Results 11 to 20 of about 33,024 (227)

Photon Mass and Very Long Baseline Interferometry [PDF]

open access: yesInternational Journal of Modern Physics D, 2010
A relation between the photon mass, its frequency, $\nu$, and the deflection parameter, $\gamma$, determined by experimentalists (which characterizes the contribution of space curvature to gravitational deflection) is found. This amazing result allows us
Accioly A.   +4 more
core   +4 more sources

Space very long baseline interferometry in China [PDF]

open access: yesAdvances in Space Research, 2020
Space very long baseline interferometry (VLBI) has unique applications in high-resolution imaging of fine structure of astronomical objects and high-precision astrometry due to the key long space-Earth or space-space baselines beyond the Earth's diameter. China has been actively involved in the development of space VLBI in recent years.
An, Tao   +21 more
openaire   +4 more sources

Very-long-baseline interferometry experiments [PDF]

open access: yes1970 Antennas and Propagation Society International Symposium, 1970
VLB observations have been made at many wavelengths from 2.8 to 270 cm. The highest resolution was obtained on the Greenbank-Crimea baseline, 2.9 x 10^8 wavelengths long at 2.8 cm on which two quasars showed interference fringes.
Cohen, M. H.
core   +3 more sources

Lorentz symmetry and Very Long Baseline Interferometry [PDF]

open access: yesPhysical Review D, 2016
Lorentz symmetry violations can be described by an effective field theory framework that contains both General Relativity and the Standard Model of particle physics called the Standard-Model extension (SME). Recently, post-fit analysis of Gravity Probe B
Hees, A.   +2 more
core   +6 more sources

A coherent fiber link for very long baseline interferometry [PDF]

open access: yesIEEE Transactions on Ultrasonics, Ferroelectrics, and Frequency Control, 2015
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.
CLIVATI, CECILIA   +10 more
openaire   +6 more sources

First Very Long Baseline Interferometry Detections at 870 μm [PDF]

open access: yesThe Astronomical Journal
The first very long baseline interferometry (VLBI) detections at 870 μ m wavelength (345 GHz frequency) are reported, achieving the highest diffraction-limited angular resolution yet obtained from the surface of the Earth and the highest-frequency ...
Alexander W. Raymond   +278 more
doaj   +7 more sources

Geophysical applications of very-long-baseline interferometry [PDF]

open access: yesReviews of Modern Physics, 1991
Very-long-baseline interferometry (VLBI) is a novel observing technique for measuring the relative positions of widely separated points on the surface of the Earth with centimeter-level accuracy. Such accuracy is two or three orders of magnitude better than was available with classical techniques only a few decades ago.
openaire   +3 more sources

Probing the solar corona with very long baseline interferometry. [PDF]

open access: yesNat Commun, 2014
AbstractUnderstanding and monitoring the solar corona and solar wind is important for many applications like telecommunications or geomagnetic studies. Coronal electron density models have been derived by various techniques over the last 45 years, principally by analysing the effect of the corona on spacecraft tracking.
Soja B, Heinkelmann R, Schuh H.
europepmc   +7 more sources

Very Long Baseline Interferometry with the SKA [PDF]

open access: yesProceedings of Advancing Astrophysics with the Square Kilometre Array — PoS(AASKA14), 2015
Adding VLBI capability to the SKA arrays will greatly broaden the science of the SKA, and is feasible within the current specifications. SKA-VLBI can be initially implemented by providing phased-array outputs for SKA1-MID and SKA1-SUR and using these extremely sensitive stations with other radio telescopes, and in SKA2 by realising a distributed ...
Paragi, Zsolt,   +81 more
  +16 more sources

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