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DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

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Ångström (Å) A unit of length used in spectroscopy,<br />

crystallography, <strong>and</strong> molecular structure,<br />

equal to 10 −10 m.<br />

angular diameter distance Distance of a<br />

galaxy or any extended astronomical object estimated<br />

by comparing its physical size to the angle<br />

subtended in the sky: ifD is the diameter of<br />

the galaxy <strong>and</strong> δ the angle measured in the sky,<br />

then dA =D/tanδD/δ. For a Friedmann<br />

model with density o in units of the critical<br />

density, <strong>and</strong> zero cosmological constant, the angular<br />

diameter dA of an object at redshift z can<br />

be given in closed form:<br />

dA =<br />

2 o<br />

2cH −1<br />

o<br />

(1 +z)2<br />

<br />

oz+(o − 2)<br />

<br />

(oz+ 1) 1/2 <br />

− 1 .<br />

Other operational definitions of distance can be<br />

made (see luminosity distance) depending on<br />

the intrinsic (assumed to be known) <strong>and</strong> the observed<br />

properties to be compared.<br />

angular momentum L = r × p, where ×<br />

indicates the vector cross product, r is the radius<br />

vector from an origin to the particle, <strong>and</strong> p is the<br />

momentum of the particle. L is a pseudovector<br />

whose direction is given by r, p via the righth<strong>and</strong><br />

rule, <strong>and</strong> whose magnitude is<br />

|L| =|r||p| sinθ,<br />

whereθ is the angle between r <strong>and</strong> p. For a body<br />

or system of particles, the total angular momentum<br />

is the vectorial sum of all its particles. In<br />

this case the position is generally measured from<br />

the center of mass of the given body. See pseudovector,<br />

right-h<strong>and</strong> rule, vector cross product.<br />

angular velocity (ω) The angle through<br />

which a body rotates per unit time; a pseudovector<br />

with direction along the axis given by the<br />

right-h<strong>and</strong> rule from the rotation.<br />

anisotropic A material whose properties<br />

(such as intrinsic permeability) vary according<br />

to the direction of flow.<br />

anisotropic scattering Scattering that is not<br />

spherically symmetric.<br />

© 2001 by CRC Press LLC<br />

anomalistic month<br />

anisotropic turbulence See isotropic turbulence.<br />

anisotropic universe A universe that exp<strong>and</strong>s<br />

at different rates in different directions.<br />

The simplest example is Kasner’s model (1921)<br />

which describes a space that has an ellipsoidal<br />

rate of expansion at any moment in time. Moreover,<br />

the degree of ellipticity changes with time.<br />

The generic Kasner universe exp<strong>and</strong>s only along<br />

two perpendicular axes <strong>and</strong> contracts along the<br />

third axis.<br />

anisotropy The opposite of isotropy (invariance<br />

under rotation), i.e., variation of properties<br />

under rotation. For example, if a rock has a fabric<br />

such as layering with a particular orientation,<br />

then phases of seismic waves may travel at different<br />

speeds in different directions through the<br />

rock, according to their alignment with the fabric.<br />

The wave speed along an axis varies when<br />

the axis is rotated through the rock with respect<br />

to the fabric, i.e., it is anisotropic. In terms of<br />

the material properties of the rock, this would<br />

be associated with an elasticity tensor that varies<br />

under rotation. This occurs in the real Earth: for<br />

example, wave speeds are observed to be faster<br />

in the upper mantle under the ocean in the direction<br />

perpendicular to the mid-ocean ridges.<br />

The Earth’s inner core has been determined to<br />

be anisotropic, with (to a first approximation)<br />

faster wave speeds parallel to the Earth’s rotation<br />

axis than in directions perpendicular to<br />

it. Many other physical properties may also be<br />

anisotropic, such as magnetic susceptibility, diffusivity,<br />

<strong>and</strong> turbulence.<br />

annual flood The maximum discharge peak<br />

flow during a given water year (October 1<br />

through September 30) or annual year.<br />

annular eclipse A solar eclipse in which the<br />

angular size of the moon is slightly too small<br />

to obscure the entire solar photosphere. As a<br />

result, a ring (“annulus”) of visible photosphere<br />

surrounds the dark central shadow of the moon.<br />

Annular eclipse occurs when the moon is near<br />

apogee, giving it a smaller angular size.<br />

anomalistic month See month.

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