Results 11 to 20 of about 22,374 (269)

Observing APOD with the AuScope VLBI Array

open access: yesSensors, 2018
The possibility to observe satellites with the geodetic Very Long Baseline Interferometry (VLBI) technique is vividly discussed in the geodetic community, particularly with regard to future co-location satellite missions.
Jamie Mccallum   +2 more
exaly   +4 more sources

Russian VLBI network “Quasar”: Current status and outlook

open access: yesGeodesy and Geodynamics, 2019
This paper presents the past, present and future status of the Russian VLBI network “Quasar”. This network has been developed for at least 20 years by the Institute of Applied Astronomy of the Russian Academy of Sciences (IAA RAS).
Igor Surkis, Mikhail Vasilyev
exaly   +4 more sources

Overview of the Observing System and Initial Scientific Accomplishments of the East Asian VLBI Network (EAVN) [PDF]

open access: yesGalaxies, 2022
The East Asian VLBI Network (EAVN) is an international VLBI facility in East Asia and is operated under mutual collaboration between East Asian countries, as well as part of Southeast Asian and European countries.
Kazunori Akiyama   +104 more
doaj   +2 more sources

Software and Techniques for VLBI Data Processing and Analysis [PDF]

open access: yesUniverse, 2022
Very-long-baseline interferometry (VLBI) is a challenging observational technique, which requires in-depth knowledge about radio telescope instrumentation, interferometry, and the handling of noisy data.
Michael Janssen   +2 more
doaj   +2 more sources

Improving VLBI analysis by tropospheric ties in GNSS and VLBI integrated processing

open access: yesJournal of Geodesy, 2022
Tropospheric delay modeling is challenging in high-precision Very Long Baseline Interferometry (VLBI) analysis due to the rapid water vapor variation and imperfect observation geometry, where observations from Global Navigation Satellite Systems (GNSS ...
Harald Schuh   +2 more
exaly   +2 more sources

Optical frequency comb integration in radio telescopes: advancing signal generation and phase calibration [PDF]

open access: yesLight: Science & Applications
Very long baseline interferometry (VLBI) enables high-angular-resolution observations in astronomy and geodesy by synthesizing a virtual telescope with baselines spanning hundreds to thousands of kilometres. Achieving high instrumental phase stability in
Minji Hyun   +10 more
doaj   +2 more sources

Optimizing schedules for the VLBI global observing system

open access: yesJournal of Geodesy, 2020
Very long baseline interferometry (VLBI) scheduling is a challenging optimization problem. With the development of the new VLBI global observing system (VGOS) consisting of smaller but very fast slewing antennas, new opportunities arise. In this work, we
Matthias Schartner   +2 more
exaly   +2 more sources

Radio Astronomical Antennas in the Central African Region to Improve the Sampling Function of the VLBI Network in the SKA Era? [PDF]

open access: yesSensors, 2022
On the African continent, South Africa has world-class astronomical facilities for advanced radio astronomy research. With the advent of the Square Kilometre Array project in South Africa (SA SKA), six countries in Africa (SA SKA partner countries) have ...
Marcellin Atemkeng   +4 more
doaj   +2 more sources

The Celestial Frame and the Weighting of the Celestial Pole Offsets in the Computation of VLBI-Based Corrections for the Main Lunisolar Nutation Terms [PDF]

open access: yesSensors, 2021
Very long baseline interferometry (VLBI) is the only technique in space geodesy that can determine directly the celestial pole offsets (CPO). In this paper, we make use of the CPO derived from global VLBI solutions to estimate empirical corrections to ...
Víctor Puente, Marta Folgueira
doaj   +2 more sources

A Comparative Study of VTEC Estimates Derived From S/X VLBI and VGOS Observations

open access: yesSpace Weather
The ionosphere, which strongly varies in time and space, is one of the largest error sources for microwave measurements, if not accounted for accurately.
Arno Rüegg   +2 more
doaj   +2 more sources

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