Data for: Filling the data gaps within GRACE missions using Singular Spectrum Analysis

Dozens of missing epochs in the monthly gravity product of the satellite mission Gravity Recovery and Climate Experiment ( GRACE ) and its follow-on ( GRACE-FO ) mission greatly inhibit the complete analysis and full utilization of the data. Despite previous attempts to handle this problem, a genera...

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Main Authors: Yi, Shuang, Sneeuw, Nico
Other Authors: Schlesinger, Ron
Language:unknown
Published: DaRUS 2021
Subjects:
SSA
Online Access:https://doi.org/10.18419/darus-807
id ftustuttdatavers:doi:10.18419/darus-807
record_format openpolar
spelling ftustuttdatavers:doi:10.18419/darus-807 2024-01-07T09:43:40+01:00 Data for: Filling the data gaps within GRACE missions using Singular Spectrum Analysis Yi, Shuang Sneeuw, Nico Schlesinger, Ron 2021-05-14 https://doi.org/10.18419/darus-807 unknown DaRUS https://doi.org/10.18419/darus-807 Earth and Environmental Sciences GRACE satellite gravimetry data gap SSA gap filling 2021 ftustuttdatavers https://doi.org/10.18419/darus-807 2023-12-10T23:54:27Z Dozens of missing epochs in the monthly gravity product of the satellite mission Gravity Recovery and Climate Experiment ( GRACE ) and its follow-on ( GRACE-FO ) mission greatly inhibit the complete analysis and full utilization of the data. Despite previous attempts to handle this problem, a general all-purpose gap-filling solution is still lacking. Here we propose a non-parametric, data-adaptive and easy-to-implement approach - composed of the Singular Spectrum Analysis (SSA) gap-filling technique, cross-validation, and spectral testing for significant components - to produce reasonable gap-filling results in the form of spherical harmonic coefficients (SHCs). We demonstrate that this approach is adept at inferring missing data from long-term and oscillatory changes extracted from available observations. A comparison in the spectral domain reveals that the gap-filling result resembles the product of GRACE missions below spherical harmonic degree 30 very well. As the degree increases above 30, the amplitude per degree of the gap-filling result decreases more rapidly than that of GRACE/GRACE-FO SHCs, showing effective suppression of noise. As a result, our approach can reduce noise in the oceans without sacrificing resolutions on land. The gap filling dataset is stored in the “SSA_filing/" folder. Each file represents a monthly result in the form of spherical harmonics. The data format follows the convention of the site ftp://isdcftp.gfz-potsdam.de/grace/. Low degree corrections (degree-1, C20, C30) have been made. The code to generate the dataset is located in the “code_share/“ folder, with an example for C30. The model-based Greenland mass balance result for data validation (results given in the paper) is provided in the "Greenland_SMB-D.txt” file. Other/Unknown Material Greenland DaRUS (University of Stuttgart) Greenland
institution Open Polar
collection DaRUS (University of Stuttgart)
op_collection_id ftustuttdatavers
language unknown
topic Earth and Environmental Sciences
GRACE
satellite gravimetry
data gap
SSA
gap filling
spellingShingle Earth and Environmental Sciences
GRACE
satellite gravimetry
data gap
SSA
gap filling
Yi, Shuang
Sneeuw, Nico
Data for: Filling the data gaps within GRACE missions using Singular Spectrum Analysis
topic_facet Earth and Environmental Sciences
GRACE
satellite gravimetry
data gap
SSA
gap filling
description Dozens of missing epochs in the monthly gravity product of the satellite mission Gravity Recovery and Climate Experiment ( GRACE ) and its follow-on ( GRACE-FO ) mission greatly inhibit the complete analysis and full utilization of the data. Despite previous attempts to handle this problem, a general all-purpose gap-filling solution is still lacking. Here we propose a non-parametric, data-adaptive and easy-to-implement approach - composed of the Singular Spectrum Analysis (SSA) gap-filling technique, cross-validation, and spectral testing for significant components - to produce reasonable gap-filling results in the form of spherical harmonic coefficients (SHCs). We demonstrate that this approach is adept at inferring missing data from long-term and oscillatory changes extracted from available observations. A comparison in the spectral domain reveals that the gap-filling result resembles the product of GRACE missions below spherical harmonic degree 30 very well. As the degree increases above 30, the amplitude per degree of the gap-filling result decreases more rapidly than that of GRACE/GRACE-FO SHCs, showing effective suppression of noise. As a result, our approach can reduce noise in the oceans without sacrificing resolutions on land. The gap filling dataset is stored in the “SSA_filing/" folder. Each file represents a monthly result in the form of spherical harmonics. The data format follows the convention of the site ftp://isdcftp.gfz-potsdam.de/grace/. Low degree corrections (degree-1, C20, C30) have been made. The code to generate the dataset is located in the “code_share/“ folder, with an example for C30. The model-based Greenland mass balance result for data validation (results given in the paper) is provided in the "Greenland_SMB-D.txt” file.
author2 Schlesinger, Ron
author Yi, Shuang
Sneeuw, Nico
author_facet Yi, Shuang
Sneeuw, Nico
author_sort Yi, Shuang
title Data for: Filling the data gaps within GRACE missions using Singular Spectrum Analysis
title_short Data for: Filling the data gaps within GRACE missions using Singular Spectrum Analysis
title_full Data for: Filling the data gaps within GRACE missions using Singular Spectrum Analysis
title_fullStr Data for: Filling the data gaps within GRACE missions using Singular Spectrum Analysis
title_full_unstemmed Data for: Filling the data gaps within GRACE missions using Singular Spectrum Analysis
title_sort data for: filling the data gaps within grace missions using singular spectrum analysis
publisher DaRUS
publishDate 2021
url https://doi.org/10.18419/darus-807
geographic Greenland
geographic_facet Greenland
genre Greenland
genre_facet Greenland
op_relation https://doi.org/10.18419/darus-807
op_doi https://doi.org/10.18419/darus-807
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