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domination cireš Fr.: domination An act or instance of dominating. Verbal noun of → dominate. |
donor dahandé (#) Fr.: donneur In a semiconductor, an impurity which may induce electric conduction by providing free electrons. → acceptor; → impurity. M.E. donour, from O.Fr. doneur, from L. donator, from donare "to give as a gift," donum "gift," dare "to give," cognate with Pers. dâdan "to give," from PIE base *do- "to give." Dahandé "giver," from dâdan "to give," Mid.Pers. dâdan "to give," O.Pers./Av. dā- "to give, grant, yield," Av. dadāiti "he gives," Skt. dadâti "he gives," Gk. didomi "I give," PIE base *do- "to give." For L. cognates see above. |
donor star setâre-ye dahandé Fr.: étoile donneuse In a → binary system, a star whose gas is → accreted by a compact companion. The donor may be a → giant or a → supergiant with an enormously distended atmosphere and a significant → stellar wind, or a star filling its → Roche lobe in a → close binary. |
double Compton scattering parâkaneš-e Compton-e dotâyi Fr.: diffusion Compton double An electron-photon interaction that can be thought of as a → Compton scattering event associated with the production or destruction of an extra photon. → double; → Compton; → scattering. |
double refraction šekast-e dotâyi Fr.: double réfraction Formation of two refracted rays of light from a single incident ray; property of certain crystals, notably calcite. → double; → refraction. |
double vision dobini (#) Fr.: vision double Same as → diplopia. |
double-diffusive convection hambaz-e do paxši Fr.: An instability involving two layers of fluid with opposite gradients of properties. Same as → fingering instability. See also → salt finger. Double-diffusive instabilities commonly occur in any astrophysical fluid that is stable according to the → Ledoux criterion, as long as the entropy and chemical stratifications have opposing contributions to the dynamical stability of the system. They drive weak forms of convection, and can cause substantial heat and compositional → mixing. Two cases can be distinguished. In fingering convection, entropy is stably stratified (∇ - ∇ad < 0), but chemical composition is unstably stratified (∇μ < 0); it is often referred to as → thermohaline convection by analogy with the oceanographic context in which the instability was first discovered. In oscillatory double-diffusive convection, entropy is unstably stratified (∇ - ∇ad > 0), but chemical composition is stably stratified (∇μ > 0); it is related to semiconvection, but can occur even when the → opacity is independent of composition (P. Garaud, 2014, arXiv:1401.0928). |
doubly convex do-kuž Fr.: double-convexe |
doubly ionized dobâr yonidé (#) Fr.: deux fois ionisé An atom that has lost two of its external electrons, for example O++ ([O III]). |
draconic month mâh-e gowzahri (#), ~ gerehi (#) Fr.: mois draconitique The time interval between two successive passages of the Moon through its → ascending node, 27.212 220 days (27d 5h 5 m 35.8s). Draconic month is important for predicting → eclipses. Also called draconitic month, nodical month. Draconic, adj. of dragon, → Draco, referring to a mythological dragon for the following reason. Since an eclipse occurs when the Earth, the Sun, and a node are aligned and moreover the Moon is situated near the node, it was believed that a dragon that resided in the node swallowed the Sun or the Moon. → month. Mâh, → month. |
Draconids eždahâiyân Fr.: Draconides Two meteor showers with radiants in the constellation → Draco. One appears early in October and the other late in June. Draconids, from → Draco constellation + → -ids suffix denoting "descendant of, belonging to the family of." |
Drake equation hamugeš-e Drake Fr.: équation de Drake A probabilistic argument used to estimate the number of
→ intelligent, communicating
→ extraterrestrial civilizations in the
→ Milky Way galaxy. The Drake equation is: Frank Donald Drake (1930-); → equation. |
Drummond light nur-e Drummond Fr.: lumière de Drummond A very brilliant white light which is the ignited flame of a mixture of oxygen and hydrogen projected against a block of calcium oxide (lime). Also called limelight. First working version produced by Lieutenant of the Royal Engineers, upon the Ordnance Trigonometrical Survey of Ireland (1826). It was used at night as a substitute for solar light. It was first employed in a theater in 1837 and was in wide use by the 1860s, among which in photography. Named after Scottish engineer Thomas Drummond (1797-1840); → light. |
Dulong-Petit law qânun-e Dulong-Petit Fr.: loi de Dulong et Petit The product of the → specific heat and → atomic weight of most solid elements at room → temperature is nearly the same. In other words, specific heat is constant for a solid and independent of temperature. Experiment shows that at moderate temperatures this law is satisfied for → crystals with rather simple structure. However, the law fails for crystals with more complex structures. More specifically the law cannot explain the variation of specific heat with temperature. The specific heat drops to zero as the temperature approaches 0 K. This behavior is explained only with the quantum theory. → Debye model. Named after Pierre L. Dulong (1785-1838) and Alexis T. Petit (1797-1820), French chemists, who proposed the law in 1819. They collaborated in several important investigations, including studies of thermal expansion of gases and of liquids and the specific heats of substances; → law. |
duplication dotâyeš, dotâkard Fr.: duplication An act or instance of duplicating; the state of being duplicated. Verbal noun of → duplicate. |
duration pâyeš Fr.: durée Continuance in time; a period of existence or persistence; length of time during which anything continues. Noun of action from L. durare "to harden," → during. Pâyeš, noun of action from pâyidan, → last (v.). |
dust coagulation mâseš-e qobâr, roceš-e ~ Fr.: coagulation de la poussière A process of formation of → dust grains in → interstellar medium and → protoplanetary disks, in which randomly colliding aggregates may stick together. → dust; → coagulation. |
dust emission gosil-e qobâr Fr.: émission des poussières Thermal emission in infrared from interstellar → dust grains receiving photons. Dust grains absorb ultraviolet and visible light emitted by nearby stars and re-radiate in the infrared wavelengths. Since the infrared light is of lower energy than the ultraviolet/visible light, the difference goes into heating the dust grain. Typical temperatures for interstellar grains are tens of degrees Kelvin. |
dust obscuration tirešod pat qobâr Fr.: obscurcissement par la poussière The → absorption of → electromagnetic radiation from an astrophysical object by → dust grains associated with that object. → dust; → obscuration. Tiregi, → obscuration, pat, → by; qobâr, → dust. |
dynamical disruption gosixt-e tavânik Fr.: rupture dynamique The process whereby a → bound system, such as a → binary system or a → globular cluster, is broken apart. → dynamical; → disruption. |
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