The tides in oceans on a rotating globe. Part III
In Part I of this series of papers a method was described by which solutions of the general dynamical equations of the tides could be obtained which were appropriate to an ocean on a rotating globe bounded by vertical cliffs along two meridians of longitude. The method was applied in that paper to a...
Published in: | Proceedings of the Royal Society of London. Series A, Containing Papers of a Mathematical and Physical Character |
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Online Access: | http://dx.doi.org/10.1098/rspa.1929.0198 https://royalsocietypublishing.org/doi/pdf/10.1098/rspa.1929.0198 |
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crroyalsociety:10.1098/rspa.1929.0198 2024-06-02T08:14:48+00:00 The tides in oceans on a rotating globe. Part III 1929 http://dx.doi.org/10.1098/rspa.1929.0198 https://royalsocietypublishing.org/doi/pdf/10.1098/rspa.1929.0198 en eng The Royal Society https://royalsociety.org/journals/ethics-policies/data-sharing-mining/ Proceedings of the Royal Society of London. Series A, Containing Papers of a Mathematical and Physical Character volume 126, issue 800, page 1-15 ISSN 0950-1207 2053-9150 journal-article 1929 crroyalsociety https://doi.org/10.1098/rspa.1929.0198 2024-05-07T14:16:04Z In Part I of this series of papers a method was described by which solutions of the general dynamical equations of the tides could be obtained which were appropriate to an ocean on a rotating globe bounded by vertical cliffs along two meridians of longitude. The method was applied in that paper to a specially chosen ocean which had a law of depth that introduced a simplification into the calculations. It is of considerable importance to apply the same method to an ocean of uniform depth. The present paper therefore gives the results for an ocean bounded by two meridians 60° apart, and having a uniform depth of 12,700 feet. Such an ocean would fairly represent the Atlantic Ocean if it were completely land-locked instead of being quite open to the Southern Ocean at one end and partially open at the other. The particular tide considered in this paper is the lunar semi-diurnal tide (M 2 ). The numerical solution is fairly complete and from the results it is possible to ascertain the character of the co-tidal lines and the values of the tide ranges corresponding to this tidal component in an ideal ocean of the form chosen. Article in Journal/Newspaper Southern Ocean The Royal Society Southern Ocean Proceedings of the Royal Society of London. Series A, Containing Papers of a Mathematical and Physical Character 126 800 1 15 |
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Open Polar |
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The Royal Society |
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crroyalsociety |
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English |
description |
In Part I of this series of papers a method was described by which solutions of the general dynamical equations of the tides could be obtained which were appropriate to an ocean on a rotating globe bounded by vertical cliffs along two meridians of longitude. The method was applied in that paper to a specially chosen ocean which had a law of depth that introduced a simplification into the calculations. It is of considerable importance to apply the same method to an ocean of uniform depth. The present paper therefore gives the results for an ocean bounded by two meridians 60° apart, and having a uniform depth of 12,700 feet. Such an ocean would fairly represent the Atlantic Ocean if it were completely land-locked instead of being quite open to the Southern Ocean at one end and partially open at the other. The particular tide considered in this paper is the lunar semi-diurnal tide (M 2 ). The numerical solution is fairly complete and from the results it is possible to ascertain the character of the co-tidal lines and the values of the tide ranges corresponding to this tidal component in an ideal ocean of the form chosen. |
format |
Article in Journal/Newspaper |
title |
The tides in oceans on a rotating globe. Part III |
spellingShingle |
The tides in oceans on a rotating globe. Part III |
title_short |
The tides in oceans on a rotating globe. Part III |
title_full |
The tides in oceans on a rotating globe. Part III |
title_fullStr |
The tides in oceans on a rotating globe. Part III |
title_full_unstemmed |
The tides in oceans on a rotating globe. Part III |
title_sort |
tides in oceans on a rotating globe. part iii |
publisher |
The Royal Society |
publishDate |
1929 |
url |
http://dx.doi.org/10.1098/rspa.1929.0198 https://royalsocietypublishing.org/doi/pdf/10.1098/rspa.1929.0198 |
geographic |
Southern Ocean |
geographic_facet |
Southern Ocean |
genre |
Southern Ocean |
genre_facet |
Southern Ocean |
op_source |
Proceedings of the Royal Society of London. Series A, Containing Papers of a Mathematical and Physical Character volume 126, issue 800, page 1-15 ISSN 0950-1207 2053-9150 |
op_rights |
https://royalsociety.org/journals/ethics-policies/data-sharing-mining/ |
op_doi |
https://doi.org/10.1098/rspa.1929.0198 |
container_title |
Proceedings of the Royal Society of London. Series A, Containing Papers of a Mathematical and Physical Character |
container_volume |
126 |
container_issue |
800 |
container_start_page |
1 |
op_container_end_page |
15 |
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1800738773471854592 |