Temporal Coherence of Single Photons Emitted by Hexagonal Boron Nitride Defects at Room Temperature. [PDF]
Martínez-Pons JV +8 more
europepmc +1 more source
Large-Diameter Diaphragm Fabry-Pérot Interferometer for High-Sensitivity Temperature Sensing Using a Hermetically Sealed Tunable Medium: Up to 190 nm/K. [PDF]
Weir A +4 more
europepmc +1 more source
Visualization of small vibrations inside an MRI scanner using video motion amplification. [PDF]
Seo Y, Wang ZJ.
europepmc +1 more source
Changes in the Interaction Properties of Antibodies with Fc Receptors upon Binding to Target Antigens. [PDF]
Grevtsev AS +9 more
europepmc +1 more source
Ultrasensitive Gas Detection via Polarization-Mode Photothermal Interferometry in a Single-Mode Nanofiber Coupler. [PDF]
Zhao P, Bao H, Ho HL, Zhao S, Jin W.
europepmc +1 more source
A coherent fiber link for very long baseline interferometry [PDF]
We realize a coherent fiber link for application in very long baseline interferometry (VLBI) for radio astronomy and geodesy. A 550-km optical fiber connects the Italian National Metrological Institute (INRIM) to a radio telescope in Italy and is used for the primary Cs fountain clock stability and accuracy dissemination.
Alberto Mura +2 more
exaly +5 more sources
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Optical Long Baseline Interferometry
Astrophysics and Space Science Library, 2016Optical Long Baseline Interferometry provides unrivalled angular resolution on bright and compact astrophysical sources. The link between the observables (interferometric phase and contrast ) and the image of the source is a Fourier transform expressed first by van Cittert and Zernike .
Jean-Baptiste LeBouquin
exaly +2 more sources
THE RAPID DEVELOPMENT of electronic technology has given man the ability to control electrical events in the time domain with extraordinary precision, just as the mechanical revolution of the last century improved, by orders of magnitude, our power to control linear dimensions of physical objects. Perhaps the only failure in the analogy is quantitative;
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Optical long-baseline interferometry in astronomy
SPIE Proceedings, 1990Optical long-baseline interferometry can yield images and spectra with fascinating angular resolution. For example, at a wavelength of 500 nm and with a baseline of lOOm a resolution of 10 arcsec can be obtained. We have studied the dependence of the SNR in the reconstructed image on the diluted pupil function, on wavefront aberrations and on photon ...
Thorsten Reinheimer, Gerd Weigelt
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Very long baseline interferometry
2005This contribution reviews the technique of Very Long Baseline Interferometry as a tool for high precision measurements of relative point positions and spatial baseline orientation. The geodetic and geophysical applications of these measurements are discussed in relation to the objectives of global and regional programs of Earth dynamics research ...
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