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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 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. |
demodulation vâ-degarâhangeš Fr.: démodulation In communications, the process of recovering the original information from a modulated signal wave. → modulation. → de- + → modulation |
demonstration padiš, padišeš Fr.: démonstration 1) The → act or → circumstance
of proving or being → proved conclusively, as
by → reasoning or a show of → evidence. Verbal noun of → demonstrate. |
demystication vâšârdeš Fr.: démystification The removal of mystery or confusion surrounding a topic or idea. |
denomination ânâmeneš Fr.: groupe, catégorie, unité; dénomination 1) A name or designation. Verbal noun of → denominate. |
dense core mass function karyâ-ye jerm-e maqze-ye cagâl Fr.: fonction de masse des cœurs denses |
density fluctuation oftâxizhâ-ye cagâli Fr.: fluctuations de densité In the early Universe, localized enhancements in the density of either matter alone or matter and radiation. According to models, very small initial fluctuations (less than 1 percent) can lead to subsequent formation of galaxies. → density; → fluctuation. |
density-bounded H II region nâhiye-ye H II-ye cagâli karânmand Fr.: bornée par la densité An → H II region which lacks enough matter to absorb all → Lyman continuum photons of the → exciting star(s). In such an H II region a part of the ionizing photons escape into the → interstellar medium. See also → ionization-bounded H II region. |
depletion tisâyeš Fr.: déplétion General: The act or process of depleting. The state of being depleted. Noun from → deplete |
depletion layer lâye-ye tisâyeš Fr.: couche de déplétion The region of a semiconductor in which the density of mobile carriers is too low to neutralize the fixed charge density of donors and acceptors. |
depletion time zamân-e tisâyeš Fr.: temps de déplétion The time it takes for a given → chemical species to be reduced below a significant level of → abundance in a → compound or → object. |
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