amplitude residuals

amplitude residuals
разности амплитуд

Англо-русский словарь по ядерным испытаниям и горному делу. 2013.

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Смотреть что такое "amplitude residuals" в других словарях:

  • Sinusoidal model — In statistics, signal processing, and time series analysis, a sinusoidal model to approximate a sequence Yi is::Y i = C + alphasin(omega T i + phi) + E i where C is constant defining a mean level, α is an amplitude for the sine wave, ω is the… …   Wikipedia

  • Seismic wave — Seismic waves are waves that travel through the Earth, most often as the result of a tectonic earthquake, sometimes from an explosion. Seismic waves are also continually excited by the pounding of ocean waves and the wind. Seismic waves are… …   Wikipedia

  • optics — /op tiks/, n. (used with a sing. v.) the branch of physical science that deals with the properties and phenomena of both visible and invisible light and with vision. [1605 15; < ML optica < Gk optiká, n. use of neut. pl. of OPTIKÓS; see OPTIC,… …   Universalium

  • Spectrum continuation analysis — (SCA) is a generalization of the concept of Fourier series to non periodic functions of which only a fragment has been sampled in the time domain.Recall that a Fourier series is only suitable to the analysis of periodic (or finite domain)… …   Wikipedia

  • HD 217107 — Starbox begin name = HD 217107 Starbox observe epoch = J2000.0 constell = Pisces ra = RA|22|58|15.54 dec = DEC|−2|23|43.39 appmag v =+6.17 Starbox character class = G8IV b v = 0.744 u b = 0.42 variable = none Starbox astrometry radial v = −14.0… …   Wikipedia

  • Bayesian experimental design — provides a general probability theoretical framework from which other theories on experimental design can be derived. It is based on Bayesian inference to interpret the observations/data acquired during the experiment. This allows accounting for… …   Wikipedia

  • HD 217107 b — Planetbox begin name = HD 217107 bPlanetbox star star = HD 217107 constell = Pisces ra = RA|22|58|15.54 dec = DEC|−2|23|43.39 dist ly = 64.3 ± 1 dist pc = 19.7 ± 0.3 class = G8IVPlanetbox orbit separation = position angle = semimajor = 0.074 ±… …   Wikipedia

  • Surface brightness fluctuation — (SBF) is a secondary distance indicator used to estimate distances to galaxies. The technique uses the fact that galaxies are made up of a finite number of stars. The number of stars in any small patch of the galaxy will vary from point to point …   Wikipedia

  • HD 217107 b — ist ein extrasolarer Planet, der einen sonnenähnlichen Stern in 7,1 Tagen umkreist. Er ist der innerste bekannte Stern seines Planetensytems und wurde vom California and Carnegie Planet Search Team entdeckt. Aufgrund seiner Größe und seiner Nähe… …   Deutsch Wikipedia


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