• Sorted by Date • Sorted by Last Name of First Author •
Zhang, Lin, Shen, Yunzhong, Ji, Kunpu, and Chen, Qiujie, 2025. An Enhanced Parameter Filtering Approach for Postprocessing GRACE Monthly Gravity Field Models. IEEE Geoscience and Remote Sensing Letters, 22:LGRS.2025, doi:10.1109/LGRS.2025.3575197.
• from the NASA Astrophysics Data System • by the DOI System •
@ARTICLE{2025IGRSL..22L5197Z,
author = {{Zhang}, Lin and {Shen}, Yunzhong and {Ji}, Kunpu and {Chen}, Qiujie},
title = "{An Enhanced Parameter Filtering Approach for Postprocessing GRACE Monthly Gravity Field Models}",
journal = {IEEE Geoscience and Remote Sensing Letters},
keywords = {Gauss-Markov process, gravity recovery and climate experiment (GRACE), parameter filtering (PF), signal extraction},
year = 2025,
month = jan,
volume = {22},
eid = {LGRS.2025},
pages = {LGRS.2025},
abstract = "{An effective filtering approach is essential for accurately interpreting
gravity recovery and climate experiment (GRACE) monthly gravity
field models. The improved parameter filtering (IPF) (Zhang et
al., 2024) simultaneously estimates signal components with
deterministic harmonic parameters and time-variable irregular
signals through Kalman filtering (KF), followed by signal
denoising based on their signal and noise covariance matrices.
However, it has two critical limitations: 1) excessive
computational burden due to redundant dynamic calculations of
deterministic parameters in KF and 2) signal attenuation
resulting from a suboptimal two-step estimation framework. For
this reason, this letter proposes an enhanced parameter
filtering (EPF) based on a more rigorous parameter estimation
criterion, which independently resolves deterministic parameters
and irregular signals, thereby avoiding dynamic estimations of
deterministic parameters while effectively integrating the two-
step procedures of IPF. Here, we employ EPF to denoise the ITSG-
Grace2018 model at degree 96 from April 2002 to December 2023,
comparing its performance with IPF. Results demonstrate that the
computational efficiency of EPF is improved by 92.3\%, with
fitting errors reduced by 62.4\% and signal-to-noise ratios
enhanced by 4.4\%. Spatial analysis of filtered global
Terrestrial Water Storage Anomalies (TWSAs) shows EPF better
matches center for space research Mascon (CSRM) RL06, jet
propulsion laboratory Mascon (JPLM) RL06, and NOAH products,
with average Nash-Sutcliffe Coefficients increased by 1.7\%,
2.9\%, and 8.3\%, respectively. Further comparisons of TWSAs
across 30 global basins, mass changes in Greenland and
Antarctica, and co-seismic gravity signals of the 2004 Sumatra-
Andaman and 2010 Chile earthquakes, reveal the superior
performance of EPF over IPF and four recently proposed filters.}",
doi = {10.1109/LGRS.2025.3575197},
adsurl = {https://ui.adsabs.harvard.edu/abs/2025IGRSL..22L5197Z},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
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