29.03.2013 Views

DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

sometimes called s<strong>and</strong> seas since they represent<br />

vast regions of s<strong>and</strong>. Most ergs are located in<br />

desert basins downwind from terrain which is<br />

experiencing high amounts of erosion. Various<br />

types of dunes occur within the ergs. Ergs are<br />

found on Earth <strong>and</strong> around the north polar cap<br />

on Mars.<br />

Ernst equation (1967) The complex partial<br />

differential equation<br />

ReEE =∇E·∇E<br />

in a Euclidean 3-space introduced by F.J. Ernst.<br />

The axially symmetric solutionsE=E(x 1 ,x 2 )<br />

represent the metric potentials of stationary, axisymmetric<br />

vacuum gravitational fields. A second<br />

form<br />

(¯ξξ− 1)ξ = 2 ¯ξ∇ξ·∇ξ<br />

is obtained by the substitutionE=(ξ−1)/(ξ+<br />

1). The Ernst equation has been found to<br />

describe additionally various physical systems,<br />

such as colliding plane waves in general relativity,<br />

monopoles in SU(2) gauge theory, <strong>and</strong> states<br />

of Heisenberg ferromagnets. The symmetries of<br />

the equation <strong>and</strong> solution generating techniques<br />

have been extensively studied.<br />

erosion Rock is destroyed by weathering.<br />

Mechanical weathering breaks up rock into<br />

small particles which can be transported hydrologically.<br />

In chemical weathering the rock is<br />

dissolved by water. In either case, the removal<br />

of the rock is erosion.<br />

ERP Earth rotation parameters.<br />

Ertel potential vorticity See potential vorticity.<br />

eruption Volcanos are subject to periodic<br />

eruptions during which molten rock (magma)<br />

<strong>and</strong>/or volcanic ash flows to the Earth’s surface.<br />

Eruptions can occur for months between periods<br />

of quiescence.<br />

eruptiveprominence Solarprominencescan<br />

become activated <strong>and</strong> exhibit several types of<br />

large-scale motion. The prominence may grow<br />

<strong>and</strong> become brighter with a corresponding in-<br />

© 2001 by CRC Press LLC<br />

Euler equations<br />

crease in helical motion or flow along the prominence<br />

axis. This type of activation can lead to<br />

an eruption, especially if it exceeds a height of<br />

50,000 km. In this case, it rises as an erupting<br />

prominence <strong>and</strong> eventually disappears. The<br />

eruption of a quiescent prominence (disparition<br />

brusque) is a slow process lasting several hours.<br />

The eruption of an active region prominence is<br />

much more rapid taking about 30 min.<br />

escape velocity In Newtonian physics, under<br />

gravitational interactions, the gravitational field<br />

contributes negatively to the total energy of a<br />

particle. The escape velocity is that speed giving<br />

a zero total energy (kinetic + gravitational potential).<br />

A particle moving without dissipation<br />

at or exceeding the escape velocity will escape<br />

to infinity.<br />

eskers Long narrow ridges of s<strong>and</strong> <strong>and</strong> gravel<br />

deposited in the middle of glaciers. They have<br />

stream-like shapes <strong>and</strong> are believed to form from<br />

meltwater streams flowing in tunnels beneath<br />

a melting glacier. Sinuous ridges in the high<br />

latitude regions of Mars have been suggested to<br />

be eskers.<br />

estuary A sheltered region that lies inshore<br />

of a sea <strong>and</strong> is subject to tidal action. Generally<br />

has a reduced salinity, compared to the adjoining<br />

sea, as a result of river <strong>and</strong> other freshwater<br />

inputs.<br />

ET See ephemeris time (ET).<br />

eternal black hole A black hole that was<br />

not formed in the collapse of matter, but was<br />

present ab initio as a stable topological structure<br />

in spacetime.<br />

Eudoxos of Cnidus Greek geometer <strong>and</strong> astronomer,<br />

born in Cnidus, Asia Minor approximately<br />

408 B.C., died about 353 B.C. Eudoxos<br />

established the foundation of geometrical principles<br />

developed by Euclid, <strong>and</strong> applied the subject<br />

to the study of the moon <strong>and</strong> the planets.<br />

Euler equations The equations of motion<br />

for an inviscid fluid. Equivalent to the Navier–<br />

Stokes equations if viscosity is taken as zero.<br />

161

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!