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piston piston (#) Fr.: piston A disk or cylindrical part tightly fitting and moving within a cylinder, either to compress or move a fluid collected in the cylinder, as air or water, or to transform energy imparted by a fluid entering or expanding inside the cylinder, as compressed air, explosive gases, or steam, into a rectilinear motion usually transformed into rotary motion by means of a connecting rod (Dictionary.com). From Fr. piston, from M.Fr. piston "large pestle," from O.It. pistone "a piston," from pestare "to pound," from L.L. pistare, from pistare "to pound." |
Planck distribution vâbâžeš-e Planck Fr.: distribution de Planck The distribution of radiation with wavelength for a blackbody, given by → Planck's radiation law. → Planck; → distribution. |
Pleistocene Pleistosen Fr.: Pléistocène The earliest Epoch of the Quaternary Period, beginning about 1.6 million years ago and ending 10,000 years ago. Commonly known as the "Ice Age," a time with episodes of widespread continental glaciation. From Gk. pleisto(s), superlative of Polys "much," cognate with Pers. por, → full, + -cene from Gk. kainos "new, recent." |
Poisson distribution vâbâžeš-e Poisson Fr.: distribution de Poisson A → probability function that characterizes → discrete → random events occurring independently of one another within some definite time or space. It may be regarded as an approximation of the → binomial distribution when the number of events becomes large and the probability of success becomes small. The Poisson distribution is expressed by: f(x) = (λxe-λ)/x!, where λ is the mean number of successes in the interval, e is the base of the → natural logarithm, and x is the number of successes we are interested in. Named after Siméon Denis Poisson (1781-1840), French mathematician, who developed the application of Fourier series to physical problems and made major contributions to the theory of probability and to the calculus of variations; → distribution. |
polar distance durâ-ye qotbi Fr.: distance polaire The angular distance of an object from a celestial pole. It is equal to 90° minus the object's declination. |
political scientist kârâhikdân Fr.: spécialiste en sciences politiques A person who studies the structure and theory of government and seeks practical and theoretical solutions to political problems. Kârâhikdân, literally "politics scientist," from kârâhik, → politics, + dân "knower," present stem of dânestan, → science. |
power-law distribution vâbâžeš bâ qânun-e tavâni Fr.: distribution en loi de puissance For a → random variable X, any → distribution which has the form: P(X ≥ x) = (k/x)α, where x is a value in the range defined for X, k > 0 is a parameter termed location parameter, and α > 0 is the → slope parameter. → power; → law; → distribution. |
principle of relativistic causality parvaz-e bonârmandi-ye bâzânigi-mand Fr.: principe de la causalité relativiste One consequence of the theory of → special relativity, according to which no two events separated by a distance greater than their separation in time multiplied by the → speed of light may have a → causal influence on each other. Violation of this principle leads to → paradoxes, such as that of an → effect preceding its → cause. → principle; → relativistic; → causality. |
probability distribution vâbâžeš-e šavânâyi Fr.: distribution de probabilité The function that describes the range of possible values that a random variable can attain and the probability that the value of the random variable is within any (measurable) subset of that range. → probability; → distribution. |
proper distance apest-e saré Fr.: distance propre A distance between two nearby events in the frame in which they occur at the same time. It is the distance measured by a ruler at the time of observation. Hence, for a cosmological time t, Dproper = DC . a(t), where DC is the → comoving distance, and a(t) is the → scale factor. In the present epoch a = a(tobs) = 1, and Dproper = DC. |
proper motion distance durâ-ye jonbeš-e saré Fr.: distance mouvement propre The distance derived from the → proper motion of an object. If an object has a known → transverse velocity u, and has an observed angular motion of dθ/dt, then the proper motion distance is defined as: d = u/(dθ/dt). |
realist 1) hasyâgerâ, hasyâbâvar; 2) hasyâmand Fr.: réaliste 1) A person who tends to view or represent things as they really are; an adherent of
→ realism. |
realistic hasyâmand Fr.: réaliste 1) Interested in, concerned with, or based on what is real or practical. From → real + -istic, from L. -isticus, Gk. -istikos, from -ikos, → -ic. |
redshift space distortion cowlegi-ye fazâ-ye sorx-kib Fr.: distorsion dûe aux vitesses particulières sur la ligne
de visée The distortion observed in → redshift space of → galaxy clusters caused by peculiar velocities of the members (→ peculiar velocity). In a perfectly homogeneous → Friedmann-Lemaitre Universe the redshifts would accurately measure radial distances from the observer, and the mapping from real space to redshift space would simply be an identity. In an inhomogeneous Universe the peculiar velocities associated with any inhomogeneous structure will introduce a distortion in this mapping (N. Kaiser, 1987, MNRAS 227, 1). See also: → fingers of God, → Kaiser effect. → redshift; → space; → distortion;. |
redshift-distance relation bâzâneš-e sorxkib-durâ Fr.: relation décalage vers le rouge-distance The correlation, first established by E. Hubble, between the cosmological recession velocities of galaxies and their distances. |
register 1) barnus; 2) barnusidan Fr.: 1) registre; 2) enregistrer 1a) A book in which records of acts, events, names, etc., are kept;
a list or → record of such acts, events, etc. M.E. registre, from M.Fr., from O.Fr. registre and directly from M.L. registrum, alteration of L.L. regesta "list, matters recorded," noun use of L. regesta, from regestus, p.p. of regerere "to record; retort," literally "to carry back, bring back" from → re- "back" + gerere "carry, bear." Barnus, from bar- "on, upon, up," → on-, + nus "to write;" cf. Kurd. (Sor.) nus, nusen "to write;" Lori nisane "to write;" variants of nevis-, neveštan, → write. |
registration barnuseš Fr.: enregistrement 1) The act or instance of registering. |
registry barnusé Fr.: registre 1) The act of registering; registration. → register + -y. |
relativist bâzâni-bâvar Fr.: relativiste An adherent or advocate of relativism. From → relative + -ist a suffix of nouns. Adj. from → relativism. |
relativistic bâzânigimand, bâzânivar Fr.: relativiste 1) Physics: Relating to the → relativity theory. From → relativist + → -ic. |
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