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  • 1
    Publication Date: 2023-10-04
    Description: Abstract
    Description: GGM05C is an unconstrained global gravity model complete to degree and order 360 determined from 1) GRACE K-band intersatellite range-rate data, GPS tracking and GRACE accelerometer data, 2) GOCE gradiometer data (ZZ+YY+XX+XZ) spanning the entire mission using a band pass filter of 10-50 mHz and polar gap filled with synthetic gradients from GGM05S to degree/order 150 evaluated at 200-km altitude, and 3) terrestrial gravity anomalies from DTU13 (Andersen et al., 2014). The value for C20 has been replaced with a value derived from satellite laser ranging. No rate terms were modeled. For additional details on the background modeling, see the CSR RL05 processing standards document available at ftp://podaac.jpl.nasa.gov/allData/grace/docs/L2-CSR0005_ProcStd_v4.0.pdf (Bettadpur 2012). Detailed information about GGM05C is available at ftp://ftp.csr.utexas.edu/pub/grace/GGM05/README_GGM05C.pdf (Ries et al., 2016).
    Keywords: ICGEM ; global gravitational model ; GRACE ; GOCE
    Language: English
    Type: Dataset , Dataset
    Format: 1734765 Bytes
    Format: 3 Files
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  • 2
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    In:  Geophysical Research Abstracts Vol. 19, EGU2017-4566
    Publication Date: 2020-02-12
    Description: As of the time of this abstract submission, the GRACE Follow-On satellites have been constructed and transferredto Ottobrunn near Munich for several months of operational testing in the IABG test centre. The Russian/UkraineDnepr launcher had to be exchanged and a corresponding new contract has been signed by GFZ and IridiumSatellite LLC. This includes a "Rideshare" between GRACE-FO and 5 Iridium-Next satellites on a Space-XFalcon-9 from Vandenberg Air Force Base in California within the launch period December 2017 till February2018.The project team is conducting tests of satellite and instrument operation and performance and evaluatingupdated simulations of expected performance on-orbit, including the assessment of inter-satellite ranging (forboth microwave and laser instruments), accelerometer, thermal variability and deformation, and other instrumentand measurement errors. In addition, all required ground analysis software of the Science Data System is in devel-opment and being tested at JPL, UTCSR, and GFZ, in preparation for fully integrated end-to-end (international)testing from Level-1 through Level-3 data within 2017. In this presentation, we will provide the detailed status ofproject integration and test, the latest simulations of science performance, and a revised schedule for remainingproject milestones.
    Language: English
    Type: info:eu-repo/semantics/conferenceObject
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  • 3
    Publication Date: 2020-12-11
    Description: Since June, 2018, the Gravity Recovery and Climate Experiment Follow‐On (GRACE‐FO) is extending the 15‐year monthly mass change record of the GRACE mission, which ended in June 2017. The GRACE‐FO instrument and flight system performance has improved over GRACE. Better attitude solutions and enhanced pointing performance result in reduced fuel consumption and gravity range rate post‐fit residuals. One accelerometer requires additional calibrations due to unexpected measurement noise. The GRACE‐FO gravity and mass change fields from June 2018 through December 2019 continue the GRACE record at an equivalent precision and spatio‐temporal sampling. During this period, GRACE‐FO observed large interannual terrestrial water variations associated with excess rainfall (Central US, Middle East), drought (Europe, Australia), and ice melt (Greenland). These observations are consistent with independent mass change estimates, providing high confidence that no inter‐mission biases exist from GRACE to GRACE‐FO, despite the 11‐month gap. GRACE‐FO has also successfully demonstrated satellite‐to‐satellite laser ranging interferometry.
    Language: English
    Type: info:eu-repo/semantics/article
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  • 4
    Publication Date: 2020-10-14
    Description: The twin satellites of the Gravity Recovery and Climate Experiment (GRACE) Follow-On mission were successfully launched in May-2018. The primary objective of the mission is to continue the 15-year GRACE (2002-2017) global data record of Earth’s monthly mass changes. These measurements have become an indispensable tool to quantify and track Earth’s water movement and surface mass changes across the planet. Monitoring changes in ice sheets and glaciers, near-surface and underground water storage, the amount of water in large lakes and rivers, as well as changes in sea level and ocean currents provides an integrated global view of how Earth’s water cycle and energy balance are evolving. In this presentation we will present the current mission status, including instrument and flight system performance, discuss science data quality and performance as well as recent science results from the first two years of observations, and address data continuity from GRACE to GRACE Follow-On.
    Language: English
    Type: info:eu-repo/semantics/conferenceObject
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  • 5
    Publication Date: 2021-04-07
    Language: English
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  • 6
    Publication Date: 2023-08-02
    Description: The GRACE Follow-On mission, a partnership between NASA (US) and GFZ (Germany), reached its nominal five-year mission lifetime in May 2023, and is entering its extended mission phase through the end of 2026. GRACE-FO continues the unique essential climate data record of mass change in the Earth system initiated in 2002 by the GRACE mission (2002-2017). The combined GRACE & GRACE-FO data records now span over 22 years and provide unique observations of monthly to decadal global mass changes and transport in the Earth system derived from temporal variations in the Earth’s gravity field. These observations have become indispensable for climate-related studies that enable process understanding of the evolving global water cycle, including ocean dynamics, polar ice mass changes, and near-surface and global ground water changes.In this presentation, we will review (1) some recent GRACE/GRACE-FO science and applications highlights, (2) key data processing and calibration approaches on GRACE-FO and lessons learned during the 5-year prime mission, and (3) the GRACE-FO mission plan to operate and collect high-quality science data through the intensifying solar cycle 25, aiming for continuity with a future Mass Change mission that is currently planned by NASA and DLR.
    Language: English
    Type: info:eu-repo/semantics/conferenceObject
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  • 7
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    In:  XXVIII General Assembly of the International Union of Geodesy and Geophysics (IUGG)
    Publication Date: 2023-07-25
    Description: A precisely determined Geocenter motion contributes to the realization of the origin of reference frame. On the other hand, A precisely defined and accurate reference frame improves the understanding Geocenter motion. We can determine Geocenter motion from the GPS data of Low-Earth Orbit (LEO) satellites. We can also estimate the motion from the Satellite Laser Ranging (SLR) data. The separate Geocenter motion solutions from LEO GPS or SLR data have been studied. The solutions have good agreements. If the solutions came from LEO GPS and SLR data, what are the differences and impacts? Based on this motivation, we investigate the Geocenter motion determination from the combination of the GPS and SLR data. In this study, the combination approach and the results will be described and analyzed.
    Language: English
    Type: info:eu-repo/semantics/conferenceObject
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  • 8
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    In:  XXVIII General Assembly of the International Union of Geodesy and Geophysics (IUGG)
    Publication Date: 2023-09-06
    Description: The goal for the next generation of terrestrial reference frames (TRF) is to achieve a 1mm and 0.1mm/yr accurate frame realization through the combination of reference station solutions by multi-technique geodetic observatories (GOs), quality benchmarks which are motivated by the user needs from commercial and scientific disciplines that rely on high precision positioning and spatial referencing. A potentially significant source of error in TRF realizations is the inter-system ties between the instruments at multi-technique stations, usually independently measured through ground-based local surveys. In this work, a successful endeavor to satisfy the tie accuracy goals while exceeding the 200m GGOS baseline guidelines is detailed for the McDonald Geodetic Observatory (MGO), located in the Davis Mountains, Texas, USA. MGO consists of a VLBI Geodetic Observing System (VGOS), infrastructure in place for a Space Geodesy Satellite Laser Ranging (SGSLR) telescope, and several GNSS stations spanning a 900m baseline and a 120m elevation change. The results of the local ties between the GNSS stations across the near-kilometer baseline, as measured between their antenna reference points, show sub-mm precision and 1mm accuracy. These results are validated through day to day repeatability across several metrology surveys conducted in 2021 and sub-mm consistency in direct comparisons with baselines derived from GPS monthly averaged solutions. This presentation will report these results, highlighting the novel designs and techniques employed in the procedure, processing, and error-budget analysis. We present framework for assessment of sensitivities of future TRF realizations to ingesting ties of this quality, and present preliminary results.
    Language: English
    Type: info:eu-repo/semantics/conferenceObject
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