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DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

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smoothing effect of molecular thermal diffusivity<br />

κT . In natural waters, χ is mostly estimated<br />

by profilers that measure the temperature fluctuations<br />

T ′ at a high rate (at least such, as to<br />

resolve the structures to the Batchelor scale). If<br />

small-scale turbulence is isotropic, the rate of<br />

dissipation of temperature variance χ[K2s−1 ]<br />

is estimated from the temperature gradient spectra<br />

by χ = 6κT , where z is<br />

the profiling direction. The vertical turbulent<br />

diffusivity κt v can be estimated by the relation<br />

κt v = χ[2(∂T/∂z)2 ] −1 , a procedure often referred<br />

to as Osborn–Cox method (Osborn <strong>and</strong><br />

Cox, 1972). See Cox number.<br />

dissipation of turbulent kinetic energy<br />

The rate at which turbulent kinetic energy ɛ[W<br />

kg−1 ] is transformed to heat by internal friction<br />

caused by viscosity ν. Dissipation is given<br />

by ɛ = 2ν <br />

ij [0.5 · (∂ui/∂xj +∂uj/∂xi)] 2<br />

(see strain rate). In natural waters, ɛ is mostly<br />

estimated by profilers that measure one velocity<br />

component u ′ in the direction perpendicular<br />

to the motion of the measuring profiler (directionz).<br />

For isotropic small-scale turbulence, the<br />

above nine terms in the summation collapse to<br />

the simple form ɛ= 7.5ν (<br />

indicates the average over a length scale, chosen<br />

typically 0.5 to several meters). An alternative<br />

estimate can be determined by the inertial dissipation<br />

method.<br />

dissipation profiler Instrument for the measurement<br />

of oceanic turbulence levels. It is<br />

equipped with fast sampling airfoil probes <strong>and</strong><br />

thermistors to resolve velocity <strong>and</strong> temperature<br />

fluctuations in the dissipation range. Generally,<br />

these instruments are designed to either fall or<br />

rise vertically in the water in order to produce a<br />

profile of the turbulent activity in the water column.<br />

For certain applications, the instruments<br />

are towed horizontally.<br />

dissipation range The range of length scales<br />

or wavenumbers at which velocity fluctuations<br />

in turbulent flows are damped out (dissipated)<br />

by molecular viscosity. See Kolmogorov scale,<br />

turbulent cascade.<br />

dissipation rate Rate at which turbulent<br />

kinetic energy ( tke) is removed from turbu-<br />

© 2001 by CRC Press LLC<br />

diurnal<br />

lent flows at length scales defined by the Kolmogorov<br />

scale. The dissipation rate enters the<br />

turbulent kinetic energy equation as the term<br />

ɛ= 2νeijeij<br />

whereν is the viscosity <strong>and</strong>eij is the fluctuating<br />

strain rate tensor defined by<br />

eij ≡ 1<br />

<br />

∂ui<br />

+<br />

2 ∂xj<br />

∂uj<br />

<br />

∂xi<br />

whereui <strong>and</strong>xi are the velocity <strong>and</strong> position, respectively,<br />

for the spatial directions i= 1, 2, 3.<br />

In oceanic turbulence studies,ɛ can be estimated<br />

from measurements of velocity gradients. Under<br />

the assumption of isotropic <strong>and</strong> steady turbulence,<br />

ɛ is estimated from<br />

ɛ= 15<br />

2 ν<br />

<br />

∂u2<br />

∂x1<br />

2<br />

where x1 is the direction along which the measurement<br />

device measures the perpendicular turbulent<br />

velocity fluctuations u2. See also airfoil<br />

probe.<br />

dissolved organic matter See colored dissolved<br />

organic matter.<br />

distance indicator See st<strong>and</strong>ard c<strong>and</strong>le.<br />

distance modulus The distance to an object<br />

can be derived by comparing its apparent magnitude<br />

(m) <strong>and</strong> absolute magnitude M, where<br />

M is defined to be the flux of the star at a st<strong>and</strong>ard<br />

distance of (10pc2 ). Using the st<strong>and</strong>ard<br />

definition for magnitude, we have<br />

<br />

L/4πR2 m − M =−2.5 log<br />

L/4π(10pc2 <br />

)<br />

where R is the distance to the star <strong>and</strong> L is the<br />

star’s intrinsic brightness (luminosity). This reduces<br />

to<br />

m − M = 5 log(R) − 5 .<br />

diurnal Due to the daily variation of the solar<br />

radiation received at the Earth’s surface, meteorological<br />

quantities, such as temperature, pressure,<br />

atmospheric pollution, wind speed <strong>and</strong> direction,<br />

etc. have daily variations. Diurnal variation<br />

is a periodic variation <strong>and</strong> does not contain

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