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Torino scale marpel-e Turin Fr.: échelle de Turin A scale used to assess the threat posed by the → impact of a → near-Earth object (NEO). It considers the impact energy as well as the probability of impact. It is designed to communicate to the public the risk associated with a NEO in more qualitative form than the → Palermo scale. The → impact hazard is expressed by a number between 0 and 10 depending on the probability that an impact will occur and the kinetic energy of the potential → impactor. The extent of damage ranges from inconsequential (0) to catastrophic (10). The scale is color-coded such that white = no consequence; green = meriting careful monitoring; yellow = meriting concern; orange = threatening events; red = impact is certain. Named for Torino, because the scale was adopted by that city in Italy in 1999; → scale. |
tornado pic-tuf, tufân-e picandé Fr.: tornade A mass of rotating air with high wind speeds at its center. It is produced in a very severe thunderstorm and appears as a funnel cloud extending from the base of a Cumulonimbus to the ground. Tornado, metathesis from Sp tronada "thunderstorm," from tronar "to thunder," from L. tonare "to thunder," → thunder. Pic-tuf, from pic present stem of picidan
"to twist, entwine, coil" (Mid.Pers. pecidan "to twist, entwine") +
tuf short for tufân, → storm. |
toroid cambarvâr (#) Fr.: toroïde A surface of revolution obtained by rotating a closed plane curve about an axis parallel to the plane which does not intersect the curve. The simplest toroid is the → torus. The solid enclosed by such a surface. |
toroidal magnetic field meydân-e meqnâtisi-ye cambarvâr Fr.: champ magnétique toroïdal A magnetic field which is generated in a → plasma inside a → toroid, as in a → tokamak, by the electric current which spirals around the toroid. Toroidal field has no radial component. → poloidal magnetic field. → toroid; → magnetic field. |
torque gaštâvar (#) Fr.: couple The tendency of a → force applied to an object to cause the object to → rotate about a given → axis or → point. Torque is the rotational analogue of or the turning effect of a force. It is equal to the product of the force and its distance from the reference axis. More specifically, if a force F acts on a single particle at a point P whose position with respect to the origin O of the inertial reference is given by the distance vector r, the torque T acting on the particle with respect to the origin O is defined as: T = r × F. Torque is a → vector quantity. Its magnitude is given by: rF sin θ, where θ is the angle between r and F; its direction is normal to the plane formed by r and F. The sense is given by the → right-hand screw rule for the → vector product of two vectors. Torque has the same dimensions as work, but work is a scalar. From L. torquere "to twist;" cf. Skt. tarku- "spindle;" maybe Mod.Pers. duk "spindle;" Mid.Pers. dôk "spindle;" O.C.S. traku "band, girdle," O.H.G. drahsil "turner," Ger. drechseln "to turn on a lathe;" O.E. thweorh "transverse, perverse, angry, cross;" E. thwart; PIE base *twork-/*twerk- "twist" Gaštâvar literally "that which makes turn, turning agent," from gašt "turning," past stem of gaštan, gardidan "to turn, to change" (Mid.Pers. vartitan; Av. varət- "to turn, revolve;" Skt. vrt- "to turn, roll," vartate "it turns round, rolls;" L. vertere "to turn;" O.H.G. werden "to become;" PIE base *wer- "to turn, bend") + âvar agent noun of âvardan "to bring; to cause, produce" (Mid.Pers. âwurtan, âvaritan; Av. ābar- "to bring; to possess," from prefix ā- + Av./O.Pers. bar- "to bear, carry," bareθre "to bear (infinitive)," bareθri "a female that bears (children), a mother;" Mod.Pers. bordan "to carry;" Skt. bharati "he carries;" Gk. pherein; L. fero "to carry"). |
torr torr (#) Fr.: torr A unit of pressure used in the field of high vacuum, equivalent to 1 mm of mercury After the Italian scientist Evangelista Torricelli (1608-1647), who invented the first barometer. |
torrent lâhez (#) Fr.: torrent A stream of water flowing with great rapidity and violence. See also → rapids. M.E., from M.Fr. torrent, from L. torrentem (nominative torrens) "a rushing (stream)," from torrere, "to parch, dry up, roast," → torrid. Lâhez, from Tabari lahez "an overwhelming flow," Baxtiyâri lâhiz "flood." The first component lâh, lah maybe related to lur, Lori, Kordi laf, Tabari lé "flood," → cataclysm. |
Torricelli's law qânun-e Torricelli Fr.: loi de Torricelli In fluid dynamics, a theorem that relates the speed of fluid flowing out of an opening to the height of fluid above the opening: v = (2gh)^{1/2}, where v is the exit velocity of the water, h is the height of the water column, and g is the acceleration due to gravity (9.81 m/s^{2}). It was later shown to be a particular case of → Bernoulli's theorem. After the Italian scientist Evangelista Torricelli (1608-1647), who found this relationship in 1643. |
torrid tafsân, tafsâ Fr.: torride Subject to the weather that is hot and dry enough to scorch land. From L. torridus "dried with heat, scorching hot," from torrere "to dry up, roast," related to terra "earth," literally "dry land;" from PIE base *ters- "to dry" (cf. Pers. tešné "thirsty;" Mid.Pers. tašnak "thirsty;" Av. taršu- "dry," taršna- "thirst;" Skt. trsta- "dry," tars- "to be thirsty;" Gk. teresesthai "to become or be dry;" Goth. þaursus "dry, barren," O.H.G. derren "to make dry," durst "thirst;" Ger. dürr "arid;" O.E. þurstig "thirsty"). Tafsân, tafsâ, from tafsidan "to become hot," variants tâftan, tâbidan "to shine;" Mid.Pers. tâftan "to heat, burn, shine;" taftan "to become hot;" Parthian t'b "to shine;" Av. tāp-, taf- "to warm up, heat," tafsat "became hot," tāpaiieiti "to create warmth;" cf. Skt. tap- "; to heat, be/become hot; to spoil, injure, damage; to suffer," tapati "burns;" L. tepere "to be warm," tepidus "warm;" PIE base *tep- "to be warm." |
Torrid Zone zonnâr-e tafsân Fr.: Zone torride The part of the Earth's surface between the tropics of Cancer and Capricorn |
torus cambar (#) Fr.: tore A surface produced by the revolution of a conic section (such as a circle) around a line lying in its plane, but not cutting the conic. The solid enclosed by such a surface. From L. torus "a round, swelling protuberance." Cambar "torus," originally "hoop, circle," from Mid.Pers. cambar "hoop; a ring-shaped headdress," cambar vâcik "playing tambourine." |
total hamâk Fr.: total Constituting or comprising the whole; entire; complete in extent or degree.
Related term → general = harvin ( M.E., from O.Fr. total, from M.L. totalis "entire, total," from L. totus "all, whole, entire," of unknown origin. Mid.Pers. hamâk, hamâg "total, all," hamâkih "totality," related to Mod.Pers. hamé- "all," variant hami "all the time, always;" Mid.Pers. hamê "all the time, always;" Av. hama- "any" (cf. Skt. sama-"any, every, whichever;" Gk. amo-then "whichever;" Goth. sums "any;" O.N. sumr "any;" O.E. sum "some;" E. some) + suffix -âk. |
total abundance farâvâni-ye hamâk Fr.: abondance totale Same as → elemental abundance. |
total eclipse gereft-e hamâk Fr.: éclipse totale An → eclipse in which the whole of the disk of the Sun or Moon is obscured. See also → annular eclipse, → partial eclipse, → totality, → totality path. |
total energy kâruž-e hamâk Fr.: énergie totale The sum of all forms of energy involved in a system. |
total function karyâ-ye hamâk Fr.: fonction totale A function whose value is defined for all possible input values. |
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. |
total internal reflection bâztâb-e hamâk-e daruni Fr.: réflexion totale interne A phenomenon occurring when a light ray traveling cross an → interface from a higher → refractive index medium to a lower refractive index medium hits the interface at an angle larger than the → critical angle. In these conditions the light will not pass through to the second → medium at all. Instead, all of it will be reflected back into the first medium. → total; → internal; → reflection. |
total lunar eclipse mâhgereft-e hamâk Fr.: éclipse lunaire totale A → lunar eclipse when the entire → Moon passes through the Earth's → umbra. The maximum duration of a total lunar eclipse is 1h 47m. It happens when the Moon crosses the umbra at its → apogee, where it moves the most slowly, and the Earth is at its → aphelion. The longest total lunar eclipse of the 21st century, lasting 1h 42m 59s, occurred on the night of 27 to 28 July 2018 (Europe, Africa, Asia, Australia, and New Zealand). See also → tetrad. |
total pressure fešâr-e hamâk Fr.: pression totale The sum of → static pressure, → dynamic pressure, and → hydrostatic pressure in the → Bernoulli equation. |
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