An Etymological Dictionary of Astronomy and Astrophysics
English-French-Persian

فرهنگ ریشه شناختی اخترشناسی-اخترفیزیک

M. Heydari-Malayeri    -    Paris Observatory

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Number of Results: 13176 Search : far
Reaumur scale
  مرپل ِ ریءومور   
marpel-e Réaumur

Fr.: échelle Réaumur   

A temperature scale in which the → freezing point and the → boiling point of → water are set to 0 and 80 degrees respectively. See also → Celsius scale, → Fahrenheit scale, → Kelvin scale, → Rankine scale.

Named after René Antoine Ferchault de Réaumur (1683-1757), who first proposed it in 1730; → scale.

rebound
  ۱) واجهیدن؛ ۲) واجست   
1) vâjahidan; 2) vâjast

Fr.: 1) rebondir; 2) rebond   

1) To bound or spring back from force of impact.
2) The act of rebounding; recoil.

M.E., from O.Fr. rebondir "leap back, resound; push back," from → re- "back" + bondir "to leap, bound."

Vâjahidan, from vâ-, → re-, + jahidan "to leap, → jump."

receding galaxy
  کهکشان ِ دورشونده   
kahkašân-e dur šavandé

Fr.: galaxie qui s'éloigne   

A galaxy whose distance increases from other galaxies due to the global expansion of the Universe.

Receding, verbal adj. of recede, M.E., from M.Fr. receder, from L. recedere "to go back, withdraw," from → re- "back" + cedere "to go;" → galaxy.

Kahkašân, → galaxy; dur šavandé "receding," from dur, → far, + šavandé agent noun of šodan "to go, to pass; to become, to be, to be doing;" Mid.Pers. šudan, šaw- "to go;" Av. š(ii)auu-, šiyav- "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."

receiver
  گیرنده   
girandé (#)

Fr.: récepteur   

An electronic device that amplifies, detects, and gives a measure of the intensity of radio signals.

M.E. receven, from O.Fr. recoivre, from L. recipere from → re- + -cipere, combining form of capere "to take, hold, seize," PIE base *kap- "to grasp" (cf. Skt. kapati "two handfuls," Gk. kaptein "to swallow," O.Ir. cacht "servant-girl," lit. "captive," Goth. haban "have, hold," O.E. habban "to have, hold," probably Mod.Pers. qâp-, qâpidan, kapidan "to seize, rob," Av. haf-, hap- "to keep, observe").

Girandé, agent noun of gereftan "to take, seize, hold;" Mid.Pers. griftan, gir- "to take, hold, restrain;" O.Pers./Av. grab- "to take, seize," cf. Skt. grah-, grabh- "to seize, take," graha- "seizing, holding, perceiving," M.L.G. grabben "to grab," from P.Gmc. *grab, E. grab "to take or grasp suddenly;" PIE *ghrebh- "to seize."

receiver noise
  نوفه‌ی ِ گیرنده   
nufe-ye girandé

Fr.: bruit de récepteur   

The unwanted signal affecting a receiver.

receiver; → noise.

recent
  ترنه   
tarné

Fr.: récent   

1) Of, belonging to, or occurring at a time immediately before the present.
2) Geology: Of, belonging to, or denoting the Holocene Epoch.

From L. recentem (nominative recens) "fresh, new, young," from → re- + PIE root *ken- "fresh, new, young;" cf. Av. kainika-, kanya- "young girl;" Mod.Pers. kaniz(ak) "maid, virigin, girl; a female slave;" Mid.Pers. kanig, kanizag "girl, maid;" Gk. kainos "new;" Skt. kanina- "young;" Old Irish cetu- "first;" O.C.S. koni "beginning."

Tarné, from Tabari tarné "fresh, new, young, recent" (tarné mâr "fresh mother," i.e. "animal that has just given birth," tarné guk "recently born calf"), related to Pers. tar "fresh, young; wet," tarké "sprout;" Mid.Pers. tarr "fresh, moist;" Proto-Ir. *tarna-; cf. Av. tauruna- "young, fresh; young boy, lad;" Skt. táruna- "young, fresh;" Gk. teren "delicate, weak."

recently
  ترنانه   
tarnâné

Fr.: récemment   

In the recent past.

recent + -ly a suffix forming adverbs from adjectives.

recentness
  ترنگی   
tarnegi

Fr.: 1) caractère récent; 2) époque récente   

1) The property of having happened or appeared not long ago.
2) A time immediately before the present.

recent; → -ness.

recession
  دورشد، واروش   
duršod, vâraveš

Fr.: éloignement, récession   

1) The act of receding, going back, or withdrawing.
2) Economics: A period of an economic contraction, sometimes limited in scope or duration (Dictionary.com).

From Fr. récession "a going backward, a withdrawing," from L. recessionem "a going back," noun of action from p.p. stem of recedere "to go back, fall back; withdraw, retire," from → re- "back" + cedere "to go," → process.

Duršod, from dur, → remote, + šod "going," past stem of šodan "to go, to become," → change. Vâraveš, from vâ-, → re-, + raveš verbal noun of raftan "to go," → method.

recession velocity
  تندای ِ دورشدن   
tondâ-ye dur šodan

Fr.: vitesse d'éloignement   

The velocity with which an object moves away from another object or a reference point.

recession; → velocity.

reciprocity theorem
  فربین ِ دوسویگی   
farbin-e dosuyegi

Fr.: théorème de réciprocité   

1) General: Any theorem that expresses various reciprocal relations for the behavior of some physical systems, in which input and output can be interchanged without altering the response of the system to a given excitation.
2) In classical electromagnetism, the theorem stating that the current in a detector divided by the voltage at the source remains constant when source and detector are interchanged, as long as the frequency and all the impedances are left unchanged.

Reciprocity, from L. reciproc(us) "returning the same way, alternating" + → -ity; → theorem.

Farbin, → theorem; dosuyegi, quality noun of dosuyé nuanced term of dosu "two-sided," from do, → two, + su "direction, side," from Mid.Pers. sôk "direction, side."

recognition
  بازشناخت   
bâzšenâxt (#)

Fr.: rconnaissance   

An act of recognizing or the state of being recognized.

Verbal noun of → recognize.

recognize
  بازشناختن   
bâzšenâxtan (#)

Fr.: rconnaître   

1) To identify as something or someone previously seen, known, etc.
2) To identify from knowledge of appearance or characteristics (Dictionary.com).

re-; → cognition; → -ize.

recoil
  ۱) پسزدن؛ ۲) پسزنی   
1) paszadan; 2) paszani

Fr.: 1) reculer; 2) recul   

1) To draw back; to rebound or fly back.
2) An act of recoiling. → Compton recoil.

M.E. recoilen, reculen, from O.Fr. reculer "to go back, recede, retreat," from V.L. *reculare, from L. → re- "back" + culus "backside."

Paszadan, from pas-, → back-, + zadan "to strike, beat, dash against," from Mid.Pers. zatan, žatan, O.Pers./Av. jan-, gan- "to strike, hit, smite, kill" (jantar- "smiter"), Skt. han- "to strike, beat" (hantar- "smiter, killer"), cf. Gk. theinein "to strike," L. fendere "to strike, push," Gmc *gundjo "war, battle;" PIE *gwhen- "to strike, kill."

recombination
  بازمیازش   
bâzmiyâzeš

Fr.: recombinaison   

1) The process or result of combining again.
2) The capture of an electron by a positive ion. It is the inverse process to → ionization.

Verbal noun of → recombine.

recombination coefficient
  همگر ِ بازمیازش   
hamgar-e bâzmiyâzeš

Fr.: coefficient de recombinaison   

A measure of the specific rate at which oppositely charged ions join to form neutral particles. It is given by the rate at which those ions recombine, divided by the product of the densities of the two species involved.

recombination; → coefficient.

recombination continuum
  پیوستار ِ بازمیازش   
peyvastâr-e bâzmiyâzeš

Fr.: continuum de recombinaison   

A recombination radiation that is continuous over a range of frequencies. Same as → continuum emission.

recombination; → continuum.

recombination epoch
  زیمه‌ی ِ بازمیازش   
zime-ye bâzmiyâzeš

Fr.: époque de recombinaison   

Same as → recombination era.

recombination; → epoch.

recombination era
  دوران ِ بازمیازش   
dowrân-e bâzmiyâzeš

Fr.: ère de recombinaison   

The era some 380,000 years after the → Big Bang (at a → redshift of about 1,100), when the Universe had cooled sufficiently so that protons and electrons combined to form → neutral hydrogen in a process called → recombination. The temperature was about 3,000 K and the ionization fraction low enough for Universe to become transparent to light. Consequently matter and radiation decouple from one another because no further → scattering of the radiation occurs. The observation of the → cosmic microwave background radiation provides a means of studying the Universe at the recombination era. Also called recombination epoch and → decoupling era.

recombination; → era.

recombination line
  خط ِ بازمیازش   
xatt-e bâzmiyâzeš

Fr.: raie de recombinaison   

An → emission line in a spectrum produced in an → H II region when a free electron combines with an ionized atom to form a neutral atom or an ion of lower → ionization stage. Same as → free-bound emission.

recombination; → line.


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