nâ- (#) Fr.: in-, non- A prefix meaning “not.” Etymology (EN): M.E., O.E. un- (cf. O.Fris., O.H.G., Ger. un-, Goth. un-, Du. on-), cognate with Pers. nâ-, as below. Etymology (PE): Nâ- “not,” variants na “no, not,” ma- “not” (prohitive); Mid.Pers. nê, ma “no, not;” O.Pers. naiy, nai “not;” Av. nôit, naē “not;” cf. Skt. ná “not;” L. ne-, in-, un-; Gk. ni; Lith. nè; O.C.S. ne “not;” E. un-, as above; PIE *ne-. |
nâ- (#) Fr.: in-, non- A prefix meaning “not.” Etymology (EN): M.E., O.E. un- (cf. O.Fris., O.H.G., Ger. un-, Goth. un-, Du. on-), cognate with Pers. nâ-, as below. Etymology (PE): Nâ- “not,” variants na “no, not,” ma- “not” (prohitive); Mid.Pers. nê, ma “no, not;” O.Pers. naiy, nai “not;” Av. nôit, naē “not;” cf. Skt. ná “not;” L. ne-, in-, un-; Gk. ni; Lith. nè; O.C.S. ne “not;” E. un-, as above; PIE *ne-. |
cašm-e biyâvar, ~ berehné Fr.: œil nu The eye unassisted by an optical instrument, except for eyeglasses. Same as → naked eye. Etymology (EN): → un- + aided, from aid, M.E. ayde, from Etymology (PE): Cašm, → eye; biyâvar “without help,” from bi- “without” + yâvar, variant yâr “helper; companion” (Mid.Pers. hayyâr “helper,” hayyârêh “help, aid, assistance,” Proto-Iranian *adyāva-bara-, cf. Av. aidū- “helpful, useful”); berehné, → naked. |
cašm-e biyâvar, ~ berehné Fr.: œil nu The eye unassisted by an optical instrument, except for eyeglasses. Same as → naked eye. Etymology (EN): → un- + aided, from aid, M.E. ayde, from Etymology (PE): Cašm, → eye; biyâvar “without help,” from bi- “without” + yâvar, variant yâr “helper; companion” (Mid.Pers. hayyâr “helper,” hayyârêh “help, aid, assistance,” Proto-Iranian *adyāva-bara-, cf. Av. aidū- “helpful, useful”); berehné, → naked. |
nâtosnidani Fr.: inévitable |
nâtosnidani Fr.: inévitable |
bi-varak Fr.: non biaisé Not biased or prejudiced. Etymology (EN): → un- + → Etymology (PE): Bi- “without” + varak, → bias. |
bi-varak Fr.: non biaisé Not biased or prejudiced. Etymology (EN): → un- + → Etymology (PE): Bi- “without” + varak, → bias. |
barâvar-e bi-varak Fr.: estimateur non biaisé |
barâvar-e bi-varak Fr.: estimateur non biaisé |
nemunân-e a bi-varak Fr.: échantillon non biaisé |
nemunân-e a bi-varak Fr.: échantillon non biaisé |
model-e nâpatumand Fr.: modèle non blanketé A stellar atmosphere model which ignores metals and their physical effects. → line-blanketed model; → line blanketing. See also: → un-; → blanketed model. |
model-e nâpatumand Fr.: modèle non blanketé A stellar atmosphere model which ignores metals and their physical effects. → line-blanketed model; → line blanketing. See also: → un-; → blanketed model. |
nâbandidé Fr.: non lié
|
nâbandidé Fr.: non lié
|
bâr-e nâbandidé Fr.: charge non liée Same as → free charge. |
bâr-e nâbandidé Fr.: charge non liée Same as → free charge. |
xuše-ye nâbandidé Fr.: amas non lié A cluster of objects, such as stars or galaxies, in which the members are not tied together gravitationally. In such a cluster the members scatter through space following different directions. → bound cluster. |
xuše-ye nâbandidé Fr.: amas non lié A cluster of objects, such as stars or galaxies, in which the members are not tied together gravitationally. In such a cluster the members scatter through space following different directions. → bound cluster. |
râžân-e nâbandidé Fr.: système non lié |
râžân-e nâbandidé Fr.: système non lié |
râžmân-e setâre-yi-ye javân-e nâbandidé Fr.: système stellaire jeune non lié A class of gravitationally loose stellar conglomerate with a
notable apparent shape making it
different from typical → bound
→ star clusters. The UYSS class |
râžmân-e setâre-yi-ye javân-e nâbandidé Fr.: système stellaire jeune non lié A class of gravitationally loose stellar conglomerate with a
notable apparent shape making it
different from typical → bound
→ star clusters. The UYSS class |
karyâ-ye bikarân Fr.: fonction non bornée The function y = f(x) in a given range of the argument x if there is no number M such that for all values of x in the range under consideration the inequality | f(x) | ≤ M will be fulfilled. → bounded function. |
karyâ-ye bikarân Fr.: fonction non bornée The function y = f(x) in a given range of the argument x if there is no number M such that for all values of x in the range under consideration the inequality | f(x) | ≤ M will be fulfilled. → bounded function. |
nâtâšigi (#) Fr.: incertitude The state of being uncertain; unpredictability; indeterminacy. → uncertainty principle. |
nâtâšigi (#) Fr.: incertitude The state of being uncertain; unpredictability; indeterminacy. → uncertainty principle. |
parvaz-e nâtâštigi Fr.: principe d'incertitude A quantum mechanical principle due to Werner Heisenberg which states that the position and momentum of a particle cannot be determined simultaneously with any arbitrary accuracy. These quantities can be determined only with accuracies limited by the relation Δx.Δp ≥ (1/2)ħ, where Δx is the error in the determination of the position and Δp is the error in the momentum. A similar relation holds for the energy of a particle and the time, ΔE.Δt ≥ (1/2)ħ. Same as → Heisenberg uncertainty principle. See also: → uncertainty; → principle. |
parvaz-e nâtâštigi Fr.: principe d'incertitude A quantum mechanical principle due to Werner Heisenberg which states that the position and momentum of a particle cannot be determined simultaneously with any arbitrary accuracy. These quantities can be determined only with accuracies limited by the relation Δx.Δp ≥ (1/2)ħ, where Δx is the error in the determination of the position and Δp is the error in the momentum. A similar relation holds for the energy of a particle and the time, ΔE.Δt ≥ (1/2)ħ. Same as → Heisenberg uncertainty principle. See also: → uncertainty; → principle. |
setâre-ye B[e]-ye bi radé Fr.: étoile B[e] non-classée A temporary designation for a → B[e] star that cannot be placed in any of the four known classes. See also: → classification; → B[e] star. |
setâre-ye B[e]-ye bi radé Fr.: étoile B[e] non-classée A temporary designation for a → B[e] star that cannot be placed in any of the four known classes. See also: → classification; → B[e] star. |
nâruné Fr.: non clair |
nâruné Fr.: non clair |
nâbutâri, nâbutârmand Fr.: inconditionnel Not limited by conditions; absolute. See also: → un-; → conditional. |
nâbutâri, nâbutârmand Fr.: inconditionnel Not limited by conditions; absolute. See also: → un-; → conditional. |
nâhâsan Fr.: non conscient |
nâhâsan Fr.: non conscient |
nâhâsani Fr.: non conscience The → state of being → unconscious. See also: → unconscious; → -ness. |
nâhâsani Fr.: non conscience The → state of being → unconscious. See also: → unconscious; → -ness. |
šen-tal Fr.: A dune on a planetary surface, used in plural form undae. Etymology (EN): From L. unda “wave,” cognate with → water. Etymology (PE): Šen-tal, from šen “sand” + tal “hill, heap.” |
šen-tal Fr.: A dune on a planetary surface, used in plural form undae. Etymology (EN): From L. unda “wave,” cognate with → water. Etymology (PE): Šen-tal, from šen “sand” + tal “hill, heap.” |
Fr.: sous-, faible A prefixal use of under, as to indicate place or situation below or beneath. Contrary to → over-. Etymology (EN): M.E., from O.E. (cf. O.H.G. untar, Ger. unter, Goth. undar), from PIE *ndhero- “lower;” cf. Av. aδara- (adj.), aδairi- (prep.) “below;” Mid.Pers. êr “below, down; low, under,” adar “low,” azêr “below, under” (Mod.Pers. zir “below, down”); Skt. ádhara- “lower;” O.E. under “under, among”). Etymology (PE): Kam- “little, few; deficient, wanting; scarce” |
Fr.: sous-, faible A prefixal use of under, as to indicate place or situation below or beneath. Contrary to → over-. Etymology (EN): M.E., from O.E. (cf. O.H.G. untar, Ger. unter, Goth. undar), from PIE *ndhero- “lower;” cf. Av. aδara- (adj.), aδairi- (prep.) “below;” Mid.Pers. êr “below, down; low, under,” adar “low,” azêr “below, under” (Mod.Pers. zir “below, down”); Skt. ádhara- “lower;” O.E. under “under, among”). Etymology (PE): Kam- “little, few; deficient, wanting; scarce” |
kamfarâvâni Fr.: sous-abondance |
kamfarâvâni Fr.: sous-abondance |
kam-mirâyi Fr.: amortissement faible The behavior of a damped system when the amount of damping is weak so that the system oscillates with the amplitude gradually decreasing to zero. → overdamping. |
kam-mirâyi Fr.: amortissement faible The behavior of a damped system when the amount of damping is weak so that the system oscillates with the amplitude gradually decreasing to zero. → overdamping. |
1) kam-baravardan; 2) kam-baravard Fr.: 1) sous-estimer; 2) sous-estimation
|
1) kam-baravardan; 2) kam-baravard Fr.: 1) sous-estimer; 2) sous-estimation
|
kamcunâyide, kamcunâmand Fr.: sousqualifié |
kamcunâyide, kamcunâmand Fr.: sousqualifié |
kam-nemunângiri Fr.: sous-échantillonage The circumstance in which there are not enough pixels in a star’s image. The number of pixels that make up a star’s image is determined by the relationship between the telescope focal length, the physical size of the pixels, and the size of the star’s image. With an undersampled image it is not possible to obtain accurate estimates of the star’s image size or its position. Undersampling occurs when the atmospheric seeing conditions are exceptionally good and the pixel size not small enough. |
kam-nemunângiri Fr.: sous-échantillonage The circumstance in which there are not enough pixels in a star’s image. The number of pixels that make up a star’s image is determined by the relationship between the telescope focal length, the physical size of the pixels, and the size of the star’s image. With an undersampled image it is not possible to obtain accurate estimates of the star’s image size or its position. Undersampling occurs when the atmospheric seeing conditions are exceptionally good and the pixel size not small enough. |
fahmidan (#) Fr.: comprendre To perceive the meaning of. Etymology (EN): M.E. understanden, understonden, O.E. understandan “comprehend, grasp the idea of,” probably literally “to stand in the midst of,” from → under- + standan “to stand,” cognate with Pers. istâdan, → standard. Etymology (PE): Fahmidan, from Ar. fahm + infinitive suffix -idan. |
fahmidan (#) Fr.: comprendre To perceive the meaning of. Etymology (EN): M.E. understanden, understonden, O.E. understandan “comprehend, grasp the idea of,” probably literally “to stand in the midst of,” from → under- + standan “to stand,” cognate with Pers. istâdan, → standard. Etymology (PE): Fahmidan, from Ar. fahm + infinitive suffix -idan. |
fahm (#) Fr.: compréhension, entendement, intelligence The ability to understand something; the → power of → abstract → thought. See also: → understand; → -ing. |
fahm (#) Fr.: compréhension, entendement, intelligence The ability to understand something; the → power of → abstract → thought. See also: → understand; → -ing. |
nâtarmidé Fr.: indéterminé
See also: → un-; → determined. |
nâtarmidé Fr.: indéterminé
See also: → un-; → determined. |
šahâbsang-e nâdegarsânidé Fr.: météorite indifférenciée A type of meteorite in which the constituting materials (stone, glass, metal) are mixed together in a disorderly mass, in contrast to → differentiated meteorites. See also: → un-; → differentiated meteorite. |
šahâbsang-e nâdegarsânidé Fr.: météorite indifférenciée A type of meteorite in which the constituting materials (stone, glass, metal) are mixed together in a disorderly mass, in contrast to → differentiated meteorites. See also: → un-; → differentiated meteorite. |
mowješ Fr.: ondulation A wave; the motion of waves. Etymology (EN): From L.L. undulatus “wavy, undulated,” from undula “wavelet,” diminutive of L. unda “wave.” Etymology (PE): Mowješ, verbal noun of mowjidan “to undulate,” from mowj→ wave. |
mowješ Fr.: ondulation A wave; the motion of waves. Etymology (EN): From L.L. undulatus “wavy, undulated,” from undula “wavelet,” diminutive of L. unda “wave.” Etymology (PE): Mowješ, verbal noun of mowjidan “to undulate,” from mowj→ wave. |
yek- (#) Fr.: uni- |
yek- (#) Fr.: uni- |
bolur-e yek-âsé Fr.: cristal uniaxe Crystal with double refraction possessing only one → optic axis. |
bolur-e yek-âsé Fr.: cristal uniaxe Crystal with double refraction possessing only one → optic axis. |
nâ-idânidé Fr.: non identifié The attribute of someone or something whose identity is not established. → unidentified flying object; → unidentified line. |
nâ-idânidé Fr.: non identifié The attribute of someone or something whose identity is not established. → unidentified flying object; → unidentified line. |
barâxt-e parande-ye nâ-idânidé, padide-ye havâ-fazâyi-ye nâ-idânidé Fr.: Objet Volant Non Identifié (OVNI) Any flying object or phenomenon that cannot be identified by the observer. See also: → unidentified; fly; M.E. flien; O.E. fleogan (cf. O.H.G. fliogan, O.N. flügja, M.Du. vlieghen, Ger. fliegen); → object. |
barâxt-e parande-ye nâ-idânidé, padide-ye havâ-fazâyi-ye nâ-idânidé Fr.: Objet Volant Non Identifié (OVNI) Any flying object or phenomenon that cannot be identified by the observer. See also: → unidentified; fly; M.E. flien; O.E. fleogan (cf. O.H.G. fliogan, O.N. flügja, M.Du. vlieghen, Ger. fliegen); → object. |
bând-e forusorx-e nâ-idânidé Fr.: bande infrarouge non identifiée A no longer in general use name for → Aromatic Infrared Band. See also: → unidentified; → infrared; → band. |
bând-e forusorx-e nâ-idânidé Fr.: bande infrarouge non identifiée A no longer in general use name for → Aromatic Infrared Band. See also: → unidentified; → infrared; → band. |
xatt-e nâ-idânidé Fr.: raie non identifiée A spectral line whose origin is not clearly established. → line identification. See also: → unidentified; → line. |
xatt-e nâ-idânidé Fr.: raie non identifiée A spectral line whose origin is not clearly established. → line identification. See also: → unidentified; → line. |
yegâneš Fr.: unification
See also: Verbal noun of → unify. |
yegâneš Fr.: unification
See also: Verbal noun of → unify. |
yekdis, yeknavâxt Fr.: uniforme Without variations; identical, always the same in quality, degree, character, or manner. Etymology (EN): → uni- + → form. Etymology (PE): Yekdis, from yek, → uni-, + dis,
|
yekdis, yeknavâxt Fr.: uniforme Without variations; identical, always the same in quality, degree, character, or manner. Etymology (EN): → uni- + → form. Etymology (PE): Yekdis, from yek, → uni-, + dis,
|
jonbeš-e dâyereyi-ye yekdis, ~ ~ yeknavâxt Fr.: mouvement circulaire uniforme |
jonbeš-e dâyereyi-ye yekdis, ~ ~ yeknavâxt Fr.: mouvement circulaire uniforme |
meydân-e yekdis, ~ yeknavâxt Fr.: champ uniforme A field that at a given instant has the same value at all points within a specified region of interest. See also: → uniform; field. |
meydân-e yekdis, ~ yeknavâxt Fr.: champ uniforme A field that at a given instant has the same value at all points within a specified region of interest. See also: → uniform; field. |
meydân-e meqnâtisi-ye yekdis Fr.: champ magnétique uniforme A → magnetic field whose direction does not change and whose strength is constant at every point. |
meydân-e meqnâtisi-ye yekdis Fr.: champ magnétique uniforme A → magnetic field whose direction does not change and whose strength is constant at every point. |
jonbeš-e yekdis, ~ yeknavâxt Fr.: mouvement uniforme Motion at a constant → velocity. The state of rest is a special case of uniform motion. → accelerated motion; → inertial motion. See also: → uniform; motion. |
jonbeš-e yekdis, ~ yeknavâxt Fr.: mouvement uniforme Motion at a constant → velocity. The state of rest is a special case of uniform motion. → accelerated motion; → inertial motion. See also: → uniform; motion. |
yekdisvâr Fr.: uniformitaire
See also: → uniformity + -arian. |
yekdisvâr Fr.: uniformitaire
See also: → uniformity + -arian. |
yekdisvârbâvari Fr.: uniformitarisme The doctrine whereby geologic processes (→ erosion, → deposition, → compaction, and → uplift) observed at Earth’s surface now are the same that have shaped Earth’s landscape over long periods of time in the past. The term uniformitarianism was first used in 1832 by William Whewell, to present an alternative explanation for the origin of the Earth. The prevailing view at that time was that the Earth was created through supernatural means and had been affected by a series of catastrophic events such as the biblical Flood. This theory is called → catastrophism. The ideas behind uniformitarianism originated with the work of Scottish geologist James Hutton. In 1785, Hutton presented at the meetings of the Royal Society of Edinburgh that the Earth had a long history and that this history could be interpreted in terms of processes currently observed. For example, he suggested that deep soil profiles were formed by the weathering of bedrock over thousands of years. He also suggested that supernatural theories were not needed to explain the geologic history of the Earth (PhysicalGeography.net). See also: → uniformitarian; → -ism. |
yekdisvârbâvari Fr.: uniformitarisme The doctrine whereby geologic processes (→ erosion, → deposition, → compaction, and → uplift) observed at Earth’s surface now are the same that have shaped Earth’s landscape over long periods of time in the past. The term uniformitarianism was first used in 1832 by William Whewell, to present an alternative explanation for the origin of the Earth. The prevailing view at that time was that the Earth was created through supernatural means and had been affected by a series of catastrophic events such as the biblical Flood. This theory is called → catastrophism. The ideas behind uniformitarianism originated with the work of Scottish geologist James Hutton. In 1785, Hutton presented at the meetings of the Royal Society of Edinburgh that the Earth had a long history and that this history could be interpreted in terms of processes currently observed. For example, he suggested that deep soil profiles were formed by the weathering of bedrock over thousands of years. He also suggested that supernatural theories were not needed to explain the geologic history of the Earth (PhysicalGeography.net). See also: → uniformitarian; → -ism. |
yekdisvâri, yekdisigi Fr.: uniformité |
yekdisvâri, yekdisigi Fr.: uniformité |
yegânestan (#), yegânidan (#) Fr.: unifier To make or become a single unit or entity. Etymology (EN): M.Fr. unifier, from L.L. unificare “to make one,” from L. uni-, → one, + facere “to make” (cf. Fr. faire, Sp. hacer), from PIE base *dhe- “to put, to do” (cognate with Mod.Pers. dâdan “to give;” O.Pers./Av. dā- “to give, grant, yield,” dadāiti “he gives; puts;” Skt. dadáti “puts, places;” Hitt. dai- “to place;” Gk. tithenai “to put, set, place;” Lith. deti “to put;” Czech diti, Pol. dziac’, Rus. det’ “to hide,” delat’ “to do;” O.H.G. tuon, Ger. tun, O.E. don “to do”). Etymology (PE): Yegânestan, yegânidan “to make one,” infinitive from yek, |
yegânestan (#), yegânidan (#) Fr.: unifier To make or become a single unit or entity. Etymology (EN): M.Fr. unifier, from L.L. unificare “to make one,” from L. uni-, → one, + facere “to make” (cf. Fr. faire, Sp. hacer), from PIE base *dhe- “to put, to do” (cognate with Mod.Pers. dâdan “to give;” O.Pers./Av. dā- “to give, grant, yield,” dadāiti “he gives; puts;” Skt. dadáti “puts, places;” Hitt. dai- “to place;” Gk. tithenai “to put, set, place;” Lith. deti “to put;” Czech diti, Pol. dziac’, Rus. det’ “to hide,” delat’ “to do;” O.H.G. tuon, Ger. tun, O.E. don “to do”). Etymology (PE): Yegânestan, yegânidan “to make one,” infinitive from yek, |
nâvinârdani Fr.: inimaginable Difficult or impossible to believe. See also: → un-; → imaginable. |
nâvinârdani Fr.: inimaginable Difficult or impossible to believe. See also: → un-; → imaginable. |
yekâyeš Fr.: union General: The act of uniting two or more things. Etymology (EN): M.E. from O.Fr. union from L.L. unionem (nominative unio) “oneness, unity,” from unus, → one, cognate with Pers. yek, as below. Etymology (PE): Yekâyeš, from yek, → one,
|
yekâyeš Fr.: union General: The act of uniting two or more things. Etymology (EN): M.E. from O.Fr. union from L.L. unionem (nominative unio) “oneness, unity,” from unus, → one, cognate with Pers. yek, as below. Etymology (PE): Yekâyeš, from yek, → one,
|
yektâ (#) Fr.: unique Existing as the only one or as the sole example. Etymology (EN): From Fr. unique, from L. unicus “single, sole,” from unus, → one. Etymology (PE): Yektâ “unique,” from yek, → one,
|
yektâ (#) Fr.: unique Existing as the only one or as the sole example. Etymology (EN): From Fr. unique, from L. unicus “single, sole,” from unus, → one. Etymology (PE): Yektâ “unique,” from yek, → one,
|
yektâyi (#) Fr.: unicité |
yektâyi (#) Fr.: unicité |
farbin-e yektâyi Fr.: théorème d'unicité
See also: → uniqueness; → theorem. |
farbin-e yektâyi Fr.: théorème d'unicité
See also: → uniqueness; → theorem. |
yekâ (#), yekân (#) Fr.: unité A quantity or dimension adopted as a standard of measurement. Etymology (EN): Back formation from → unity. Etymology (PE): Yekâ, yekân, from yek, → one. |
yekâ (#), yekân (#) Fr.: unité A quantity or dimension adopted as a standard of measurement. Etymology (EN): Back formation from → unity. Etymology (PE): Yekâ, yekân, from yek, → one. |
bordâr-e yekâ Fr.: vecteur unité |
bordâr-e yekâ Fr.: vecteur unité |
yekâyigi Fr.: unitarité
|
yekâyigi Fr.: unitarité
|
yekâyi Fr.: unitaire |
yekâyi Fr.: unitaire |
goruh-e yekâyi, ~ yekâni Fr.: groupe unitaire The set of n × n unitary matrices (→ unitary matrix). |
goruh-e yekâyi, ~ yekâni Fr.: groupe unitaire The set of n × n unitary matrices (→ unitary matrix). |
mâtris-e yekâyi, ~ yekâni Fr.: matrice unitaire |
mâtris-e yekâyi, ~ yekâni Fr.: matrice unitaire |
âpârgar-e yekâyi Fr.: opérateur unitaire A linear operator whose inverse is its → adjoint. In addition to → Hermitian operators, unitary operators constitute a fundamentally important class of quantum-mechanical operators. |
âpârgar-e yekâyi Fr.: opérateur unitaire A linear operator whose inverse is its → adjoint. In addition to → Hermitian operators, unitary operators constitute a fundamentally important class of quantum-mechanical operators. |
tarâdis-e yekâyi, ~ yekâni Fr.: transformation unitaire A transformation whose reciprocal is equal to its Hermitian conjugate. See also: → unitary; → transformation. |
tarâdis-e yekâyi, ~ yekâni Fr.: transformation unitaire A transformation whose reciprocal is equal to its Hermitian conjugate. See also: → unitary; → transformation. |
âyekidan, ham-yekidan Fr.: unir To join, combine, or incorporate so as to form a single whole or unit. Etymology (EN): M.E. uniten, from L. unitus, p.p. of unire “to unite,” from unus, → one. Etymology (PE): Âyekidan, from â- nuance/strengthening prefix + yek, → one, + -idan infinitive suffix; ham-yekidan, from ham- “together,” → syn-,
|
âyekidan, ham-yekidan Fr.: unir To join, combine, or incorporate so as to form a single whole or unit. Etymology (EN): M.E. uniten, from L. unitus, p.p. of unire “to unite,” from unus, → one. Etymology (PE): Âyekidan, from â- nuance/strengthening prefix + yek, → one, + -idan infinitive suffix; ham-yekidan, from ham- “together,” → syn-,
|
âyekidé, ham-yekidé Fr.: uni Formed by or resulting from the union of two or more persons or things. See also: P.p. of → unite. |
âyekidé, ham-yekidé Fr.: uni Formed by or resulting from the union of two or more persons or things. See also: P.p. of → unite. |
yeki (#) Fr.: unité |
yeki (#) Fr.: unité |
yekvartâ Fr.: univarié |
yekvartâ Fr.: univarié |
seri-ye zamâni-ye yekvartâ Fr.: série temporelle univariée A sequence of measurements of the same variable collected over time. Most often, the measurements are made at regular time intervals. See also: → univariate; → time; → series. |
seri-ye zamâni-ye yekvartâ Fr.: série temporelle univariée A sequence of measurements of the same variable collected over time. Most often, the measurements are made at regular time intervals. See also: → univariate; → time; → series. |
1a) hargâni; 1b) gitik, gitiyâné (#); 1c) jahâni (#); 2) hargâné Fr.: universal 1a) Of, pertaining to, or characteristic of all or the whole;
relating to, affecting, or including everyone in a group or situation. 1b) Of or pertaining to the → Universe,
all nature, or all existing things.
See also: → Coordinated Universal Time,
→ universal astrolabe,
→ universal gas constant,
→ universal IMF,
→ universal quantifier,
→ Universal Time. Related concepts: |
1a) hargâni; 1b) gitik, gitiyâné (#); 1c) jahâni (#); 2) hargâné Fr.: universal 1a) Of, pertaining to, or characteristic of all or the whole;
relating to, affecting, or including everyone in a group or situation. 1b) Of or pertaining to the → Universe,
all nature, or all existing things.
See also: → Coordinated Universal Time,
→ universal astrolabe,
→ universal gas constant,
→ universal IMF,
→ universal quantifier,
→ Universal Time. Related concepts: |
ostorlâb-e hargâni Fr.: astrolabe universel |
ostorlâb-e hargâni Fr.: astrolabe universel |
pâyâ-ye hargâni-ye gâzhâ Fr.: constante universelle des gaz Same as → gas constant. |
pâyâ-ye hargâni-ye gâzhâ Fr.: constante universelle des gaz Same as → gas constant. |
IMF-e hargâni Fr.: IMF universelle Same as → canonical IMF. See also: → universal; → initial mass function. |
IMF-e hargâni Fr.: IMF universelle Same as → canonical IMF. See also: → universal; → initial mass function. |
candigâr-e harvin Fr.: quantificateur universel A symbol of → predicate logic which expresses that the statements within its scope are → true for everything, or every instance of a specific thing. The symbol ∀ “for all” is used as the universal quantifier. Universal quantifiers are normally used in logic in conjunction with predicate symbols, which say something about a variable or constant, in this case the variable being quantified. See also: → universal; → quantifier. |
candigâr-e harvin Fr.: quantificateur universel A symbol of → predicate logic which expresses that the statements within its scope are → true for everything, or every instance of a specific thing. The symbol ∀ “for all” is used as the universal quantifier. Universal quantifiers are normally used in logic in conjunction with predicate symbols, which say something about a variable or constant, in this case the variable being quantified. See also: → universal; → quantifier. |
zamân-e jahâni Fr.: temps universel |
zamân-e jahâni Fr.: temps universel |
zamân-e jahâni-ye hamrâyânidé Fr.: temps universel coordonné Sale as → Coordinated Universal Time (UTC). See also: → Coordinated Universal Time (UTC). |
zamân-e jahâni-ye hamrâyânidé Fr.: temps universel coordonné Sale as → Coordinated Universal Time (UTC). See also: → Coordinated Universal Time (UTC). |
hargânigi Fr.: universalité |
hargânigi Fr.: universalité |
hargânigi-ye oft-e âzâd Fr.: universlité de chute libre Same as → weak equivalence principle. See also: → universality; → free; → fall. |
hargânigi-ye oft-e âzâd Fr.: universlité de chute libre Same as → weak equivalence principle. See also: → universality; → free; → fall. |
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. See also: → universality; → initial mass function. |
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. See also: → universality; → initial mass function. |
1) giti (#); 2) hargân Fr.: univers
2a) Math.: A → set made of 2b) Statistics: The entire population under study. See also: → all, → general, → omni-, → public, → total. Etymology (EN): M.E., from O.Fr. univers, from L. universum “the universe,” noun use of neuter of adj. universus “all together,” literally “turned into one,” from unus, → one, + versus, p.p. of vertere “to turn,” akin to Pers. gar-, gardidan “to turn, to change” (Mid.Pers. vartitan; Av. varət- “to turn, revolve;” cf. 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”). Etymology (PE): 1) Giti “world, material world, time,” variants
jahân, keyhân, geyhân “world;”
|
1) giti (#); 2) hargân Fr.: univers
2a) Math.: A → set made of 2b) Statistics: The entire population under study. See also: → all, → general, → omni-, → public, → total. Etymology (EN): M.E., from O.Fr. univers, from L. universum “the universe,” noun use of neuter of adj. universus “all together,” literally “turned into one,” from unus, → one, + versus, p.p. of vertere “to turn,” akin to Pers. gar-, gardidan “to turn, to change” (Mid.Pers. vartitan; Av. varət- “to turn, revolve;” cf. 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”). Etymology (PE): 1) Giti “world, material world, time,” variants
jahân, keyhân, geyhân “world;”
|
dânešgâh (#) Fr.: université An institution of higher education composed of several faculties for teaching and research and authorized to grant academic degrees. Etymology (EN): 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. Etymology (PE): Dânešgâh, from dâneš, → science,
|
dânešgâh (#) Fr.: université An institution of higher education composed of several faculties for teaching and research and authorized to grant academic degrees. Etymology (EN): 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. Etymology (PE): Dânešgâh, from dâneš, → science,
|
yekvâz Fr.: univoque |
yekvâz Fr.: univoque |
yekvâzi Fr.: monosémie |
yekvâzi Fr.: monosémie |
nâdânest Fr.: inconnu |
nâdânest Fr.: inconnu |
vâxabândan Fr.: activer le son |
vâxabândan Fr.: activer le son |
nâšunik Fr.: non ordinaire Uncommon, unusual. → extraordinary. |
nâšunik Fr.: non ordinaire Uncommon, unusual. → extraordinary. |
nur-e nâqotbidé (#) Fr.: lumière non polarisée A light whose electric vector of vibration is randomly oriented.
Light is an → electromagnetic wave possessing
an electric vector and an associated orthogonal magnetic vector. Both vectors
are → transverse to the axis
of propagation. In unpolarized light the electric and magnetic vibrations See also: → un-; → polarized light. |
nur-e nâqotbidé (#) Fr.: lumière non polarisée A light whose electric vector of vibration is randomly oriented.
Light is an → electromagnetic wave possessing
an electric vector and an associated orthogonal magnetic vector. Both vectors
are → transverse to the axis
of propagation. In unpolarized light the electric and magnetic vibrations See also: → un-; → polarized light. |
nâcunâyid, nâcunâmand Fr.: non qualifié |
nâcunâyid, nâcunâmand Fr.: non qualifié |
setâre-ye nâsorxidé Fr.: étoile non rougie A star whose light is not affected by→ interstellar absorption. → reddening See also: → un-; → reddened star. |
setâre-ye nâsorxidé Fr.: étoile non rougie A star whose light is not affected by→ interstellar absorption. → reddening See also: → un-; → reddened star. |
nâvâgošudé Fr.: non résolu Describing an image whose constituent or elementary parts are not resolved. → unresolved source. |
nâvâgošudé Fr.: non résolu Describing an image whose constituent or elementary parts are not resolved. → unresolved source. |
xan-e nâvâgošudé Fr.: source non résolue A source of radiation whose angular size is too small for details of its structure to be revealed. See also: → unresolved; → source. |
xan-e nâvâgošudé Fr.: source non résolue A source of radiation whose angular size is too small for details of its structure to be revealed. See also: → unresolved; → source. |
vine-ye nâtig, tasvir-e ~ Fr.: image floue An image in which finer details are not visible. → blurred image See also: → un-; → sharp image. |
vine-ye nâtig, tasvir-e ~ Fr.: image floue An image in which finer details are not visible. → blurred image See also: → un-; → sharp image. |
mâskzad-e nâtig Fr.: masque floue |
mâskzad-e nâtig Fr.: masque floue |
nâpâydâr (#) Fr.: instable Not → stable, as in → unstable atom, → unstable equilibrium. |
nâpâydâr (#) Fr.: instable Not → stable, as in → unstable atom, → unstable equilibrium. |
atom-e nâpâydâr (#) Fr.: atome instable An atom whose nuclei → decay by → radioactivity. |
atom-e nâpâydâr (#) Fr.: atome instable An atom whose nuclei → decay by → radioactivity. |
tarâzmandi-ye nâpâydâr Fr.: équilibre instable An equilibrium state of a system in which if a small perturbation away
from equilibrium is applied, the system will move farther away from
equilibrium state. For example, mechanical equilibrium in
which the potential energy is a maximum, as a sphere placed on top of
a hill. Mathematically, if the second derivative of the energy with respect
to the coordinate of interest is negative, See also: → unstable; → equilibrium. |
tarâzmandi-ye nâpâydâr Fr.: équilibre instable An equilibrium state of a system in which if a small perturbation away
from equilibrium is applied, the system will move farther away from
equilibrium state. For example, mechanical equilibrium in
which the potential energy is a maximum, as a sphere placed on top of
a hill. Mathematically, if the second derivative of the energy with respect
to the coordinate of interest is negative, See also: → unstable; → equilibrium. |
Onoqelhayyé (#) Fr.: Unukalhai The brightest star as well as the Alpha star of → Serpens, thus
also known as α Serpentis. It is a third magnitude (V = 2.65)
an orange giant of spectral type K2 with a radius 15 times as large as that of the Sun
and a surface temperature of 4300 kelvins. It is approximately 73.2 light years from Earth. See also: From Ar. ‘unuq al-hayyah ( |
Onoqelhayyé (#) Fr.: Unukalhai The brightest star as well as the Alpha star of → Serpens, thus
also known as α Serpentis. It is a third magnitude (V = 2.65)
an orange giant of spectral type K2 with a radius 15 times as large as that of the Sun
and a surface temperature of 4300 kelvins. It is approximately 73.2 light years from Earth. See also: From Ar. ‘unuq al-hayyah ( |