- very long baseline interferometer
English-Russian dictionary of telecommunications and their abbreviations. A.V. Alexandrov.. 2004.
English-Russian dictionary of telecommunications and their abbreviations. A.V. Alexandrov.. 2004.
Very Long Baseline Interferometry — (VLBI) is a type of astronomical interferometry used in radio astronomy. It allows observations of an object that are made simultaneously by many telescopes to be combined, emulating a telescope with a size equal to the maximum separation between … Wikipedia
Very Long Baseline Interferometry — VLBI Beobachtung zwischen den Stationen Kashima (Japan) und TIGO (Chile) Very Long Baseline Interferometry (VLBI) bzw. Langbasisinterferometrie ist eine Methode der Radioastronomie für Messungen mit höchster räumlicher Auflösung und… … Deutsch Wikipedia
Very Large Array — Das VLA in New Mexico USGS Luftaufnah … Deutsch Wikipedia
Very Large Array — Infobox Telescope name = Very Large Array organization = nowrap|National Radio Astronomy Observatory location = Socorro, New Mexico, USA coords = coord|34|04|43.497|N|107|37|05.819|W|type:landmark altitude = 2124 m (6970 ft) weather = wavelength … Wikipedia
Interferometer (Radioastronomie) — Ein Interferometer aus Radioteleskopen wird benutzt, um mit kleineren Anlagen eine hohe Winkelauflösung zu erreichen. Eine höhere Auflösung führt zu trennschärferen Bildern von nahe beieinander liegenden Radioquellen oder bei kompakten Quasaren,… … Deutsch Wikipedia
Astronomical interferometer — An astronomical interferometer is an array of telescopes or mirror segments acting together to probe structures with higher resolution. Astronomical interferometers are widely used for optical astronomy, infrared astronomy, submillimetre… … Wikipedia
Palomar Testbed Interferometer — The Palomar Testbed Interferometer is a near IR, long baseline stellar interferometer located at Palomar Observatory in north San Diego County. It was built by Caltech/JPL and is intended to serve as a testbed for developing interferometric… … Wikipedia
VLBI — Beobachtung zwischen den Stationen Kashima (Japan) und TIGO (Chile) Very Long Baseline Interferometry (VLBI) ist eine Methode der Radioastronomie für Messungen mit höchster räumlicher Auflösung und Positionsgenauigkeit. Sie dient sowohl für… … Deutsch Wikipedia
Meanings of minor planet names: 10001–11000 — As minor planet discoveries are confirmed, they are given a permanent number by the IAU s Minor Planet Center, and the discoverers can then submit names for them, following the IAU s naming conventions. The list below concerns those minor planets … Wikipedia
SELENE — Saltar a navegación, búsqueda SELENE Infografía de la sonda Datos de la misión Nombre: SELENE (o Kaguya) Organización: JAXA … Wikipedia Español
OVLBI — Orbital Very Long Baseline Interferometer ( > IEEE Standard Dictionary ) … Acronyms