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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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particle forces due to electrical charges are significant<br />

compared to particle weight.<br />

clear air turbulence (CAT) Vigorous smallscale<br />

motions within the lowest kilometer of the<br />

atmosphere. Most clear air turbulence is the result<br />

of small-scale wavelike undulations that develop<br />

spontaneously when the vertical shear of<br />

the horizontal flow exceeds some critical value.<br />

cleft, polar See cusp, polar.<br />

climate regimes (Charney <strong>and</strong> DeVore,<br />

1979). The equilibrium states in the extratropical<br />

circulation in the atmosphere.<br />

climatic optimum Mid-Holocene event in<br />

which summer temperatures in the Northern<br />

hemisphere averaged 1 to 2 ◦ C above current<br />

temperatures. Dated as the period approximately<br />

8000 to 5000 years ago.<br />

closed magnetosphere A model of a magnetosphere<br />

(usually the Earth’s), in which all<br />

planetary magnetic field lines are confined inside<br />

some surface, usually identified with the<br />

magnetopause. The Earth’s magnetosphere resembles<br />

a closed magnetosphere, except for two<br />

details: (1) on the night side, field lines extend<br />

to great distances <strong>and</strong> no well-defined closure<br />

surface has been observed there; (2) indications<br />

exist that a small amount of interconnection usually<br />

exists. See open magnetosphere.<br />

closed universe A model of the universe that<br />

is finite in total volume <strong>and</strong> age. It evolves from<br />

a “big bang” to a point of maximum expansion<br />

before contracting back to a “big crunch” of high<br />

density <strong>and</strong> temperature.<br />

cloudclassification Aschemeofdistinguishing<br />

<strong>and</strong> grouping clouds based on their appearance,<br />

elevation, <strong>and</strong> the physical processes generating<br />

them. The World Meteorological Organization<br />

classifies 10 genera in three major<br />

groups — cumulus, stratus, <strong>and</strong> cirrus, by criteria<br />

essentially according to the cloud formation<br />

processes. The major cloud genera are, cirrus<br />

(Ci), cirrocumulus (Cc), cirrostratus (Cs), altocumulus<br />

(Ac), altostratus (As), nimbostratus<br />

(Ns), stratocumulus (Sc), stratus (St ), cumulus<br />

© 2001 by CRC Press LLC<br />

coastal jet<br />

(Cu), <strong>and</strong> cumulonimbus (Cb). Clouds can also<br />

be referred to, according to their composition,<br />

as water clouds, ice clouds, or mixed clouds.<br />

clump star A metal-rich star of a few solar<br />

masses that has begun helium burning. Because<br />

of the difference in opacity, such stars do not<br />

reach the giant branch but instead spend a long<br />

period of time in the red clump in the HR diagram,B−V=<br />

1mag, <strong>and</strong> M= 0mag.<br />

CNO cycle (or tricycle) A set of nuclear<br />

reactions in which hydrogen is fused to helium,<br />

with the liberation of about 7 × 10 18 ergs<br />

per gram, 5 to 10% of which is lost in neutrinos,<br />

depending on the precise temperature<br />

at which the reactions occur, generally in the<br />

range 15–25 ×10 6 K. These reactions, which<br />

require the presence of carbon, nitrogen, or<br />

oxygen as catalysts, are the primary source<br />

of energy for stars larger than about 2 solar<br />

masses during their main sequence lifetimes<br />

<strong>and</strong> for all stars during the red giant phase.<br />

They are the primary source of nitrogen in the<br />

universe <strong>and</strong> contribute to the production of<br />

13 C, 15 N, 17 O, 18 O, <strong>and</strong>, through extensions<br />

toheaviercatalystsathighertemperatures, probably<br />

also to 19 F, 21 Ne, 22 Ne, 23 Na, <strong>and</strong> perhaps<br />

26 Al.<br />

The primary reaction sequence is (see nuclear<br />

reactions for explanation of the symbols):<br />

12 C(p,γ) 13 N(e + νe) 13 C(p,γ) 14 N(p,γ)<br />

15 O(e + νe) 15 N(p,α) 12 C,<br />

thus the net effect is to convert four protons (hydrogen<br />

atoms) to one helium nucleus or alpha<br />

particle, returning the 12 C to its original form.<br />

Other closures include<br />

15 16 17 +<br />

N(p,γ) O(p,γ) F(e νe) 17 O(p,γ)<br />

18 +<br />

F(e νe) 18 O(p,α) 15 N.<br />

See nuclear reactions.<br />

cnoidal wave A nonlinear theory for periodic<br />

waves, attributed to Korteweg <strong>and</strong> Devries<br />

(1895), in which the water surface profile is expressed<br />

in terms of a Jacobian elliptical integral,<br />

cn(u).<br />

coastal jet a coastal current system that intensifies<br />

toward the coast.

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