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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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conserves energy; if the column is conditionally<br />

unstable <strong>and</strong> the humidity exceeds a specified<br />

value, the column is adjusted to moist static<br />

neutrality.<br />

convective cloud A type of cloud that is<br />

generated by convective activities in the atmosphere.<br />

The main feature of it is its strongly<br />

vertical development. Strong vertically developed<br />

clouds are also called heap clouds.<br />

convective heat transfer Transfer of heat<br />

by mass movement, due to free or forced convection.<br />

The latter case is also referred to as<br />

advective heat transfer.<br />

convective instability Stratification instability<br />

caused by convective activities, i.e., the lower<br />

layer has higher moisture <strong>and</strong> becomes saturated<br />

first when being lifted, <strong>and</strong> hence cools<br />

thereafter at a rate slower than does the upper,<br />

drier portion, until the lapse rate of the whole<br />

layer becomes equal to the saturation adiabatic<br />

<strong>and</strong> any further lifting results in instability. In<br />

general, use ∂θsw<br />

∂Z<br />

< 0 or ∂θse<br />

∂Z<br />

< 0 as the cri-<br />

terion of the convective instability, where θsw<br />

<strong>and</strong> θse are pseudo-wet-bulb potential temperature<br />

<strong>and</strong> pseudo-equivalent potential temperature,<br />

respectively.<br />

convective scaling In the boundary layer,<br />

pure convective turbulence depends only on the<br />

thickness Hcon of the convectively well-mixed<br />

layer <strong>and</strong> the boundary buoyancy flux J o b [Monin<br />

<strong>and</strong> Obukhov, 1954]. Dimensional analysis provides<br />

the scaling relations as a function of Hcon<br />

<strong>and</strong> J o b by:<br />

Length Lcs ∼ Hcon<br />

Time τcs ∼ Hcon/wcs<br />

Velocity wcs ∼ (HconJ o b )1/3<br />

Diffusivity Kcs ∼ wcsHcon<br />

Dissipation of turbulent<br />

kinetic energy εcs ∼ J o b<br />

If convection is driven purely by heat fluxes (i.e.,<br />

J o b = gαFth/(cpρ)), further scaling relations for<br />

temperature are as shown in the table on page 86.<br />

convective turbulence If density increases<br />

at the top of a fluid (i.e., cooling, evaporation<br />

© 2001 by CRC Press LLC<br />

convergent plate boundaries<br />

of salty water at the surface, etc.) or if density<br />

decreases at the bottom of a fluid (i.e., warming<br />

from below, etc.), convective plumes (thermals<br />

for temperature) will set in <strong>and</strong> mix a progressively<br />

thicker boundary layer. Convective<br />

scaling allows the quantification of the relevant<br />

physical parameters of convection as a function<br />

of the boundary buoyancy flux Jo b <strong>and</strong> the thickness<br />

Hcon of the convectively unstable layer. See<br />

also penetrative convection.<br />

convergent boundary Plates are destroyed<br />

or severely deformed at convergent boundaries.<br />

Two types of convergent boundaries exist: subduction<br />

<strong>and</strong> collision. A subduction convergent<br />

boundary occurs when two plates composed of<br />

oceanic crust (thin, basalt composition) or an<br />

ocean plate <strong>and</strong> a continental plate (thick, more<br />

silicic composition) meet. At the ocean-ocean<br />

boundary, one of the oceanic plates dives down<br />

under the other plate. At an ocean-continent<br />

boundary, the oceanic plate is always subducted<br />

under the continental plate. The location where<br />

the first plate subducts under the second plate is<br />

characterized by a deep trough, called a trench.<br />

As the oceanic plate dives deeper into the Earth’s<br />

interior, the temperature rises <strong>and</strong> sediments<br />

which accumulated on the ocean floor begin to<br />

melt. This magma rises towards the surface<br />

<strong>and</strong> erupts on the overriding plate, creating the<br />

very explosive volcanos called stratovolcanos<br />

(or composite volcanos). Subduction boundaries<br />

are characterized by this explosive volcanism<br />

<strong>and</strong> earthquakes from a variety of depths<br />

(down to about 200 km). Japan is an example<br />

of an ocean-ocean subduction boundary, while<br />

the Cascade volcanos (including Mt. St. Helens)<br />

in the northwestern U.S. are an example of the<br />

ocean-continent subduction boundary. If both<br />

plates are composed of continental crust, neither<br />

plate is subducted. Instead the two plates crumple<br />

to form high mountain ranges, such as the<br />

Himalayas. This type of convergent boundary is<br />

called a collision boundary <strong>and</strong> is characterized<br />

by earthquakes but no volcanism. Convergent<br />

boundaries are believed to occur over the descending<br />

portions of convection cells within the<br />

Earth’s asthenosphere.<br />

convergent plate boundaries See convergent<br />

boundary.

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