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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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diurnal motion<br />

the non-periodic variation caused by synoptic<br />

situations (such as advection processes). The<br />

strength of diurnal variation is related to location,<br />

stronger in continental areas <strong>and</strong> weaker in<br />

maritime areas, e.g., the strongest diurnal variation<br />

region is the Tibetan Plateau. The diurnal<br />

range in equatorial areas exceeds the annual<br />

variation in average temperature. More strictly,<br />

diurnal pertains to occurrences during the day,<br />

as opposed to nocturnal occurrences; diel occurrences<br />

are those that happen once per day.<br />

diurnal motion Apparent motion of objects<br />

on the celestial sphere due to the rotation of<br />

Earth from west to east, which causes objects<br />

to appear to rise in the east <strong>and</strong> set in the west<br />

daily.<br />

divergence Branching off or moving in different<br />

directions. Also denotes a mathematical<br />

operation; the divergence of a vector u is denoted<br />

by ∇ ·u.<br />

divergence law for irradiance See Gershun’s<br />

law.<br />

divergence theorem Also called Gauss’ theorem:<br />

<br />

<br />

B ·n dA = ∇·B dV<br />

A<br />

with V being a volume enclosed by surface A<br />

<strong>and</strong> n is a unit normal toA. Used, for instance, to<br />

convert between integral <strong>and</strong> differential forms<br />

of Maxwell’s equations.<br />

divergent boundary In tectonics, two plates<br />

moveapartfromeachotheratadivergentboundary.<br />

Magma moves up from the Earth’s asthenosphere<br />

at the divergent boundary. The magma<br />

rises to the surface, where it cools <strong>and</strong> solidifies<br />

as the volcanic rock basalt. Continued<br />

magma ascent forces the newly formed basaltic<br />

crust to move to the sides as the process repeats.<br />

Thus, divergent boundaries are areas where new<br />

crust is formed <strong>and</strong> where the plates move apart.<br />

Divergent boundaries are characterized by volcanism<br />

(quiet eruptions with very fluid lavas)<br />

<strong>and</strong> shallow earthquakes. Divergent boundaries<br />

are believed to occur over the uprising portions<br />

of convection cells within the Earth’s astheno-<br />

© 2001 by CRC Press LLC<br />

V<br />

sphere. The Mid-Atlantic Rift <strong>and</strong> the East<br />

African Rift Valley are examples of divergent<br />

boundaries.<br />

divergent plate boundary See divergent<br />

boundary, seafloor spreading.<br />

diversity reception Often, a radio circuit will<br />

have many different possible paths between the<br />

transmitter <strong>and</strong> receiver. There may be differences<br />

in the quality of the service on these paths<br />

<strong>and</strong> the quality may vary in time, space, <strong>and</strong> frequency.<br />

Diversity methods seek to exploit these<br />

differences. In the simplest form, signals on two<br />

different paths may be received <strong>and</strong> the maximum<br />

signal selected. More complex diversity<br />

systems may make use of redundancy between<br />

signals collected from several paths. See ionospheric<br />

radio propagation path.<br />

dividedbar Thenameofanapparatususedto<br />

measure thermal conductivities of disk-shaped<br />

rock samples. Two metal, usually brass, heads<br />

with circular cross-sections are maintained at<br />

different constant temperatures. Rock samples<br />

with known <strong>and</strong> unknown thermal conductivities<br />

are s<strong>and</strong>wiched in between. The heat flux<br />

q through the axis (z) of the system is determined<br />

from the measured temperature gradient<br />

dT/dz across the rock sample of known thermal<br />

conductivityλk from Fourier’s law of heat conduction.<br />

The thermal conductivity of the other<br />

sample is then given by this heat flux <strong>and</strong> the<br />

measured temperature gradient across it. See<br />

conductive heat transfer.<br />

D-layer The D-layer is the lowest ionospheric<br />

layer at heights between 60 <strong>and</strong> 85 km.<br />

In contrast to the other ionospheric layers, it is<br />

still inside the mesosphere. Ionization is primarily<br />

due to energetic particles of solar <strong>and</strong> galactic<br />

origin <strong>and</strong> some UV lines which penetrate deep<br />

into the atmosphere, such as the Lyman-α-line.<br />

The main constituent is NO, which results from<br />

a combination of atomar oxygen O <strong>and</strong> molecular<br />

nitrogen N2. The layer can be described<br />

very well by a Chapman profile. Due to the<br />

high densities, free electrons are rare <strong>and</strong> ion<br />

clusters <strong>and</strong> negative ions form instead. Polar<br />

cap absoptions (PCAs) <strong>and</strong> sudden ionospheric<br />

disturbances (SID) strongly modify this layer.

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