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expansion parameter pârâmun-e sopâneš Fr.: paramètre d'expansion A → scale factor that relates the size of the Universe R = R(t) at time t to the size of the Universe R0 = R(t0) at time t0 by R = aR0. The expansion parameter represents the history of expansion of the Universe. |
expectation bayuseš Fr.: espérance, attente Statistics: Same as → mathematical expectation, → expected value. From L. expectare "to await, hope," from → ex- "thoroughly" + spectare "to look," from → specere "to look at," → -scope. Bayusesš, verbal noun of bayusidan "to expect;" Mid.Pers. pyws- "to hope for, desire" (prefixed *pati-); O.Pers. vasiy "at will, greatly, utterly," vašna- "will, favor;" Av. vas- "to will, desire, wish, long for," vasəmi "I wish," vasna- "will, favor," ušti- "desire, wish, will," vasô, vasə "at one's will." This word is extant in several Mod.Pers. dialects, Tabari vessen "to wish, desire," Gilaki vâssan "to wish, desire," vâsti "desire," Kurd. wistin "to desire, wish," Lâri avessa "to desire," colloquial Tehrâni vâsé "for" (Mid.Pers. vasnâd "because"); cf. Skt. vaś- "to wish, want, desire," váśa- "wish, desire," vasēna "for, because;" Gk. ekon "voluntary;" PIE base *uek- "to wish." |
explanation ostâheš Fr.: explication 1) The act or process of explaining. Verbal noun of → explain. |
explicit function karyâ-ye ostâhi Fr.: fonction explicite The most usual form of a function in which the dependent variable (written on the left hand side of the Same as → equality sign) is expressed directly in terms of independent variables written on the left (on the right hand side). See also → implicit function. |
exploration puyeš (#) Fr.: exploration 1) An act or instance of exploring or investigating; examination. Verbal noun of → explore. |
explosion oskaft Fr.: explosion The sudden and violent release of mechanical, chemical, or nuclear energy from a confined space which creates a heat wave that travels at → subsonic speeds. → detonation; → deflagration; → implosion. Verbal noun of → explode. |
exponential equation hamugeš-e nemâyi Fr.: équation exponentielle An equation in which unknowns appear as exponents. Examples: 23x + 1 = 32. → exponential; → equation. |
exponential function karyâ-ye nemâyi Fr.: fonction exponentielle A function in the form of y = bx defined for every → real number x, with positive base b > 1. → exponential; → function. |
exposition osneheš Fr.: exposition 1) The act of setting forth information or a viewpoint. Verbal noun of → expose. |
expression zohâveš Fr.: expression 1) The act or an instance of expressing. |
extension ostaneš (#) Fr.: extension 1) An act or instance of extending; the state of being extended. Verbal noun of → extend. |
externalization boruneš Fr.: extériorisation Verbal noun of → externalize. → externalize + → -tion. |
extinction xâmuši (#) Fr.: extinction 1) Dimming of light by an intervening medium (the Earth's atmosphere or the interstellar medium).
It is usually due to both scattering and absorption. Noun of extinct, from L. extinctus, p.p. of extinguere "to quench, wipe out," from → ex- "out" + stinguere "to quench," from PIE base *steig- "to prick, stick, pierce;" cf. Mod.Pers. tiz, tež, tig, tej, tij, tiq "sharp;" Av. tiγra- "pointed," tiγray- "arrow;" → deblur. Xâmuši, noun of xâmuš "extinguished; silent," Mid.Pers. xâmôš "silent;" cf. Skt. amrs- "to bear patiently." |
extinction coefficient hamgar-e xâmuši Fr.: coefficient d'extinction Gradient of apparent magnitude with air mass. → extinction; → coefficient. |
extinction correction aršâyeš-e xâmuši Fr.: correction d'extinction In → photometric calibration, the correction for energy loss undergone by radiation due to the → atmospheric extinction. Extinction correction is done using → standard stars observed at different → airmasses. → extinction; → correction. |
extinction curve xam-e xâmuši Fr.: courbe de l'extinction interstellaire A graph representing the variation of the → interstellar extinction against → wavelength. Usually it displays the → normalized values of extinction as a function of (the → inverse) of the wavelength (in → microns). See, e.g., Sandage & Mathis, 1979, Ann. Rev. Astron. Astrophys. 17, 73. → extinction; → curve. |
extinction stars setâregân-e xâmuši Fr.: étoiles d'extinction Stars specifically observed at selected air masses in view of determining the atmospheric extinction coefficients. → extinction; → star. |
extraction barhanješ Fr.: extraction 1) The act of extracting or the condition of being extracted. |
extrapolation borunyâbeš (#) Fr.: extrapolation Predicting the value of unknown data points by projecting a function beyond the range of known data points. Verbal noun of → extrapolate. |
Faber-Jackson relation bâzâneš-e Faber-Jackson Fr.: relation Faber-Jackson An empirical power-law correlation between the luminosity (L) and the velocity dispersion of stars (σ) in the center of a elliptical galaxies. The original relation can be expressed mathematically as: L ∝ σγ, where the index γ is observed to be approximately equal to 4, but depends on the range of galaxy luminosities that is fitted. → Tully-Fisher relation. After the astronomers Sandra M. Faber and Robert Earl Jackson, who first noted this relation in 1976 (ApJ 204, 668); → relation. |
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