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direction angle zâviye-ye râstâ Fr.: angle de direction An angle made by a given vector and a coordinate axis. |
Dirichlet condition butâr-e Dirichlet Fr.: condition de Dirichlet One of the following conditions for a → Fourier series
to converge: Named after Peter Gustav Lejeune Dirichlet (1805-1859), German mathematician who made valuable contributions to → number theory, → analysis, and → mechanics; → condition. |
disallocation vâtesk Fr.: desallouation The act of disallocating or the state of being disallocated. |
discontinuity nâpeyvastegi (#) Fr.: discontinuité A break in sequence or continuity of anything.
→ Balmer discontinuity M.L. discontinuitas, from discontinuus, from → dis- + continuus, → continuous. Nâpeyvastegi, noun from nâpeyvasté "discontinuous," from nâ- "non, un-," → a-, + peyvasté, → continuous. |
discrete absorption component (DAC) hamne-ye daršami-ye gosasté Fr.: composante d'absorption discrète The rapid, systematic changes in the absorption parts of the → P Cygni profiles of the ultraviolet → resonance lines (Si IV, C IV, and N V) observed in a majority of massive → hot stars. DACs are typically seen to accelerate to the → blue wing of the profile over a few days, becoming narrower as they approach the → terminal velocity. → discrete; → absorption; → component. |
discrete transition gozareš-e gosasté Fr.: transition discrète A transition between two quantum-mechanical energy levels. See also → discrete spectrum. → discrete; → transition. |
discrimination vâkarbeš Fr.: discrimination 1) An act or instance of discriminating, or of making a distinction. Verbal noun of → discriminate. |
discussion bahs Fr.: discussion An act or instance of discussing; → consideration or → examination by → argument, → comment, etc., especially to explore solutions; informal debate (Dictionary.com). Verbal noun from → discuss. |
disintegration vâpâši, forupâši (#) Fr.: desintégration The breaking up of a body into fragments. For example, that of an unstable nuclei either spontaneously or as a result of bombardment by fast-moving particles, or the breaking up of a comet. Disintegration, verbal noun of disintegrate, from → dis- + → integration. Vâpâši, forupâši, from vâ-, frou-→ de- + pâši, noun of pâšidan→ disperse. |
disjunction vâjuheš Fr.: disjonction A → proposition of the form "A or B" (A ∨ B), where A and B are themselves propositions. A disjunction is → true when one or the other of its components (called → disjuncts) is true, and false otherwise. |
disk accretion farbâl-e gerde-yi, ~ pat geredé, ~ ~ disk Fr.: accrétion par disque An accretion process involving an → accretion disk. |
disk partition parkeš-e disk, ~ gerde Fr.: partition de disque A logical division of a hard disk that is treated as a separate unit by operating systems and file systems. |
disk population porineš-e gerdé, ~ disk Fr.: population disque Of a spiral galaxy, those stars that lie in a flattened disk and move in nearly circular orbits around its centre. They are Population I stars of all ages up to the age of the disk, but in general are younger than stars in → halo population. → disk; population, from L.L. populationem "a people, multitude," from populatio, from populare "to inhabit," from populus "people," related to plebes "the common people," cf. Gk. plethos "people, multitude, great number," from PIE base *pel- "to be full;" Mod.Pers. por "full," O.Pers. paru- "much, many," Av. pouru- "much, many," pərəna- "full," par- "to fill," Skt. puru-, Gk. polus, O.E. full "completely, full," from P.Gmc. *fullaz, O.H.G. fol, Ger. voll, Goth. full. Like Gk., Pers. uses the concepts of "multitude, many, full" to denote "people, group, herd, flock". The following examples are all terms derived from O.Pers. paru- "much, many," Av. par- "to fill," pouru- "much, many," pərəna- "full" (Mod.Pers. por "full"): literary Pers. bâré "herd, flock," parré "a rank or file of soldiers, a circular disposition of troops," Lori, Qâyeni bor "group, tribe, herd," Torbat-Heydariyeyi, Qomi borr "heap, bundle, group," Qomi borreh "group, assemblage of people," Pashtu parrak "flock, herd," Urdu para "flock, herd," Lârestâni baila "group, tribe," Tabari balik "herd, flock." With this introduction, porineš "population," verbal noun of porinidan "to populate," infinitive of porin "populous," from por "mutitude, many, full" + -in attribution suffix. |
disk truncation kolkard-e disk, ~ gerdé Fr.: troncature de disque In models of magnetized → accretion disks, the process whereby the disk is disrupted at a radius where the → magnetic pressure overcomes the → ram pressure of the accreted material. This occurs at a distance typically 3-7 stellar radii, below the → corotation radius. → disk; → truncation. |
dispersion pâšeš (#) Fr.: dispersion 1) The resolution of white light into its component wavelengths,
either by → refraction or by → diffraction.
Dispersion is actually an effect in which radiations having → different
wavelengths travel at different speeds in the medium. Since
the → angle of refraction
of each radiation vary as a function of
its → wavelength, the component waves deviate from each other. Verbal noun of → disperse. |
dispersion curve xam-e pâšeš Fr.: courbe de dispersion A graph displaying the variation of the → refractive index of a substance against the wavelength of the electromagnetic wave passing through the substance. → dispersion; → curve. |
dispersion equation hamugeš-e pâšeš Fr.: équation de dispersion An equation representing the variation of → refractive index as a function of → wavelength; for example → Cauchy's equation and → Sellmeier's equation. → dispersion; → equation. |
dispersion measure andâze-ye pâšeš Fr.: mesure de dispersion A parameter used in radio astronomy which describes the amount of dispersion in a radio signal due to its passage through an intervening plasma. It is proportional to the product of the interstellar electron density and the distance to the source. → dispersion; → measure. |
dispersion relation bâzâneš-e pâšeš Fr.: relation de dispersion An equation that describes how the → angular frequency, ω, of a wave depends on its → wave number, k. For the simplest of waves, where the speed of propagation, c, is a constant, ω(k) = ck. If the → phase velocity depends on k, that is for a dispersive medium, the function ω(k) is nonlinear. → dispersion; → relation. |
disqualification vâcunâyeš Fr.: disqualification An act or instance of disqualifying; the state of being disqualified. → disqualify; → -tion. |
<< < "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 > >>