Results 21 to 30 of about 348,356 (178)

A novel type of very long baseline astronomical intensity interferometer [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2013
This article presents a novel type of very long baseline astronomical interferometer that uses the fluctuations, as a function of time, of the intensity measured by a quadratic detector, which is a common type of astronomical detector. The theory on which the technique is based is validated by laboratory experiments.
openaire   +2 more sources

Development of a digital astronomical intensity interferometer: laboratory results with thermal light [PDF]

open access: yesJournal of Modern Optics, 2017
13 pages, 5 figures, Accepted into special issue of the Journal of Modern ...
Nolan Matthews   +2 more
openaire   +2 more sources

Sirius: a prototype astronomical intensity interferometer using avalanche photodiodes in linear mode [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2020
ABSTRACT Optical intensity interferometry, developed in the 1950s, is a simple and inexpensive method for achieving angular resolutions on microarcsecond scales. Its low sensitivity has limited intensity interferometric observations to bright stars so far.
Oh, J.   +5 more
openaire   +3 more sources

Optical coherence tomography with a Fizeau interferometer configuration [PDF]

open access: yes, 2005
We report the investigation of a Fizeau interferometer-based OCT system. A secondary processing interferometer is necessary in this configuration, to compensate the optical path difference formed in the Fizeau interferometer between the end of the ...
H. D. Ford   +7 more
core   +1 more source

Phase Feedback Active Stabilisation Of A Multiplexed Fibre Interferometer [PDF]

open access: yes
Current optical technologies for surface measurement such as white light scanning interferometry (WLSI) can produce sub-nanometric resolution areal height information.
Martin, Haydn, Jiang, Xiang
core   +4 more sources

Stabilized fiber-optic Mach–Zehnder interferometer for carrier-frequency rejection

open access: yes, 2013
We have demonstrated stabilization of a fiber-optic Mach–Zehnder interferometer, with a centimeter-scale path difference, to the transmission minimum for the carrier wave of a frequency-modulated laser beam.
Freegarde, Tim   +4 more
core   +1 more source

An active fiber sensor for mirror vibration metrology in astronomical interferometers [PDF]

open access: yesAstronomische Nachrichten, 2009
AbstractWe present a fiber sensor based on an active integrated component which could be effectively used to measure the longitudinal vibration modes of telescope mirrors in an interferometric array. We demonstrate the possibility to measure vibrations with frequencies up to ⋍100 Hz with a precision better than 10 nm (© 2009 WILEY‐VCH Verlag GmbH &
Minardi, S.   +6 more
openaire   +2 more sources

Dynamic Evolution of a Storm‐Time “Super‐EPB” Event Over China on the Magnetically Disturbed Night of 01 December 2023

open access: yesSpace Weather, Volume 24, Issue 10, October 2026.
Abstract This paper investigates the dynamic evolution of a storm‐time “Super‐EPB” event over China on 1 December 2023 (Kp ≤ 7, SYM/H ≥ −130 nT) using multi‐instrument observations. Occurring near sunset as the IMF‐Bz abruptly turned southward, with auroral extension to midlatitudes, the “Super‐EPB” extended to 40°N with an apex height of ∼2,460 km ...
Longchang Sun   +11 more
wiley   +1 more source

The Benefits of Using XML Technologies in Astronomical Data Retrieval and Interpretation [PDF]

open access: yes, 2016
This paper describes a solution found during recent research that could provide improvements in the efficiency, reliability and cost of retrieving stored astronomical data.
Doicu, Adrian   +69 more
core   +2 more sources

Impact of Two Radio Occultation Constellations on Numerical Weather Prediction: Polar‐Orbits Only and Mixed Polar‐Equatorial Orbits

open access: yesEarth and Space Science, Volume 13, Issue 10, October 2026.
Abstract This study explores the relative impact of two orbital configurations for Global Navigation Satellite System radio occultation (RO) observations in numerical weather prediction using observing system simulation experiments (OSSE). Three experiments are carried out: a Control experiment with no RO observations and two experiments with 14,000 RO
Nikki C. Privé   +6 more
wiley   +1 more source

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