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DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

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saturation<br />

Satellite ephemeris, r<br />

Altimetric satellite<br />

h, Observed satellite altitude<br />

h DSSH<br />

h MSS<br />

r el , Reference ellipsoid height<br />

Earth’s center of mass<br />

Fundamental measurements of satellite altimetry.<br />

from the station, reflecting it from the prisms,<br />

<strong>and</strong> receiving the reflected laser beam. Since<br />

the location of the satellite can be determined<br />

independently, geodetic location of the station<br />

can be determined within an accuracy of several<br />

centimeters if the two-point distances are measured<br />

for at least three different locations of the<br />

satellite. Such observations are currently carried<br />

out at different stations in the world; one<br />

application is to measure the relative motion of<br />

tectonic plates. Satellite laser ranging is also<br />

used to provide information on Earth rotation<br />

<strong>and</strong> Earth orientation.<br />

saturation See current saturation.<br />

saturation adiabat A type of adiabatic process<br />

in movement of saturation moist air. Under<br />

the saturation adiabatic condition, when a saturated<br />

air parcel ascends, part of the vapor will<br />

condense to water or ice, <strong>and</strong> the air parcel will<br />

be still saturated. The latent heat released partly<br />

compensates the ascending adiabatic cooling,<br />

<strong>and</strong> the condensed water or ice remains in the<br />

saturated air parcel.<br />

saturation adiabatic lapse rate The adiabatic<br />

cooling rate of rising air parcel which is<br />

saturated, <strong>and</strong> in which condensation is taking<br />

place as it rises, so that the latent heat release<br />

moderates the adiabatic cooling, <strong>and</strong> causes the<br />

saturation adiabatic lapse rate to be less than<br />

the dry adiabatic lapse rate. The saturation adiabatic<br />

lapse rate is not a constant, <strong>and</strong> varies<br />

inversely with the temperature <strong>and</strong> somewhat<br />

with change of pressure. The difference between<br />

the saturation adiabatic lapse rate <strong>and</strong> dry<br />

adiabatic lapse rate is determined by the possibly<br />

released latent heat. Since the temperature at<br />

© 2001 by CRC Press LLC<br />

408<br />

higher level atmosphere is lower, the saturation<br />

adiabatic lapse rate has a smaller value at low<br />

level <strong>and</strong> larger value at high level which can<br />

approach or equal the dry adiabatic lapse rate.<br />

saturation vapor pressure The pressure exerted<br />

by the water vapor which is equilibrium<br />

with its condensed phase, which may be water<br />

or ice, the moist surface (or ice surface) saturation<br />

vapor pressure. In this state the same number<br />

of water molecules leave the water (ice) into<br />

the air as move from the air into the water (ice).<br />

Saturation vapor pressure is only a function of<br />

temperature. Its formula for water surface is<br />

E = E0 10 7.45t/(t+235)<br />

where E is saturation vapor pressure, E0 =<br />

6.1078 hPa, is the saturation vapor pressure at<br />

0 ◦ C, t is vapor temperature( ◦ C).<br />

The ice surface saturation vapor pressure is<br />

E = E0 10 9.5t/(t+265) .<br />

Saturn The sixth planet from the sun. Named<br />

after the Roman elder god of agriculture, Saturn<br />

has a mass M = 5.6841 × 10 29 g, <strong>and</strong> an<br />

equatorial radius of R = 60,330 km, giving it a<br />

mean density of 0.71 g cm −3 <strong>and</strong> a surface gravity<br />

of 1.08 that of Earth. Its rotational period is<br />

10 h 14 min. The rotation axis has an obliquity<br />

of 26.7 ◦ . The rapid rotation gives the planet an<br />

oblateness of 0.09. Saturn’s orbit around the sun<br />

is characterized by a mean distance of 9.54 AU,<br />

an eccentricity of e = 0.056, <strong>and</strong> an orbital inclination<br />

of i = 2.5 ◦ . Its sidereal period is 29.46<br />

years <strong>and</strong> its synodic period is 378 days. Its average<br />

albedo is 0.47 but its atmospheric temperature<br />

is determined by an internal heat source.<br />

At one bar the temperature is about 140 K <strong>and</strong><br />

increases inward. Saturn is a “gas giant” being<br />

composed primarily of hydrogen <strong>and</strong> helium <strong>and</strong><br />

is the least dense, most oblate planet in the solar<br />

system. Saturn has prominent rings composed<br />

of large particles <strong>and</strong> numerous moons including<br />

Pan, Atlas, Prometheus, P<strong>and</strong>ora, Epimetheus,<br />

Janus, Mimas, Enceladus, Tethys, Telesto, Calypso,<br />

Dione, Helene, Rhea, Titan, Hyperion,<br />

Iapetus, <strong>and</strong> Phoebe.<br />

scalar A function or physical property that<br />

depends only on the position <strong>and</strong> time at which it

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