K-band (24 GHz) VLBI signal path delays caused by the troposphere and ionosphere
K-band (24 GHz) Very Long Baseline Interferometry (VLBI) reference frame observations, originally motivated by astrometric goals, are now providing accurate geodetic products such as station locations, Earth orientation, and atmospheric parameters. These results from the K-band Astro2Geo VLBI project, launched in 2013, allow for multi-frequency VLBI comparisons as well as multi-technique comparisons.
Institutions
- Jet Propulsion Laboratory (US)
- TU Wien (AT)
- ETH Zurich (CH)
- South African Radio Astronomy Observatory (ZA)
- United States Naval Observatory (US)
Publication Details
- Journal
- Zenodo (CERN European Organization for Nuclear Research)
- Published
- 2024-10-17
- DOI
- https://doi.org/10.5281/zenodo.13945877
- Primary Topic
- Radio Astronomy Observations and Technology
- Type
- article
- Field-Weighted Citation Impact
- 0.00