- speckle reference point source
- точечный источник диффузного опорного излучения
Англо-русский словарь промышленной и научной лексики. 2014.
speckle reference point source
Смотреть что такое "speckle reference point source" в других словарях:
Holography — (from the Greek, ὅλος hólos whole + γραφή grafē writing, drawing) is a technique that allows the light scattered from an object to be recorded and later reconstructed so that it appears as if the object is in the same position relative to the… … Wikipedia
Astronomical seeing — Schematic diagram illustrating how optical wavefronts from a distant star may be perturbed by a layer of turbulent mixing in the atmosphere. The vertical scale of the wavefronts plotted is highly exaggerated. Astronomical seeing refers to the… … 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
Hubble Space Telescope — Infobox Space telescope name = Hubble Space Telescope (HST) caption = The Hubble Space Telescope as seen from Space Shuttle Discovery during its second servicing mission (STS 82) organization = NASAESASTScI alt names = nssdc id =… … Wikipedia
Adaptive optics — (AO) is a technology used to improve the performance of optical systems by reducing the effects of rapidly changing optical distortion. It is used in astronomical telescopes and laser communication systems to remove the effects of atmospheric… … Wikipedia
Optical heterodyne detection — is an important special case of heterodyne detection. In heterodyne detection, a signal of interest at some frequency is non linearly mixed with a reference local oscillator (LO) that is set at a close by frequency. The desired outcome is the… … Wikipedia
INTERFÉRENCES LUMINEUSES — Lorsqu’on éclaire un plan matériel par deux sources ponctuelles, le phénomène observé ne résulte pas toujours de la superposition des intensités lumineuses émises par les deux sources. Si elles émettent des vibrations parallèles et… … Encyclopédie Universelle
HOLOGRAPHIE — Divers cas d’intervention de l’optique cohérente ont été considérés dans les articles INTERFÉRENCES LUMINEUSES et LUMIÈRE Diffraction, ainsi que dans l’article OPTIQUE Images optiques. Pour les sources usuelles, dites «thermiques», la phase… … Encyclopédie Universelle
star — starless, adj. /stahr/, n., adj., v., starred, starring. n. 1. any of the heavenly bodies, except the moon, appearing as fixed luminous points in the sky at night. 2. Astron. any of the large, self luminous, heavenly bodies, as the sun, Polaris,… … Universalium
Lucky imaging — M15 coreLucky imaging (also called lucky exposures) is one form of speckle imaging used for astronomical photography. Speckle imaging techniques use a high speed camera with exposure times short enough (100 ms or less) so that the changes in the… … Wikipedia
INTERFÉROMÉTRIE STELLAIRE OPTIQUE — Née dans la seconde moitié du XIXe siècle, l’interférométrie stellaire optique a été utilisée jusque dans les années 1920, puis fut quelque peu délaissée. Elle devait renaître dans les années 1950; elle a depuis lors enregistré de grands succès.… … Encyclopédie Universelle
