GGOS Topical Meeting on the Atmosphere
Published October 17, 2024 | Version v1
Poster Open

K-band (24 GHz) VLBI signal path delays caused by the troposphere and ionosphere

Authors/Creators

  • 1. TU Wien
  • 2. ROR icon South African Radio Astronomy Observatory
  • 3. ROR icon Jet Propulsion Laboratory
  • 4. ROR icon United States Naval Observatory
  • 5. ROR icon ETH Zurich

Description

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.

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Krasna_GGOSatm_Kband.pdf

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