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angular velocity tondâ-ye zâviye-yi Fr.: vitesse angulaire A measure of the angular displacement per unit time. Of a particle traveling on a circular path or a rotating body, the ratio of the angle traversed to the amount of time it takes to traverse that angle: ω = dθ/dt. For a rigid body, all lines in it rotate through the same angle in the same time, and the angular velocity is the characteristic of the body as a whole. The angular velocity is related to the linear velocity by the equation v = rω, where r is the distance of the point from the rotation axis. → vector angular velocity. |
anisoplanicity anizobirâhigi Fr.: anisoplanicité The departure from → isoplanicity. → an-; → isoplanicity. |
annularity halqevâri Fr.: annularité The maximum phase of an → annular eclipse during which the Moon's entire disk is seen silhouetted against the Sun. Annularity is the period between second and → third contact during an annular eclipse. It can last from a fraction of a second to a maximum of 12 minutes 29 seconds (F. Espenak, NASA). |
anomalous luminosity effect oskar-e tâbandegi-ye nâsân Fr.: effet luminosité anormale Discrepant luminosity classes derived for the same → Am star when different criteria are used. Lore specifically, a luminosity criterion may indicate a → giant star, wheras another criterion indicates a → supergiant. → anomalous; → luminosity; → effect. |
aridity kamâbi (#) Fr.: aridité A measure of the degree to which a climate lacks effective moisture. Aridity, noun from → arid. Kamâbi, noun from amâbi, → arid. |
Aristarchus' inequality nâhamugi-ye Aristarchus Fr.: inégalité d'Aristarque Put in modern notation, if α and β are acute angles and if β <α, then sin α / sin β <α / β < tan α / tan β. Aristarchus probably used this inequality to show that the Sun is between 18 and 20 times as far from the Earth as the Moon is. Aristarchus of Samos (c.310-c.230 BC); → inequality. |
asperity zafti Fr.: aspérité 1) Roughness or unevenness of surface. M.E. asperite, from O.Fr. asperité "difficulty, painful situation," from L. asperitas, from asper "rough, harsh," of unknown origin. From zaft "thick, gross, rude," (Steingass, Dehxodâ), + noun suffix -i. |
associativity âhazandegi Fr.: associativité Of or relating to association; state of being associative. → associative + → -ity. |
asymptotic velocity tondâ-ye nâhamsâvi Fr.: vitesse asymptotique For → stellar winds, same as → terminal velocity. → asymptotic; → velocity. |
authority dâtârgân Fr.: autorité 1) The power to determine, adjudicate, or otherwise settle issues or
disputes; jurisdiction; the right to control, command, or determine (Dictionary.com). Dâtârgân, from dâtâr, → author, + -gân, on the model of xodâygân "a great lord." |
average velocity tondâ-ye miyângin Fr.: vitesse moyenne The ratio of the displacement (Δx) of a particle, as it moves from point A to point B, to the corresponding time interval: v = Δx/Δt. |
Balmer discontinuity nâpeyvastegi-ye Bâlmer Fr.: discontinuité de Balmer An abrupt decrease in the intensity of the continuum at the limit of the → Balmer series of hydrogen (at about 3650 Å), caused by the energy absorbed when electrons originally in the second → energy level are ionized. Same as → Balmer jump. → Balmer; → discontinuity. |
baroclinic instability nâpâydâri-ye fešâršibi Fr.: instabilité barocline 1) A type of instability occurring within a rapidly → rotating star
where non-axisymmetric motions can separate surfaces of constant pressure from
→ equipotential surfaces. → baroclinic; → instability. |
baroclinicity fešâršibi Fr.: baroclinie The state of stratification in a fluid in which surfaces of constant pressure do not coincide with those of constant density, but intersect. Where baroclinicity is zero, the fluid is → barotropic. Same as baroclinity. → baroclinic; → -ity. |
barotropic instability nâpâydâri-ye fešârgard Fr.: instabilité barotrope A hydrodynamical instability that arises when the horizontal → shear gradient becomes very large. Barotropic instabilities grow by extracting kinetic energy from the mean flow field. → barotropic; → instability. |
Bell's inequality nâhamugi-ye Bell Fr.: inégalité de Bell Any of a large number of inequality relations developed to study the → hidden variable hypothesis suggested in the → EPR paradox. Using Bell's inequalities, the → Aspect experiment showed that no local hidden variable theory can make predictions in agreement with those of quantum mechanics. If, in a measurement, the inequality is violated, the measurement is in agreement with the predictions of the quantum theory. If the equality is satisfied, it suggests that a classical, causal, and local model is adequate to explain the outcome of the measurements. See also → quantum entanglement. John Stewart Bell (1928-1990); → inequality. |
Big Bang singularity takini-ye Big Bang Fr.: singularité du Big Bang A hypothetical state of → infinite energy density representing an infinite → gravitational field and infinite → space-time curvature. The singularity arises from using Einstein's theory of → general relativity concerning gravity. We know, however, that when the density and heat become extremely large, quantum physics of gravity becomes important. Yet Einstein's equations ignore quantum effects. In other words, in certain extreme conditions, Einstein's equations do not apply. → Big Bang; → singularity. |
bimodality domodi Fr.: bimodalité The quality or state of being → bimodal. |
binarity dorini Fr.: binarité The quality or condition of being binary. |
biodiversity zistgunâguni Fr.: biodiversité The → variety of → plant and → animal → species in a particular → environment. |
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