An Etymological Dictionary of Astronomy and Astrophysics

فرهنگ ریشه شناختی اخترشناسی-اخترفیزیک

M. Heydari-Malayeri    -    Paris Observatory



<< < abs col den Glo mag per pos rad spe tra > >>

Number of Results: 192 Search : sit
density-bounded H II region
  ناحیه‌ی ِ H IIی ِ چگالی‌کرانمند   
nâhiye-ye H II-ye cagâli karânmand

Fr.: bornée par la densité   

An → H II region which lacks enough matter to absorb all → Lyman continuum photons of the → exciting star(s). In such an H II region a part of the ionizing photons escape into the → interstellar medium. See also → ionization-bounded H II region.

density; → bounded; → region.

  ۱) لرد؛ ۲) لرد انداختن، ~ افتادن، لردیدن   
1) lerd; 2) lerd andâxtan, lerd oftâdan, lerdidan

Fr.: 1) dépôt, gisement, lie, tarte; 2) déposer, se déposer   

1a) Something precipitated, delivered and left, thrown down, or accumulated, as by a natural process.
1b) Substance which settles down from a solution or a suspension, such as the natural sediment of wine in a bottle. See also → sediment.
2) To leave or form a layer of some substance (sand, sediment, etc.) as a gradual process in one place, or be left in this way.

From L. depositus, p.p. of deponere "to lay aside, put down," from → de- "away" + ponere "to put," → position.

Lerd "sediment, tartar of wine," probably a variant of dord "dregs, lees, sediment, tartar of wine."


Fr.: dépôt   

The process by which water vapor changes directly to ice without first becoming a liquid. This is how snow forms in clouds, as well as frost and hoar frost on the ground. The opposite of deposition is → sublimation. → condensation.

M.E., from O.Fr. deposition, from L. deposition- "putting aside, testimony, burial," from deposit(us) "laid down," p.p. of deponere "to put down," from → de- + ponere "to put, place."

Vâneheš, from vâ-de- + neheš verbal noun of nehâdan "to put, place," Mid.Pers. nihâtan, O.Pers./Av. ni- "down; into," → ni-, + dā- "to put; to establish; to give," dadāiti "he gives," cf. Skt. dadâti "he gives," Gk. didomi "I give," L. do "I give;" PIE base *do- "to give."

discrete transition
  گذرش ِ گسسته   
gozareš-e gosasté

Fr.: transition discrète   

A transition between two quantum-mechanical energy levels. See also → discrete spectrum.

discrete; → transition.

gunâguni (#)

Fr.: diversité   

The state or fact of being diverse; difference; unlikeness.

diverse; → -ity.

dynamic viscosity
  وشکسانی ِ توانیک   
vošksâni-y tavânik

Fr.: viscosité dynamique   

Same as → viscosity and → absolute viscosity.

dynamic; → viscosity.

Eddington luminosity
  تابندگی ِ ادینگتون   
tâbandegi-ye Eddington

Fr.: luminosité d'Eddington   

Same as → Eddington limit.

Eddington limit; → luminosity.

Einstein-de Sitter effect
  اسکر ِ اینشتین-دو سیتر   
oskar-e Einstein-de Sitter

Fr.: effet Einstein-de Sitter   

Same as → geodetic precession.

Einstein-de Sitter Universe; → effect.

Einstein-de Sitter Universe
  گیتی ِ اینشتین-دو سیتر   
giti-ye Einstein-de Sitter

Fr.: Univers Einstein-de Sitter   

The → Friedmann-Lemaitre model of → expanding Universe that only contains matter and in which space is → EuclideanM > 0, ΩR = 0, ΩΛ = 0, k = 0). The Universe will expand at a decreasing rate for ever.

Einstein; de Sitter, after the Dutch mathematician and physicist Willem de Sitter (1872-1934) who worked out the model in 1917; → Universe.

electric intensity
  درتنویی ِ برقی   
dartanuyi-e barqi (#)

Fr.: intensité électrique   

The strength of an electric field at any point as measured by the force exerted upon a unit positive charge placed at that point.

electric; → intensity.

electron density
  چگالی ِ الکترونی   
cagâli-ye elektroni (#)

Fr.: densité électronique   

The number of electrons per unit volume in an ionized medium, like an → H II region, as determined from → emission lines.

electron; → density.

electron-positron pair
  جفت ِ الکترون-پوزیترون   
joft-e elektron-pozitron (#)

Fr.: paire électron-positron   

The simultaneous formation of an → electron and a → positron in the → pair production process.

electron; → positron; → pair.

electronic transition
  گذرش ِ الکترونی   
gozareš-e elektroni

Fr.: transition électronique   

The → transfer of an → electron from one → energy level to another.

electronic; → transition.

energy density
  چگالی ِ کاروژ   
cagâli-ye kâruž

Fr.: densité d'énergie   

The amount of energy in the form of radiation per unit volume, expressed in ergs cm-3. In particular, the energy density of blackbody radiation at temperature T is aT4, where the radiation constant a = 7.56 × 10-15 erg cm-3 (K)-4.

energy; → density.

ephemeris transit
  گذر ِ روزیجی   
gozar-e ruziji

Fr.: transit au méridien des éphémérides   

The passage of a celestial body or point across the → ephemeris meridian.

ephemeris; → transit.

equilibrium position
  نهش ِ ترازمندی   
naheš-e tarâzmandi (#)

Fr.: position d'équilibre   

The position of an oscillating body at which no net force acts on it.

equilibrium; → position.

equivalent positions
  نهش‌های ِ هموگ‌ارز   
nehešhâ-ye hamug-arz


Complete set of points in any given space group which are obtained by performing the symmetry operations of the space group on a single point (x, y, z).

equivalent; → position.



The quality or condition of being → false. Opposite of → truth.

false; → -ity.

flux density
  چگالی ِ شار   
cagâli-ye šârr

Fr.: densité de flux   

Flux of radiation that falls on a detector per unit surface area of the detector per unit bandwidth of the radiation per unit time.

flux; → density.

forbidden transition
  گذرش ِ بژکم   
gozareš-e bažkam

Fr.: transition interdite   

A transition between two quantum mechanical → states that → violates the quantum mechanical → selection rules.

forbidden; → transition.

<< < abs col den Glo mag per pos rad spe tra > >>