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DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

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heard as “whistles” with steadily falling pitch<br />

that lasts for a few tenths of a second (short<br />

whistlers) to several seconds (long whistlers).<br />

Whistlers are generated by lightning sources or<br />

atmospherics. The electromagnetic energy produced<br />

in the lightning sources travels along the<br />

Earth’s magnetic lines in the ionosphere almost<br />

without any attenuation to the other hemisphere.<br />

A part of this energy in the other hemisphere<br />

is reflected back along the same magnetic lines<br />

producing whistlers in a radio receiver in the<br />

hemisphere of origin, <strong>and</strong> another part enters<br />

the ionosphere <strong>and</strong> propagates in the Earth –<br />

ionosphere waveguide mode to the hemisphere<br />

of origin producing short whistlers. Since the<br />

losses in the ionosphere are small, many echoes<br />

may occur in what is known as an “echo” train<br />

beforetheyarelostinthebackgroundnoise. The<br />

changing pitch indicates that the path time “t”<br />

along the magnetic line of force is related to the<br />

frequency “f” by the dispersion relation<br />

D = t √ f<br />

where D is the dispersion <strong>and</strong> may range from<br />

about 10 to 200 √ sec. Since t will depend on<br />

the line of force along which the energy travels<br />

<strong>and</strong> the electron density which decreases with<br />

height, D is found to increase with increase in<br />

electron density. The whistler properties can be<br />

explainedbytheapplicationofthemagnetoionic<br />

theory to low frequency wave propagation in the<br />

ionosphere. Whistlers are used as a research<br />

tool to study the electron density <strong>and</strong> associated<br />

properties in the Earth’s magnetosphere.<br />

whistler waves A low-frequency plasma<br />

wave which propagates parallel to the magnetic<br />

field at a frequency less than the electroncyclotron<br />

frequency. Whistler waves are circularly<br />

polarized, rotating in the same sense as the<br />

electrons in the plasma. Whistlers are so-named<br />

because of their characteristic audio frequency<br />

tone.<br />

white dwarf A star supported entirely by<br />

electron degeneracy pressure, formed by contraction<br />

when internal fusion energy sources are<br />

exhausted.<br />

white hole The time-reverse of a black hole,<br />

i.e., a region of the spacetime that can only eject<br />

© 2001 by CRC Press LLC<br />

Wien’s displacement law<br />

matter <strong>and</strong> radiation but can accrete none of it.<br />

A white hole would be a naked singularity, with<br />

a past event horizon, which does not shield it<br />

from our view. Light from a white hole would<br />

be blue-shifted. A white hole can be imagined<br />

as a Big Bang taking place in a limited volume<br />

of space, while the remaining part of the space<br />

already exists. White holes are natural in inhomogeneous<br />

models of the universe — they are<br />

places where the Big Bang occurs later <strong>and</strong> was<br />

still going on while it had already been completed<br />

elsewhere. Since literally everything can<br />

come out of these holes, thus strongly violating<br />

causality, a cosmic censorship principle has<br />

been invoked to avoid their existence in our universe.<br />

There is currently no evidence that they<br />

exist. See black hole, future/past event horizon,<br />

naked singularity.<br />

white light Solar radiation integrated over the<br />

visible portion of the spectrum (4000 to 7000 Å)<br />

to produce a broad-b<strong>and</strong> (white light) signal.<br />

Best used to observe the photosphere <strong>and</strong> also in<br />

eclipse or coronagraph observations of the solar<br />

corona.<br />

white light flare A major flare in which compact<br />

regions become visible in white light. Such<br />

flares are usually strong X-ray, radio, <strong>and</strong> particle<br />

emitters.<br />

Widmanstä tten pattern A distinctive pattern<br />

of crystal faces found in nickel-rich iron meteorites.<br />

When an iron-nickel mixture is heated<br />

to near melting <strong>and</strong> slowly cooled, two types of<br />

crystals are formed: a nickel-poor phase (kamacite)<br />

<strong>and</strong> a nickel-rich phase (taenite). The<br />

pattern formed by the growth of these two crystal<br />

phases can be seen when the meteorite is polished<br />

<strong>and</strong> etched with acid.<br />

Wien’s displacement law (Wien law) The<br />

wavelength λm at which the maximum radiation<br />

intensity (ergs/sec/cm 2 /steradian/wavelength<br />

interval) of a black body radiator occurs is inversely<br />

proportional to the absolute temperature<br />

T , so:<br />

Tλm = C,<br />

where C is a constant, equal to 0.28978 cm-K.<br />

515

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