Results 21 to 30 of about 160 (88)

The Vienna VLBI raw data simulator and correlator in the VGOS era [PDF]

open access: yes, 2022
Die Very Long Baseline Interferometry (VLBI) ist ein Verfahren, bei der weltweit verteilte Radioteleskope eingesetzt werden, um die elektromagnetischen Feldstärken von natürlichen Radiosignalen von kosmischen Quellen zu messen.
Gruber, Jakob Franz; orcid:
core   +1 more source

Impact of the image alignment over frequency for the VLBI Global Observing System

open access: yes, 2022
Aims. The VLBI Global Observing System (VGOS), which is the next generation of geodetic very long baseline interferometry (VLBI), observes simultaneously in four frequency bands in the range 3.0-10.7 GHz (expected to be extended to 14 GHz).
Xu, Ming H.   +6 more
core   +1 more source

Impacts of the image alignment over frequency for VLBI Global Observing System

open access: yes, 2021
The VLBI Global Observing System, which is the next generation of geodetic VLBI and is called VGOS, observes simultaneously at four frequency bands in the range 3.0--10.7 GHz (expected to be extended to 14 GHz).
Xu, Ming H.   +15 more
core   +1 more source

Radiometry performance of the VGOS receivers of the Onsala twin telescopes [PDF]

open access: yes, 2023
With the introduction of the VLBI Global Observing System (VGOS) the parallel use of the VGOS receiver asradiometer in order to estimate the wet propagation delay was recognised as a future possibility.
Forkman, Peter   +8 more
core   +1 more source

Geodetic data analysis of VGOS experiments

open access: yes, 2021
Very Long Baseline Interferometry (VLBI) serves as one of the common geodetic methods to define the global reference frames and monitor Earth\u27s orientation variations. The technical upgrade of the VLBI method known as the VLBI Global Observing System (
Mueskens, Arno,   +145 more
core   +1 more source

The NTSC VLBI System and its application in UT1 measurement

open access: yes, 2023
In order to measure the Universal Time (UT1) in real time, National Time Service Center (NTSC) has built a VGOS-like (VLBI Global Observing System) broadband VLBI network, which includes three 13-m radio telescopes located in Jilin, Sanya and Kashi, and ...
Wu, Yuan-Wei   +10 more
core   +1 more source

The Potential for Unifying Global‐Scale Satellite Measurements of Ground Displacements Using Radio Telescopes

open access: yesGeophysical Research Letters, Volume 46, Issue 21, Page 11841-11849, 16 November 2019., 2019
Abstract The expansion of globally consistent satellite‐radar imagery presents new opportunities to measure Earth‐surface displacements on intercontinental scales. Yet global applications, including a complete assessment of the land contribution to relative sea‐level rise, first demand new solutions to unify relative satellite‐radar observations in a ...
A. L. Parker   +4 more
wiley   +1 more source

Realization Status of the VLBI Global Observing System

open access: yes, 2021
American Geophysical Union (AGU) Fall Meeting, 13-17 December 2021, New OrleansThe International VLBI Service for Geodesy and Astrometry (IVS) currently employs a two-band VLBI system (legacy S/X system) as its operational system for product creation ...
Macmillan, Daniel S.   +4 more
core  

Gravitational deformation of ring-focus antennas for VGOS: first investigations at the Onsala twin telescopes project [PDF]

open access: yes, 2019
The receiving properties of radio telescopes used in geodetic and astrometric very long baseline interferometry (VLBI) depend on the surface quality and stability of the main reflector.
Lösler, Michael,   +7 more
core   +1 more source

Cross‐Polarization Gain Calibration of Linearly Polarized VLBI Antennas by Observations of 4C 39.25

open access: yesRadio Science, Volume 59, Issue 4, April 2024.
Abstract Radio telescopes with dual linearly polarized feeds regularly participate in Very Long Baseline Interferometry. One example is the VLBI Global Observing System (VGOS), which is employed for high‐precision geodesy and astrometry. In order to achieve the maximum signal‐to‐noise ratio, the visibilities of all four polarization products are ...
F. Jaron   +14 more
wiley   +1 more source

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