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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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figure of the Earth<br />

See cosmic topological defect, Derrick theorem,<br />

spontaneous symmetry breaking.<br />

figure of the Earth The shape of the Earth.<br />

To a first approximation it is an oblate spheroid<br />

with a polar radius of 6357 km <strong>and</strong> an equator<br />

radius of 6378 km.<br />

filament A structure in the corona consisting<br />

of cool (∼ 7000 K), dense ( 10 12 cm −3 )<br />

plasma supported by magnetic fields <strong>and</strong> seen<br />

as dark lines threaded over the solar disk. When<br />

seen in emission at the solar limb, a filament<br />

appears as a protuberance: a bright arc of matter<br />

extending high above the photosphere, spanning<br />

latitudes of up to some 10 ◦ . Their density is<br />

about a factor of ten higher than the ambient density<br />

(therefore the arc is bright when seen above<br />

the solar limb), <strong>and</strong> the filament can extend up to<br />

about 100 times the scale height in the corona.<br />

Filaments are aligned along the separation of<br />

opposing magnetic field patches in the photosphere.<br />

Their existence therefore is related to<br />

solar activity with only a few filaments observed<br />

during solar minimum <strong>and</strong> a much larger number<br />

during solar maximum. Filaments can have<br />

very long lifetimes, lasting 2 to 3 solar rotations<br />

in some cases. They are found, preferentially,<br />

in two latitude belts on the sun; in a strip at high<br />

latitudes known as the polar crown <strong>and</strong> in active<br />

mid-latitudes. Typical magnetic fields are ∼ 5<br />

to 10 G in quiescent filaments <strong>and</strong> may be as<br />

high as 200 G in active region filaments fields.<br />

The cold end dense matter of the filament/protuberance<br />

is held against gravity by<br />

magnetic tension in the anchoring magnetic field<br />

lines. Two configurations can be distinguished<br />

by comparing the photospheric magnetic field<br />

pattern with that of the filament:<br />

1. Kippenhahn–Schlüter configuration, also<br />

called normal configuration: the magnetic field<br />

inside the filament has the same direction as the<br />

photospheric field below it.<br />

2. Raadu–Kuperus configuration, also called<br />

inverse configuration: the magnetic field inside<br />

the filament is directed opposite to the one in the<br />

photosphere. This is possible only because the<br />

anchoring field lines have a neutral point below<br />

the filament. In particular, in large <strong>and</strong> highrising<br />

filaments, which tend to give rise to coronal<br />

mass ejections, the Raadu–Kuperus configu-<br />

© 2001 by CRC Press LLC<br />

172<br />

ration seems to be the dominant one. This is attributed<br />

to the X-point below the filament where<br />

reconnection is likely to occur, leading to the expulsion<br />

of the filament (coronal mass ejection)<br />

<strong>and</strong> the generation of electromagnetic emission<br />

due to the accelerated electrons (the flare). See<br />

coronal mass ejection, reconnection.<br />

filament channel A broad pattern of fibrils<br />

in the chromosphere, marking where a filament<br />

may soon form or where a filament recently disappeared.<br />

filter layer In civil or coastal engineering, denotes<br />

a layer of material (typically stone, gravel,<br />

or s<strong>and</strong>, possibly combined with a geotextile<br />

fabric) intended to prevent migration of fine material<br />

into or out of a structure. May also be<br />

employed to reduce settlement. As an example,<br />

breakwaters are often built with a filter layer in<br />

the base to help prevent scouring <strong>and</strong> settlement.<br />

finestructure In atmospheric dynamics,<br />

structures with scales from tens of meters to<br />

decimeters, covering the processes of internal<br />

waves <strong>and</strong> intrusions. Finestructure processes<br />

are intermediary between the large-scale (overall<br />

stratification) structures <strong>and</strong> the small-scale<br />

(turbulence).<br />

fine structure constant Dimensionless constant<br />

relating to strength of electromagnetic interactions:<br />

α = e 2 / (4πɛ0 ¯hc) = 7.297352533(27)×10 −3 .<br />

fingering See double diffusion.<br />

finger regime The double-diffusive regime,<br />

where temperature stabilizes <strong>and</strong> salinity destabilizes<br />

(i.e., warmer <strong>and</strong> saltier water is on<br />

top of cooler <strong>and</strong> fresher water). In this case,<br />

the non-dimensional stability ratio is defined as<br />

Rρ = (α∂/∂z)/(β∂S/∂z). The term “finger”<br />

refers to the saltier finger-like plumes driving<br />

the double-diffusive convection. Classical locations<br />

of the finger regime are under the Mediterranean<br />

Outflow, in the East North-Atlantic <strong>and</strong><br />

the C-SALT field east of Barbados.

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