Please use this identifier to cite or link to this item: http://hdl.handle.net/10397/100707
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dc.contributorDepartment of Land Surveying and Geo-Informaticsen_US
dc.creatorChen, Qen_US
dc.creatorShen, Yen_US
dc.creatorChen, Wen_US
dc.creatorFrancis, Oen_US
dc.creatorZhang, Xen_US
dc.creatorChen, Qen_US
dc.creatorLi, Wen_US
dc.creatorChen, Ten_US
dc.date.accessioned2023-08-11T03:12:49Z-
dc.date.available2023-08-11T03:12:49Z-
dc.identifier.issn2169-9313en_US
dc.identifier.urihttp://hdl.handle.net/10397/100707-
dc.language.isoenen_US
dc.publisherJohn Wiley & Sonsen_US
dc.rights©2019. American Geophysical Union. All Rights Reserved.en_US
dc.titleAn optimized short‐arc approach : methodology and application to develop refined time series of Tongji‐Grace2018 GRACE monthly solutionsen_US
dc.typeJournal/Magazine Articleen_US
dc.identifier.spage6010en_US
dc.identifier.epage6038en_US
dc.identifier.volume124en_US
dc.identifier.issue6en_US
dc.identifier.doi10.1029/2018JB016596en_US
dcterms.abstractConsidering the unstable inversion of ill-conditioned intermediate matrix required in each integral arc in the short-arc approach presented in Chen et al. (2015, https://doi.org/10.1002/2014JB011470), an optimized short-arc method via stabilizing the inversion is proposed. To account for frequency-dependent noise in observations, a noise whitening technique is implemented in the optimized short-arc approach. Our study shows that the optimized short-arc method is able to stabilize the inversion and eventually prolong the arc length to 6 hr. In addition, the noise whitening method is able to mitigate the impacts of low-frequency noise in observations. Using the optimized short-arc approach, a refined time series of Gravity Recovery and Climate Experiment (GRACE) monthly models called Tongji-Grace2018 has been developed. The analyses allow us to derive the following conclusions: (a) During the analyses over the river basins (i.e., Amazon, Mississippi, Irrawaddy, and Taz) and Greenland, the correlation coefficients of mass changes between Tongji-Grace2018 and others (i.e., CSR RL06, GFZ RL06, and JPL RL06 Mascon) are all over 92% and the corresponding amplitudes are comparable; (b) the signals of Tongji-Grace2018 agree well with those of CSR RL06, GFZ RL06, ITSG-Grace2018, and JPL RL06 Mascon, while Tongji-Grace2018 and ITSG-Grace2018 are less noisy than CSR RL06 and GFZ RL06; (c) clearer global mass change trend and less striping noise over oceans can be observed in Tongji-Grace2018 even only using decorrelation filtering; and (d) for the tests over Sahara, over 36% and 19% of noise reductions are achieved by Tongji-Grace2018 relative to CSR RL06 in the cases of using decorrelation filtering and combined filtering, respectively.en_US
dcterms.accessRightsopen accessen_US
dcterms.bibliographicCitationJournal of geophysical research. B, Solid earth, June 2019, v. 124, no. 6, p. 6010-6038en_US
dcterms.isPartOfJournal of geophysical research. B, Solid earthen_US
dcterms.issued2019-06-
dc.identifier.scopus2-s2.0-85067837811-
dc.identifier.eissn2169-9356en_US
dc.description.validate202305 bckwen_US
dc.description.oaVersion of Recorden_US
dc.identifier.FolderNumberLSGI-0199-
dc.description.fundingSourceOthersen_US
dc.description.fundingTextNational Natural Science Foundation of China; National Key R&D Program of China; Alexander von Humboldt Foundation in Germanyen_US
dc.description.pubStatusPublisheden_US
dc.identifier.OPUS52664057-
dc.description.oaCategoryVoR alloweden_US
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