An Etymological Dictionary of Astronomy and Astrophysics

English-French-Persian

فرهنگ ریشه‌شناختی اخترشناسی-اخترفیزیک



188 terms — U › UN
  نا-  
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. “not;” L. ne-, in-, un-; Gk. ni; Lith. ; O.C.S. ne “not;” E. un-, as above; PIE *ne-.

  نا-  
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. “not;” L. ne-, in-, un-; Gk. ni; Lith. ; O.C.S. ne “not;” E. un-, as above; PIE *ne-.

  چشم ِ بی‌یاور، ~ ِ برهنه  
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
O.Fr. aidier, from L. adjutare, frequentative of adjuvare “to give help to,” from → ad- “to” + juvare “to help;” → eye.

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.

  چشم ِ بی‌یاور، ~ ِ برهنه  
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
O.Fr. aidier, from L. adjutare, frequentative of adjuvare “to give help to,” from → ad- “to” + juvare “to help;” → eye.

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.

  ناتسنیدنی  
nâtosnidani
Fr.: inévitable

Impossible to avoid.

See also:avoid; → -ance.

  ناتسنیدنی  
nâtosnidani
Fr.: inévitable

Impossible to avoid.

See also:avoid; → -ance.

  بی‌وَرَک  
bi-varak
Fr.: non biaisé

Not biased or prejudiced.
Statistics: With an expected value that is equal to the parameter being estimated.

Etymology (EN):un- + → biased.

Etymology (PE): Bi- “without” + varak, → bias.

  بی‌وَرَک  
bi-varak
Fr.: non biaisé

Not biased or prejudiced.
Statistics: With an expected value that is equal to the parameter being estimated.

Etymology (EN):un- + → biased.

Etymology (PE): Bi- “without” + varak, → bias.

  بر‌آور ِ بی‌وَرَک  
barâvar-e bi-varak
Fr.: estimateur non biaisé

A sample statistics when the mean of the sampling distribution of that statistic can be shown to be equal to the parameter being estimated.

See also:unbiased; → estimator.

  بر‌آور ِ بی‌وَرَک  
barâvar-e bi-varak
Fr.: estimateur non biaisé

A sample statistics when the mean of the sampling distribution of that statistic can be shown to be equal to the parameter being estimated.

See also:unbiased; → estimator.

  نمونان ِ بی‌وَرَک  
nemunân-e a bi-varak
Fr.: échantillon non biaisé

A sample in which every individual element in the population has
an equal chance of being selected.

See also:unbiased; → sample.

  نمونان ِ بی‌وَرَک  
nemunân-e a bi-varak
Fr.: échantillon non biaisé

A sample in which every individual element in the population has
an equal chance of being selected.

See also:unbiased; → sample.

  مدل ِ ناپتومند  
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.

  مدل ِ ناپتومند  
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.

  نابندیده  
nâbandidé
Fr.: non lié
  1. Not bound or tied up.

    1. Not held by a → chemical bond, → gravity, or other physical force (OxfordDictionaries.com).
      See: → unbound charge, → unbound cluster, → unbound system.

See also:un-; → bound.

  نابندیده  
nâbandidé
Fr.: non lié
  1. Not bound or tied up.

    1. Not held by a → chemical bond, → gravity, or other physical force (OxfordDictionaries.com).
      See: → unbound charge, → unbound cluster, → unbound system.

See also:un-; → bound.

  بار ِ نابندیده  
bâr-e nâbandidé
Fr.: charge non liée

Same as → free charge.

See also:unbound; → charge.

  بار ِ نابندیده  
bâr-e nâbandidé
Fr.: charge non liée

Same as → free charge.

See also:unbound; → charge.

  خوشه‌ی ِ نابندیده  
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.

See also:unbound; → cluster.

  خوشه‌ی ِ نابندیده  
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.

See also:unbound; → cluster.

  راژمان ِ نابندیده  
râžân-e nâbandidé
Fr.: système non lié

An association of bodies which are not gravitationally tied together.

See also:unbound; → system.

  راژمان ِ نابندیده  
râžân-e nâbandidé
Fr.: système non lié

An association of bodies which are not gravitationally tied together.

See also:unbound; → system.

  راژمان ِ ستاره‌ای ِ جوان ِ نابندیده  
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
includes a large range of objects, which extend at various size scales and at various degrees of self-binding; from small (semi-)compact → unbound systems named → stellar associations, to huge extended superstructures of → massive stars that make up whole parts of Galactic → spiral arms, known as → stellar complexes (Gouliermis, D. A., 2018, PASP 130:072001; arXiv:1806.11541).

See also:unbound; → young; → stellar; → system.

  راژمان ِ ستاره‌ای ِ جوان ِ نابندیده  
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
includes a large range of objects, which extend at various size scales and at various degrees of self-binding; from small (semi-)compact → unbound systems named → stellar associations, to huge extended superstructures of → massive stars that make up whole parts of Galactic → spiral arms, known as → stellar complexes (Gouliermis, D. A., 2018, PASP 130:072001; arXiv:1806.11541).

See also:unbound; → young; → stellar; → system.

  کریای ِ بیکران  
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.

See also:unbound; → function.

  کریای ِ بیکران  
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.

See also:unbound; → function.

  ناتاشتیگی  
nâtâšigi (#)
Fr.: incertitude

The state of being uncertain; unpredictability; indeterminacy. → uncertainty principle.

See also:un- + → certainty.

  ناتاشتیگی  
nâtâšigi (#)
Fr.: incertitude

The state of being uncertain; unpredictability; indeterminacy. → uncertainty principle.

See also:un- + → certainty.

  پَروَز ِ ناتاشتیگی  
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.

  پَروَز ِ ناتاشتیگی  
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.

  ستاره‌یِ B[e]ی ِ بی‌رده  
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.

  ستاره‌یِ B[e]ی ِ بی‌رده  
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.

  نارونه  
nâruné
Fr.: non clair

Difficult to see, hear, understand, or to be sure about.

See also:un-; → clear.

  نارونه  
nâruné
Fr.: non clair

Difficult to see, hear, understand, or to be sure about.

See also:un-; → clear.

  نابوتاری، نابوتارمند  
nâbutâri, nâbutârmand
Fr.: inconditionnel

Not limited by conditions; absolute.

See also:un-; → conditional.

  نابوتاری، نابوتارمند  
nâbutâri, nâbutârmand
Fr.: inconditionnel

Not limited by conditions; absolute.

See also:un-; → conditional.

  ناهاسن  
nâhâsan
Fr.: non conscient

Not awake and aware; not responding to one’s environment.

See also:non-; → conscious.

  ناهاسن  
nâhâsan
Fr.: non conscient

Not awake and aware; not responding to one’s environment.

See also:non-; → conscious.

  ناهاسنی  
nâhâsani
Fr.: non conscience

The → state of being → unconscious.

See also:unconscious; → -ness.

  ناهاسنی  
nâhâsani
Fr.: non conscience

The → state of being → unconscious.

See also:unconscious; → -ness.

  شن-تل  
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.”

  شن-تل  
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.”

  کم-  
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”
(Mid.Pers. kam “little, small, few,” O.Pers./Av. kamna- “small, few”).

  کم-  
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”
(Mid.Pers. kam “little, small, few,” O.Pers./Av. kamna- “small, few”).

  کم‌فراوانی  
kamfarâvâni
Fr.: sous-abondance

The abundance of a chemical element being lower than a reference value, in particular compared to that of the Sun.

Etymology (EN):under-; → abundance.

  کم‌فراوانی  
kamfarâvâni
Fr.: sous-abondance

The abundance of a chemical element being lower than a reference value, in particular compared to that of the Sun.

Etymology (EN):under-; → abundance.

  کم‌میرایی  
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.

See also:under-; → damping.

  کم‌میرایی  
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.

See also:under-; → damping.

  ۱) کم-بر‌آوردن؛ ۲) کم-بر‌آورد  
1) kam-baravardan; 2) kam-baravard
Fr.: 1) sous-estimer; 2) sous-estimation
  1. To estimate at too low a value, rate, or the like.
  2. An estimate that is too low. → overestimate.

See also:under-; → estimate

  ۱) کم-بر‌آوردن؛ ۲) کم-بر‌آورد  
1) kam-baravardan; 2) kam-baravard
Fr.: 1) sous-estimer; 2) sous-estimation
  1. To estimate at too low a value, rate, or the like.
  2. An estimate that is too low. → overestimate.

See also:under-; → estimate

  کمچوناییده، کمچونامند  
kamcunâyide, kamcunâmand
Fr.: sousqualifié

Insufficiently qualified for a particular job (OxfordDictionaries.com).

See also:under-; → qualified.

  کمچوناییده، کمچونامند  
kamcunâyide, kamcunâmand
Fr.: sousqualifié

Insufficiently qualified for a particular job (OxfordDictionaries.com).

See also:under-; → qualified.

  کم‌نمونان‌گیری  
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.

See also:under-; → sampling.

  کم‌نمونان‌گیری  
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.

See also:under-; → sampling.

  فهمیدن  
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.

  فهمیدن  
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.

  فهم  
fahm (#)
Fr.: compréhension, entendement, intelligence

The ability to understand something; the → power of → abstract  → thought.

See also:understand; → -ing.

  فهم  
fahm (#)
Fr.: compréhension, entendement, intelligence

The ability to understand something; the → power of → abstract  → thought.

See also:understand; → -ing.

  ناترمیده  
nâtarmidé
Fr.: indéterminé
  1. Not definitely or authoritatively decided or settled.

    1. Not known.

See also:un-; → determined.

  ناترمیده  
nâtarmidé
Fr.: indéterminé
  1. Not definitely or authoritatively decided or settled.

    1. Not known.

See also:un-; → determined.

  شهاب‌سنگ ِ نا-دگرسانیده  
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.

  شهاب‌سنگ ِ نا-دگرسانیده  
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.

  موجش  
mowješ
Fr.: ondulation

A wave; the motion of waves.
A wavelike motion in any medium.

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 mowjwave.

  موجش  
mowješ
Fr.: ondulation

A wave; the motion of waves.
A wavelike motion in any medium.

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 mowjwave.

  یک-  
yek- (#)
Fr.: uni-

A prefix with the meaning of “one” occurring in loanwords from L., such as → uniform, → uniaxial, → universe, etc.

Etymology (EN): From uni- a combining form meaning “one,” from L. uni-, from unus, → one;

Etymology (PE): Yek-, from yek, → one.

  یک-  
yek- (#)
Fr.: uni-

A prefix with the meaning of “one” occurring in loanwords from L., such as → uniform, → uniaxial, → universe, etc.

Etymology (EN): From uni- a combining form meaning “one,” from L. uni-, from unus, → one;

Etymology (PE): Yek-, from yek, → one.

  بلور ِ یک‌آسه  
bolur-e yek-âsé
Fr.: cristal uniaxe

Crystal with double refraction possessing only one → optic axis.

See also:uni-; axial adj. from → axis; → crystal.

  بلور ِ یک‌آسه  
bolur-e yek-âsé
Fr.: cristal uniaxe

Crystal with double refraction possessing only one → optic axis.

See also:uni-; axial adj. from → axis; → crystal.

  نا-ایدانیده  
nâ-idânidé
Fr.: non identifié

The attribute of someone or something whose identity is not established. → unidentified flying object; → unidentified line.

See also:un-; → identify.

  نا-ایدانیده  
nâ-idânidé
Fr.: non identifié

The attribute of someone or something whose identity is not established. → unidentified flying object; → unidentified line.

See also:un-; → identify.

  بر‌آخت ِ پرنده‌ی ِ نا-ایدانیده، پدیده‌ی ِ هوا-فضایی ِ نا-ایدانیده  
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.

  بر‌آخت ِ پرنده‌ی ِ نا-ایدانیده، پدیده‌ی ِ هوا-فضایی ِ نا-ایدانیده  
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.

  باند ِ فروسرخ ِ نا-ایدانیده  
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.

  باند ِ فروسرخ ِ نا-ایدانیده  
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.

  خط ِ نا-ایدانیده  
xatt-e nâ-idânidé
Fr.: raie non identifiée

A spectral line whose origin is not clearly established. → line identification.

See also:unidentified; → line.

  خط ِ نا-ایدانیده  
xatt-e nâ-idânidé
Fr.: raie non identifiée

A spectral line whose origin is not clearly established. → line identification.

See also:unidentified; → line.

  یگانش  
yegâneš
Fr.: unification
  1. The process of unifying or uniting; union.

  2. The state or condition of being unified (Dictionary.com).

See also: Verbal noun of → unify.

  یگانش  
yegâneš
Fr.: unification
  1. The process of unifying or uniting; union.

  2. The state or condition of being unified (Dictionary.com).

See also: Verbal noun of → unify.

  یکدیس، یکنواخت  
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,
form; yeknavâxt, literally “with one rhythm,”
from yek, → one, + navâxt “rhythm,” from navâxtan, navâzidan “to play an instrument; to gratify,” navâ “music, song, melody” (Mid.Pers. nw’c “to treat kindly, honour,” niwag “music, melody;” Proto-Iranian *ni-uac-, from ni- “down; into,” → ni- (PIE),

  • *uac- “to speak, treat kindly”).
  یکدیس، یکنواخت  
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,
form; yeknavâxt, literally “with one rhythm,”
from yek, → one, + navâxt “rhythm,” from navâxtan, navâzidan “to play an instrument; to gratify,” navâ “music, song, melody” (Mid.Pers. nw’c “to treat kindly, honour,” niwag “music, melody;” Proto-Iranian *ni-uac-, from ni- “down; into,” → ni- (PIE),

  • *uac- “to speak, treat kindly”).
  جنبش ِ دایره‌ای ِ یکدیس، ~ ~ یکنواخت  
jonbeš-e dâyereyi-ye yekdis, ~ ~ yeknavâxt
Fr.: mouvement circulaire uniforme

The motion of an object around a fixed point at a constant angular speed, and at constant radius.

See also:uniform; → circular; → motion.

  جنبش ِ دایره‌ای ِ یکدیس، ~ ~ یکنواخت  
jonbeš-e dâyereyi-ye yekdis, ~ ~ yeknavâxt
Fr.: mouvement circulaire uniforme

The motion of an object around a fixed point at a constant angular speed, and at constant radius.

See also:uniform; → circular; → motion.

  میدان ِ یکدیس، ~ ِ یکنواخت  
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.

  میدان ِ یکدیس، ~ ِ یکنواخت  
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.

  میدان ِ مغناتیسی ِ یکدیس  
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.

See also:uniform; → magnetic; → field.

  میدان ِ مغناتیسی ِ یکدیس  
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.

See also:uniform; → magnetic; → field.

  جنبش ِ یکدیس، ~ ِ یکنواخت  
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.

  جنبش ِ یکدیس، ~ ِ یکنواخت  
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.

  یکدیسوار  
yekdisvâr
Fr.: uniformitaire
  1. Of, characterized by, or conforming to → uniformity.

    1. Of or relating to → uniformitarianism.

See also:uniformity + -arian.

  یکدیسوار  
yekdisvâr
Fr.: uniformitaire
  1. Of, characterized by, or conforming to → uniformity.

    1. Of or relating to → uniformitarianism.

See also:uniformity + -arian.

  یکدیسوارباوری  
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.

  یکدیسوارباوری  
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.

  یکدیسواری، یکدیسیگی  
yekdisvâri, yekdisigi
Fr.: uniformité

The state or quality of being uniform.

See also:uniform; → -ity.

  یکدیسواری، یکدیسیگی  
yekdisvâri, yekdisigi
Fr.: uniformité

The state or quality of being uniform.

See also:uniform; → -ity.

  یگانستن، یگانیدن  
yegânestan (#), yegânidan (#)
Fr.: unifier

To make or become a single unit or entity.
grand unified theory

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,
one.

  یگانستن، یگانیدن  
yegânestan (#), yegânidan (#)
Fr.: unifier

To make or become a single unit or entity.
grand unified theory

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,
one.

  ناویناردنی  
nâvinârdani
Fr.: inimaginable

Difficult or impossible to believe.

See also:un-; → imaginable.

  ناویناردنی  
nâvinârdani
Fr.: inimaginable

Difficult or impossible to believe.

See also:un-; → imaginable.

  یکایش  
yekâyeš
Fr.: union

General: The act of uniting two or more things.
A number of persons, organizations, states, etc., joined or associated together for some common purpose, e.g. → International Astronomical Union (IAU).
Math.: A set containing all the elements of two or more sets being combined.
It is represented by ∪.

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,

  • -ây- epenthetic vowel, + -eš verbal noun suffix, → -tion.
  یکایش  
yekâyeš
Fr.: union

General: The act of uniting two or more things.
A number of persons, organizations, states, etc., joined or associated together for some common purpose, e.g. → International Astronomical Union (IAU).
Math.: A set containing all the elements of two or more sets being combined.
It is represented by ∪.

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,

  • -ây- epenthetic vowel, + -eš verbal noun suffix, → -tion.
  یکتا  
yektâ (#)
Fr.: unique

Existing as the only one or as the sole example.
Limited to a single outcome or result. → uniqueness theorem.

Etymology (EN): From Fr. unique, from L. unicus “single, sole,” from unus, → one.

Etymology (PE): Yektâ “unique,” from yek, → one,

  • “fold, plait, ply; piece, part” (Mid.Pers. tâg “piece, part”).
  یکتا  
yektâ (#)
Fr.: unique

Existing as the only one or as the sole example.
Limited to a single outcome or result. → uniqueness theorem.

Etymology (EN): From Fr. unique, from L. unicus “single, sole,” from unus, → one.

Etymology (PE): Yektâ “unique,” from yek, → one,

  • “fold, plait, ply; piece, part” (Mid.Pers. tâg “piece, part”).
  یکتایی  
yektâyi (#)
Fr.: unicité

The state or condition of being → unique.

See also: Noun from → unique.

  یکتایی  
yektâyi (#)
Fr.: unicité

The state or condition of being → unique.

See also: Noun from → unique.

  فربین ِ یکتایی  
farbin-e yektâyi
Fr.: théorème d'unicité
  1. Physics: A → potential that satisfies both → Poisson’s equation and the → boundary conditions pertinent to a particular field is the only possible potential.

  2. Math.: If two → continuous functions φ(t) and ψ(t) have one and the same → Laplace transform F(p), then these functions are identically equal.

  3. Astro.: A → black hole can only be characterized by its → mass, → electric charge, and → angular momentum. See also → no hair theorem.

See also:uniqueness; → theorem.

  فربین ِ یکتایی  
farbin-e yektâyi
Fr.: théorème d'unicité
  1. Physics: A → potential that satisfies both → Poisson’s equation and the → boundary conditions pertinent to a particular field is the only possible potential.

  2. Math.: If two → continuous functions φ(t) and ψ(t) have one and the same → Laplace transform F(p), then these functions are identically equal.

  3. Astro.: A → black hole can only be characterized by its → mass, → electric charge, and → angular momentum. See also → no hair theorem.

See also:uniqueness; → theorem.

  یکا، یکان  
yekâ (#), yekân (#)
Fr.: unité

A quantity or dimension adopted as a standard of measurement.
Math.: The lowest positive natural number.
The first digit to the left of the decimal point in decimal notation, representing a whole number less than ten.
An element in a ring that has a multiplicative inverse.

Etymology (EN): Back formation from → unity.

Etymology (PE): Yekâ, yekân, from yek, → one.

  یکا، یکان  
yekâ (#), yekân (#)
Fr.: unité

A quantity or dimension adopted as a standard of measurement.
Math.: The lowest positive natural number.
The first digit to the left of the decimal point in decimal notation, representing a whole number less than ten.
An element in a ring that has a multiplicative inverse.

Etymology (EN): Back formation from → unity.

Etymology (PE): Yekâ, yekân, from yek, → one.

  بردار ِ یکا  
bordâr-e yekâ
Fr.: vecteur unité

A vector of length 1, also called a direction vector.

See also:unit; → vector.

  بردار ِ یکا  
bordâr-e yekâ
Fr.: vecteur unité

A vector of length 1, also called a direction vector.

See also:unit; → vector.

  یکاییگی  
yekâyigi
Fr.: unitarité
  1. The condition of being → unitary.

    1. quantum unitarity.

See also:unitary; → -ity.

  یکاییگی  
yekâyigi
Fr.: unitarité
  1. The condition of being → unitary.

    1. quantum unitarity.

See also:unitary; → -ity.

  یکایی  
yekâyi
Fr.: unitaire
  1. Of or pertaining to a unit or units; having the indivisible character of a unit.

  2. Math.: An → operator  U satisfying the relations: U+ U = 1, U U+ = 1, where U+ is the → adjoint .

See also:unit + -ary.

  یکایی  
yekâyi
Fr.: unitaire
  1. Of or pertaining to a unit or units; having the indivisible character of a unit.

  2. Math.: An → operator  U satisfying the relations: U+ U = 1, U U+ = 1, where U+ is the → adjoint .

See also:unit + -ary.

  گروه ِ یکایی، ~ یکانی  
goruh-e yekâyi, ~ yekâni
Fr.: groupe unitaire

The set of n × n unitary matrices (→ unitary matrix).

See also:unitary; → group.

  گروه ِ یکایی، ~ یکانی  
goruh-e yekâyi, ~ yekâni
Fr.: groupe unitaire

The set of n × n unitary matrices (→ unitary matrix).

See also:unitary; → group.

  ماتریس ِ یکایی، ~ یکانی  
mâtris-e yekâyi, ~ yekâni
Fr.: matrice unitaire

A square matrix whose inverse equals its adjoint.

See also:unitary; → matrix.

  ماتریس ِ یکایی، ~ یکانی  
mâtris-e yekâyi, ~ yekâni
Fr.: matrice unitaire

A square matrix whose inverse equals its adjoint.

See also:unitary; → matrix.

  آپارگر ِ یکایی  
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.

See also:unitary; → operator.

  آپارگر ِ یکایی  
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.

See also:unitary; → operator.

  ترادیس ِ یکایی، ~ یکانی  
tarâdis-e yekâyi, ~ yekâni
Fr.: transformation unitaire

A transformation whose reciprocal is equal to its Hermitian conjugate.

See also:unitary; → transformation.

  ترادیس ِ یکایی، ~ یکانی  
tarâdis-e yekâyi, ~ yekâni
Fr.: transformation unitaire

A transformation whose reciprocal is equal to its Hermitian conjugate.

See also:unitary; → transformation.

  آیکیدن، هم‌یکیدن  
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-,

  • yekidan.
  آیکیدن، هم‌یکیدن  
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-,

  • yekidan.
  آیکیده، هم‌یکیده  
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.

  آیکیده، هم‌یکیده  
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.

  یکی  
yeki (#)
Fr.: unité

The state or condition of being one.
Math.: One.

Etymology (EN): M.E. unite, from O.Fr., from L. unitatem “oneness, sameness, agreement,” from unus, → one.

Etymology (PE): Yeki, noun from yek, → one.

  یکی  
yeki (#)
Fr.: unité

The state or condition of being one.
Math.: One.

Etymology (EN): M.E. unite, from O.Fr., from L. unitatem “oneness, sameness, agreement,” from unus, → one.

Etymology (PE): Yeki, noun from yek, → one.

  یکورتا  
yekvartâ
Fr.: univarié

Statistics: Involving only one variable.

See also:uni-; → variate.

  یکورتا  
yekvartâ
Fr.: univarié

Statistics: Involving only one variable.

See also:uni-; → variate.

  سری ِ زمانی ِ یکورتا  
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.

  سری ِ زمانی ِ یکورتا  
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.

  ۱) هرگانی؛ گیتیک، گیتیانه؛ جهانی؛ ۲) هرگانه  
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.

  1. A trait, characteristic, or property, as distinguished from a particular individual or event, that can be possessed in common, as the care of a mother for her young (Dictionary.com).

See also:

Coordinated Universal Time, → universal astrolabe, → universal gas constant, → universal IMF, → universal quantifier, → Universal Time.

Related concepts:

all, → general, → omni-, → public, → total.

See also:universe; → -al.

  ۱) هرگانی؛ گیتیک، گیتیانه؛ جهانی؛ ۲) هرگانه  
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.

  1. A trait, characteristic, or property, as distinguished from a particular individual or event, that can be possessed in common, as the care of a mother for her young (Dictionary.com).

See also:

Coordinated Universal Time, → universal astrolabe, → universal gas constant, → universal IMF, → universal quantifier, → Universal Time.

Related concepts:

all, → general, → omni-, → public, → total.

See also:universe; → -al.

  اسطرلاب ِ هرگانی  
ostorlâb-e hargâni
Fr.: astrolabe universel

An → astrolabe which could be used at any → latitude.

See also:universal; → astrolabe.

  اسطرلاب ِ هرگانی  
ostorlâb-e hargâni
Fr.: astrolabe universel

An → astrolabe which could be used at any → latitude.

See also:universal; → astrolabe.

  پایای ِ هرگانی ِ گاز‌ها  
pâyâ-ye hargâni-ye gâzhâ
Fr.: constante universelle des gaz

Same as → gas constant.

See also:universal; → gas; → constant.

  پایای ِ هرگانی ِ گاز‌ها  
pâyâ-ye hargâni-ye gâzhâ
Fr.: constante universelle des gaz

Same as → gas constant.

See also:universal; → gas; → constant.

  IMF ِ هرگانی  
IMF-e hargâni
Fr.: IMF universelle

Same as → canonical IMF.

See also:universal; → initial mass function.

  IMF ِ هرگانی  
IMF-e hargâni
Fr.: IMF universelle

Same as → canonical IMF.

See also:universal; → initial mass function.

  چنداگر ِ هروین  
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.

  چنداگر ِ هروین  
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.

  زمان ِ جهانی  
zamân-e jahâni
Fr.: temps universel

A measure of time that conforms, within a close approximation, to the mean diurnal motion of the Sun and serves as the basis off all civil timekeeping. The local civil time for a position on the Greenwich meridian.

See also:universal; → time.

  زمان ِ جهانی  
zamân-e jahâni
Fr.: temps universel

A measure of time that conforms, within a close approximation, to the mean diurnal motion of the Sun and serves as the basis off all civil timekeeping. The local civil time for a position on the Greenwich meridian.

See also:universal; → time.

  زمان ِ جهانی ِ همرایانیده  
zamân-e jahâni-ye hamrâyânidé
Fr.: temps universel coordonné
  زمان ِ جهانی ِ همرایانیده  
zamân-e jahâni-ye hamrâyânidé
Fr.: temps universel coordonné
  هرگانیگی  
hargânigi
Fr.: universalité

The character or state of being universal.

See also:universal; → -ity.

  هرگانیگی  
hargânigi
Fr.: universalité

The character or state of being universal.

See also:universal; → -ity.

  هرگانیگی ِ افت ِ آزاد  
hargânigi-ye oft-e âzâd
Fr.: universlité de chute libre

Same as → weak equivalence principle.

See also:universality; → free; → fall.

  هرگانیگی ِ افت ِ آزاد  
hargânigi-ye oft-e âzâd
Fr.: universlité de chute libre

Same as → weak equivalence principle.

See also:universality; → free; → fall.

  هرگانی ِ کریای ِ آغازین ِ جرم  
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.

  هرگانی ِ کریای ِ آغازین ِ جرم  
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.

  ۱) گیتی؛ ۲) هرگان  
1) giti (#); 2) hargân
Fr.: univers
  1. The totality of all matter and energy that exists in the vastness of cosmos whether known to human beings or not. Related concepts: → world,
    cosmos,
    multiverse.

2a) Math.: A → set made of
subsets that contains all the elements relevant to a particular discussion or problem.

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;”
Mid.Pers. gêhân “world,” gêtig “the material world; wordly;” Av. gaēθā- “being, world, matter, mankind,” gaya- “life, manner of living”, root gay- “to live” (present tense jiva-), O.Pers. gaiθā- “live-stock,” cognate with Skt. jīv- “to live,” jīva- “alive, living;” Gk. bios “life,” L. vivus “living, alive,” vita “life;” PIE base *gwei- “to live” (cf. O.E. cwic “alive;” O.C.S. zivo “to live;” Lith. gyvas “living, alive;” O.Ir. bethu “life,” bith “age;” Welsh byd “world”). The Pers. words zistan “to live,” zendé “alive,” zendegi “life,” and jân “vital spirit, soul; mind” belong to this family.

  1. Hargân, from har “every, all, each,” → holo-,
  • -gân suffix forming plural entities, from Mid.Pers. -gânag, -gâna, on the model of hamegân, → public.
  ۱) گیتی؛ ۲) هرگان  
1) giti (#); 2) hargân
Fr.: univers
  1. The totality of all matter and energy that exists in the vastness of cosmos whether known to human beings or not. Related concepts: → world,
    cosmos,
    multiverse.

2a) Math.: A → set made of
subsets that contains all the elements relevant to a particular discussion or problem.

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;”
Mid.Pers. gêhân “world,” gêtig “the material world; wordly;” Av. gaēθā- “being, world, matter, mankind,” gaya- “life, manner of living”, root gay- “to live” (present tense jiva-), O.Pers. gaiθā- “live-stock,” cognate with Skt. jīv- “to live,” jīva- “alive, living;” Gk. bios “life,” L. vivus “living, alive,” vita “life;” PIE base *gwei- “to live” (cf. O.E. cwic “alive;” O.C.S. zivo “to live;” Lith. gyvas “living, alive;” O.Ir. bethu “life,” bith “age;” Welsh byd “world”). The Pers. words zistan “to live,” zendé “alive,” zendegi “life,” and jân “vital spirit, soul; mind” belong to this family.

  1. Hargân, from har “every, all, each,” → holo-,
  • -gân suffix forming plural entities, from Mid.Pers. -gânag, -gâna, on the model of hamegân, → public.
  دانشگاه  
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,

  • -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”).
  دانشگاه  
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,

  • -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”).
  یکواز  
yekvâz
Fr.: univoque
  1. Having one meaning only.
  2. A word or term that has only one meaning

See also: L.L. univocus, from L. → uni- + voc-, vox, → voice. “voice,”

  یکواز  
yekvâz
Fr.: univoque
  1. Having one meaning only.
  2. A word or term that has only one meaning

See also: L.L. univocus, from L. → uni- + voc-, vox, → voice. “voice,”

  یکوازی  
yekvâzi
Fr.: monosémie

The character of being → univocal. Same as → monosemy.

See also:univocal; → ity.

  یکوازی  
yekvâzi
Fr.: monosémie

The character of being → univocal. Same as → monosemy.

See also:univocal; → ity.

  نادانست  
nâdânest
Fr.: inconnu

Math.: A → variable or → function whose → value is to be found.

See also:un-, + known, p.p. of → know.

  نادانست  
nâdânest
Fr.: inconnu

Math.: A → variable or → function whose → value is to be found.

See also:un-, + known, p.p. of → know.

  واخباندن  
vâxabândan
Fr.: activer le son

To remove a mute from (a musical instrument).

See also:un-; → mute.

  واخباندن  
vâxabândan
Fr.: activer le son

To remove a mute from (a musical instrument).

See also:un-; → mute.

  ناشونیک  
nâšunik
Fr.: non ordinaire

Uncommon, unusual. → extraordinary.

See also:un-; → ordinary.

  ناشونیک  
nâšunik
Fr.: non ordinaire

Uncommon, unusual. → extraordinary.

See also:un-; → ordinary.

  نور ِ ناقطبیده  
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
occur in all possible planes. Ordinary light emitted by the Sun, by a living room lamp,
or by a candle flame is unpolarized light. → polarization.

See also:un-; → polarized light.

  نور ِ ناقطبیده  
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
occur in all possible planes. Ordinary light emitted by the Sun, by a living room lamp,
or by a candle flame is unpolarized light. → polarization.

See also:un-; → polarized light.

  ناچوناییده، ناچونامند  
nâcunâyid, nâcunâmand
Fr.: non qualifié

Not qualified; not fit; lacking requisite qualifications (Dictionary.com).

See also:un-; → qualified.

  ناچوناییده، ناچونامند  
nâcunâyid, nâcunâmand
Fr.: non qualifié

Not qualified; not fit; lacking requisite qualifications (Dictionary.com).

See also:un-; → qualified.

  ستاره‌ی ِ ناسرخیده  
setâre-ye nâsorxidé
Fr.: étoile non rougie

A star whose light is not affected by→ interstellar absorption. → reddening

See also:un-; → reddened star.

  ستاره‌ی ِ ناسرخیده  
setâre-ye nâsorxidé
Fr.: étoile non rougie

A star whose light is not affected by→ interstellar absorption. → reddening

See also:un-; → reddened star.

  ناواگشوده  
nâvâgošudé
Fr.: non résolu

Describing an image whose constituent or elementary parts are not resolved. → unresolved source.

See also:un- + → resolved.

  ناواگشوده  
nâvâgošudé
Fr.: non résolu

Describing an image whose constituent or elementary parts are not resolved. → unresolved source.

See also:un- + → resolved.

  خن ِ ناواگشوده  
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.

  خن ِ ناواگشوده  
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.

  وینه‌ی ِ ناتیگ، تصویر ِ ~  
vine-ye nâtig, tasvir-e ~
Fr.: image floue

An image in which finer details are not visible. → blurred image

See also:un-; → sharp image.

  وینه‌ی ِ ناتیگ، تصویر ِ ~  
vine-ye nâtig, tasvir-e ~
Fr.: image floue

An image in which finer details are not visible. → blurred image

See also:un-; → sharp image.

  ماسک‌زد ِ ناتیگ  
mâskzad-e nâtig
Fr.: masque floue

A process for amplifying fine details in a registered image. Generally speaking, the process consists of creating a mask which contains larger scale features of the image and then subtracting the mask from the initial image.

See also:un-; → sharp; → masking.

  ماسک‌زد ِ ناتیگ  
mâskzad-e nâtig
Fr.: masque floue

A process for amplifying fine details in a registered image. Generally speaking, the process consists of creating a mask which contains larger scale features of the image and then subtracting the mask from the initial image.

See also:un-; → sharp; → masking.

  ناپایدار  
nâpâydâr (#)
Fr.: instable

Not → stable, as in → unstable atom, → unstable equilibrium.

See also:un-; → stable.

  ناپایدار  
nâpâydâr (#)
Fr.: instable

Not → stable, as in → unstable atom, → unstable equilibrium.

See also:un-; → stable.

  اتم ِ ناپایدار  
atom-e nâpâydâr (#)
Fr.: atome instable

An atom whose nuclei → decay by → radioactivity.

See also:unstable; → atom.

  اتم ِ ناپایدار  
atom-e nâpâydâr (#)
Fr.: atome instable

An atom whose nuclei → decay by → radioactivity.

See also:unstable; → atom.

  ترازمندی ِ ناپایدار  
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,
the system is in an unstable equilibrium. → stable equilibrium.

See also:unstable; → equilibrium.

  ترازمندی ِ ناپایدار  
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,
the system is in an unstable equilibrium. → stable equilibrium.

See also:unstable; → equilibrium.

  عنق‌الحیّه  
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.
Unukalhai is in fact a triple star system. The second star (α Serpentis B) is 58 arcseconds from the primary and has a magnitude of 11.8. The third star (α Serpentis C), 13th magnitude, lies 2.3 arcminutes from A. Other designations: Cor Serpentis, HR 5854, HD 140573.

See also: From Ar. ‘unuq al-hayyah (عنق‌الحیه) “Neck of the Snake,” from ‘unuq “neck” + al-hayyah “snake.”

  عنق‌الحیّه  
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.
Unukalhai is in fact a triple star system. The second star (α Serpentis B) is 58 arcseconds from the primary and has a magnitude of 11.8. The third star (α Serpentis C), 13th magnitude, lies 2.3 arcminutes from A. Other designations: Cor Serpentis, HR 5854, HD 140573.

See also: From Ar. ‘unuq al-hayyah (عنق‌الحیه) “Neck of the Snake,” from ‘unuq “neck” + al-hayyah “snake.”