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DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

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Located near Socorro, NM at 34 ◦ 04 ′ 43".497N,<br />

107 ◦ 37 ′ 03".819W. The array has a maximum<br />

resolution of 0".04 <strong>and</strong> can be used over the frequency<br />

range 300 to 50,000 MHz (90 to 0.7 cm).<br />

Vlasov equation The kinetic equation governing<br />

the velocity distributions of electrons <strong>and</strong><br />

ions in an environment where Coulomb collisions<br />

may be neglected. For non-relativistic particles<br />

of charge q <strong>and</strong> mass m in the presence<br />

of an electric field E(x,t)<strong>and</strong> a magnetic field<br />

B(x,t), the Vlasov equation is (cgs units)<br />

<br />

∂ ∂ q<br />

<br />

+ v · + E +<br />

∂t ∂x m<br />

v<br />

c ×B<br />

<br />

· ∂<br />

<br />

f= 0 ,<br />

∂v<br />

where f(v, x,t) is the velocity distribution.<br />

Here v <strong>and</strong> x are, respectively, the velocity <strong>and</strong><br />

spatial coordinates, <strong>and</strong> t is the time.<br />

Moment equations for macroscopic quantities<br />

are obtained by multiplying the Vlasov<br />

equation by 1, v, etc. <strong>and</strong> integrating over velocity<br />

space. For example, the zero-order moment<br />

equation is<br />

∂n<br />

∂t<br />

+∇·(nV) = 0 ,<br />

where the zeroth moment of f<br />

<br />

n= fd 3 v<br />

is the particle number density, <strong>and</strong> the first moment<br />

(divided by n)<br />

V = 1<br />

<br />

vfd<br />

n<br />

3 v<br />

is the mean vector velocity. Another useful moment<br />

is the stress (or pressure) tensor<br />

<br />

P=m (v − V)(v − V)fd 3 v;<br />

note that the stress tensor need not be isotropic<br />

in a collisionless plasma.<br />

The electric charge <strong>and</strong> current densities in<br />

the plasma are<br />

<br />

<br />

fαd 3 v<br />

<strong>and</strong><br />

α<br />

<br />

α<br />

qα<br />

© 2001 by CRC Press LLC<br />

qα<br />

<br />

vfαd 3 v,<br />

Voigt profile<br />

respectively, where the summation is taken over<br />

all charge species α.<br />

Vlasov–Maxwell equations The fundamental<br />

equations governing the behavior of a<br />

plasma in which Coulomb collisions are negligible.<br />

A solution of the Vlasov–Maxwell system<br />

is comprised of velocity distributions for<br />

all charge-species <strong>and</strong> the associated electric<br />

charge <strong>and</strong> current densities, together with electric<br />

<strong>and</strong> magnetic fields, all consistent with the<br />

Maxwell equations governing electrodynamics.<br />

See Vlasov equation.<br />

voids Large regions of the universe in<br />

which the matter-density is distinctly lower than<br />

the average. Voids are surrounded by relatively<br />

thin layers into which nearly all galaxies<br />

are crowded. Typical diameters of voids<br />

are between 20h −1 Mpc <strong>and</strong> 60h −1 Mpc (h is<br />

the dimensionless Hubble parameter, i.e., H0<br />

/100/km/sec/Mpc), <strong>and</strong> the mass-density within<br />

a void is believed to be about 10% of the cosmic<br />

average matter-density. Hence, the large-scale<br />

distribution of matter in the universe is somewhat<br />

similar to a foam, with the voids being<br />

analogs of the air-bubbles <strong>and</strong> the layers with<br />

galaxies being analogs of the soap films.<br />

Voids were observationally discovered in<br />

1978–1979 <strong>and</strong> hailed at that time as a surprising<br />

discovery. However, papers were already<br />

published in 1934 that predicted that<br />

the Friedmann–Lemaître cosmological models<br />

were unstable against the formation of local<br />

minima in matter-density. Had the faith in the<br />

cosmological principle not prevailed later, voids<br />

would have been, in fact, expected.<br />

Voigt body Also called Kelvin body. A kind<br />

of material with both properties of elastic body<br />

<strong>and</strong> viscous fluid. A Voigt body is represented<br />

by the sum of two terms for which stresses are<br />

proportional to elastic strain <strong>and</strong> viscous strain<br />

rate. Most elastic bodies containing many pores<br />

filled with viscous fluid are examples of Voigt<br />

bodies.<br />

Voigt profile An expression that describes<br />

the shape of an absorption line considering the<br />

effects of natural <strong>and</strong> thermal Doppler broadening<br />

mechanisms. The total absorption coeffi-<br />

505

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