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DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

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western boundary currents Ocean currents<br />

flowing on the western boundary at speeds much<br />

higher than those in the rest of an ocean basin.<br />

This western intensification of ocean currents is<br />

a combined effect of rotation <strong>and</strong> surface curvature<br />

of the Earth, or the so-called beta-effect.<br />

The Gulf Stream <strong>and</strong> Kuroshio Current are the<br />

surface western boundary currents of the North<br />

Atlantic <strong>and</strong> North Pacific, respectively. In the<br />

Atlantic, deep western boundary currents are<br />

also observed, transporting deep water formed<br />

in the Nordic <strong>and</strong> Labrador Seas.<br />

western boundary intensification The intensification<br />

of current toward the western<br />

boundary of the ocean due to the variation of the<br />

Coriolis parameter with latitude (the β-effect).<br />

west Greenl<strong>and</strong> current A branch of the east<br />

Greenl<strong>and</strong> current that branches northwestward<br />

along the southwest coast of Greenl<strong>and</strong>.<br />

westward drift The movement of features<br />

of the geomagnetic field to the west. This was<br />

first noticed by Halley in the 17th century, who<br />

hypothesized that the Earth’s magnetic field emanates<br />

from magnetized layers in the Earth’s interior<br />

that are in rotation with respect to the surface.<br />

It is now understood that the magnetic<br />

field is generated in a molten iron outer core,<br />

<strong>and</strong> that changes in the magnetic field observed<br />

at the Earth’s surface are related either to flows<br />

at the top of the core, or diffusion of the magnetic<br />

field. If the former is responsible for the<br />

westward drift, then it would be related to a general<br />

westward flow of the core’s surface. The<br />

magnitude of the drift is around 0.2 to 0.4 ◦ per<br />

year, although it appears to vary with time <strong>and</strong><br />

latitude. It is better determined in some places<br />

than others: for example, the field in the Pacific<br />

region is relatively plain, so it is difficult to tell<br />

whether or not it is drifting, <strong>and</strong> some models of<br />

core flow show flows to the east there. Part of<br />

the time variation of the westward drift may be<br />

related to torsional oscillations. See core flow.<br />

wet-bulb temperature The temperature to<br />

which a parcel of air is cooled by evaporating<br />

water into it gradually, adiabatically, <strong>and</strong> at constant<br />

pressure until it is saturated. It is measured<br />

© 2001 by CRC Press LLC<br />

Weyl tensor<br />

directly by a thermometer whose bulb is covered<br />

by a moist cloth over which air is drawn.<br />

wetness (or degree of saturation) (S) The<br />

proportion of pore space that contains water:<br />

S =<br />

Vw<br />

= θ<br />

φ<br />

Va + Vw<br />

where Vw is the volume of water in the sample,<br />

<strong>and</strong> Va is the volume of air in the sample. When<br />

a soil or rock sample is saturated with water the<br />

volume of air goes to zero, the volumetric water<br />

content equals porosity, <strong>and</strong> wetness equals one.<br />

wetted perimeter A linear measure of the<br />

length of a river or canal cross-section that is<br />

wetted by flowing fluid.<br />

Weyl space-times (1917) The static <strong>and</strong> axially<br />

symmetric vacuum metrics of the form<br />

ds 2 = −e 2U dt 2 + e −2U<br />

<br />

e 2γ (dρ 2 + dz 2 ) + ρ 2 dφ 2<br />

where ρ <strong>and</strong> z are generalized cylindrical coordinates.<br />

The function U = U(ρ,z)satisfies the<br />

Laplace equation U = 0 as follows from the<br />

vacuum Einstein equations. The linearity of the<br />

Laplace equation allows a superposition of solutions.<br />

The function γ = γ(ρ,z)is determined<br />

by the line integral in the (ρ, z) plane<br />

∂U 2 <br />

2<br />

∂U<br />

γ = ρ<br />

− dρ<br />

∂ρ ∂z<br />

+2 ∂U ∂U<br />

∂z ∂ρ dz<br />

<br />

.<br />

The solution U = m/(ρ 2 + z 2 ) 1/2 yields the<br />

axisymmetric Curzon metric (rather than the<br />

spherical Schwarzschild solution).<br />

Weyl tensor A tensor, components of which<br />

are the following linear combination of the components<br />

of the curvature tensor:<br />

Cαβρσ =Rαβρσ − 2<br />

n − 2<br />

<br />

Rα[ρ gσ ]β − Rβ[ρ gσ ]α<br />

2 R<br />

+<br />

(n − 1)(n − 2) gα[ρ gσ ]β .<br />

513

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