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Vienna mapping functions in VLBI analyses

Boehm, Johannes, Schuh, Harald·2004·Geophysical Research Letters

Abstract

In the past few years, numerical weather models (NWM) have been investigated to improve mapping functions which are used for tropospheric delay modeling in VLBI and GPS data analyses. The Vienna Mapping Functions VMF are based on direct raytracing through NWM, and so they are able to exploit the full information provided in the NWM. On the other hand, the Isobaric Mapping Functions IMF are using intermediate parameters calculated from the NWM. In this study, pressure level data from ECMWF (European Centre for Medium‐Range Weather Forecasts) are applied to determine the coefficients of the VMF and the IMF. Used for the analyses of IVS‐R1 and IVS‐R4 VLBI sessions, both mapping functions improve the repeatability of baseline lengths (by ∼10% for IVS‐R1 and ∼5% for IVS‐R4) compared to the Niell Mapping Functions NMF.

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Metadata

Authors
Boehm, J., & Schuh, H.
Venue
Geophysical Research Letters
Published
2004-01
Volume
31
Issue
1
Pages
277
ISSN
  • 0094-8276 (ISSN-L)
  • 1944-8007
OpenAlex
W2021214714
Cited by
271
References
4
FWCI
13.71
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Vienna mapping functions in VLBI analyses. https://app.cochat.ai/papers/10.1029/2003gl018984
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Boehm, J., & Schuh, H. (2004). Vienna mapping functions in VLBI analyses. Geophysical Research Letters. https://doi.org/10.1029/2003gl018984

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