Very Long Baseline Interferometry observation oor Frans
Very Long Baseline Interferometry observation
Vertalings in die woordeboek Engels - Frans
observation RILB
observation radiointerférométrie à très longue base
Geskatte vertalings
Vertoon algoritmies gegenereerde vertalings
voorbeelde
Advanced filtering
Voorbeelde moet herlaai word.
The WSRT is often combined with other telescopes around the world to perform very-long-baseline interferometry (VLBI) observations, being part of the European VLBI Network.
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To include it, the scientists conducted the first real-time electronic Very Long Baseline Interferometry (e-VLBI) observation.
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In addition, although individual portions of the model sources are highly polarized, as also seen with very long baseline interferometry, the integrated polarizations are relatively small, as observed.
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Nowadays, UT in relation to International Atomic Time (TAI) is determined by Very Long Baseline Interferometry (VLBI) observations of distant quasars, a method which has an accuracy of microseconds.
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(e) Support the observation, analysis and development of national global navigation satellite systems, satellite laser ranging and very long baseline interferometry infrastructure and their interconnection for reference frame improvement, and provide an Asia and the Pacific perspective to the global geodetic community;
Non déterminéUN-2 UN-2
The Committee noted the importance of supporting the observation, analysis and development of national global navigation satellite system, satellite laser ranging and very long baseline interferometry infrastructure and their interconnection for reference frame improvement and for providing an Asia and Pacific perspective to the global geodetic community.
Procédure d' arrêt d' urgence annuléeUN-2 UN-2
These observations were transmitted in real-time at an aggregated rate of 1.44 Gbps to a super computer located at the Joint Institute for Very Long Baseline Interferometry (JIVE), in Dwingeloo, the Netherlands.
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In this study, we examine the alignment of Very Long Baseline Interferometry scale structure with arcsecond scale structure for a much larger sample of core-dominated radio sources and compare the distribution of observed misalignment angles with theoretical distributions calculated from models using a range of intrinsic bend angles, ξ, and Lorentz factors, γ.
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The project uses Very Long Baseline Interferometry at short wavelengths to directly observe the area around a black hole.
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The EHT observations use a technique called very-long-baseline interferometry (VLBI), which synchronizes telescope facilities around the world and exploits the rotation of our planet to form one huge, Earth-sized telescope observing at a wavelength of 1.3mm.
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The EHT observations use a technique called very-long-baseline interferometry (VLBI) which synchronises telescope facilities around the world and exploits the rotation of our planet to form one huge, Earth-size telescope observing at a wavelength of 1.3mm.
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This image was captured by ESO’s Very Large Telescope as part of the Cosmic Gems programme. The_Tech The EHT observations use a technique called very-long-baseline interferometry (VLBI) which synchronises telescope facilities around the world and exploits the rotation of our planet to form one huge, Earth-size telescope observing at a wavelength of 1.3mm.
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UT1 is a time scale directly related to the Earth rotation determined by the IERS essentially from the observation of extragalactic quasars extra galactiques using VLBI (Very Long Baseline Interferometry).
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(b) the relevant space geodetic (such as Satellite Laser Ranging, Very Long Baseline Interferometry, Global Positioning SDystem and Dynthetic Apertune Radar) and terrestrial techniques (such as gravimetry, tide gauge measurmenet, meteorological observation) be employed in support on fhis project;
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