u00E8 uguale alla velocit\u00E0 di gruppo dell'energia del moto ondoso a tutte le frequenze e questo implica che essa mantiene la sua forma nel tempo mentre si muove lungo la direzione della costa."@it . . . "Kelvinv\u00E5g \u00E4r en geostrofisk v\u00E5g i atmosf\u00E4ren eller havet som balanserar corioliskraften mot en topografisk gr\u00E4ns som till exempel en kustlinje. Karakt\u00E4riserande f\u00F6r en Kelvinv\u00E5g \u00E4r att den \u00E4r icke-dispersiv, det vill s\u00E4ga v\u00E5gtopparnas fashastighet sammanfaller med v\u00E5genergins grupphastighet vid samtliga frekvenser. F\u00F6reteelsen beskrevs av William Whewell 1836, men \u00E4r uppkallad efter William Thomson (fr\u00E5n 1892 Lord Kelvin) som f\u00F6rklarade den 1879."@sv . "Fala Kelvina"@pl . . "\u30B1\u30EB\u30D3\u30F3\u6CE2\uFF08\u82F1\u8A9E: Kelvin wave\uFF09\u306F\u3001\u6D77\u6D0B\u6CE2\u52D5\u306E1\u3064\u3067\u3042\u308B\u3002"@ja . . . "Onda Kelvin"@es . "Kelvin wave"@en . . "Las ondas Kelvin son ondas oce\u00E1nicas paralelas extremadamente largas que se propagan de oeste a este en los oc\u00E9anos, especialmente notorio en el Pac\u00EDfico, donde hace que la capa superior del mar relativamente c\u00E1lido se concentre y el nivel del mar aumente.\u200B Una onda de Kelvin, en oceanograf\u00EDa y como parte de la din\u00E1mica de fluidos, es lineal o no dispersiva; es tambi\u00E9n un modo de perturbaci\u00F3n a gran escala de un v\u00F3rtice en la din\u00E1mica de superfluidos; en t\u00E9rminos de la derivaci\u00F3n meteorol\u00F3gica u oceanogr\u00E1fica, se puede suponer que el componente de velocidad meridional desaparece, es decir, no hay flujo en la direcci\u00F3n norte-sur, lo que hace que las ecuaciones de movimiento y continuidad sean mucho m\u00E1s simples.\u200B Esta ola lleva el nombre del descubridor, Lord Kelvin (1879).\u200B"@es . . . "9332"^^ . . . "935830"^^ . .