SLR, GRACE and SWARM gravity field determination and combination

At the Astronomical Institute of the University of Bern (AIUB) long time-series (1995 - 2017) of low resolution (spherical harmonic degree/order 6) gravity field coefficients have been determined from a combination of LAGEOS and geodetic SLR satellites in low Earth orbit, namely: Beacon-C, Ajisai, S...

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Main Authors: Meyer, Ulrich, Sosnica, Krzsztof, Andritsch, Florian, Dach, Rolf, Jäggi, Adrian, König, Daniel, Thaller, Daniela
Format: Text
Language:English
Published: (:null) 2019
Subjects:
Online Access:https://dx.doi.org/10.7892/boris.132229
https://boris.unibe.ch/132229/
id ftdatacite:10.7892/boris.132229
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spelling ftdatacite:10.7892/boris.132229 2023-05-15T16:29:18+02:00 SLR, GRACE and SWARM gravity field determination and combination Meyer, Ulrich Sosnica, Krzsztof Andritsch, Florian Dach, Rolf Jäggi, Adrian König, Daniel Thaller, Daniela 2019 application/pdf https://dx.doi.org/10.7892/boris.132229 https://boris.unibe.ch/132229/ en eng (:null) info:eu-repo/semantics/openAccess 520 Astronomy Text article-journal ScholarlyArticle 2019 ftdatacite https://doi.org/10.7892/boris.132229 2021-11-05T12:55:41Z At the Astronomical Institute of the University of Bern (AIUB) long time-series (1995 - 2017) of low resolution (spherical harmonic degree/order 6) gravity field coefficients have been determined from a combination of LAGEOS and geodetic SLR satellites in low Earth orbit, namely: Beacon-C, Ajisai, Starlette, Stella, Larets, and Lares. Monthly gravity fields, excluding degree 1 terms, are co-estimated with orbits (10-day LAGEOS and 1-day LEO arcs), station coordinates, range biases, geocenter variations and Earth orientation parameters. For the period 2003-2016 also GRACE monthly gravity fields were produced at AIUB with a significantly higher resolution (degree/order 90). After truncation of the gravity field corresponding to SLR the derived mass variations match well in selected areas with strong mass transport signals and SLR can thus serve to shed light on mass transport in the pre-GRACE period. Finally monthly gravity fields have been determined from high-low tracking data of the three SWARM satellites and are combined with SLR at normal equation level. The combined gravity fields turn out to be well suited for Greenland ice mass observation at low spatial resolution and therefore bridge the gap between GRACE and GRACE-FO. Text Greenland DataCite Metadata Store (German National Library of Science and Technology) Greenland Stella ENVELOPE(-64.254,-64.254,-65.249,-65.249)
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language English
topic 520 Astronomy
spellingShingle 520 Astronomy
Meyer, Ulrich
Sosnica, Krzsztof
Andritsch, Florian
Dach, Rolf
Jäggi, Adrian
König, Daniel
Thaller, Daniela
SLR, GRACE and SWARM gravity field determination and combination
topic_facet 520 Astronomy
description At the Astronomical Institute of the University of Bern (AIUB) long time-series (1995 - 2017) of low resolution (spherical harmonic degree/order 6) gravity field coefficients have been determined from a combination of LAGEOS and geodetic SLR satellites in low Earth orbit, namely: Beacon-C, Ajisai, Starlette, Stella, Larets, and Lares. Monthly gravity fields, excluding degree 1 terms, are co-estimated with orbits (10-day LAGEOS and 1-day LEO arcs), station coordinates, range biases, geocenter variations and Earth orientation parameters. For the period 2003-2016 also GRACE monthly gravity fields were produced at AIUB with a significantly higher resolution (degree/order 90). After truncation of the gravity field corresponding to SLR the derived mass variations match well in selected areas with strong mass transport signals and SLR can thus serve to shed light on mass transport in the pre-GRACE period. Finally monthly gravity fields have been determined from high-low tracking data of the three SWARM satellites and are combined with SLR at normal equation level. The combined gravity fields turn out to be well suited for Greenland ice mass observation at low spatial resolution and therefore bridge the gap between GRACE and GRACE-FO.
format Text
author Meyer, Ulrich
Sosnica, Krzsztof
Andritsch, Florian
Dach, Rolf
Jäggi, Adrian
König, Daniel
Thaller, Daniela
author_facet Meyer, Ulrich
Sosnica, Krzsztof
Andritsch, Florian
Dach, Rolf
Jäggi, Adrian
König, Daniel
Thaller, Daniela
author_sort Meyer, Ulrich
title SLR, GRACE and SWARM gravity field determination and combination
title_short SLR, GRACE and SWARM gravity field determination and combination
title_full SLR, GRACE and SWARM gravity field determination and combination
title_fullStr SLR, GRACE and SWARM gravity field determination and combination
title_full_unstemmed SLR, GRACE and SWARM gravity field determination and combination
title_sort slr, grace and swarm gravity field determination and combination
publisher (:null)
publishDate 2019
url https://dx.doi.org/10.7892/boris.132229
https://boris.unibe.ch/132229/
long_lat ENVELOPE(-64.254,-64.254,-65.249,-65.249)
geographic Greenland
Stella
geographic_facet Greenland
Stella
genre Greenland
genre_facet Greenland
op_rights info:eu-repo/semantics/openAccess
op_doi https://doi.org/10.7892/boris.132229
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