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DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

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equatorial surface of the magnetosphere A<br />

surface with respect to which the Earth’s magnetospheric<br />

field <strong>and</strong> its trapped plasma exhibit<br />

approximate north-south symmetry. It is usually<br />

defined as a collection of the points of weakest<br />

magnetic intensity |B| on “closed” field lines<br />

which start <strong>and</strong> end on the surface of Earth. In<br />

the plasma sheet the surface is often called the<br />

“neutral sheet” <strong>and</strong> it undergoes a periodic deformation<br />

(“warping”) due to the daily <strong>and</strong> annual<br />

variation of the geomagnetic tilt angle ψ.<br />

See minimum-B surface.<br />

equatorial undercurrent A strong narrow<br />

eastward current found in the region of strong<br />

density gradient below the ocean mixed layer<br />

<strong>and</strong> with its core close to the equator. Its vertical<br />

thickness is around 100 m <strong>and</strong> its half-width is<br />

a degree of latitude. The maximum current is<br />

typically 1 ms −1 . This eastward current is a<br />

majorfeatureoftheequatorialoceancirculation,<br />

particularly in the Pacific <strong>and</strong> Atlantic Oceans.<br />

equatorial upwelling The resultant volume<br />

transport in the Ekman layer is at right angles<br />

to <strong>and</strong> to the right of the wind direction in the<br />

northern hemisphere. If the wind is easterly, water<br />

in the Ekman layer will tend to move away<br />

from the equator on both sides of the equator<br />

<strong>and</strong> will be replaced by water moving upward<br />

from below the layer. This is called equatorial<br />

upwelling. If the wind is westerly, water in the<br />

Ekman layer will tend to move toward the equator<br />

in both sides of the equator <strong>and</strong> repel the<br />

water below the layer. This is called equatorial<br />

downwelling.<br />

equatorial waveguide An oceanic or atmospheric<br />

wave that is confined to propagate near<br />

the equator due to the vanishing of the Coriolis<br />

force at the equator. While the conditions<br />

for geostrophic balance theoretically fail at the<br />

equator, in practice any mass crossing the equator<br />

will be influenced by the Coriolis force on<br />

either side. The force turns such motion back<br />

towards the equator, thus creating a trap or a<br />

waveguide.<br />

equatorial waves A class of equatorially<br />

trapped wave solutions first obtained by Taroh<br />

Matsuno in 1966, consisting of the Rossby, in-<br />

© 2001 by CRC Press LLC<br />

equilibrium tide (gravitational tide)<br />

ertial gravity, mixed Rossby-gravity, <strong>and</strong> Kelvin<br />

waves. The Rossby <strong>and</strong> inertial gravity waves<br />

are waves of rotating fluid, having their counterparts<br />

in off-equatorial regions. The Kelvin <strong>and</strong><br />

mixed Rossby-gravity waves are unique to the<br />

equatorial waveguide arising from the singularity<br />

of the equator where the Coriolis parameter<br />

f = 2 sinθ vanishes. Here is the angular<br />

velocity of the Earth’s rotation around the north<br />

pole <strong>and</strong> θ is latitude.<br />

equilibrium In mechanics, a configuration<br />

in which the total force on a system vanishes,<br />

so if placed in such a configuration the system<br />

remains in it.<br />

equilibrium beach profile A theoretical<br />

beach profile shape that results if wave conditions<br />

<strong>and</strong> water level are held constant for an<br />

indefinite period. It has a monotonic, concaveup<br />

shape.<br />

equilibrium range High-wavenumber part<br />

of the turbulent kinetic energy spectrum that includes<br />

the inertial subrange <strong>and</strong> the dissipation<br />

range. The turbulence at these wavenumbers is<br />

nearly isotropic <strong>and</strong> the shape of the spectrum<br />

at these wavenumbers does not depend on the<br />

amount of kinetic energy present at larger scales<br />

or the size of these energy containing scales.<br />

Kinetic energy is merely transferred by inertial<br />

forces through the inertial subrange until the energy<br />

is dissipated into heat at the Kolmogorov<br />

microscale.<br />

equilibrium space-times Stationary electrovacuum<br />

space-times describing the external<br />

fields of an arbitrary array of electrically<br />

charged, massive sources. Equilibrium is<br />

achieved by the balance of gravitational <strong>and</strong><br />

electromagnetic forces. The static equilibrium<br />

space-times were found by S.D. Majumdar<br />

<strong>and</strong> A. Papapetrou (1947). See Israel–Wilson–<br />

Perjés space-times.<br />

equilibrium tide (gravitational tide) Ahypothetical<br />

ocean tide that responds instantly to<br />

tide producing forces, forming an equilibrium<br />

surface. The effects of friction, inertia, <strong>and</strong> the<br />

irregular distribution of l<strong>and</strong> mass are ignored.<br />

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