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231.
Errors in high-frequency ocean tide models alias to low frequencies in time-variable gravity solutions from the Gravity Recovery
and Climate Experiment (GRACE). We conduct an observational study of apparent gravity changes at a period of 161 days, the
alias period of errors in the S2 semidiurnal solar tide. We examine this S2 alias in the release 4 (RL04) reprocessed GRACE monthly gravity solutions for the period April 2002 to February 2008, and
compare with that in release 1 (RL01) GRACE solutions. One of the major differences between RL04 and RL01 is the ocean tide
model. In RL01, the alias is evident at high latitudes, near the Filchner-Ronne and Ross ice shelves in Antarctica, and regions
surrounding Greenland and Hudson Bay. RL04 shows significantly lower alias amplitudes in many of these locations, reflecting
improvements in the ocean tide model. However, RL04 shows continued alias contamination between the Ronne and Larson ice shelves,
somewhat larger than in RL01, indicating a need for further tide model improvement in that region. For unknown reasons, the
degree-2 zonal spherical harmonics (C20) of the RL04 solutions show significantly larger S2 aliasing errors than those from RL01. 相似文献
232.
Since its launch in 2002, the Gravity Recovery and Climate Experiment (GRACE) mission has been providing measurements of the
time-varying Earth gravity field. The GRACE mission architecture includes two satellites in near-circular, near-polar orbits
separated in the along-track direction by approximately 220 km (e.g. collinear). A microwave ranging instrument measures changes
in the distance between the spacecraft, while accelerometers on each spacecraft are used to measure changes in distance due
to non-gravitational forces. The fact that the satellites are in near-polar orbits coupled with the fact that the inter-satellite
range measurements are directed in the along-track direction, contributes to longitudinal striping in the estimated gravity
fields. This paper examines four candidate mission architectures for a future gravity recovery satellite mission to assess
their potential in measuring the gravity field more accurately than GRACE. All satellites were assumed to have an improved
measurement system, with an inter-satellite laser ranging instrument and a drag-free system for removal of non-gravitational
accelerations. Four formations were studied: a two-satellite collinear pair similar to GRACE; a four-satellite architecture
with two collinear pairs; a two-satellite cartwheel formation; and a four-satellite cartwheel formation. A cartwheel formation
consists of satellites performing in-plane, relative elliptical motion about their geometric center, so that inter-satellite
measurements are, at times, directed radially (e.g. parallel to the direction towards the center of the Earth) rather than
along-track. Radial measurements, unlike along-track measurements, have equal sensitivity to mass distribution in all directions
along the Earth’s surface and can lead to higher spatial resolution in the derived gravity field. The ability of each architecture
to recover the gravity field was evaluated using numerical simulations performed with JPL’s GIPSY-OASIS software package.
Thirty days of data were used to estimate gravity fields complete to degree and order 60. Evaluations were done for 250 and
400 km nominal orbit altitudes. The sensitivity of the recovered gravity field to under-sampled effects was assessed using
simulated errors in atmospheric/ocean dealiasing (AOD) models. Results showed the gravity field errors associated with the
four-satellite cartwheel formation were approximately one order of magnitude lower than the collinear satellite pair when
only measurement system errors were included. When short-period AOD model errors were introduced, the gravity field errors
for each formation were approximately the same. The cartwheel formations eliminated most of the longitudinal striping seen
in the gravity field errors. A covariance analysis showed the error spectrum of the cartwheel formations to be lower and more
isotropic than that of the collinear formations. 相似文献
233.
LEO星载GPS双向滤波定轨研究 总被引:1,自引:1,他引:0
介绍了目前常用的LEO(low Earth orbiter)星载GPS定轨方法,分析了LEO星载GPS双向滤波定轨方法与其他几种主要定轨方法的区别.从卫星运动方程和星载GPS非差定轨观测方程出发,给出了LEO星载GPS双向滤波定轨方法的原理,采用自行研制的定轨软件对两颗GRACE(gravity recovery and climate ex-periment)卫星进行了定轨试验,通过与JPL(Jet Propulsion Laboratory)轨道的对比及KBR(k-band rangingsystem)观测数据的外部检核发现:①双向滤波定轨技术不仅能显著提高单向滤波开始阶段的定轨精度,而且可以从整体上提高卫星的定轨精度;②LEO星载GPS双向滤波定轨方法切实可行,相应的星载GPS定轨软件对GRACE卫星定轨精度在径向、沿轨方向和法向优于5 cm. 相似文献
234.
??????????????λ???????????????????????????????仯?????????С????????????????GRACE????????????????λ????????????????е??????????????????????????????????????????????????????????????????????????????????????仯???????????????????????????????????????????????????????????????????6????????????? 相似文献
235.
匡翠林 《大地测量与地球动力学》2009,29(4):88-92
???????л??????????????????ж???????????????????????????????????????????????????????????????????????????????????????????ж???????????????о???????????CHAMP??GRACE????????顣??????????÷???????????????????????????????????????????????????????????????????????????????? 相似文献
236.
����GRACE�����������������������ļ��� 总被引:8,自引:3,他引:5
???????????????????????????????????????????PEM??????С????Э????????LSM????????120??GRACE???????????????????????????1??????????JPL??????GRACE???????????????????????120?????????PEM??LSM???????????λ?????????5.192??10-10????6.633??10-10????2????????PEM??LSM???120?????????λ???????????1?GFZ??????EIGEN-GRACE02S???????????????????????????????????????????PEM??LSM????????????????????????Ч???3?????????PEM??LSM?????????????λ????????????????????????????????????????????????????????????120??GRACE??????????????????? 相似文献
237.
?о???????漰????GPS?????????????????CHAMP??GRACE????GPS???????????????????????????????????????????????????????????????????PANDA??????????????????????????????????????????????ν??????????????????????????????????????????????? 相似文献
238.
239.
Recent hydrological behavior of the East African great lakes region inferred from GRACE,satellite altimetry and rainfall observations 总被引:1,自引:0,他引:1
Mélanie Becker William LLovel Anny Cazenave Andreas Güntner Jean-François Crétaux 《Comptes Rendus Geoscience》2010,342(3):223-233
We have jointly analysed space gravimetry data from the GRACE space mission, satellite altimetry data and precipitation over the East African Great Lakes region, in order to study the spatiotemporal variability of hydrological parameters (total water storage, lake water volume and rainfall). We find that terrestrial water storage (TWS) from GRACE and precipitation display a common mode of variability at interannual time scale, with a minimum in late 2005, followed by a rise in 2006–2007. We argue that this event is due to forcing by the strong 2006 Indian Ocean Dipole (IOD) on East African rainfall. We also show that GRACE TWS is linked to the El Niño-Southern Oscillation cycle. Combination of the altimetry-based lake water volume with TWS from GRACE over the lakes drainage basins allows estimating soil moisture and groundwater volume variations. Comparison with the WGHM hydrological model outputs is performed and discussed. 相似文献
240.
介绍了自主开发的卫星重力测量数据处理软件--GRASTAR,给出了该软件的整体设计框架和功能.该软件主要采用动力学法实现,应用CHAMP卫星和GRACE卫星的观测数据反演地球重力场模型.利用模拟方法验证了该软件的正确性,并利用GRASTAR处理了126 d的CHAMP卫星数据,解算出直到40阶次重力场模型的初步结果. 相似文献