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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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Thus, four-velocity is the tangent four-vector<br />

u α =dx α /ds of an affinely parametrized timelike<br />

curve γ ={x α (s)} in the space-time. The<br />

norm isg(u,u) =−1. See signature, spacelike<br />

vector, timelike vector.<br />

f-plane approximation In calculating motions<br />

on the Earth’s surface, the effects of the<br />

Earth’s sphericity are retained by approximating<br />

the value of the Coriolis parameter, f, as a<br />

constant.<br />

fractal A geometrical object that is selfsimilar<br />

under a change of scale; i.e., that appears<br />

similar at all levels of magnification. Fractals<br />

can be considered to have fractional dimensionality.<br />

A statistical distribution is fractal if the<br />

number of “objects” N has a fractional inverse<br />

power dependence on the linear dimension of<br />

the objects r.<br />

N ∼ r −D<br />

where D is the fractal dimension. Examples<br />

occur in diverse fields such as geography<br />

(rivers <strong>and</strong> shorelines), biology (trees), geology,<br />

<strong>and</strong> geophysics (the number-size distribution of<br />

fragments often satisfies this fractal relation; the<br />

Guttenberg–Richter frequency-magnitude relation<br />

for earthquakes is fractal), <strong>and</strong> solid state<br />

physics (amorphous materials).<br />

fractionation In geophysics, separation of<br />

different minerals during the melting of rocks,<br />

<strong>and</strong> refreezing of a solid; applied to the geophysical<br />

processes modifying rocks.<br />

fracture In geophysics, the Earth’s crust is<br />

filled with fractures on a range of scales from<br />

centimeters to thous<strong>and</strong>s of kilometers. The<br />

term fracture covers both joints <strong>and</strong> faults. If<br />

no lateral displacement has occurred across a<br />

fracture, it is classified as a joint; if a lateral<br />

displacement has occurred, it is classified as a<br />

fault.<br />

fracture zone In geophysics, deep valleys<br />

caused by faults on the ocean floor. The ocean<br />

floor on the two sides of a fracture zone can be of<br />

very different ages <strong>and</strong> this leads to differential<br />

elevations <strong>and</strong> subsidence.<br />

© 2001 by CRC Press LLC<br />

frame dragging<br />

fragmentation The breaking up of a mass<br />

into fragments. Applied in astrophysics to discuss<br />

collisions of minor planets, <strong>and</strong> in geophysics<br />

to describe rock processing where fragmentation<br />

takes place on a wide range of scales<br />

<strong>and</strong> occurs on joints <strong>and</strong> faults. On the largest<br />

scale the plates of plate tectonics are fragments<br />

that are the result of fragmentation.<br />

frame dragging The phenomenon in relativistic<br />

theories of gravitation, particularly in<br />

general relativity in which the motion of matter,<br />

e.g., translating or rotating matter “drags” the<br />

inertial frame, meaning the inertial frames near<br />

the moving matter are set in motion with respect<br />

to the distant stars, in the direction of the matter<br />

motion. For instance, the plane of a circular<br />

polar orbit around a rotating primary rotates in<br />

the direction of the central rotating body. In the<br />

case of an orbit around the Earth, the gravitational<br />

fields are weak, <strong>and</strong> the effect was first<br />

calculated by Lense <strong>and</strong> Thining in 1918. The<br />

plane of the polar orbit rotates in this case at a<br />

rate:<br />

˙ = 2GJ<br />

c 2 r<br />

3 .<br />

Here c is the speed of light, G is Newton’s gravitational<br />

constant, <strong>and</strong> J is the angular momentum<br />

of the isolated rotating planet. For an orbit<br />

close to the surface of the Earth, this rate is approximately<br />

220 milliarc sec/year.<br />

This result actually applies to the dragging of<br />

the line of nodes of any orbit, with the following<br />

modification due to eccentricity e:<br />

2J<br />

˙ =<br />

a3 (1 − e2 .<br />

) 3/2<br />

The pointing direction of a gyroscope near<br />

a rotating object is also affected by the frame<br />

dragging. The precession rate due to this effect<br />

for a gyroscope in circular orbit is:<br />

3ˆr(J · ˆr) − J<br />

˙δ =<br />

r3 ,<br />

where ˆr is the unit vector to the gyroscope position.<br />

For a gyroscope in orbit at about 650 km<br />

altitude above this rate is approximately 42 milliarc<br />

sec/year. A second relativistic effect, the<br />

deSitter precession, constitutes<br />

3 M<br />

(ˆr × v),<br />

2 r2 181

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