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theory of relativity negare-ye bâzânigi Fr.: théorie de la relativité Any of the two theories put forward by Albert Einstein: → special relativity (1905) and → general relativity (1916). → theory; → relativity; |
thermal conductivity hâzandegi-ye garmâyi Fr.: conductivité thermale In → thermal conduction, the amount of heat passing across unit area per unit time and per unit → temperature gradient. → thermal; → conductivity. |
thermoelectricity damâbarq (#) Fr.: thermo-éléctricité The electricity produced by heat or temperature difference in a conductor. → thermo- + → electricity. |
total gravity gerâni-ye hamâk Fr.: gravité totale In a → rotating star, the sum of the → gravitational, → centrifugal, and → radiative accelerations. See also → effective gravity. |
totality hamâki Fr.: totalité The period during a → solar eclipse when the → Sun is completely blocked by the → Moon. Totality for a → lunar eclipse is the period when the Moon is in the complete → shadow of the → Earth. For a solar eclipse totality can last from only several fractions of a second to a theoretical maximum of 7m 31s, depending on the → distance from the Moon to the Earth. For a lunar eclipse totality can last up to 1h 47m, also depending on the distance from the Moon to the Earth and on its → passage through the shadow. See also → totality path. |
totality path pah-e hamâki, gozargâh-e ~ Fr.: ligne de totalité Of a → solar eclipse, the path of the → umbra across the → Earth. The totality path is usually about 100 km across, but under the most favorable conditions, when the → Moon is at its nearest → distance to Earth and the Earth is at its farthest distance from the Sun, the umbra can have a diameter of about 270 km. |
transition probability šavânâyi-ye gozareši Fr.: probabilité de transition The probability that a quantum-mechanical system will make a transition from a given initial state to a given final state. → transition; → probability. |
transverse velocity tondâ-ye tarâgozar Fr.: vitesse transverse Same as → tangential velocity. → transverse; → velocity. |
triangle inequality nâhamugi-ye sebari Fr.: inégalité triangulaire 1) A theorem according to which any side of a triangle is always shorter than the sum of the
other two sides. → triangle; → inequality. |
triviality zabi Fr.: trivialité The quality or state of being → trivial; something trivial. |
turbidity târi (#) Fr.: turbidité 1) Meteo.: A measure of vertical extinction of solar radiation in the
atmosphere. Turbidity is directly related to aerosol concentrations in the
tropospheric and stratospheric layers. → visibility. |
ubiquity visp-bâšandegi, visp-bâši, visp-bâšâyi Fr.: ubiquité, omniprésence The state or capacity of being everywhere, especially at the same time; omnipresence. From M.Fr. ubiquité, from L. ubique "everywhere," → ubiquitous; → -ity. Noun from visp-bâšandé, visp-bâš, visp-bâšâyi, → ubiquitous. |
uniformity yekdisvâri, yekdisigi Fr.: uniformité The state or quality of being uniform. |
unitarity yekâyigi Fr.: unitarité 1) The condition of being → unitary. |
unity yeki (#) Fr.: unité The state or condition of being one. M.E. unite, from O.Fr., from L. unitatem "oneness, sameness, agreement," from unus, → one. Yeki, noun from yek, → one. |
universality hargânigi Fr.: universalité The character or state of being universal. |
universality of free fall hargânigi-ye oft-e âzâd Fr.: universlité de chute libre Same as → weak equivalence principle. → universality; → free; → fall. |
universality of the IMF hargâni-ye karyâ-ye âqâzin-e jerm Fr.: universalité de l'IMF The hypothesis whereby there exists a universal parent → distribution function which describes the stellar → initial mass function in individual star forming events. A consensus appears to have emerged in the community that the stellar IMF is largely invariant for star formation conditions as are found throughout the Local Group of galaxies at the present time. For details and discussion see Pavel Kroupa (2012), Recent advances on IMF research, arXiv.org/abs/astro-ph/1210.1211, and references therein. |
university dânešgâh (#) Fr.: université An institution of higher education composed of several faculties for teaching and research and authorized to grant academic degrees. M.E., from O.Fr. universitei, from M.L. universitatem (nominative. universitas), in L.L. "corporation, society," from L., "the whole, aggregate," from universus "whole, entire," → universe. Dânešgâh, from dâneš, → science, + -gâh "place; time" (Mid.Pers. gâh, gâs "time;" O.Pers. gāθu-; Av. gātav-, gātu- "place, throne, spot;" cf. Skt. gâtu- "going, motion; free space for moving; place of abode;" PIE *gwem- "to go, come"). |
univocity yekvâzi Fr.: monosémie |
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