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DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

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decibel<br />

universe <strong>and</strong> . indicates the time derivative. This<br />

definition assumes an approximately isotropic<br />

universal expansion (as is observed). The quantity<br />

˙R is related to the Hubble parameter: H0 =<br />

˙R/R.<br />

decibel A dimensionless measure of the ratio<br />

of two powers, P1 <strong>and</strong> P2, that is equal to 10<br />

times the logarithm to the base 10 of the ratio<br />

of two powers (P1/P2). The units expressed this<br />

way are one-tenth of a bel <strong>and</strong> are referred to as<br />

decibels. The power P2 may be some reference<br />

power. For instance, in electricity, the reference<br />

power is sometimes taken as 1 milliwatt (abbreviated<br />

to dBm).<br />

declination In terrestrial magnetism, at any<br />

given location, the angle between the geographical<br />

meridian <strong>and</strong> the magnetic meridian; that is,<br />

the angle between true north <strong>and</strong> magnetic north<br />

is the declination. Declination is measured either<br />

east or west as the compass needle points<br />

to the east or west of the geographical meridian.<br />

East is taken as the positive direction. Lines of<br />

constant declination are called isogonic lines,<br />

<strong>and</strong> the one of zero declination is called the agonic<br />

line. See dip, magnetic. In astronomy, an<br />

angle coordinate on the celestial sphere corresponding<br />

to latitude, measured in degrees north<br />

or south of the celestial equator.<br />

decollement A near horizontal detachment<br />

zone between distinct bodies of rocks.<br />

deep(-focus) earthquake Earthquakes at<br />

depths ranging from about 300 to 700 km that<br />

occur along the Wadati–Benioff zone, which is<br />

inclined from a trench toward a continental side<br />

beneath the subduction zone of an oceanic plate.<br />

Fault plane solutions with down-dip compression<br />

are dominant. Since a deep(-focus) earthquake<br />

takes place under high-pressure conditions,<br />

where friction is large, it is difficult to<br />

explain its generation mechanism by frictional<br />

sliding processes such as those for a shallow<br />

earthquake. Recent laboratory experiments indicate<br />

that shear melting, a self-feedback system<br />

of phase transformations of olivine <strong>and</strong><br />

fault growth, <strong>and</strong> brittle fracturing due to pore<br />

pressure are possible generation mechanisms of<br />

deep(-focus) earthquakes.<br />

© 2001 by CRC Press LLC<br />

Deep Space 1 (DS1) A New Millennium<br />

spacecraft launched October 24, 1998. It is the<br />

first mission under NASA’s New Millennium<br />

Program to test new technologies for use on future<br />

science missions. Its objective is to test<br />

12 advanced technologies in deep space to lower<br />

the cost <strong>and</strong> risk to future science-driven missions<br />

that use them for the first time. Among<br />

these technologies are a xenon ion propulsion<br />

system (performing beyond expectations), autonomous<br />

navigation, a high-efficiency solar array,<br />

<strong>and</strong> a miniature camera/spectrometer. By<br />

December 1, 1998, DS1 had accomplished<br />

enough testing to satisfy the technology validation<br />

aspects of the minimum mission success<br />

criteria <strong>and</strong> is well on its way toward meeting<br />

maximum criteria.<br />

It carried out a flyby of the near-Earth asteroid<br />

1992 KD on July 28, 1998 at an altitude of<br />

10 km. The primary mission ended on September<br />

18, 1999. It is now on a new trajectory to<br />

encounter Comets Wilson–Harrington <strong>and</strong> Borrelly.<br />

Deep Space 2 Two microprobes that were<br />

onboard the Mars Polar L<strong>and</strong>er spacecraft<br />

launched on January 3, 1999 <strong>and</strong> lost in the<br />

l<strong>and</strong>ing on Mars on December 3, 1999. The primary<br />

purpose of the Mars Microprobe Mission<br />

was to demonstrate key technologies for future<br />

planetary exploration while collecting meaningful<br />

science data (thus, it was named Deep Space<br />

2). In this case, the scientific objectives were<br />

to determine if ice is present below the Martian<br />

surface; to characterize the thermal properties<br />

of the Martian subsurface soil; to characterize<br />

the atmospheric density profile; to characterize<br />

the hardness of the soil <strong>and</strong> the presence of any<br />

layering at a depth of 10 cm to 1 m. See Mars<br />

Microprobe, Deep Space 1.<br />

Deep Space Network (DSN) The NASA<br />

Deep Space Network is a world-wide network<br />

of large antennas with the principal function<br />

of maintaining communications with spacecraft<br />

beyond the moon’s orbit. The three main<br />

tracking complexes are in Goldstone, California<br />

(U.S.), near Canberra (Australia), <strong>and</strong> Madrid<br />

(Spain).

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