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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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multiple ring basins<br />

all be possible). This can lead to severe amplitude<br />

fading, <strong>and</strong> hence signal distortion, because<br />

of the small time delays (up to 1 msec <strong>and</strong> more<br />

for several modes) in radio signals traveling by<br />

different modes. The effects of this form of multipath<br />

may be minimized by choosing a working<br />

frequency that is supported on fewer modes, <strong>and</strong><br />

by selecting antennas that favor one mode over<br />

others. A single ionospheric mode (e.g., 1-F<br />

mode) may encompass four separate paths: the<br />

ordinary <strong>and</strong> extraordinary paths <strong>and</strong> a high <strong>and</strong><br />

low ray for each of these polarizations. This<br />

situation is common near the maximum useable<br />

frequency for the circuit <strong>and</strong> time delays of the<br />

order of 0.5 msec are possible. See fading.<br />

multiple ring basins Very large impact<br />

basins often display a pattern of three or more<br />

complete or partial rings of mountainous materials.<br />

These multiple ring basins provide information<br />

on the thickness of the crust at the<br />

time the basin formed. Multiple ring basins<br />

are created by impact into a rigid surface layer<br />

(lithosphere) which overlies a more fluid layer<br />

(asthenosphere). If the crater resulting from<br />

the impact is smaller than the thickness of the<br />

lithosphere, a normal impact crater is produced.<br />

However, if the impact crater is greater than<br />

the thickness of the lithosphere, the asthenosphere<br />

can flow inward beneath the portion of<br />

the lithosphere which is pushed down by the<br />

impact. This flow exerts a drag force on the descending<br />

segment of the lithosphere, which can<br />

cause fracturing in the lithosphere surrounding<br />

the crater. The number of rings in a multi-ring<br />

basin is related to the thickness of the crust at<br />

the time of basin formation — fewer rings are<br />

produced in a thicker crust, while many rings<br />

indicate a relatively thin crust.<br />

multiple shock An earthquake composed of<br />

several spatially <strong>and</strong> temporally discontinuous<br />

© 2001 by CRC Press LLC<br />

326<br />

subevents. Most large earthquakes are multiple<br />

shocks. From detailed analysis of seismograms,<br />

we can find that an earthquake source fault does<br />

not spread continuously <strong>and</strong> smoothly, but exp<strong>and</strong>s<br />

intermittently <strong>and</strong> heterogeneously. This<br />

kind of rupture pattern is considered to reflect<br />

the inhomogeneous structure of a source region.<br />

mushy zone As a melt containing more than<br />

one component (e.g., a rock magma with diverse<br />

chemistry, or the fluid of the Earth’s outer<br />

core, which is thought to be composed of iron,<br />

nickel, <strong>and</strong> some lighter elements) is cooled, the<br />

composition of the first crystals to solidify are<br />

generally different from the bulk composition of<br />

the melt as a whole. As cooling continues, the<br />

chemical makeup of the material being solidified<br />

evolves, both because temperature of the melt<br />

is changing <strong>and</strong> because the chemical makeup<br />

of the remaining melt is itself changing (becoming<br />

more enriched in the material excluded from<br />

the first crystals). These factors also come into<br />

play at the boundary between the Earth’s inner<br />

core <strong>and</strong> outer core: Between the depths where<br />

a parcel of outer core fluid would start to crystallize<br />

<strong>and</strong> finish crystallizing, the boundary region<br />

may be a mixture of liquid <strong>and</strong> solid material,<br />

commonly referred to as a mushy zone. As neither<br />

the composition of the core nor the thermodynamic<br />

conditions at the inner core boundary<br />

are particularly well constrained, the existence<br />

<strong>and</strong> depth of the mushy zone are not known, but<br />

it may be a factor both for the seismic properties<br />

of the top of the inner core <strong>and</strong> the dynamic<br />

boundary conditions for the geodynamo at the<br />

base of the outer core. The crystallization of<br />

aqueous analogs reveals some of the nature of<br />

mushy zones: liquid circulates through the zone,<br />

creating organized structures such as channels<br />

called “chimneys”.

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