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DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

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Fata Morgana A complex mirage made up<br />

of multiple images as of cliffs <strong>and</strong> buildings, distorted<br />

<strong>and</strong> magnified, which occasionally gives<br />

the impression of elaborate castles floating in<br />

the air. A Fata Morgana can only occur where<br />

there are alternating warm <strong>and</strong> cold layers of air<br />

near the ground or surface of water. Named after<br />

the effect seen in the Straits of Medina, <strong>and</strong><br />

attributed to the sorcery of King Arthur’s halfsister,<br />

Morgan Le Fay.<br />

fathom A nautical unit of depth, equal to<br />

6 ft. It is also sometimes used for horizontal<br />

measure; a related unit is the cable, equal to 100<br />

fathoms. Also, a nautical mile is approximately<br />

1000 fathoms. See nautical mile.<br />

fault A seismic fracture across which lateral<br />

motion occurs. In some cases a fracture is simply<br />

a crack in rocks where slip has occurred.<br />

Major faults may be broad zones of granulated<br />

rock (fault gouge) accommodating lateral motions<br />

of 1000 km or more. Faults can be classified<br />

as thrust faults, normal faults, or strike-slip<br />

faults.<br />

fault constitutive law A representation<br />

of fault mechanical properties using relations<br />

among stress, strain rate, <strong>and</strong> displacement on<br />

fault planes. A variety of constitutive laws<br />

have been proposed such as the slip weakening<br />

model which represents the relation between<br />

shear stress <strong>and</strong> slip, <strong>and</strong> the rate- <strong>and</strong> statedependent<br />

friction law which represents the relation<br />

between friction <strong>and</strong> slip accompanied by<br />

changes in slip rate. These are empirical laws<br />

derived from laboratory experiments of rock<br />

friction. There are two modes for friction: stable<br />

sliding <strong>and</strong> unstable sliding. It is thought that<br />

aseismic slips such as fault creep <strong>and</strong> slow earthquakes<br />

correspond to the former, while usual<br />

earthquakes correspond to the latter. Numerical<br />

simulations are being carried out to tackle<br />

problems of earthquake cycle <strong>and</strong> seismic nucleation<br />

process of large earthquakes, using the<br />

fault constitutive laws.<br />

fault gouge The granulated material on a<br />

fault that has been generated during the many<br />

earthquakes that have occurred on the fault.<br />

© 2001 by CRC Press LLC<br />

fault scarp<br />

fault parameter Parameter that characterizes<br />

faulting. As a geometrical quantity, there<br />

is the strike of a fault plane, dip angle <strong>and</strong> slip<br />

direction, while as quantities which represent<br />

fault size, there is fault area (length times width)<br />

<strong>and</strong> the amount of slip. Furthermore, rupture<br />

velocity, rise time, <strong>and</strong> slip rate are physical<br />

parameters which represent source processes.<br />

From these fault parameters, seismic moment<br />

<strong>and</strong> stress drop can be calculated. These fault<br />

parameters can be obtained from radiation patterns<br />

of seismic waves, waveforms, <strong>and</strong> aftershock<br />

distributions.<br />

fault plane solution An earthquake is generated<br />

by the relative motion of rocks across a<br />

fault. The movement has to be parallel to the<br />

fault plane, i.e., a vector representing the motion<br />

of one side with respect to the other will lie<br />

on the fault plane, <strong>and</strong> therefore there will be<br />

a plane normal to this vector (termed the “auxiliary<br />

plane”) that will be perpendicular to the<br />

fault plane. For the simplest type of earthquake<br />

— simple movement along a flat fault plane,<br />

known as a “double-couple” earthquake — the<br />

pattern of radiation is divided into four lobes<br />

separated by the fault <strong>and</strong> auxiliary planes. The<br />

reason for this is that these planes divide the rock<br />

into areas in which the released stress is compressive<br />

or extensional, <strong>and</strong> thereby directions<br />

in which the first motions of the propagated radiation<br />

are compressions or rarefactions. With<br />

sufficient seismic data from around the world, it<br />

is possible to reconstruct the pattern of radiation<br />

for these first motions, <strong>and</strong> so to pick out the fault<br />

<strong>and</strong> auxiliary planes. This is known as the fault<br />

plane solution. Without other information it is<br />

difficult to tell which plane is the fault plane <strong>and</strong><br />

which is the auxiliary plane, but local observations<br />

of the fault where the earthquake occurred<br />

or knowledge of the tectonic setting can help<br />

to determine this. The fault plane solution is<br />

invaluable in discriminating between different<br />

types of fault (e.g., thrust faults <strong>and</strong> transcurrent<br />

faults).<br />

fault scarp When there is vertical movement<br />

on a fault during an earthquake, one side of the<br />

fault is elevated relative to the other. This is a<br />

fault scarp.<br />

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