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recursive definition hedâreš-e bâzâyeši Fr.: définition récursive Math.: A definition of a function from which values of the same function can be calculated in a finite number of steps. In mathematical logic and computer science, a recursive definition is used to define an object in terms of itself. An example is the → factorial: n! = n*(n-1)! → recursive; → definition. |
red horizontal branch star setâre-ye sorx-e šâxe-ye ofoqi Fr.: étoile rouge de la branche horizontale A star found on the red part of the → horizontal branch. According to theoretical models, these stars result from the evolution of stars with a mass around 0.8 Msun, higher than that giving rise to → BHB stars. Upon helium burning in their cores, the remnant envelope of the red giant collapses. → red; → horizontal; → branch; → star. |
reddening function karyâ-ye sorxeš Fr.: fonction de rougissement The normalized interstellar extinction at a given wavelength. It is defined by f(λ) = A(λ)/A(Hβ) - 1, where A(λ) is the extinction at the given wavelength and A(Hβ) the extinction at Hβ, with f(Hβ) = 0. It is used to → de-redden observed fluxes: I(λ)/I(Hβ) = F(λ)/F(Hβ).10c(Hβ).f(λ), where I represents the flux in the absence of extinction and F the observed flux affected by extinction, c(Hβ) being the → reddening coefficient. |
redshift space distortion cowlegi-ye fazâ-ye sorx-kib Fr.: distorsion dûe aux vitesses particulières sur la ligne
de visée The distortion observed in → redshift space of → galaxy clusters caused by peculiar velocities of the members (→ peculiar velocity). In a perfectly homogeneous → Friedmann-Lemaitre Universe the redshifts would accurately measure radial distances from the observer, and the mapping from real space to redshift space would simply be an identity. In an inhomogeneous Universe the peculiar velocities associated with any inhomogeneous structure will introduce a distortion in this mapping (N. Kaiser, 1987, MNRAS 227, 1). See also: → fingers of God, → Kaiser effect. → redshift; → space; → distortion;. |
redshift-distance relation bâzâneš-e sorxkib-durâ Fr.: relation décalage vers le rouge-distance The correlation, first established by E. Hubble, between the cosmological recession velocities of galaxies and their distances. |
reduced Planck constant pâyâ-ye Planck-e bâzhâzidé Fr.: constante de Planck réduite The → Planck constant divided by 2π and denoted ħ, pronounced h-bar. Also called the → Dirac constant. Reduced, p.p. of → reduce; → Planck's constant. |
reduced Planck's constant pâyâ-ye Planck-e bâzhâzidé Fr.: constante de Planck réduite |
reduction bâzhâzeš Fr.: réduction 1) In → data processing, the transformation of data from
a "raw" form to some usable form. Verbal noun of → reduce. |
reflection bâztâb (#) Fr.: réflexion The return of radiation after striking a surface, without change in wavelength. If the surface is smooth, reflection is regular, otherwise it is diffuse. → diffuse reflection; → specular reflection. Verbal noun of → reflect. |
reflection coefficient hamgar-e bâztâb (#) Fr.: coefficient de réflexion The ratio given by the → amplitude (or energy) of a reflected wave divided by the amplitude (or energy) of the incident wave. → reflection; → coefficient. |
reflection factor karvand-e bâztâb Fr.: facteur de réflexion The ratio of total flux that is reflected from a surface to the incident flux. Also called reflectance, reflectivity. → reflection; → factor. |
reflection nebula miq-e bâztâbi Fr.: nébuleuse par réflexion A type of nebula that is visible from its reflection of starlight. Bright stars near reflection nebulae emit light into the region that is reflected by the large amount of dust there. The size of the dust grains causes blue light to be reflected more efficiently than red light, so these reflection nebulae frequently appear blue in color. → reflection; → nebula. |
refraction šekast (#) Fr.: réfraction 1) Optics: The change of direction which a beam of light undergoes as it
enters a medium of different → refractive index. From L.L. refractionem (nominative refractio) "a breaking up," from L. refractus, p.p. of refringere "to break up," from re- "back" + combining form of frangere "to break," from PIE base *bhreg- "to break" (cf. Goth. brikan, O.E. brecan "to break;" Lith. brasketi "crash, crack"). Šekast, past stem of šekastan "to break, split;" Mid.Pers. škastan "to break;" Av. scind-, scand "to beak, cleave;" Proto-Iranian *skand- "to break, cleave;" PIE sken- "to cut off." |
refutation vâkuteš Fr.: réfutation The act or process of refuting. |
regeneration bâz-âzâneš Fr.: regénération 1) Act of regenerating; state of being regenerated. → re-; → generation. |
region nâhiyé (#) Fr.: région A large, usually continuous segment of a surface or space; area. → H II region. M.E., from Anglo-Fr. regioun; O.Fr. region, from L. regionem (nominative regio) "district, country, direction, boundary," from regere "to direct," cognate with Pers. râst, → right. Nâhiyé, loan from Ar. nâHiyat. |
registration barnuseš Fr.: enregistrement 1) The act or instance of registering. |
regression 1) pasraft (#); 2) vâyâzi (#), vâyâzeš (#) Fr.: régression 1) Astro.: → retrograde motion. From L. regression-, from regress-, stem of regredi "to go back," from → re- "back" + gradi "to step, walk." 1) → retrograde. |
regression analysis anâlas-e vâyâzeš Fr.: analyse de régression A statistical technique used to determine the values of parameters for a function that best fits a given set of data. → regression, → analysis. |
regression coefficient hamgar-e vâyâzeš (#) Fr.: coefficient de régression The slope of the straight line that most closely relates two correlated variables. → regression, → coefficient. |
<< < "no abe acc act aff ama ani ant aps ast atm aut bar bic Boh bou cal car cel che cla col com com Com con con con con con con con con con con con con Cor cor cot cul de- dec dem des dif dil dir dis dom dyn Edd ele ele emi equ Eve exc exp fac fin for fre fuz gen Glo gra gra Ham hel hor hyd ign inc inf Inf int Int int ion irr jum Lag lea lig lin Lor Lyo mag mat met min Mon moo NaC neg New New non non non nul obs one opt Ori oxi par per per phl pho pla Pla pol pos pre pro pro pse qua rad rad rea rec reg rel res ret rot Ryd sci sec sec sep sim Soc son spe sta Ste Sto sub sup syn the Tho top tra Tro unc vec vio Was Wil Zhe > >>