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obrit
Fr.: aubrite
A type of → achondrite meteorite composed mostly of the magnesium silicate mineral → enstatite (Mg2Si2O6). The group is named for the small Aubres → meteorite that fell near Nyons, France, on Sep. 14, 1836. Outside Antarctica only about 10 aubrites are known, mostly the result of witnessed falls. Aubrites make up only 0.14% of all known meteorites in our terrestrial meteorite collection. See also: From Fr. Aubres, a commune in the Drôme department in southeastern France; + → -ite. |
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elektron-e Auger
Fr.: électron d'Auger
An electron that is emitted when an electron from a higher → energy level falls into a → vacancy in an inner shell, according to the → Auger-Meitner effect. The process usually occurs when the atom is bombarded with high energy electrons. If the collision ejects an inner-shell electron, an electron from a higher level will quickly drop to this lower level to fill the vacancy. Most of the time, the energy is released in the form of a photon. But sometimes the energy is transferred to another electron, which is ejected from the atom. See also: → Auger-Meitner effect; → electron. |
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oskar-e Auger-Meitner
Fr.: effet Auger-Meitner
The → emission of an → electron when an → atom transits to a less → excited state. More specifically, → ionization of an atom by a very energetic photon can bring about the ejection of an inner electron of the atom. Consequently, the atom becomes unstable and rapidly undergoes a → spontaneous transition. As a result, an outer electron moves inward and fills the → vacancy produced in the inner orbit. Energy conservation requires that this transition be accompanied by the emission of a photon or a peripheral electron. The latter is called the → Auger electron. Knowing the electron energy leads us to characterize the atom from which it was ejected. This effect is used, in the Auger spectroscopy, to analyze the surface compositions of materials. See also: This effect was discovered in 1923 Lise Meitner (1878-1968) and in 1925 independently by Pierre Auger (1899-1993). |
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Arrâbe-rân, Gardune-rân
Fr.: Cocher
The Charioteer. A conspicuous northern constellation lying midway between
→ Perseus and → Ursa Major
and in a region crossed by the → Milky Way.
The brightest star is → Capella. Etymology (EN): L. auriga “a charioteer, driver,” from aureæ “bridle of a horse” + agere “set in motion, drive, lead.” Etymology (PE): Arrâberân “charioteer,” from arrâbé “chariot, cart”
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ušé
Fr.: aurore
A phenomenon consisting of luminous colorful arcs, rays, and streamers that appear in the Earth’s upper atmosphere during the night with the greatest frequency in the northern and southern polar magnetic zones. This → non-thermal radiation is caused by the emission of light from atoms excited by electrons accelerated along the planet’s magnetic field lines at the magnetic poles. Fluorescent emission from atomic oxygen at 5557 Å results in a greenish glow, and there is a weaker effect from the red line at 6300 Å. Blue and purple colors are emitted by atomic and molecular nitrogen. Etymology (EN): L. Aurora, the Roman goddess of dawn, akin to Av. uš-, ušah- “dawn,” Skt. usas-, usah- “dawn,” Gk. eos “dawn,” Lith. ausra “dawn,” O.E. east “east,” PIE *ausus- “dawn,” from *aus- “to shine.” Etymology (PE): Ušé, from Av. uš-, ušah-, as above. |
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uše-ye daštari
Fr.: aurore australe
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uše-ye hudari
Fr.: aurore boréale
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uše-yi
Fr.: auroral
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gosil-e uše-yi
Fr.: émission aurorale
The → electromagnetic radiation emitted in planetary atmospheres involving the → aurora phenomenon. |
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xatt-e uše-yi
Fr.: raie aurorale
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zonâr-e uše-yi
Fr.: zone aurorale
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râstin šomârdan
Fr.: authentifier
Etymology (EN): From L.L. authenticus, from Gk. authentikos “original, primary, at first hand,” from authent(es) “one who does things himself,” from aut-, from autos “self, one’s own,” of unknown origin,
Etymology (PE): Râstin “genuine, authentic,” from râst “right, true; just, straight”
(Mid.Pers. râst “true, straight, direct;” O.Pers. rāsta-
“straight, true,” rās- “to be right, straight, true;” Av. rāz-
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râstinšomâri, râstin-âzmâyi
Fr.: authentification
Computers: The process by which a user’s identity is checked within the network to ensure that the user has access to the requested resources. See also: Verbal noun of → authenticate. |
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dâtâr
Fr.: auteur
Etymology (EN): M.E. auctour, from O.Fr. autor, from L. auctor, “creator, enlarger, founder, master, leader,” literally “one who causes to grow,” from auctus, p.p. of augere “to increase,” from PIE root aug- “to increase”. Etymology (PE): Dâtâr, from Mid.Pers. dâtâr/dâdâr “creator,” from
Av. and O.Pers. dâtâr “creator,” from dâ-
“to create, make, appoint,” Skt. dhatr
“author, creator, preserver, bearer.” |
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dâtârgânvarz
Fr.: autoritaire
Of, relating to, or characterized by strict obedience to authority. See also: From authorit(y), → authority, + suffix -arian. |
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dâtârgânvarzi
Fr.: autoritarisme
See also: → authoritarian; → -ism. |
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dâtârgânmand
Fr.: qui fait autorité, digne de foi
See also: From authorit(y), → authority, + suffix -ative. |
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dâtârgân
Fr.: autorité
Etymology (EN): → author; → -ity. Etymology (PE): Dâtârgân, from dâtâr, → author, + -gân, on the model of xodâygân “a great lord.” |
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Fr.: paternité
See also: → author. |
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xod- (#)
Fr.: auto-, aut-
Etymology (EN): Gk., from autos “self, one’s own,” of unknown origin. Etymology (PE): Xod-, from xod “self,” Av. hva- “self, own.” |
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xod-hambâzâneš
Fr.: autocorrélation
Etymology (EN): Autocorrelation, from → auto- “self” + → correlation. Etymology (PE): Xod-hambâzâneš, from xod- “self” + hambâzâneš, |
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karyâ-ye xod-hambâzâneš
Fr.: fonction d'autocorrélation
A mathematical function that describes the correlation between two values of the same variable at different points in time. See also: → autocorrelation; → function. |
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xod-hambâzângar
Fr.: autocorrélateur
In radio astronomy, a spectrograph which correlates the signal with itself with various time delays, and extracts the frequency spectrum of the signal. → correlator. Etymology (EN): Autocorrelator, agent n. from → autocorrelate + → -or. Etymology (PE): Xod-hambâzângar, agent n. from xod-, → auto-,
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xod-hamvartâyi
Fr.: autocovariance
The → covariance of a → time series overt time. See also: → auto-; → covariance. |
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karyâ-ye xod-hamvartâyi
Fr.: fonction d'autocovariance
The autocovariance function (ACF) is defined as the sequence of
covariances of a stationary process. A mathematical function that expresses the autocovariance of a series in terms of the interval of separation. See also: → autocovariance; → function. |
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xodrâhbar, râhbar-e xodkâr
Fr.: autoguideur
An electronic equipment used to automatically guide a telescope during long exposures. Etymology (EN): Autoguider from → auto- “self” + guider, from O.Fr. guider “to guide, lead, conduct,” from Germanic origin; akin to O.E. wltan “to look after” witan “to know,” akin to O.H.G. wizzan “to know,” L. videre “to see,” Gk. eidenai “to know,” idein “to see,” Av. vaêd- “to know,” Skt. veda “knowledge; finding.” Etymology (PE): Xodrâhbar from xod-, → auto + râhbar “guide,” from râh “way” + bar, from bordan “to lead.” |
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xodrâhbord, râhbord-e xodkâr
Fr.: autoguidage
The act or process of guiding a telescope automatically. See also: → autoguider. |
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xodkâr (#)
Fr.: automatique
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durbin-e šidsanjik-e xodkâr, teleskop-e ~ ~
Fr.: télescope photométrique automatique
A telescope developed to perform photometric observations automatically. See also: → automatic; → photometric; → telescope. |
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xod-rixtmandi
Fr.: automorphisme
An → isomorphism between an → object and itself. |
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xoddât
Fr.: autonome
See also: Adjective from → autonomy. |
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xoddâti
Fr.: autonomie
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pâyiz (#)
Fr.: automne
The season of the year between summer and winter; it begins in the northern hemisphere at the → autumnal equinox and ends at the → winter solstice. Etymology (EN): O.Fr., from L. autumnus, a word probably of Etruscan origin. Etymology (PE): Pâyiz, from Mid.Pers. pâdiz or pâtez, from Proto-Iranian *pâti-z(a)ya- “near winter,” from pâti “near” + *z(a)ya- “winter,” compare with Av. zyan- or zyam- “winter” (Skt. heman, Gk. xeimon, L. hiems). |
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hamugân-e pâyizi
Fr.: équinoxe d'automne
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hamugân-e pâyizi
Fr.: équinoxe d'automne
One of the two points where the → ecliptic crosses the → celestial equator. At the autumnal equinox the Sun appears to be moving across the equator from the northern celestial hemisphere to the southern celestial hemisphere. The instant of the event. |