Time-variable gravity signal during the water impoundment of China's Three-Gorges Reservoir

2002 ◽  
Vol 29 (24) ◽  
pp. 53-1-53-4 ◽  
Author(s):  
Jean-Paul Boy ◽  
Benjamin F. Chao
Keyword(s):  
Three Gorges Reservoir ◽  
Time Variable ◽  
Three Gorges ◽  
Time Variable Gravity ◽  
Variable Gravity ◽  
Gravity Signal ◽  
Water Impoundment

scholarly journals Time-variable gravity signal in Greenland revealed by high-low satellite-to-satellite tracking

2013 ◽  
Vol 118 (7) ◽  
pp. 3848-3859 ◽  
Author(s):  
M. Weigelt ◽  
T. van Dam ◽  
A. Jäggi ◽  
L. Prange ◽  
M. J. Tourian ◽  
...  
Keyword(s):  
Satellite Tracking ◽  
Time Variable ◽  
Time Variable Gravity ◽  
Variable Gravity ◽  
Gravity Signal

Water Storage Changes in Three Gorges Water Systems Area Inferred from Grace Time-Variable Gravity Data

2007 ◽  
Vol 50 (3) ◽  
pp. 650-657 ◽  
Author(s):  
Han-Sheng WANG ◽  
Zhi-Yong WANG ◽  
Xu-Dong YUAN ◽  
Patrick Wu ◽  
Elena Rangelova
Keyword(s):  
Gravity Data ◽  
Water Storage ◽  
Water Systems ◽  
Time Variable ◽  
Three Gorges ◽  
Time Variable Gravity ◽  
Variable Gravity

scholarly journals Time-variable gravity fields derived from GPS tracking of Swarm

2016 ◽  
Vol 205 (3) ◽  
pp. 1665-1669 ◽  
Author(s):  
Aleš Bezděk ◽  
Josef Sebera ◽  
João Teixeira da Encarnação ◽  
Jaroslav Klokočník
Keyword(s):  
Regional Scale ◽  
Time Variable ◽  
Gps Tracking ◽  
Gps Data ◽  
Time Variable Gravity ◽  
Grace Data ◽  
Gravity Fields ◽  
Grace Satellites ◽  
Variable Gravity ◽  
Gravity Signal

Abstract Since 2002 Gravity Recovery and Climate Experiment (GRACE) provides monthly gravity fields from K-band ranging (KBR) between two GRACE satellites. These KBR gravity monthlies have enabled the global observation of time-varying Earth mass signal at a regional scale (about 400 km resolution). Apart from KBR, monthly gravity solutions can be computed from onboard GPS data. The newly reprocessed GPS monthlies from 13 yr of GRACE data are shown to yield correct time-variable gravity signal (seasonality, trends, interannual variations) at a spatial resolution of 1300 km (harmonic degree 15). We show that GPS fields from new Swarm mission are of similar quality as GRACE GPS monthlies. Thus, Swarm GPS monthlies represent new and independent source of information on time-variable gravity, and, although with lower resolution and accuracy, they can be used for its monitoring, particularly if GRACE KBR/GPS data become unavailable before GRACE Follow-On is launched (2017 August).

scholarly journals Evaluation of GRACE/GRACE Follow-On Time-Variable Gravity Field Models for Earthquake Detection above Mw8.0s in Spectral Domain

2021 ◽  
Vol 13 (16) ◽  
pp. 3075
Author(s):  
Ming Xu ◽  
Xiaoyun Wan ◽  
Runjing Chen ◽  
Yunlong Wu ◽  
Wenbing Wang
Keyword(s):  
Signal To Noise Ratio ◽  
Time Variable ◽  
Model Errors ◽  
Signal To Noise ◽  
Time Variable Gravity ◽  
Earthquake Detection ◽  
Gravity Fields ◽  
Variable Gravity ◽  
Gravity Recovery ◽  
Gravity Field Models

This study compares the Gravity Recovery And Climate Experiment (GRACE)/GRACE Follow-On (GFO) errors with the coseismic gravity variations generated by earthquakes above Mw8.0s that occurred during April 2002~June 2017 and evaluates the influence of monthly model errors on the coseismic signal detection. The results show that the precision of GFO monthly models is approximately 38% higher than that of the GRACE monthly model and all the detected earthquakes have signal-to-noise ratio (SNR) larger than 1.8. The study concludes that the precision of the time-variable gravity fields should be improved by at least one order in order to detect all the coseismic gravity signals of earthquakes with M ≥ 8.0. By comparing the spectral intensity distribution of the GFO stack errors and the 2019 Mw8.0 Peru earthquake, it is found that the precision of the current GFO monthly model meets the requirement to detect the coseismic signal of the earthquake. However, due to the limited time length of the observations and the interference of the hydrological signal, the coseismic signals are, in practice, difficult to extract currently.

scholarly journals Earth’s Time-Variable Gravity from GRACE Follow-On K-Band Range-Rates and Pseudo-Observed Orbits

2021 ◽  
Vol 13 (9) ◽  
pp. 1766
Author(s):  
Igor Koch ◽  
Mathias Duwe ◽  
Jakob Flury ◽  
Akbar Shabanloui
Keyword(s):  
Gravity Field ◽  
Time Variable ◽  
Time Variable Gravity ◽  
Gravity Field Recovery ◽  
Variable Gravity ◽  
Earth’S System ◽  
Grace Mission ◽  
Insight Into ◽  
K Band

During its science phase from 2002–2017, the low-low satellite-to-satellite tracking mission Gravity Field Recovery And Climate Experiment (GRACE) provided an insight into Earth’s time-variable gravity (TVG). The unprecedented quality of gravity field solutions from GRACE sensor data improved the understanding of mass changes in Earth’s system considerably. Monthly gravity field solutions as the main products of the GRACE mission, published by several analysis centers (ACs) from Europe, USA and China, became indispensable products for quantifying terrestrial water storage, ice sheet mass balance and sea level change. The successor mission GRACE Follow-On (GRACE-FO) was launched in May 2018 and proceeds observing Earth’s TVG. The Institute of Geodesy (IfE) at Leibniz University Hannover (LUH) is one of the most recent ACs. The purpose of this article is to give a detailed insight into the gravity field recovery processing strategy applied at LUH; to compare the obtained gravity field results to the gravity field solutions of other established ACs; and to compare the GRACE-FO performance to that of the preceding GRACE mission in terms of post-fit residuals. We use the in-house-developed MATLAB-based GRACE-SIGMA software to compute unconstrained solutions based on the generalized orbit determination of 3 h arcs. K-band range-rates (KBRR) and kinematic orbits are used as (pseudo)-observations. A comparison of the obtained solutions to the results of the GRACE-FO Science Data System (SDS) and Combination Service for Time-variable Gravity Fields (COST-G) ACs, reveals a competitive quality of our solutions. While the spectral and spatial noise levels slightly differ, the signal content of the solutions is similar among all ACs. The carried out comparison of GRACE and GRACE-FO KBRR post-fit residuals highlights an improvement of the GRACE-FO K-band ranging system performance. The overall amplitude of GRACE-FO post-fit residuals is about three times smaller, compared to GRACE. GRACE-FO post-fit residuals show less systematics, compared to GRACE. Nevertheless, the power spectral density of GRACE-FO and GRACE post-fit residuals is dominated by similar spikes located at multiples of the orbital and daily frequencies. To our knowledge, the detailed origin of these spikes and their influence on the gravity field recovery quality were not addressed in any study so far and therefore deserve further attention in the future. Presented results are based on 29 monthly gravity field solutions from June 2018 until December 2020. The regularly updated LUH-GRACE-FO-2020 time series of monthly gravity field solutions can be found on the website of the International Centre for Global Earth Models (ICGEM) and in LUH’s research data repository. These operationally published products complement the time series of the already established ACs and allow for a continuous and independent assessment of mass changes in Earth’s system.

scholarly journals Decorrelated GRACE time-variable gravity solutions by GFZ, and their validation using a hydrological model

2009 ◽  
Vol 83 (10) ◽  
pp. 903-913 ◽  
Author(s):  
J. Kusche ◽  
R. Schmidt ◽  
S. Petrovic ◽  
R. Rietbroek
Keyword(s):  
Hydrological Model ◽  
Time Variable ◽  
Time Variable Gravity ◽  
Variable Gravity
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