Significance of secular trends of mass variations determined from GRACE solutions

authored by: Holger Steffen, Svetozar Petrovic, Jürgen Müller, Roland Schmidt, Johann Wünsch, Franz Barthelmes, Jürgen Kusche
Abstract: Since 2002 the Earth's gravity field is globally observed by the Gravity Recovery and Climate Experiment (GRACE) satellite mission. The GRACE monthly gravity field solutions, available from several analysis centres, reflect mass variations in the atmosphere, hydrosphere and geosphere. Due to correlated noise contained in these solutions, it is, however, first necessary to apply an appropriate filtering technique. The resulting, smoothed time series are applied not only to determine variations with different periodic signatures (e.g., seasonal, short and medium-term), but to derive long-periodic mass variations and secular trends as well. As the GRACE monthly solutions always show the integral effect of all mass variations, for separation of single processes, like the GIA (Glacial isostatic adjustment)-related mass increase in Fennoscandia, appropriate reduction models (e.g. from hydrology) are necessary. In this study we show for the example of the Fennoscandian uplift area that GRACE solutions from different analysis centres yield considerably different secular trends. Furthermore, it turns out that the inevitable filtering of the monthly gravity field models affects not only the amplitudes of the signals, but also their spatial resolution and distribution such as the spatial form of the detected signals. It also becomes evident that the determination of trends has to be performed together with the determination of periodic components. All periodic terms which are really contained in the data, and only such, have to be included. The restricted time span of the available GRACE measurements, however, limits the separation of long-periodic and secular signals. It is shown that varying the analysis time span affects the results considerably. Finally, a reduction of hydrological signals from the detected integral secular trends using global hydrological models (WGHM, LaDWorld, GLDAS) is attempted. The differences among the trends resulting from different models illustrate that the state-of-the-art hydrology models are not suitable for this purpose as yet. Consequently, taking the GRACE monthly gravity field solutions from one centre, choosing a single filter and applying an insufficiently reliable reduction model leads sometimes to a misinterpretation of considered geophysical processes. Therefore, one has to be cautious with the final interpretation of the results.
Organisation(s): Institute of Geodesy
External Organisation(s): University of Calgary
Helmholtz Centre Potsdam - German Research Centre for Geosciences
Airbus Group
Astrium GmbH
Type: Article
Journal: Journal of geodynamics
Volume: 48
Pages: 157-165
No. of pages: 9
ISSN: 0264-3707
Publication date: 30.09.2009
Publication status: Published
Peer reviewed: Yes
ASJC Scopus subject areas: Geophysics, Earth-Surface Processes
Sustainable Development Goals: SDG 13 - Climate Action
Electronic version(s): https://doi.org/10.1016/j.jog.2009.09.029 (Access: Unknown)
: Details in the research portal "Research@Leibniz University"

BibTeX

@article{d33a6d878fa14a5a819ca31b886dcda2,
title = "Significance of secular trends of mass variations determined from GRACE solutions",
abstract = "Since 2002 the Earth's gravity field is globally observed by the Gravity Recovery and Climate Experiment (GRACE) satellite mission. The GRACE monthly gravity field solutions, available from several analysis centres, reflect mass variations in the atmosphere, hydrosphere and geosphere. Due to correlated noise contained in these solutions, it is, however, first necessary to apply an appropriate filtering technique. The resulting, smoothed time series are applied not only to determine variations with different periodic signatures (e.g., seasonal, short and medium-term), but to derive long-periodic mass variations and secular trends as well. As the GRACE monthly solutions always show the integral effect of all mass variations, for separation of single processes, like the GIA (Glacial isostatic adjustment)-related mass increase in Fennoscandia, appropriate reduction models (e.g. from hydrology) are necessary. In this study we show for the example of the Fennoscandian uplift area that GRACE solutions from different analysis centres yield considerably different secular trends. Furthermore, it turns out that the inevitable filtering of the monthly gravity field models affects not only the amplitudes of the signals, but also their spatial resolution and distribution such as the spatial form of the detected signals. It also becomes evident that the determination of trends has to be performed together with the determination of periodic components. All periodic terms which are really contained in the data, and only such, have to be included. The restricted time span of the available GRACE measurements, however, limits the separation of long-periodic and secular signals. It is shown that varying the analysis time span affects the results considerably. Finally, a reduction of hydrological signals from the detected integral secular trends using global hydrological models (WGHM, LaDWorld, GLDAS) is attempted. The differences among the trends resulting from different models illustrate that the state-of-the-art hydrology models are not suitable for this purpose as yet. Consequently, taking the GRACE monthly gravity field solutions from one centre, choosing a single filter and applying an insufficiently reliable reduction model leads sometimes to a misinterpretation of considered geophysical processes. Therefore, one has to be cautious with the final interpretation of the results.",
keywords = "Filtering, Glacial isostatic adjustment, Global hydrology models, GRACE, Mass variation",
author = "Holger Steffen and Svetozar Petrovic and J{\"u}rgen M{\"u}ller and Roland Schmidt and Johann W{\"u}nsch and Franz Barthelmes and J{\"u}rgen Kusche",
note = "Funding information: We would like to thank the GRACE science team for the overall support, CSR, University of Texas, JPL Pasadena, ITG Bonn , and CNES Toulouse for providing the GRACE monthly solutions, and Petra D{\"o}ll and her group for making the WGHM data available. We would also like to thank Andreas G{\"u}ntner (GFZ), Sean Swenson (University of Colorado), Wouter van der Wal (TU Delft), and Matthias Weigelt (Universit{\"a}t Stuttgart) for helpful discussions. We are very grateful for the excellent reviews and numerous valuable suggestions of two anonymous referees, which have greatly improved this manuscript. This research was funded by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) through research grant MU1141/8-1 (SPP 1257) and by the German Ministry of Education and Research (BMBF) within the geoscientific R + D programme GEOTECHNOLOGIEN under grant 03F0424A .",
year = "2009",
month = sep,
day = "30",
doi = "10.1016/j.jog.2009.09.029",
language = "English",
volume = "48",
pages = "157--165",
journal = "Journal of geodynamics",
issn = "0264-3707",
publisher = "Elsevier Ltd.",
number = "3-5",
}