29.03.2013 Views

DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

polycyclic aromatic hydrocarbons (PAHs)<br />

entirely on spherical surfaces, while the poloidal<br />

potentialP can only be zero on a spherical surface<br />

if the radial component of v is also zero on<br />

that surface. It can further be shown that the curl<br />

of the toroidal term is poloidal, <strong>and</strong> the curl of<br />

the poloidal term is toroidal.<br />

polycyclic aromatic hydrocarbons (PAHs)<br />

Flat molecules made primarily of carbon atoms<br />

arranged in the graphitic form; in hexagons so<br />

that their skeleton looks like chicken wire. Pollutants<br />

on Earth, they are commonly observed in<br />

meteorites, <strong>and</strong> are widely distributed throughout<br />

the galaxy, accounting for 15 to 20% of the<br />

galactic carbon. The UV absorption of these stable<br />

molecules may be the source of the diffuse<br />

interstellar b<strong>and</strong>s, <strong>and</strong> their emission in the IR<br />

is seen towards H II <strong>and</strong> star forming regions.<br />

polynya An area of the ocean that persists<br />

in being either partially or totally free of sea ice<br />

under surface conditions where the sea would be<br />

expected to be ice covered. Polynyas appear in<br />

winter when air temperatures are well below the<br />

freezing point of sea water <strong>and</strong> are bordered by<br />

water that is covered with ice. They are typically<br />

rectangular or elliptical in shape <strong>and</strong> tend to recur<br />

in the same regions of the Arctic <strong>and</strong> Southern<br />

Ocean. The size of polynyas can range from<br />

a few hundred meters to hundreds of kilometers.<br />

Polynyas form via two mechanisms, which<br />

often operate simultaneously. In the first, ice<br />

is continually formed <strong>and</strong> removed by winds,<br />

ocean currents, or both. The latent heat of fusion<br />

of the ice provides the energy necessary to<br />

maintain open water. The second mechanism<br />

requires oceanic heat to enter a region in quantities<br />

sufficient to prevent local ice formation.<br />

Polynyas are sites for active brine formation,<br />

which may affect the local water density structure<br />

<strong>and</strong> current field, which in turn modifies<br />

large-scale water masses. They are also an interface<br />

for gas exchange between the ocean <strong>and</strong><br />

atmosphere in polar regions. The large sensible<br />

heat fluxes (along with fluxes due to evaporation<br />

<strong>and</strong> longwave radiation) tend to dominate regional<br />

heat budgets. They are also of biological<br />

interest because their regular occurrence makes<br />

them important habitats.<br />

© 2001 by CRC Press LLC<br />

372<br />

polytropic process In thermodynamics, any<br />

process that can be described by the statement<br />

pV n = constant (for some fixed n). Here p<br />

is the pressure in the experiment, <strong>and</strong> V is the<br />

volume of the sample. Thus n= 0 yields p=<br />

constant (constant pressure process), n = ∞<br />

yieldsV= constant (constant volume process).<br />

For a process at constant temperature in an ideal<br />

gas, n = 1, <strong>and</strong> for a constant entropy process<br />

in an ideal gas, n is the ratio of specific heat at<br />

constant pressure to that at constant volume.<br />

poorly graded sediment A sediment with<br />

grain sizes that have a small st<strong>and</strong>ard deviation.<br />

Most grains are very close to the median grain<br />

size.<br />

Pop I See Population I.<br />

Pop II See Population II.<br />

Population I Stars having a composition similar<br />

to the sun. See also main sequence star,<br />

metallicity.<br />

Population II Stars significantly deficient,<br />

relative to the sun, in elements beyond helium.<br />

See also metallicity, main sequence star.<br />

pore fluid pressure ratio The ratio of pore<br />

fluid pressure to lithostatic pressure, defined as<br />

λ = pf − ps<br />

pl − ps<br />

where pf is the pore fluid pressure, ps is pressure<br />

at the surface, <strong>and</strong> pl is the lithostatic pressure,<br />

the weight of the rock column above containing<br />

the pore fluid.<br />

poroelastic medium A porous medium that<br />

deforms elastically under loading. A poroelastic<br />

medium can be envisaged to consist of an<br />

elastic matrix frame hosting an interstitial fluid.<br />

The elastic moduli of the matrix frame are defined<br />

under the drained condition, a situation in<br />

which the pore fluid freely enters <strong>and</strong> exits the<br />

medium such that the pore fluid pressure does<br />

not affect matrix deformation. In a poroelastic<br />

medium, strain <strong>and</strong> effective stress of the matrix<br />

frame are governed by its constitutive law<br />

(such as Hooke’s law for infinitesimal strain),

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!