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DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

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Ballerina model<br />

tosphere through lunar valleys. If only one bead<br />

is apparent, a “diamond ring effect” is produced.<br />

Ballerina model Shape of the heliospheric<br />

current sheet as proposed by H. Alfvén in the<br />

early 1970s. The wavy neutral line on the source<br />

surface is carried outwards by the solar wind,<br />

resulting in a wavy heliospheric current sheet<br />

that resembles the skirt of a dancing ballerina.<br />

The waviness of this current sheet is described<br />

by the tilt angle. See heliospheric current sheet,<br />

source surface, tilt angle.<br />

Balmer series The series of lines in the<br />

spectrum of the hydrogen atom which corresponds<br />

to transitions between the state with principal<br />

quantum number n = 2 <strong>and</strong> successive<br />

higher states. The wavelengths are given by<br />

1/λ =RH(1/4 − 1/n 2 ), where n = 3, 4,...<br />

<strong>and</strong> RH is the Rydberg constant for hydrogen.<br />

The first member of the series (n = 2 ↔ 3),<br />

which is often called theHα line, falls at a wavelength<br />

of 6563 Å. See Rydberg constant.<br />

banner cloud An altocumulus lenticularis<br />

cloud, (lenticular cloud) which forms on the lee<br />

side of the top of a mountain <strong>and</strong> remains a stationary<br />

feature with one edge attached to the<br />

ridge of the mountain.<br />

bar A unit of pressure, defined as 10 6<br />

dyne/cm 2 (10 5 N/m 2 ). The bar is commonly<br />

divided into 1000 mb. The pressure of atmosphere<br />

at sea level is about 1013 hPa = 1.013 bar.<br />

bar detectors Solid bars, made of metallic<br />

alloys, for detecting gravitational waves. The<br />

technology was pioneered by J. Weber. The sensitivity<br />

of h = 10 −18 (relative strain) has been<br />

reached in second-generation cryogenic detectors.<br />

At this level of sensitivity, no gravitational<br />

wave event has yet been reliably detected. See<br />

LIGO.<br />

barium release An experimental procedure<br />

near-Earth space physics, in which barium is<br />

evaporated by a thermite charge, usually in a<br />

sunlit region above the (denser) atmosphere,<br />

creating a greenish cloud. Barium atoms are<br />

rapidly ionized (within 10 sec or so), <strong>and</strong> the<br />

ions form a purple cloud, which responds to<br />

© 2001 by CRC Press LLC<br />

magnetic <strong>and</strong> electric fields <strong>and</strong> therefore often<br />

drifts away from the neutral one.<br />

The technique was pioneered by Gerhard<br />

Haerendel in Germany, <strong>and</strong> many releases have<br />

been conducted from rockets above the atmosphere,<br />

often with the barium squirted out by a<br />

shaped explosive charge. Typically releases are<br />

made after sunset or before sunrise, so that the<br />

rocket rises into sunlight but the clouds are seen<br />

against a dark sky. Effects of electric fields have<br />

been observed, striations like those of the aurora,<br />

even abrupt accelerations along field lines.<br />

Some releases have taken place in more distant<br />

space, notably an artificial comet in the solar<br />

wind, produced in 1984 by the AMPTE mission.<br />

Barnard’s star Star of spectral type M3.8,<br />

5.9ly distant with magnitude m = 9.5 <strong>and</strong> absolute<br />

magnitude M = 13.2; located at Right<br />

Ascension 17 h 58 m , declination +04 ◦ 41 ′ . Discovered<br />

in 1916 by E.E. Bernard, it has the<br />

largest known proper motion: 10.29 arcsec/year.<br />

Measurements by van de Kamp had suggested<br />

that there were perturbations of the motion corresponding<br />

to an associated planet, but recent<br />

observations using the Hubble space telescope<br />

have not confirmed this claim.<br />

baroclinic atmosphere or ocean An atmosphere<br />

or ocean in which the density depends<br />

on both the temperature <strong>and</strong> the pressure. In a<br />

baroclinic atmosphere or ocean, the geostrophic<br />

wind or current generally has vertical shear, <strong>and</strong><br />

this shear is related to the horizontal temperature<br />

or density gradient by the thermal wind relation.<br />

baroclinic instability A wave instability that<br />

is associated with vertical shear of the mean flow<br />

<strong>and</strong> that grows by converting potential energy<br />

associated with the mean horizontal temperature<br />

or density gradient.<br />

baroclinic wave Wave in the baroclinic flow.<br />

barotropic atmosphere or ocean An atmosphere<br />

(or ocean) in which the density depends<br />

only on the pressure. In the barotropic atmosphere<br />

or ocean, the geostrophic wind or current<br />

is independent of height.

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