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submillimeter radiation tâbeš-e zir-milimetri Fr.: rayonnement sub-millimétrique That part of the → electromagnetic radiation with a → wavelength beyond 300 → microns. → submillimeter; → radiation. |
submission dar-sepord Fr.: soumission An act or instance of submitting. The condition of having submitted. → submit Verbal noun of → submit. |
subscription zirvešt Fr.: souscription 1) A sum of money given or pledged as a contribution, payment, investment, etc. 2) The right to receive a periodical for a sum paid, usually for an agreed number of issues (Dictionary.com). |
subtraction zirkaršeš Fr.: soustraction The operation of finding the difference between two numbers or quantities. Verbal noun of → subtract. |
suggestion pišnehâd (#) Fr.: suggestion 1) The act of suggesting. Verbal noun of → suggest. |
supergranulation cell yâxte-ye abar-dâne-bandi Fr.: cellule de supergranulation One of a number of large convective cells (about 15,000-30,000 km in diameter) in the solar photosphere, distributed fairly uniformly over the solar disk, that last longer than a day. → super-; → granulation; → cell. |
superion abaryon Fr.: superion An ion which is responsible for the existence of a strong → P Cygni profile observed in many early O stars. Since the → effective temperature of the star is too low to produce such an ion appreciably, the ion is termed a superion. For example, the ion O5+ which is at the origin of a strong O VI λλ1031, 1038 P Cygni profile observed in many O stars. Similarly, the lines due to N V λλ1238, 1242 belong to the superion category, while in later spectral types C IV λλ1548, 1552 also falls into this category. Initial modeling of the → ultraviolet line superions assumed the → stellar winds were smooth and homogeneous. However it is now generally accepted that the winds are (→ clumped wind), and this can have a profound influence on the formation of the superion profiles. We know that the strength of lines due to the superions is strongly influenced by the → interclump medium. Indeed, the interclump medium may be more important for producing the lines than are the clumps -- this is simply a consequence of the higher ionization in the interclump medium which occurs because of its lower density (see D. John Hillier, 2020, https://www.mdpi.com/2075-4434/8/3/60/htm, and references therein). |
superior conjunction hamistân-e zabarin Fr.: conjonction supérieure The conjunction of a planet with the Sun which occurs when the planet is beyond the Sun. → inferior conjunction. → superior; → conjunction. |
superior culmination bâlest-e zabarin Fr.: culmination supérieure The meridian transit of a star between the celestial pole and the south point of the horizon. Same as → upper culmination. → inferior culmination. → superior; → culmination. |
superluminal motion jonbeš-e abar-nuri Fr.: mouvement superluminal Apparent proper motion exceeding the velocity of light seen toward certain astronomical objects, such as the jets of radio galaxies and quasars. However, these jets are not actually moving at speeds in excess of the speed of light: the apparent superluminal motion is a projection effect caused by objects moving near the speed of light and at a small angle to the line of sight. |
supernova explosion oskaft-e abar-now-axtar Fr.: explosion de supernova The very short and violent phenomenon that occurs when a star undergoes → core collapse or → thermonuclear runaway. |
superposition barhamneheš Fr.: superposition 1) The act of placing upon; the state of being placed upon. Barhamneheš, from bar- "on, upon, up" (Mid.Pers. abar; O.Pers. upariy "above; over, upon, according to;" Av. upairi "above, over," upairi.zəma- "located above the earth;" cf. Gk. hyper- "over, above;" L. super-; O.H.G. ubir "over;" PIE base *uper "over") + -ham- "together, with," → syn-, + neheš, → position. |
superposition principle parvaz-e barhamneheš Fr.: principe de superposition 1) Math.: The principle concerned with homogeneous and
non-homogeneous → linear differential equations,
stating that two or more solutions to a linear equation or set of linear equations can be added
together so that their sum is also a solution. → superposition; → principle. |
supersaturation abar-anjâleš Fr.: super-saturation The process whereby the amount of → water vapor in the air exceeds that needed to → saturate. In other words, the condition of air in which the → humidity is above the level required for saturation at a given temperature (i.e. the → relative humidity is greater than 100%). When the temperature drops below freezing, this can lead to a situation where more water vapor is present in the air than the air can hold. At every temperature, there is a maximum amount of water vapor that can be supported in the air. The higher the temperature, the more water vapor can be accommodated. But if the air that is already at 100% relative humidity is cooled then it becomes supersaturated, and this situation is unstable. As a result, the excess water vapor crystallizes out, either into water droplets or directly into ice. → super-; → saturation. |
suppression nehâveš Fr.: suppression The act of suppressing; the state of being suppressed. → Compton suppression, → zero suppression. |
surface tension taeš-e ruye-yi Fr.: tension superficielle The inward → attraction of the → molecules at the → surface of a → liquid. The reason is that the molecules at the surface do not have other like molecules on all sides of them and consequently they cohere more strongly to those directly associated with them on the surface. Also called surface energy and capillary forces. |
surjection baršâneš Fr.: surjection A mapping f of a set A onto a set B in such a way that every b element of B is the image of at least one element a of A. In other words, for any element b of B, the equation f(a) = b yields at least one solution. Allso called → surjective mapping. |
suspicion bargâseš Fr.: suspicion 1) The state of mind or feeling of one who suspects. M.E., from suspecioun, from O.Fr. suspicion, sospeçon "mistrust, suspicion," from L.L. suspectionem "mistrust, suspicion, fear," noun of state from past participle stem of L. suspicere "to look up at," → suspect. Verbal noun from bargâsidan, → suspect. |
symmetric relation bâzâneš-e hamâmun Fr.: relation symétrique A relation between two quantities such that the first is to the second as the second is to the first. In symbols: a R b = b R a. For example, multiplication is an operation with a symmetric relation between the factors: 5 x 3 = 3 x 5. |
synchronous rotation carxeš-e hamgâm (#) Fr.: rotation synchrone Of a body orbiting another, where the orbiting body takes as long to rotate on its axis as it does to make one orbit. Therefore it always keeps the same hemisphere pointed at the body it is orbiting. Both bodies are tidally locked (→ tidal locking). This phenomenon is a natural consequence of → tidal braking. Synchronous rotation is common throughout the → solar system. It is found among the satellites of → Mars (→ Phobos and → Deimos), → Jupiter (most of Jupiter satellites, including the → Galilean Moons) and → Saturn (e.g. → Iapetus). Similarly, → Pluto and its moon → Charon are locked in mutual synchronous rotation, with both of them keeping the same faces towards each other. → synchronous; → rotation. |
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