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DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

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a propagation velocity, c, which is numerically<br />

equal to the observed speed of the light.<br />

Minkowksi, Lorentz, <strong>and</strong> especially Einstein<br />

in his 1905 exposition, modified concepts of<br />

space <strong>and</strong> time in a way that accommodates<br />

the fact that every observer, regardless of his<br />

motion, will always measure exactly the same<br />

speed for light as experimentally observed by<br />

Michelson <strong>and</strong> Morley. To accomplish this required<br />

accepting that time is involved in Lorentz<br />

transformation, the change of coordinate frame<br />

between moving observers, just as spatial position<br />

is involved. The Lorentz transformation<br />

also predicts length contraction, time dilation,<br />

<strong>and</strong> relativistic mass increase, <strong>and</strong> led Einstein<br />

to his famous result E=mc 2 .<br />

A consequence of the universality of the<br />

speed of light is that velocities are not additive.<br />

If the system B (say, an airliner) moves with respect<br />

to the system A (say, the surface of the<br />

Earth) with a given velocity v1 (say, 900 km/h)<br />

<strong>and</strong> an object C (say, a flight attendant) moves in<br />

the same direction with a velocity v2 (suppose,<br />

4 km/h), then the velocity of the object C with<br />

respect to the system A is not simply v1 + v2,<br />

v1+v2<br />

but V =<br />

1+(v1v2/c2 , where c is the velocity<br />

)<br />

of light (in the example given, the flight attendant<br />

moves with respect to the surface of the<br />

Earth with the velocity 904 ·(1 − 0.31 · 10−12 )<br />

km/h). As is seen from the example, at velocities<br />

encountered in everyday life the corrections<br />

provided by special relativity to Newton’s mechanics<br />

are negligible. However, for velocities<br />

large compared toc, the difference is profound.<br />

In particular, if v2 =c, then V =c. Also, if<br />

v1 ≤c <strong>and</strong>v2 ≤c, thenV≤c, i.e., the velocity<br />

of light cannot be exceeded by adding velocities<br />

smaller than c. The geometric arena of special<br />

relativity is not the three-dimensional EuclideanspacefamiliarfromNewton’stheory,<br />

but<br />

a four-dimensional Minkowski spacetime. The<br />

Euclidean space is contained in the Minkowski<br />

spacetime as the subspace of constant time, but<br />

it is not universally defined, i.e., every observer<br />

will see a different Euclidean space in his/her<br />

own reference system. See Lorentz transformation,<br />

Michelson–Morley experiment.<br />

specific The adjective used to express a quantity<br />

per unit mass.<br />

© 2001 by CRC Press LLC<br />

specific photosynthetic rate<br />

specific absorption coefficient The absorption<br />

coefficient [m −1 ] per unit mass of material,<br />

e.g., for unit chlorophyll a concentration (Units:<br />

[mg chl a m −3 ]); one obtains a specific absorption<br />

coefficient with units [m 2 (mg chl a) −1 ].<br />

specific discharge See Darcy velocity.<br />

specific energy A term used in the study of<br />

open channel flow to denote the energy of a fluid<br />

relative to the channel bottom. Specific energy<br />

is defined as E = y + V 2 /2g, where y is flow<br />

depth, V is flow speed, <strong>and</strong> g is acceleration of<br />

gravity. Specific energy has units of length <strong>and</strong><br />

corresponds to energy per unit weight of fluid.<br />

specific gravity Ratio of the density of a substance<br />

to that of water.<br />

specific heat Specific heats, also called specific<br />

heat capacity or heat capacity, are defined<br />

under constant volume (cv, Cv, also called isochoric<br />

specific heat) <strong>and</strong> constant pressure (cp,<br />

Cp, also called isobaric specific heat). The constant<br />

volume specific heat of a pure substance<br />

is the change of molecular internal energy u for<br />

a unit mass (or 1 mole) per degree change of<br />

temperature when the end states are equilibrium<br />

states of the same volume:<br />

<br />

<br />

∂u<br />

∂ū<br />

cv ≡ <strong>and</strong> Cv ≡ ,<br />

∂T v<br />

∂T v<br />

where cv is for unit mass <strong>and</strong> Cv is called the<br />

molal specific heat, u is the specific internal energy,<br />

ū is internal energy for 1 mole; Cv = Mcv.<br />

The constant pressure specific heat of a pure substance<br />

is the change of enthalpy for a unit mass<br />

(or 1 mole) between two equilibrium states at<br />

the same pressure per degree change of temperature:<br />

<br />

<br />

∂h<br />

∂ ¯h<br />

<br />

cp ≡ <strong>and</strong> Cp ≡<br />

∂T p<br />

∂T p<br />

where h = (u+pv) is the specific enthalpy, <strong>and</strong><br />

¯h is the enthalpy for 1 mole; Cp = Mcp.<br />

specific humidity The mass of water vapor<br />

per unit mass of air.<br />

specific photosynthetic rate Photosynthetic<br />

rate, net or gross, per unit biomass or per unit<br />

435

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