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closed curve xam-e basté (#) Fr.: courbe fermée A curve whose ends are joined. |
closed space fazâ-ye basté (#) Fr.: espace fermé A bounded space the surface of which has the property that if one travels in any direction upon it without changing direction, one will end up back to the departure point. An example is a sphere. Triangles which lie on the surface of a closed space will have a sum of angles which is greater than 180°. An closed space has a positive → curvature. See also → closed Universe, → open space. |
closed system râžmân-e basté Fr.: système fermé Thermodynamics: A system which can exchange energy with the surroundings but not matter. → open system; → isolated system. |
closed Universe giti-ye basté (#) Fr.: Univers fermé A → cosmological model, first formulated by Friedmann and Lemaître, in which the Universe has a → finite size and lifetime and → space has a → positive → curvature, e.g. a Universe with a density greater than the → critical density. See also → closed space. |
closed wff wff basté Fr.: FBF fermée In → predicate logic, a → wff with no → free occurrences of any → variable. Also called a → sentence. |
closure bandeš (#) Fr.: clôture Math.:
The property of a set in which the application of a given
mathematical operation to any member of the set always has another
member of the set as its result. M.E., from M.Fr., from O.Fr. closure "that which encloses," from L. clausura "lock, fortress, a closing," from p.p. stem of claudere "to close." Bandeš, verbal noun of bastan "to shut, bind; to clot; to form seed buds," from Mid.Pers. bastan/vastan "to bind, shut," Av./O.Pers. band- "to bind, fetter," banda- "band, tie;" Skt. bandh- "to bind, tie, fasten;" PIE *bhendh- "to bind," cf. Ger. binden, E. bind. |
closure axiom bondâšt-e bandeš Fr.: axiome de clôture A basic rule in → group theory stating that if a and b are a group element then a * b is also a group element. |
closure phase fâz-e bandeš Fr.: clôture de phase In astronomical interferometry, a method using triplets of telescopes in an array to calculate the phase information and get over the effects of atmospheric turbulence. The method, used in high-resolution astronomical observations, both at radio and at optical wavelengths, allows imaging of complex objects in the presence of severe aberrations. |
clothoid klotoid Fr.: clothoïde A plane curve of spiral form, → Cornu's spiral. From Gk. kloth, from klothein "to spin" + epenthetic vowel -o- + eides "form," → -oid; because the curve is reminiscent of the thread that winds around a weaving loom. → Klotho. |
cloud abr (#) Fr.: nuage 1) A visible mass of water droplets and/or ice particles in the atmosphere above the
Earth's surface. Cloud, from O.E. clud "mass of rock," from P.Gmc. *kludas. Abr, from Mid.Pers. awr, abr (Laki owr, Baluchi haur, Kordi Soriani hewr), Av. awra- "rain cloud, rain," cf. Skt. abhra-"thunder cloud," Gk. afros "scum, foam," L. imber "rain;" also Sk. ambha- "water," Gk. ombros "rain," PIE *mbhros "rain cloud, rain," from *mbh-. |
cloud chamber otâqak-e abr Fr.: chambre à nuage An early type of → bubble chamber used for detecting particles of ionizing radiation. It was invented in 1900 by Charles Thomson Rees Wilson (1869-1959), a Scottish physicist, who along with Arthur Compton (1892-1962 ) received the Nobel Prize for physics in 1927. |
cloud cover pušeš-e abri (#) Fr.: couverture nuageuse The fraction of the sky covered by clouds. It is expressed in tenths, so that 0.0 indicates a clear sky and 1.0 (or 10/10) indicates a completely covered sky. |
cloud fragmentation latpâreš-e abr Fr.: fragmentation de nuage Process by which a → collapsing → giant molecular cloud breaks into dense → clumps, eventually bringing about → pre-stellar cores. → cloud; → fragmentation. |
cloudbow abrkamân Fr.: A large, faintly colored arc formed usually by sunlight falling on a cloud. Also called white rainbow, fogbow, and mistbow. Cloudbow appears white because the water droplets in the cloud or fog are very small compared with those of ordinary rainbows. |
cloudburst ragbâr (#) Fr.: averse Any sudden and heavy fall of → rain, always of the → shower type. Ragbâr, from rag + bâr. The second component bâr, variant bârân "rain," from bâridan "to rain." The origin of the first component is not clear. Rag in Persian means "blood vein, vessel," but this sense seems irrelevant here. In Gilaki the bare râk (without bâr) means cloudburst. Râk/rag may be related (via an extinct Iranian parent) to the Skt. stem ri- "to flow, to drop, to become liquid." |
cloudiness abrâludegi (#) Fr.: état nuageux, nébulosité Same as → cloud cover. |
cloudshine abr-tâb Fr.: éclat de nuage Light from nearby stars scattered by → dust grains in low-density outer regions of → molecular clouds. It is seen not only in the → near infrared bands JHK, but also continuously from the visible to 5 μm. Cloudshine could be considered as an intermediate between → scattering in the visible and the → coreshine effect (Foster & Goodman, 2006, ApJ 636, L105). See also |
clover šabdar (#) Fr.: trèfle Any of various plants of the genus Trifolium with three round, green leaves that are joined together. Clovers occasionally have leaves with four leaflets, instead of the usual three. M.E. clovere; O.E. clafre; cf. M.L.G. klever, M.Du. claver, Du. klaver, O.S. kle, O.H.G. kleo, Ger. Klee "clover," of uncertain origin. Šabdar, of unknown origin. |
cloverleaf quasar (H1413+117) kuâsâr-e barg-e šabdar Fr.: quasar du trèfle à quatre feuilles A bright → quasar whose image is split into four spots due to → gravitational lensing (Magain et al. 1988, Nature 334, 325). The four images of comparable brightness all lie within 0.7 arc seconds of the image center. The quasar has a → redshift of 2.56, corresponding to a distance of about 11 billion → light-years. Observations indicate that the lensing galaxy is located approximately at the geometrical center of the four images. A firm spectroscopic redshift of the lens has yet to be obtained; however, a → cluster of galaxies at a redshift of z = 1.7 has been suggested to account for the lensing of this system. H1413+117 was the first quasar to be detected in the → submillimeter wave → continuum and in → carbon monoxide emission. So named because of the optical image; → clover; → leaf; → quasar. |
clump gude Fr.: grumeau 1) A compact mass, in particular that contained in a less dense environment. Clump, from Du. klomp "lump, mass," or Low Ger. klump. Gudé "ball, bowl, tumour" in Gilaki, cf. Skt. guda- "ball, mouthful, lump, tumour," Gk. gloutos "rump," L. glomus "ball," globus "globe," Ger. Kugel, E. clot, PIE *gel- "to make into a ball." |
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