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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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Tethys system. Calypso orbits at the other. Its<br />

orbit has a semimajor axis of 2.95 ×10 5 km. Its<br />

size is 17 × 14 × 13 km, but its mass has not<br />

been measured. It has a geometric albedo of 0.5<br />

<strong>and</strong> orbits Saturn once every 1.888 Earth days.<br />

temperature (1.) In thermodynamics, the<br />

integrating factor in the first law of thermodynamics:<br />

dE=dU+TdS<br />

where the energy E, the internal energy U, <strong>and</strong><br />

the entropy S are functions of the state of the<br />

equilibrium system, <strong>and</strong> dE, dU,dS are their<br />

functional differentials; a function proportional<br />

to the pressure of a hypothetical perfect gas held<br />

at constant volume.<br />

(2.) In statistical mechanics, a measure of the<br />

translational molecular kinetic energy.<br />

(3.) The degree of hotness measured on a<br />

conventional temperature scale.<br />

(Definitions (1.) <strong>and</strong> (2.) agree for equilibrium<br />

systems, as does (3.) for some appropriate<br />

range of temperature specific to the device.)<br />

(4.) In equilibrium photon dynamics, the<br />

inverse multiplier of E/k (where k = Boltzmann’s<br />

constant) in the Plack distribution f =<br />

f(E/kT); the temperature of a black body radiation.<br />

In non-equilibrium situations, e.g., astronomical<br />

observations, a derived measure which<br />

agrees with one of the above definitions for some<br />

range of applicability.<br />

If the object radiates like a true black body, all<br />

of these temperatures are equivalent; however,<br />

a perfect black body in nature is rare. A perfect<br />

black body is thermalized, that is, the atoms or<br />

molecules of the object are in perfect thermodynamic<br />

equilibrium. Most stars have a radiation<br />

distribution with wavelength that closely<br />

but not exactly approximates that of a black<br />

body. The sun, for example, has a radiation temperature<br />

that approximates a black body with<br />

TB = 6300 K; however, its effective temperature,<br />

which compares the total output power to<br />

that of a black body, is better approximated by<br />

aTeff = 5800 K, <strong>and</strong> the color temperature of<br />

the sun which compares the energy output ratio<br />

over two wavelength intervals is Tc = 6500 K.<br />

See excitation temperature, effective temperature,<br />

blackbody temperature, brightness temperature,<br />

color temperature.<br />

© 2001 by CRC Press LLC<br />

tension (cosmic string)<br />

temperature inversion An increase of atmospheric<br />

temperature with altitude. Under this<br />

condition the typical lapse rate is reversed, <strong>and</strong><br />

great stability is created, which strongly damps<br />

vertical motions <strong>and</strong> vertical turbulent transport.<br />

Wind shear will exist between the top <strong>and</strong> the<br />

bottom of the temperature inversion layer. A<br />

temperature inversion acts as a ceiling, preventing<br />

further upward convection, <strong>and</strong> is generally<br />

the limit for cloud development. Marked <strong>and</strong><br />

persistent inversions occur at lower levels, with<br />

subsiding air in major anti-cyclonic cells, such<br />

as the Azores high-pressure zone <strong>and</strong> cold anticyclones<br />

over continents. Temperature inversion<br />

arises for different reasons, such as frontal<br />

inversion, subsidence inversion, trade-wind inversion,<br />

radiation inversion, advective inversion,<br />

turbulence inversion, <strong>and</strong> stratospheric inversion.<br />

See density inversion.<br />

temperature variance dissipation rate<br />

Measure of the rate at which gradient fluctuations<br />

of temperature are smoothed out by turbulence.<br />

It is defined by<br />

χT = 2κT (∇T ) 2<br />

where κT is the thermal diffusivity, T is the temperature,<br />

z is the vertical coordinate, <strong>and</strong> ∇ denotes<br />

the gradient operator. The temperature<br />

variance dissipation rate can be regarded as the<br />

thermal equivalent of the dissipation rate of velocity<br />

fluctuations ɛ.<br />

In oceanic or atmospheric studies, generally<br />

only one component of the temperature gradient<br />

is measured, <strong>and</strong> χT is estimated from<br />

χT 2λκT<br />

2 ∂T<br />

.<br />

∂z<br />

The factor λ is a scaling parameter that reflects<br />

the level isotropy. For a completely isotropic<br />

turbulence field λ = 3.<br />

tension (cosmic string) For a stringlike topological<br />

defect, the quantity<br />

<br />

T =−2π rdrT zz ,<br />

where r is the radial coordinate in a cylindrical<br />

reference frame aligned with the string, <strong>and</strong> T µν<br />

471

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