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INDIAN OCEAN

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Originally appearing in Volume V14, Page 452 of the 1911 Encyclopedia Britannica.
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INDIAN OCEAN , the ocean bounded N. by See also:India and See also:Persia; W. by See also:Arabia and See also:Africa, and the See also:meridian passing southwards from Cape Agulhas; and E. by Farther India, the Sunda Islands, See also:West and See also:South See also:Australia, and the meridian passing through South Cape in See also:Tasmania. As in the See also:case of the See also:Atlantic and Pacific Oceans, the See also:southern boundary is taken at either 4o° S., the See also:line of separation from the See also:great Southern Ocean, or, if the See also:belt of this ocean between the two meridians named be included, at the See also:Antarctic Circle. It attains its greatest breadth, more than 6000 m. between the south points of Africa and Australia, and becomes steadily narrower towards the See also:north, until it is divided by the Indian See also:peninsula into two arms, the Arabian See also:Sea on the west and the See also:Bay of See also:Bengal on the See also:east. Both branches meet the See also:coast of See also:Asia almost exactly on the Tropic of See also:Cancer, but the Arabian Sea communicates with the Red Sea and the See also:Persian Gulf by the Straits of Bab-el-Mandeb and Ormuz respectively. Both of these, again, extend in a north-See also:westerly direction to 30° N. See also:Murray gives the See also:total See also:area, reckoning to 4o° S. and including the Red Sea and Persian Gulf, as 17,320,550 See also:English square See also:miles, See also:equivalent to 13,042,000 See also:geographical square miles. Karstens gives the area as 48,182,413 square kilometres, or 14,001,000 geographical square miles; of these 10,842,000 square kilometres, or 3,150,000 geographical square miles, about 22% of the whole, See also:lie north of the See also:equator. For the area from 4o° S. to the Antarctic Circle, Murray gives 9,372,600 English square miles, equivalent to 7,057,568 geographical square miles, and Karstens 24,718,000 square kilometres, equivalent to 7,182,474 geographical square miles. The Indian Ocean receives few large See also:rivers, the See also:chief being the See also:Zambezi, the Shat-el-Arab, the See also:Indus, the See also:Ganges, the See also:Brahmaputra and the Irawadi. Murray estimates the total See also:land area draining to the Indian Ocean at 5,050,000 geographical square miles, almost the same as that draining to the Pacific. The See also:annual rainfall draining from this area is estimated at 4380 cubic miles. See also:Relief.—Large portions of the See also:bed still remain unexplored, but a See also:fair knowledge of its See also:general See also:form has been gained from the soundings of H.M.S.

" Challenger," the See also:

German " Gazelle " Expedition, and various See also:cable See also:ships, and in 1898 See also:information was greatly added to by the German " See also:Valdivia " Expedition. A See also:ridge, less than 2000 fathoms from the See also:surface, extends south-eastwards from the Cape. This ridge, on which the Crozet Islands and Kerguelen are situated, is directly connected with the submarine See also:plateau of the Antarctic. From it the See also:depth increases north-eastwards, and the greatest depression is found in the See also:angle between Australia and the Sunda Islands, where " See also:Wharton deep," below the 3000-See also:fathom line, covers an area of nearly 50,000 sq. m. Immediately to the north of Wharton deep is the smaller " Maclear deep," and the See also:long narrow " See also:Jeffreys deep " off the south of Australia completes the See also:list of depressions below 3000 fathoms in the Indian Ocean. The 2000-fathom line approaches See also:close to the coast except (I) in the Bay of Bengal, which it does not enter; (2) to the south-west of India along a ridge on which are the Laccadive and Maldive Islands; and (3) in the See also:Mozambique Channel, and on a See also:bank north and east of See also:Madagascar, on which are the See also:Seychelles, Mascarene Islands and other See also:groups. Islands.—Like the Pacific, the Indian Ocean contains more islands in the western than in the eastern See also:half. Towards the centre, the Maldive, See also:Chagos and Cocos groups are of characteristic See also:coral formation, and coral reefs occur on most parts of the tropical coasts. There are many volcanic islands, as See also:Mauritius, the Crozet Islands, and St See also:Paul's. The chief See also:continental islands are Madagascar, See also:Sokotra and See also:Ceylon. Kerguelen, a desolate and uninhabited See also:island near the centre of the Indian Ocean at its southern border, is See also:note-worthy as providing a See also:base station for Antarctic exploration. Deposits.—The bottom of the Bay of Bengal, of the See also:northern See also:part of the Arabian Sea, of the Red Sea and the Persian Gulf, and of the narrow coastal strips on the east and west sides of the ocean, are chiefly covered by See also:blue and See also:green muds.

Off the See also:

African coasts there are large deposits of Glauconitic sands and muds at depths down to moo fathoms, and on See also:banks where coral formation occurs there are large deposits of coral muds and sands. In the deeper parts the bed of the ocean is covered on the west and south by See also:Globigerina See also:ooze except for an elongated patch of red See also:clay extending most of the distance from Sokotra to the Maldives. The red clay covers a nearly square area in the eastern part of the See also:basin bounded on two sides by the Sunda Islands and the west coast of Australia, as well as two strips extending east and west from the southern margin of the square along the south of Australia and nearly to Madagascar. In the northern portion of the square, north and east of Wharton deep, the red clay is replaced over a large See also:tract by Radiolarian ooze. Temperature.—The mean temperature of the surface See also:water is over 8o° F. in all parts north of 13° S., except in the north-west of the Arabian Sea, where it is somewhat See also:lower. South of 13° S. temperature falls uniformly and quickly to the Southern Ocean. Between the depths of See also:Ioo and boo fathoms temperature is high in the north-west, and in the south centre and south-west, and See also:low in the north-east, the type of See also:distribution remaining substantially the same. At 1500 fathoms temperature has become very See also:uniform, ranging between 35° and 370 F., but still exhibiting the same type of distribution, though in a very degenerate form. Salinity.—The saltest surface water is found in (a) the Arabian Sea and (b) along a. belt extending from West Australia to South Africa, the highest salinity in this belt occurring at the Australian end. South of the belt salinity falls quickly as See also:latitude increases, while to the north of it, in the See also:monsoon region, the surface water is very fresh off the African coast and to the north-east. Little is known with certainty about the distribution of salinity in the depths, the number of trustworthy observations available being still very small. Probably the northern and north-eastern region, within the monsoon area, contains relatively fresh water down to very considerable depths.

Circulation.—North of the equator the surface circulation is under the See also:

control of the monsoons, and changes with them, the currents consisting chiefly of north-east and south-west drifts in the open sea, and induced streams following the coasts. During the northern summer the south-west monsoon, which is sufficiently strong to bring See also:navigation practically to a standstill except for powerful steamers, sets up a strong north-easterly See also:drift in the Arabian Sea, and the water removed from the east African coast is replaced by the upwelling of See also:cold water from below; this is one of the best illustrations of this See also:action extant. Along the line of the equator the Indian See also:counter-current flows eastwards all the See also:year See also:round, acting . as See also:compensation to the great See also:Equatorial current flowing westwards between the See also:parallels of 7° and 2o° S. The equatorial current, on See also:meeting the northern extremity of Madagascar, sends a See also:branch southwards along the east coast of that island, sometimes called the Mascarene current. When the See also:main equatorial current reaches-the African coast a See also:minor stream is sent northwards to the source of the Indian counter-current, but the See also:discharge is chiefly by the Mozambique current, which south of Cape See also:Corrientes becomes the Agulhas current, one of the most powerful stream currents of the globe. On the west coast of Madagascar and on the banks of the African coast south of 3o° S., reaction currents or " back• drifts " move in the opposite direction along the flanks of the Agulhas current; these back-drifts are of great importance to navigation. On clearing the land south of the Cape the See also:waters of the Agulhas current meet those of the west See also:wind drift of the Southern Ocean, and mingle with them in such a manner as to produce, by interdigitation, alternate strips of warm and cold water, which are met with at great distances south-west and south of the Cape. Between South Africa and Australia the waters form a part of the great west wind drift. The waters of this drift are, in general, of very low temperature, but it is remarkable that the interdigitation just mentioned continues far to the eastward, at least as far as Kerguelen. This fact is probably due partly to the actual intrusion of warm water from the Mascarene current east of Madagascar, and partly to the circumstance that the different temperatures of the waters are so compensated by their See also:differences of salinity that they have almost precisely the same specific gravity in situ. The west wind drift sends a stream northwards along the west coast of Australia, the West Australia current, the homologue of the Benguela current in the South Atlantic. The See also:principal feature in the circulation in the depths of the Indian Ocean is a slow See also:movement of Antarctic water northwards along the bottom to take the See also:place of that removed from the surface by evaporation, and by currents in the lower latitudes.

Little is known beyond the See also:

bare fact that such movement does take place. (H. N.

End of Article: INDIAN OCEAN

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