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RED See also:SEA , a narrow See also:strip of See also:water extending S.S.E. from See also:Suez to the Strait of Bab el-Mandeb in a nearly straight See also:line, and separating the coasts of See also:Arabia from those of See also:Egypt, See also:Nubia and See also:Abyssinia. Its See also:total length is about 1200 m., and its breadth varies from about 25o M. in the See also:southern See also:half to 130 M. in 27° 45' N., where it divides into two parts, the Gulf of Suez and the Gulf of See also:Akaba, separated from each other by the See also:peninsula of See also:Sinai.
The Gulf of Suez is shallow, and slopes regularly down to
the See also:northern extremity of the Red Sea See also:basin, which has a
Depths. maximum See also:depth of 64o fathoms, and then over a
shoal of 6o fathoms goes down to 1200 fathoms in
22° 7' N. The Gulf of Akaba is separated from the Red Sea by
a submarine See also:bank only 70 fathoms from the See also:surface, and in
28° 39' N. and 34° 43' E. it attains the depth of 700 fathoms.
See also:South of the 'zoo-See also:fathom depression a See also:ridge rises to 500 fathoms
in the See also:latitude of See also:Jidda, and south of this again a similar depres-
See also:sion goes down to 1190 fathoms. Throughout this northern See also:part,
i.e. to the See also:banks of See also:Suakin and Farsan in 20° N., the See also:loo-fathom
line keeps to a See also:belt of See also:coral See also:reef See also:close inshore, but in See also:lower
latitudes the shallow coral region, 300 M. See also:long and 7o to 8o m.
across, extends farther and farther seaward, until in the latitude
of See also:Hodeda the deep channel (marked by the loo-fathom line) is
only 20 M. broad, all the See also:rest of the See also:area being dangerous to See also:navigation, even for small vessels. In the See also:middle of the gradually narrowing channel three depressions are known to exist; soundings in two of these are: rrio fathoms in 20° N. and 890 fathoms in 16° N., a little to the See also:north of See also:Massawa. To the north-See also:west of the volcanic See also:island of Zebayir the depth is less than 500 fathoms; the bottom of the channel rises to the ioofathom line at Hanish Island (also volcanic), then shoals to 45 fathoms, and sinks again in about the latitude of See also:Mokha in a narrow channel which curves westward See also:round the island of See also:Perim (depth 170 fathoms), to lose itself in the See also:Indian Ocean. This western channel is x6 m. wide in the Strait of Bab el-Mandeb; the eastern channel of the strait is 2 M. broad and 16 fathoms deep.
See also: Both these computations, however, were made before the date of the See also:Austrian exploring expeditions (1896—98). Bludau's measurements give the total area draining to the Red Sea at about 255,000 sq. geographical m. Krummel's more See also:recent calculations (see OCEAN) give values somewhat higher than those of Karstens. The Red Sea is formed by a line of fracture, probably dating from See also:Pliocene times, See also:crossing the centre of a See also:dome of Archean rocks, on both flanks of which, in Egypt and Arabia, Forma. rest Secondary and See also:Tertiary deposits. The See also:granite rocks tton. forming the core of the dome appear at the surface on the Red Sea See also:coast, at the western end of the transverse line of heights crossing See also:Nejd. Along the line of fracture traces of volcanic activity are frequent; a See also:group of volcanic islands occurs in 14° N., and on See also:Jebel Teir, farther north, a See also:volcano has only recently become See also:extinct. The margin of the Red Sea itself consists, on the Arabian See also:side, of a strip of See also:low See also:plain backed by ranges of barren hills of coral and See also:sand formation, and here and there by mountains of consider-able height. The greater elevations are for the most part formed of limestones, except in the south, where they are largely volcanic. The coasts of the Gulf of Akaba are steep, with numerous coral reefs on both sides. On the See also:African side there are in the north wide stretches of See also:desert plain, which towards the south rise to elevated tablelands, and ultimately to the mountains of Abyssinia. The shores of the Red Sea are little indented; See also:good harbours are almost wanting in the desert regions of the north, while in the south the See also:chief inlets are at Massawa, and at Kamaran, almost directly opposite. Coral formations are abundant; immense reefs, both barrier and fringing, skirt both coasts, often enclosing wide channels between the reef and the See also:land. The reefs on the eastern side are the more extensive; they occur in places as much as 25 m. from the land. It has long been known that the whole Red Sea area is undergoing See also:gradual See also:elevation, and much has been done in recent years in investigating the levels of raised beaches found in different localities. In the northern part, down to almost 19° N., the prevailing winds are north and north-west. The middle region, to 14°–16° N., has variable winds in an area of low barometric pressure, while in the southern Red Sea south-See also:east and okay. east winds prevail. From See also:June to See also:August the north-west See also:wind blows over the entire' area ; in See also:September it retreats again as far as 16° N., south of which the winds are for a See also:time variable. In the Gulf of Suez the See also:westerly, or " See also:Egyptian," wind occurs frequently during See also:winter, sometimes blowing with violence, and generally accompanied by See also:fog and clouds of dust. Strong north-north-east winds prevail in the Gulf of Akaba during the greater part of the See also:year; they are weakest in See also:April and May, sometimes giving See also:place at that See also:season to southerly breezes. The high temperature and See also:great relative humidity make the summer See also:climate of the Red Sea one of the most disagreeable in the See also:world. The mean See also:annual temperature of the surface See also:waters near the See also:head is 77° F.; it rises to 8o° in about 22° N., to 84° in 16° N., and drops again to 82° at the Strait of Bab el-Mandeb. See also:Tempera- Daily See also:variations of temperature are observable to a taredepth of over 5o fathoms. Temperature is. on the whole, higher near the Arabian than the Egyptian side, but it everywhere diminishes with increase of depth and latitude, down to 38o fathoms from the surface; below this depth a See also:uniform See also:constant temperature of 70.7° F. is observed throughout. In the Gulf of Suez temperature is relatively low, falling rapidly from south to north. The waters of the Gulf of Akaba are warmer towards_ the Arabian than the Sinai coasts; a uniform temperature of 70.2° is observed at all depths below 270 fathoms. The salinity of the waters is relatively great, the highest re-corded being 42.7 per mille (Gulf of Suez), and the lowest 36-2 salinity. (Perim See also:harbour). The See also:distribution is, speaking generally, the opposite to that of temperature; salinity increases from the surface downwards, and from the south north-wards, and it is greater towards the western than the eastern side. This statement holds good for the Gulf of Suez, in which the water is much See also:salter than in the open sea; but in the Gulf of Akaba the distribution is exceedingly uniform, nowhere differing much from an See also:average of 40.6 per mille. The movements of the waters are of great irregularity and complexity, rendering navigation difficult and dangerous. Two features stand out with See also:special distinctness: the ex-Circula- See also:change of water between the Red Sea and the Indian See also:Lion. Ocean, and the tidal streams of the Gulf of Suez. From the observations of salinity it is inferred that a surface current flows inwards to the Red Sea in the eastern channel of the Strait of Bab el-Mandeb, while a current of very See also:salt water flows outward to the Indian Ocean, through the western channel, at a depth of 5o to Too fathoms from the surface. In the Gulfs of Suez and Akaba, almost the only part of the Red Sea in which tidal phenomena are well See also:developed, a sharply defined tidal circulation is found. Elsewhere the surface movements at least are controlled by the prevailing winds, which give rise in places to complex " transverse " currents, and near the coast are modified by the channels enclosed by the coral reefs. During the prevalence of the north and north-west winds the surface level of the northern part of the Red Sea is depressed by as much as 2 ft. The great evaporation going on from the surface probably causes a slow See also:vertical circulation in the depth, the salter colder waters sinking, and ultimately escaping to the Indian Ocean. Extensive collections of the deposits forming the See also:bed were made by the expeditions of the Austrian See also:ship " See also:Pola " (1896 and 1898). These were analysed by Dr K. Natterer, whose conclusions, however, have been disputed by a number of other investigators. The zoological collections of the " Pola " expeditions show that certain well-defined districts are extremely See also:rich in See also:plankton, while others are correspondingly poor; and it appears that the latter occur in districts surrounded by currents of relatively low temperature, while the richer parts are where the movements of water are blocked by irregularities in the coast-line. Additional information and CommentsThere are no comments yet for this article.
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