Monthly gravity field models derived from GRACE Level 1B data using a modified short-arc approach

被引:47
|
作者
Chen, Qiujie [1 ,2 ,3 ]
Shen, Yunzhong [1 ,2 ]
Zhang, Xingfu [4 ]
Hsu, Houze [5 ]
Chen, Wu [3 ]
Ju, Xiaolei [1 ]
Lou, Lizhi [1 ]
机构
[1] Tongji Univ, Coll Surveying & Geoinformat, Shanghai 200092, Peoples R China
[2] Ctr Spatial Informat Sci & Sustainable Dev, Shanghai, Peoples R China
[3] Hong Kong Polytech Univ, Dept Land Surveying & Geoinformat, Hong Kong, Hong Kong, Peoples R China
[4] Guangdong Univ Technol, Dept Surveying & Mapping, Guangzhou, Guangdong, Peoples R China
[5] Chinese Acad Sci, Inst Geodesy & Geophys, State Key Lab Geodesy & Earths Dynam, Wuhan, Peoples R China
基金
中国国家自然科学基金;
关键词
satellite gravimetry; monthly gravity field model; GRACE; short-arc approach; MASS-BALANCE; VARIABILITY; RECOVERY;
D O I
10.1002/2014JB011470
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
In this study, a new time series of Gravity Recovery and Climate Experiment (GRACE) monthly solutions, complete to degree and order 60 spanning from January 2003 to August 2011, has been derived based on a modified short-arc approach. Our models entitled Tongji-GRACE01 are available on the website of International Centre for Global Earth Models (http://icgem.gfz-potsdam.de/ICGEM/). The traditional short-arc approach, with no more than 1h arcs, requires the gradient corrections of satellite orbits in order to reduce the impact of orbit errors on the final solution. Here the modified short-arc approach has been proposed, which has three major differences compared to the traditional one: (1) All the corrections of orbits and range rate measurements are solved together with the geopotential coefficients and the accelerometer biases using a weighted least squares adjustment; (2) the boundary position parameters are not required; and (3) the arc length can be extended to 2h. The comparisons of geoid degree powers and the mass change signals in the Amazon basin, the Antarctic, and Antarctic Peninsula demonstrate that our model is comparable with the other existing models, i.e., the Centre for Space Research RL05, Jet Propulsion Laboratory RL05, and GeoForschungsZentrum RL05a models. The correlation coefficients of the mass change time series between our model and the other models are better than 0.9 in the Antarctic and Antarctic Peninsula. The mass change rates in the Antarctic and Antarctic Peninsula derived from our model are -92.738.0Gt/yr and -23.912.4Gt/yr, respectively, which are very close to those from other three models and with similar spatial patterns of signals.
引用
收藏
页码:1804 / 1819
页数:16
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