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dissipative system râžmân-e eftâli Fr.: système dissipatif A → dynamical system which undergoes energy → dissipation. Such a system gives rise to → irreversible processes, associated with a time-asymmetric evolution of observable quantities. → dissipative; → system. |
dissociate vâhazidan Fr.: dissocier General: To separate from association of any kind. Verbal form of → dissociation. |
dissociation vâhazeš Fr.: dissociation General: An act or instance of dissociating; the state of being dissociated. From → dis- + (as)sociation, → association. |
dissociation energy kâruž-e vâhazeš Fr.: énergie de dissociation Energy required to dissociate a molecule. → dissociate. → dissociation; → energy. |
dissociative vâhazeši Fr.: dissociatif Of, relating to, or tending to produce → dissociation. Adj. of → dissociate. |
dissociative recombination bâzmiyâzeš-e vâhazeši Fr.: recombinaison dissociative A process where a positive molecular ion recombines with an electron, and as a result it dissociates into two neutral products. For example, AB^{+} + e^{-}→ A + B, where e^{-} is an electron, AB^{+} is a diatomic or polyatomic molecular ion, and A and B are the neutral fragmentation products. Dissociative recombination is the dominant recombination process in planetary ionospheres and interstellar clouds. → dissociative; → recombination. |
dissolution vâluyeš Fr.: dissolution Chemistry: The process by which a solid, gas, or liquid is dispersed homogeneously in a gas, solid, or a liquid. Verbal noun of → dissolve. |
dissolve vâluyidan Fr.: dissoudre To make a solution of, as by mixing with a liquid; pass into solution. From L. dissolvere "to loosen up, break apart," from → dis- "apart" + solvere "to loose, loosen, untie," from PIE *se-lu-, from reflexive pronoun *swe- + base *leu- "to loosen, divide, cut apart" (cf. Gk. lyein "to loosen, release, untie," Skt. lunati "cuts, cuts off," lavitram "sickle," O.E. leosan "to lose," leas "loose." Vâluyidan, infinitive from stem vâlu(y)-, from vâ-→ de- + lu, variant of Mod.Pers. las "loose," lâ "slit, cut," luš "torn," lok "torn, piece," lâc "open, wide open" (→ analysis), from PIE *leu- "to loosen, divide, cut apart." |
dissymmetry nâhmâmuni Fr.: dissymétrie Absence or lack of symmetry |
distal ejecta ešânâk-e dur Fr.: éjecta distaux Geology: Impact ejecta found at distances more than 5 crater radii from the rim of the source crater. |
distance apest, durâ (#), duri (#) Fr.: distance 1) The separation/length in space/time between two things/events. M.E., from O.Fr., from L. distantia "a standing apart," from distantem (nominative distans) "standing apart, separate, distant," pr.p. of distare "to stand apart," from → dis- "apart, off" + stare "to stand," (cf. Mod.Pers. istâdan "to stand," O.Pers./Av. sta- "to stand, stand still; set," Skt. sthâ- "to stand," Gk. histemi "put, place, weigh," stasis "a standing still"). Apest, literally "standing apart," from apa- prefix denoting
"separation, away, off," → dis-, + est variant of
ist, present stem of istâdan, to stand," as above;" cf.
Choresmian bst "to stand apart," from *apa- + st-
"to stand," → stand. |
distance function karyâ-ye apest Fr.: fonction de distance Same as → metric. |
distance modulus peymun-e apest Fr.: module de distance The difference between the → apparent magnitude (m) of a star or galaxy and its → absolute magnitude (M). It is given by m - M = 5 log d - 5, where d is the distance in → parsecs. For an object that is 10 pc away, the distance modulus is zero. |
distance to the horizon apest-e ofoq Fr.: distance à l'horizon The distance separating an observer and the → apparent horizon of the place. Neglecting the → atmospheric refraction, it is given by: d = (2Rh)^{1/2}, where R is the radius of the Earth and h is the observer's height. This can be approximated to: d (km) = 3.57(h)^{1/2} for a typical value of R = 6378 km. The atmospheric refraction, however, makes the thing more complex, depending on the temperature and density variations along the line of sight. Generally, refraction pushes the apparent horizon about 10% farther. |
distort cowlé kardan, cowlidan Fr.: déformer, altérer To twist awry or out of shape; make crooked or deformed (Dictionary.com). From L. distortus, p.p. of distorquere "to distort," from → dis-, + torquere "to twist." Cowlé "distorted, crooked, bent," variants [Mo'in] kowlé, kal, kil, Lori cowel, Laki hoval, hol, Malâyeri caval, hol, Tabari, Aftari val, Mid.Pers. xwahl "bent, crooked;" PIE base *klei- "to lean, incline" from which is also derived Gk. klinein "to cause to slope, slant, incline," L. clinare "to bend," → declination. |
distortion cowlegi (#), cowleš Fr.: distorsion, déformation 1) Extent to which a system, optical, acoustic, or electronic, fails to reproduce
accurately at its output the characteristics of the input. Verbal noun of → distort. |
distribute vâbâžidan (#) Fr.: distribuer 1) (v.tr.) To divide and dispense in portions; to disperse through a space or
over an area. Distribute, from L. distributus p.p. of distribute "deal out in portions," from → dis- + tribuere "to pay, assign, allot," from tribus "tribe." Vâbâžidan, infinitive of vâbâž, from vâ-→ dis- + bâž "tribute, toll, impost," from Mid.Pers. bâj, bâž "tribute, tax," baxtan "to distribute," baxt "luck, fate," O.Pers. bāji- "tribute, tax," Av. bag- "to distribute, divide, allot," cf. Skt. bhaj- "to share, distribute, apportion," Gk. phagein "to eat (to have a share of food)"; PIE base *bhag- "to share out, apportion;" → division. |
distribution vâbâžeš (#) Fr.: distribution An act or instance of distributing; the state or manner of being distributed; something that is distributed. → binomial distribution, → Bose-Einstein distribution, → brightness distribution, → chi-square distribution, → cumulative distribution function, → distribution function, → Gaussian distribution, → Gibbs canonical distribution, → lognormal distribution, → Maxwell-Boltzmann distribution, → normal distribution, → Poisson distribution, → power-law distribution, → probability distribution, → spectral energy distribution. Verbal noun of → distribute |
distribution function karyâ-ye vâbâžeš Fr.: fonction de distribution A function that gives the relative frequency with which the value of a statistical variable may be expected to lie within any specified interval. For example, the Maxwellian distribution of velocities gives the number of particles, in different velocity intervals, in a unit volume. → distribution; → function. |
distributive vâbâžeši Fr.: distributif Characterized by or relating to → distribution. → distributive law. → distibution; → -ive. |
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