An Etymological Dictionary of Astronomy and Astrophysics
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فرهنگ ریشه شناختی اخترشناسی-اخترفیزیک

M. Heydari-Malayeri    -    Paris Observatory

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Number of Results: 13116 Search : far
multiplet
  بستایه   
bastâyé

Fr.: multiplet   

A group of spectral lines arising from transitions having a common lower energy level.

From → multi- + -plet on the model of triplet.

Bastâyé, from bastâ-multi- + euphonic -yé, from nuance suffix.

multiplicand
  بستاشو   
bastâšow

Fr.: multiplicande   

A number to be multiplied by another.

From L. multiplicandum, from multiplicandus "to be multiplied," gerundive of multiplicare, → multiply.

Bastâšow, literally "that undergoes multiplication," from bastâ, → multiple, + šow, present stem and agent noun of šodan "to become, to be, to be doing, to go, to pass," from Mid.Pers. šudan, šaw- "to go;" Av. šiyav-, š(ii)auu- "to move, go," šiyavati "goes," šyaoθna- "activity; action; doing, working;" O.Pers. šiyav- "to go forth, set," ašiyavam "I set forth;" cf. Skt. cyu- "to move to and fro, shake about; to stir," cyávate "stirs himself, goes;" Gk. kinein "to move;" Goth. haitan "call, be called;" O.E. hatan "command, call;" PIE base *kei- "to move to and fro."

multiplication
  بستایش   
bastâyeš

Fr.: multiplication   

In general, the process of repeatedly adding a quantity to itself a certain number of times, or any other process which has the same result.

Verbal noun of → multiply.

multiplication sign
  نشانه‌ی ِ بستایش   
nešâne-ye bastâyeš

Fr.: croix de multiplication   

The sign used to indicate multiplication, either a times sign (×), a centered dot (·), or an asterisk. The multiplication sign was introduced by William Oughtred in 1631.

multiplication; → sign.

multiplicative
  بستایشی   
bastâyeši

Fr.: multiplicatif   

Involving → multiplication.

From multiplicate, → multiply, + → -ive.

multiplicative identity
  ایدانی ِ بستایشی   
idâni-ye bastâyeši

Fr.: identité multiplicative   

The number which when used as the multiplier of another number leaves the second unchanged; one.

multiplicative; → identity.

multiplicative inverse
  وارون ِ بستایشی   
vârun-e bastâyeši

Fr.: inverse multiplicative   

The number which when used as a multiplier of another number (except 0) produces 1. For example (1/5) x 5 = 1; each of the numbers is the multiplicative inverse of the other.

multiplicative; → inverse.

multiplicity
  بستاییگی   
bastâyigi

Fr.: multiplicité   

1) The state of being multiple, made of several components.
2) In atomic and nuclear physics, the number of → levels into which the energy of an atom, molecule, or nucleus splits as a result of → Russell-Saunders coupling between → orbital angular momentum and → spin angular momentum. It is given by 2S+1, where S is the total electron → spin quantum number. The multiplicity of an energy level is indicated by a left superscript to the value of L, where L is the resultant electron orbital angular momentum of the individual electron orbital angular momenta.
3) In → statistical mechanics, the number of → microstates corresponding to a given → macrostate.

multiple; → -ity.

multiplier
  بستاگر   
bastâgar

Fr.: multiplicateur   

Arithmetic: A number by which another is multiplied. Physics: A device for intensifying some effect.

Agent noun of → multiply.

multiply
  بستاییدن   
bastâyidan

Fr.: multiplier   

To make many or manifold; increase the number, quantity, etc., of.
Arithmetic: To find the product of by multiplication.

O.Fr. multiplier, from L. multiplicare "to increase," from multiplex (gen. multiplicis) "having many folds, many times as great in number," from multi- "many" + base of plicare "to lay, fold, twist."

Bastâyidan, from bastâ, → multiple, + -idan infinitive suffix.

multipole
  بس‌قطبه   
basqotbé

Fr.: multipôle   

An entity consisting of several poles.

multi-; → pole.

multipole index
  دیشن ِ بس‌قطبه   
dišan-e basqotbé

Fr.: indice multipolaire   

A variable used in → spherical harmonic expansions. Each spherical harmonic is characterized by its multipole index l: l = 0 for a → monopole, l = 1 for a → dipole, and so on. It is used in particular to describe the → cosmic microwave background anisotropy: ΔT/T0 (θ,φ) = Σ almYlm(θ,φ), where θ and φ are the → spherical polar coordinates, Ylm is the → spherical harmonic functions, and the sum runs over l = 1, 2, ..., ∞ and m = -l, ..., l, where the multipole index l corresponds to angular scales ≅ 180°/l.

multipole; → index.

multipole moment
  گشتاور ِ بس‌قطبه   
gaštâvar-e basqotbé

Fr.: moment multipolaire   

The quantity that gives the electric potential field due to a distribution of charges, such as a → dipole, → quadrupole, → octupole, etc. A multipole moment usually involves powers of the distance to the origin, as well as some angular dependence.

multi-; → pole; → moment.

multitude
  بسینه   
basiné

Fr.: multitude   

1) A great number.
2) A great number of people gathered together; crowd; throng.
3) The state or character of being many; numerousness.

M.E., from O.Fr. multitude and directly from L. multitudo "a great number, a crowd; the common people," from multus "many, much," → multi-, + suffix -tudo "-tude."

Basiné, from basin + superlative of bas "many, much," → multi-, + suffix -in + noun/nuance suffix (as bišiné, kaminé, etc.).

multivariate
  بسورتا   
basvartâ

Fr.: multivarié   

Statistics: Having more than one → variable.

multi-; → variate.

multivariate time series
  سری ِ زمانی ِ بسورتا   
seri-ye zamâni-ye basvartâ

Fr.: série temporelle multivariée   

A → time series consisting of two or more → univariate time series which share the same time period. As an example, if we record wind velocity and wind direction at the same instant of time, we have a multi-variate time series, specifically a bivariate one.

multivariate; → time; → series.

multiverse
  گیتی‌گان   
gitigân

Fr.: multivers   

A → hypothetical set of → multiple universes, including our → Universe, that together comprise all of physical reality.

Initially coined by William James (1895) "an alternative to universe meant to convey absence of order and unity." In modern cosmology coined from -verse in → universe, by replacing uni- with multi- to denote "multiple universes."

Gitigân, from giti, → universe, + -gân multiplicity suffix.

multiwire proportional chamber
  اتاقک ِ بسیار-سیم ِ برپارشی   
otâqak-e besyâr-sim-e barpâreši

Fr.: chambre proportionnelle multifils   

Same as → Charpak's detector.

multi-; → wire; → proportional; → chamber.

muon
  موءون   
muon (#)

Fr.: muon   

A short-lived → elementary particle with negative → electric charge, represented by the symbol μ-. The muon was discovered in 1936 by Carl Anderson (1905-1991) in → cosmic rays. It shares several properties with the electron: it is a → lepton with the same charge and → spin as the electron. But it is heavier than the electron (105 MeV/c2), about 200 times more massive. The muon is instable and decays after 2.197 × 10-6 s into → electron, → neutrino, and → antineutrino-e- + νμ + anti νe) .

A shortening of mu meson, from mu the 12th letter of the Gk. alphabet, + → meson.

muon telescope
  تلسکوپ ِ موءونی   
teleskop-e muoni

Fr.: télescope muonique   

An → instrument used in → geophysics to determine the average → density of geological bodies by measuring the → attenuation produced by → rocks on the flux of → atmospheric muons. This density muon → radiography is or example used to study the physical conditions inside → volcanoes.

muon; → telescope.

<< < -es -iv -ti 21 a p abe abs abs aca acc acc acr act ada adh Adr aer aga air Alf Alg alk Alp alt alu amm ana And ang ani ano ant ant Ap apo app app Aqu Arc arg arr asc ass ast ast asy atm ato att aur aut axi B-m bad Bal bar bar Bay Bed ber Bet bif bim bin bio bis bla ble blu Bod Bol bor bou Bra Bre bro bul C-t Cal Cam can car Car Cas cat cav cel cen cer Cha cha Cha che chl Cir cir cir Cla cli clo clu co- coc coh col col col Com com com com com com com com Com con con con con con con con con con con con con coo Cor Cor cor cos cos cos Cou cou Cra Cre cri cro cub cur cyc cyl Dan dat Dav de- Deb dec dec dee def deg del Den den der det deu dew dic dif dif dil Dip dir dis dis dis dis dis diu dod Dop dou Dra dua dus dwa dyn DZ Ear ecc eco edi EHB Ein ela ele ele ele ele ell eme emp end Eng ent epi equ equ era ESP eth Eur evi exa exc exe exi exp exp ext ext ext fac fal far fec Fer fer fie fin fir fis fla Flo flu fog for for Fou fra fre fre Fro fun G s Gal gal gal Gar gau geg gen geo geo geo ger gla gly gra gra gra gra gra Gre gro GYR Had Hal hap Har HD hea hel hel Hen Her hex hig Hil hol Hoo hor hou Hub hum hyb hyd hyd hyp hys ide ign ima imp imp in- inc Ind ind ine inf inf inf ini ins ins ins int int int int Int int int int inv ion iri irr iso iso iso Jea Jor jum K c Kep Ker kin kno lab Lam Lan Lap las lat Le lef len lev lig lig lin lin lin liq Lit loc log lon lou LS lun lun Lym M s Mag mag mag mag mag mag maj man Mar mas mas mat May mea mec mel mer mes met met met mic mid mil Min Mir mix mod mod mol mon mor mov mul mur mys nan nat nav nec Nep neu New New NGC nob nom non non nor nos nuc nuc num nut obj obl obs occ oct off oli oni ope opp opt opt orb ord org orp osc out ove oxi P-w pal par par par par Pas pat pej per per per per per per pha Phe pho pho pho phy pin pla Pla pla pla pla plu poi pol pol Pol pol por pos pot Poy pre pre pre pre pri pri pri pro pro pro pro pro pro Psa pul pum Q i qua qua qua qua R A rad rad rad rad rad rad Ram Ran rat rea rea rec rec red red ref ref reg rei rel rel rem rep res res res ret rev Rho Rie ril riv rog Ros rot rul S A Sag sam sat sca sca Sch Sco Sec sec sec seg sel sem sen set Sha sha shi sho sid sig sim sin Sir ske sli Smo soc sof sol sol sol sol sou sou spa spe spe Spe spe sph spi Spi spr sta sta sta sta sta ste ste ste Sto str str sub sub sub suc sun sup sup sup sup sur swa syn syn tac tas tel tem ter tes the the the the thi thr tid til tip ton tor tou tra tra tra tra Tri tri tru tsu tur two Typ UHE ult unc uni uni uni upg ura uti val var vec Vel ver Ver vie Vir vis vis vol W-R war wav wav wea Wei wha wid win WN3 Wol wri xen yok zen zij > >>