Results 1 to 10 of about 689 (120)
Research on Instrument Visibility of Ozone Wind Imaging Interferometer [PDF]
Remote Sensing, 2021 This paper discussed the principle of the ozone wind imaging interferometer developed by our group, which used remote sensing method to detect wind field and ozone concentration simultaneously, focused on the analysis and calculation of the instrument visibility and gave the theoretical representation of the instrument visibility.
Chunmin Zhang +3 more
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Keck Interferometer nuller instrument performance [PDF]
SPIE Proceedings, 2010 The Keck Interferometer combines the two 10 m Keck telescopes as a long baseline interferometer. It is funded by NASA as a joint development among the Jet Propulsion Laboratory, the W. M. Keck Observatory, and the NASA Exoplanet Science Institute. In February 2008, the 10 um nulling mode began a 32 night observing program with three key science teams ...
Colavita, M. M. +4 more
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The Sydney University Stellar Interferometer -- I. The instrument [PDF]
Monthly Notices of the Royal Astronomical Society, 1999 ABSTRA C T The Sydney University Stellar Interferometer (SUSI) is a new long-baseline optical interferometer located in northern New South Wales, Australia. SUSI has been developed to tackle a range of problems in stellar astrophysics, and its design is based on a successful prototype instrument. In its initial configuration, observations are made with
J. Davis +5 more
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The Micro-Precision Interferometer Testbed Instrument Design [PDF]
Symposium - International Astronomical Union, 1994 The Micro-Precision Interferometer Testbed is essentially a space-based Michelson interferometer suspended in a ground-based laboratory. The purpose of the testbed is to serve as a proving ground for technologies needed for future space-based missions requiring low-vibration environments.
B. Hines +4 more
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Quantum-assisted optical interferometers: instrument requirements [PDF]
Optical and Infrared Interferometry and Imaging VII, 2020 It has been recently suggested that optical interferometers may not require a phase-stable optical link between the stations if instead sources of quantum-mechanically entangled pairs could be provided to them, enabling extra-long baselines and benefiting numerous topics in astrophysics and cosmology.
Nomerotski, Andrei +19 more
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Computer simulations of interferometric imaging with the VLT Interferometer and the AMBER instrument [PDF]
SPIE Proceedings, 2000 10 pages including 6 PostScript figures, also available from http://www.mpifr-bonn.mpg.de/div/speckle/publications.html, SPIE Conf. Vol.
Bloecker, T. +3 more
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Instrumentation for Radio Interferometers with Antennas on a Regular Grid
, 2022 PhD thesis, published at Proquest 2021 ...
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Long-baseline optical fiber interferometer instruments and science [PDF]
SPIE Proceedings, 2003 Developments of fiber linked optical interferometer are reported. This interferometer is a part of MIRA-I.2 interferometer (Mitaka InfraRed and optical Array). MIRA-I.2 is an optical interferometer with a 30 meters long baseline. It consists of two 30cm siderostats, tip-tilt mirrors, vacuum pipes delay lines and detectors.
Takayuki Kotani +10 more
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Science and instrumentation update from the Palomar testbed interferometer [PDF]
SPIE Proceedings, 2004 The Palomar Testbed Interferometer (PTI) is a near-infrared, long-baseline interferometer located at the Palomar Observatory. PTI obtained first fringes in 1995, and has been in routine scientific operations since 1998. PTI was primarily designed as a technology demonstration experiment for the Keck Interferometer, and has been successful in ...
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Signatures of correlation of spacetime fluctuations in laser interferometers. [PDF]
Nat CommunSharmila B, Vermeulen SM, Datta A.
europepmc +1 more source