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decretion disk gerde-ye vâbâl Fr.: disque de décrétion A disk that would form around a star when the star injects matter into a close orbit. This is in contrast to an → accretion disk, which transfers matter from outside to the star. The mass gets injected into the decretion disk by a not yet well-known mechanism, most probably a combination of → non-radial pulsation, fast rotation, and possibly small-scale → magnetic fields. See also → viscous decretion disk. |
decryption vânehâneš (#) Fr.: décryptage The process of restoring encrypted data back to the original information. See also → encryption and → decoding. |
deduction foruhâzeš Fr.: déduction 1) The act or process of deducting; something that is or may be deduced. Verbal noun from → deduce. |
deductive reasoning râyaneš-e foryhâzeši Fr.: raisonnement déductif Reasoning from the → general to the → particular (or from → cause to → effect). |
definition hedâreš Fr.: définition 1) The act or process of establishing some value or condition with precision. Verbal noun of → define. |
deflagration taškaft Fr.: déflagration A rapid → chemical reaction in which the → output of → heat is enough to enable the reaction to proceed and be accelerated without input of heat from another source. The effect of a true deflagration under confinement is an → explosion. See also: → detonation; → explosion. Verbal noun of → deflagrate. |
deflection vâcaft Fr.: déflexion The act or state of deflecting or the state of being deflected. Amount
of deviation. Verbal noun of → deflect. |
deflection angle zâviye-ye vâcaft Fr.: angle de déflexion 1) The angle by which a light ray is curved by the gravitational field of a massive body.
Einstein's general relativity predicts that a light
ray which tangentially grazes the surface of the Sun is deflected by
1''.7. This result was confirmed in 1919 when
the apparent angular shift of stars close to the limb of the Sun was
measured during a total solar eclipse. → deflection; → angle. |
deflection of light vâcaft-e nur Fr.: déflexion de la lumière The bending of a light ray under the gravitational effect of a massive body. → deflection angle. → deflection; → light. |
deformation vâdis, vâdiseš, vâdisâneš Fr.: déformation Altering in the size or shape of a body. See also → deformable. Verbal noun of → deform. |
defuzzification vâporzvâreš Fr.: défuzzification, concrétisation The process of producing a quantifiable result in a → fuzzy logic system, given → fuzzy sets and corresponding → membership functions. Defuzzification is the last step in a fuzzy logic system. After → fuzzy inferencing, the overall result is a → fuzzy value. This result should be defuzzified to obtain a final → crisp value. |
degree of ionization daraje-ye yoneš (#) Fr.: degré d'ionisation The number of electrons a neutral atom has lost in an ionizing physical process (radiation, shock, collision). In spectroscopy, the degree of ionization is indicated by a Roman numeral following the symbol for the element. A neutral atom is indicated by the Roman numeral I, a singly ionized atom, one which has lost one electron, is indicated by II, and so on. Thus O VI indicates an oxygen atom which has lost five electrons. → degree; → ionization. |
degree of polarization daraje-ye qotbeš Fr.: degré de polarisation The ratio of the intensity of polarized portion of light to the total intensity at a point in the beam. → degree; → polarization. |
dehumanization martugân zodâyi Fr.: déshumanisation The act or process or an instance of dehumanizing. Verbal noun of → dehumanize. |
deionization vâyoneš Fr.: désionisation Chemistry: A process in which all charged species are removed from
a solution. From → de- + → ionization. |
delayed neutrons notronhâ-ye derangidé Fr.: neutrons retardés Neutrons resulting from nuclear fission which are emitted with a measurable time delay. Delayed neutrons are responsible for the ability to control the rate at which power can rise in a reactor. → prompt neutrons. |
delayed supernova explosion oskaft-e bâderang-e abar-novâ, ~ ~ abar-now-axtar Fr.: explosion retardée de supernova A mechanism predicted by theoretical models of → supernova explosion that operates after the → supernova shock fails to deliver a → prompt supernova explosion. The delayed supernova explosion mechanism assumes that a few tenth of a second after the → iron core collapse, the supernova shock is stalled due to energy dissipation. The material between the → protoneutron star and the stalled shock is mainly disintegrated into neutrons and protons due to the high temperatures (a few MeV) in this region. As the → neutrinos coming from the protoneutron star run through this material, a fraction of the neutrinos are captured by the → nucleons, and their energy is deposited in the material. As a result, the material behind the shock is heated by the neutrinos. If this neutrino heating is efficient enough, the stalled shock can be reinvigorated to bring about a supernova explosion. |
deletion rušé Fr.: suppression 1) An act or instance of deleting. The state of being deleted. A deleted word, passage, etc. Verbal noun from → delete. |
delta function karyâ-ye delta Fr.: fonction delta Same as → Dirac function. |
Delta Orionis Deltâ Šekârgar Fr.: delta Orionis Same as → Mintaka. |
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