Unpredictability of internal M 2

Current observations from a shelf sea, continental slopes and the abyssal North-East Atlantic Ocean are all dominated by the semidiurnal lunar (M 2 ) tide. It is shown that motions at M 2 vary at usually large barotropic and coherent baroclinic scales, >50 km horizontally and >0.5 H vertically...

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Main Author: H. van Haren
Format: Article in Journal/Newspaper
Language:English
Published: Copernicus Publications 2007
Subjects:
G
Online Access:https://doaj.org/article/75bbbaa3580a45388893501f9fcad3e7
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spelling ftdoajarticles:oai:doaj.org/article:75bbbaa3580a45388893501f9fcad3e7 2023-05-15T17:38:35+02:00 Unpredictability of internal M 2 H. van Haren 2007-06-01T00:00:00Z https://doaj.org/article/75bbbaa3580a45388893501f9fcad3e7 EN eng Copernicus Publications http://www.ocean-sci.net/3/337/2007/os-3-337-2007.pdf https://doaj.org/toc/1812-0784 https://doaj.org/toc/1812-0792 1812-0784 1812-0792 https://doaj.org/article/75bbbaa3580a45388893501f9fcad3e7 Ocean Science, Vol 3, Iss 2, Pp 337-344 (2007) Geography. Anthropology. Recreation G Environmental sciences GE1-350 article 2007 ftdoajarticles 2022-12-30T22:13:49Z Current observations from a shelf sea, continental slopes and the abyssal North-East Atlantic Ocean are all dominated by the semidiurnal lunar (M 2 ) tide. It is shown that motions at M 2 vary at usually large barotropic and coherent baroclinic scales, >50 km horizontally and >0.5 H vertically. H represents the waterdepth. Such M 2 -scales are observed even close to topography, the potential source of baroclinic, "internal" tidal waves. In contrast, incoherent small-scale, ~10 km horizontally and ~0.1 H vertically, baroclinic motions are dominated around f, the local inertial frequency, and/or near 2Ω&#x2248;S 2 , the semidiurnal solar tidal frequency. Ω represents the Earth's rotational vector. This confirms earlier suggestions that small-scale baroclinic M 2 -motions generally do not exist in the ocean in any predictable manner, except in beams very near, <10 km horizontally, to their source. As a result, M 2 -motions are not directly important for generating shear and internal wave induced mixing. Indirectly however, they may contribute to ocean mixing if transfer to small-scale motions at f and/or S 2 and at high internal wave frequencies can be proven. Also far from topography, small-scale motions are found at either one or both of the latter frequencies. Different suggestions for the scales at these particular frequencies are discussed, ranging from the variability of "background" density gradients and associated divergence and focusing of internal wave rays to the removal of the internal tidal energy by non-linear interactions. Near f and S 2 particular short-wave inertio-gravity wave bounds are found in the limits of strong and very weak stratification, which are often observed in small-scale layers. Article in Journal/Newspaper North East Atlantic Directory of Open Access Journals: DOAJ Articles
institution Open Polar
collection Directory of Open Access Journals: DOAJ Articles
op_collection_id ftdoajarticles
language English
topic Geography. Anthropology. Recreation
G
Environmental sciences
GE1-350
spellingShingle Geography. Anthropology. Recreation
G
Environmental sciences
GE1-350
H. van Haren
Unpredictability of internal M 2
topic_facet Geography. Anthropology. Recreation
G
Environmental sciences
GE1-350
description Current observations from a shelf sea, continental slopes and the abyssal North-East Atlantic Ocean are all dominated by the semidiurnal lunar (M 2 ) tide. It is shown that motions at M 2 vary at usually large barotropic and coherent baroclinic scales, >50 km horizontally and >0.5 H vertically. H represents the waterdepth. Such M 2 -scales are observed even close to topography, the potential source of baroclinic, "internal" tidal waves. In contrast, incoherent small-scale, ~10 km horizontally and ~0.1 H vertically, baroclinic motions are dominated around f, the local inertial frequency, and/or near 2Ω&#x2248;S 2 , the semidiurnal solar tidal frequency. Ω represents the Earth's rotational vector. This confirms earlier suggestions that small-scale baroclinic M 2 -motions generally do not exist in the ocean in any predictable manner, except in beams very near, <10 km horizontally, to their source. As a result, M 2 -motions are not directly important for generating shear and internal wave induced mixing. Indirectly however, they may contribute to ocean mixing if transfer to small-scale motions at f and/or S 2 and at high internal wave frequencies can be proven. Also far from topography, small-scale motions are found at either one or both of the latter frequencies. Different suggestions for the scales at these particular frequencies are discussed, ranging from the variability of "background" density gradients and associated divergence and focusing of internal wave rays to the removal of the internal tidal energy by non-linear interactions. Near f and S 2 particular short-wave inertio-gravity wave bounds are found in the limits of strong and very weak stratification, which are often observed in small-scale layers.
format Article in Journal/Newspaper
author H. van Haren
author_facet H. van Haren
author_sort H. van Haren
title Unpredictability of internal M 2
title_short Unpredictability of internal M 2
title_full Unpredictability of internal M 2
title_fullStr Unpredictability of internal M 2
title_full_unstemmed Unpredictability of internal M 2
title_sort unpredictability of internal m 2
publisher Copernicus Publications
publishDate 2007
url https://doaj.org/article/75bbbaa3580a45388893501f9fcad3e7
genre North East Atlantic
genre_facet North East Atlantic
op_source Ocean Science, Vol 3, Iss 2, Pp 337-344 (2007)
op_relation http://www.ocean-sci.net/3/337/2007/os-3-337-2007.pdf
https://doaj.org/toc/1812-0784
https://doaj.org/toc/1812-0792
1812-0784
1812-0792
https://doaj.org/article/75bbbaa3580a45388893501f9fcad3e7
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