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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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electromagnetic penetration depth) complicates<br />

somewhat the interpretation (e.g., the Meissner<br />

effect) in usual condensed matter terms.<br />

See Abelian Higgs model, conducting string,<br />

Nielsen–Olesen vortex, spontaneous symmetry<br />

breaking, winding number.<br />

wolf number An historic term for the sunspot<br />

number.<br />

work In Newtonian mechanics, the product<br />

of an applied force <strong>and</strong> the displacement in the<br />

direction of the force.<br />

work W= F · d = |F||d| sinθ,<br />

where θ is the angle between the force <strong>and</strong> the<br />

displacement.<br />

Work has units of Joules: 1 Joule =<br />

1 Newton·meter, or of ergs: 1 erg = 1 dyne·cm.<br />

worldsheet charge See electric regime<br />

(string).<br />

worldsheet geometry See fundamental tensors<br />

of a worldsheet.<br />

wormhole A connection between two locations<br />

in space-time. This involves a curvature of<br />

space-time which acts as a bridge between two<br />

distant points that may lie in the same region or<br />

in different regions <strong>and</strong> which are otherwise inaccessible<br />

to each other. There is currently no<br />

evidence of their existence. See curved spacetime,<br />

Einstein–Roser bridge.<br />

© 2001 by CRC Press LLC<br />

WWSSN (World-Wide St<strong>and</strong>ardized Seismograph Network)<br />

wrinkle ridges Features that occur in the<br />

northern plains of Mars, probably of volcanic<br />

origin. They are classically described as consisting<br />

of a rise, a broad arch, <strong>and</strong> an associated<br />

narrow sinuous ridge. They may be segmented<br />

to form an “en echelon” arrangement.<br />

Detailed analysis shows that almost all wrinkle<br />

ridges mark a regional elevation offset <strong>and</strong> so are<br />

asymmetrical. Dimensions are ≈10 km wide,<br />

≈100 m high, with a regional elevation offset<br />

range between ≈10 to 1000 m where detectable.<br />

W Ursa Majoris (W UMa) See contact binary.<br />

WWSSN (World-Wide St<strong>and</strong>ardized Seismograph<br />

Network) In 1960, three-component<br />

Press–Ewing type seismographs <strong>and</strong> shortperiod<br />

Benioff type seismographs with identical<br />

properties were deployed at about 120 stations<br />

throughout the world by U.S. Coast <strong>and</strong> Geodetic<br />

Survey (USCGS), mainly aiming at detection<br />

of underground nuclear tests. This world-wide<br />

seismograph network is called WWSSN. Seismic<br />

waveforms recorded by the seismograph network<br />

have contributed substantially to research<br />

on the source process of large earthquakes <strong>and</strong><br />

structure of the Earth’s interior using surface<br />

waves. In the 1970s, digital recording type seismograph<br />

networks began to be deployed. To<br />

date, there are IDA, SRO, DWWSSN, RSTN,<br />

<strong>and</strong> GEOSCOPE as seismograph networks deployed.<br />

Recently, principal observation stations<br />

of WWSSN have been moved to IRIS (Incorporated<br />

Research Institutions for Seismology).<br />

519

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