基于拉格朗日多项式的精密星历坐标插值

为获得任意时刻的卫星坐标位置,采用拉格朗日插值模型对精密星历坐标内插实验验证,并探讨插值模型的适用范围。实验表明,拉格朗日多项式的插值阶数高于10阶时可以获得毫米级的精度,插值阶数高于13阶时精度趋于稳定。利用此方法能满足实际测量工作的要求。     

电源及负载电阻对PTB220型气压传感器检定结果的影响

为保证检定结果的准确可靠,对多台自动气象站用PTB220型气压传感器进行了供电电压及负载电阻的试验。试验结果表明:在12~30V的范围内,随着供电电压的提高,PTB220型气压传感器模拟量输出测量误差存在着逐渐变大的现象,这种变化最大达到了-0.28hPa;而数字量输出则不存在这一问题;当负载电阻在10~500kΩ之间变化时,PTB220型气压传感器的模拟量输出测量误差在测量范围下限附近呈现出随着负载电阻的增加而逐渐增大的现象。基于这一发现,对PTB220型气压传感器检定方法的完善提出了针对性建议。     

A plausible link between the asteroid 21 Lutetia and CH carbonaceous chondrites

A crucial topic in planetology research is establishing links between primitive meteorites and their parent asteroids. In this study, we investigate the feasibility of a connection between asteroids similar to 21 Lutetia, encountered by the Rosetta mission in July 2010, and the CH3 carbonaceous chondrite Pecora Escarpment 91467 (PCA 91467). Several spectra of this meteorite were acquired in the ultraviolet to near‐infrared (0.3–2.2 μm) and in the midinfrared to thermal infrared (2.5–30.0 μm or 4000 to ~333 cm⁻¹), and they are compared here to spectra from the asteroid 21 Lutetia. There are several similarities in absorption bands and overall spectral behavior between this CH3 meteorite and 21 Lutetia. Considering also that the bulk density of Lutetia is similar to that of CH chondrites, we suggest that this asteroid could be similar, or related to, the parent body of these meteorites, if not the parent body itself. However, the apparent surface diversity of Lutetia pointed out in previous studies indicates that it could simultaneously be related to other types of chondrites. Future discovery of additional unweathered CH chondrites could provide deeper insight in the possible connection between this family of metal‐rich carbonaceous chondrites and 21 Lutetia or other featureless, possibly hydrated high‐albedo asteroids.     

TEQC在GPS数据质量检查中的常见问题及解决方案

TEQC是进行GPS数据格式转换、编辑、质量检查的常用工具,在目前GPS数据预处理中应用较为广泛。介绍了TEQC在GPS数据处理中的常用语法及常用命令,总结了使用TEQC进行GPS原始观测数据质量检查时的常见问题,并给出了具体解决方案。     

Changes in hydrodynamic process dominance (wave,tide or river) in foreland sequences: The subalpine Miocene Molasse revisited (France)

A comprehensive sedimentological study was undertaken in the Miocene of the subalpine massifs and southern Jura (France) with the aim to constrain the evolution of process changes in third-order sequences of peripheral foreland basins during the overfilled phase (i.e. sediment supply higher than accommodation space). Fieldwork analyses based on 35 sedimentological sections allowed the identification of four depositional models: wave dominated, mixed wave-tide, river to tide and river dominated. The sections were dated using chemostratigraphy (i.e. marine strontium isotopic ratios), revealing three-third-order sequences between the Upper Aquitanian and the Langhian. Chronostratigraphical and sedimentological results document prominent and recurrent changes in depositional models along third-order sequences: (i) in the earliest stage of the transgression, mixed-energy coastal environments influenced by the local coastal morphology prevailed (in palaeo-highs or incised valleys); (ii) during the course of the transgression, Gilbert delta deposits suggest a prominent steepening linked to a tectonic uplift in the proximal depozone (between the tectonically active frontal part of the orogenic wedge and the proximal foredeep). Instead, in the distal depozone (between the proximal foredeep and the proximal border of the flexural uplifted forebulge), deposits were characterized either by wave-dominated or mixed wave-tide environments and are likely eustatically-driven; (iii) during the maximum flooding stage, water depth remained shallow below the storm-weather wave base; and (iv) during the regression, the proximal depozone is characterized by the progradation of gravel-rich fan deltas. In the distal depozone, mixed wave-tide systems preceded the development of river to tidal depositional environments. These results were integrated and compared with facies models from other basin analogues worldwide. A model tackling the evolution of process changes within third-order sequences (of the overfilled phase) of foreland basins is proposed, thereby improving sequence stratigraphic predictions in foreland basins.     

A SPH framework for dynamic interaction between soil and rigid body system with hybrid contact method

A smoothed particle hydrodynamics (SPH) framework for three-dimensional dynamic soil-multibody interaction modeling is presented, where both soils and rigid bodies are discretized using SPH particles. In the framework, soils are modeled using the Drucker-Prager model, while rigid bodies are considered with a multibody dynamics solver. A hybrid contact method suitable for three-dimensional simulations is developed to model the soil-body and body-body frictionless and frictional contacts, where contact forces are calculated based on ideal plastic collision and the unit normal/tangential vectors of the actual surface. Owing to its simplicity in contact detection and accuracy in contact force calculation, the hybrid contact method can be easily incorporated into SPH. Furthermore, graphics processing unit (GPU) parallelization is utilized to improve efficiency. The presented numerical framework and the hybrid contact method are validated using several examples. Numerical results are compared with analytical solutions and results from the literature. Furthermore, two three-dimensional simulations involving dynamic soil-multibody interaction are included to demonstrate the application.     

灌注桩钢筋笼磁异常的定量化研究(英文)

本文利用数值计算方法首次定量化研究了钢筋笼的磁异常场,总结了钢筋笼的磁异常特征,重点讨论了测孔方位、桩孔距、多节钢筋笼等影响因素,并为磁法检测钢筋笼提供了定量化的参考值.通过模型桩试验,验证了理论计算的正确性,并利用理论计算所得的规律合理的对实测曲线进行了解释.结果显示:数值计算和现场试验基本吻合,通过钢筋笼曲线特征可以较好的判断钢筋笼长度和配筋率变化.本文的研究完善了基于磁法的钢筋笼检测方法,并可以做进一步推广.该方法也对其他构筑物内部的配筋检测有一定的指导意义.     

Near surface velocity and QS structure of the Quaternary sediment in Bohai basin,China

Heavily populated by Beijing and Tianjin cities, Bohai basin is a seismically active Cenozoic basin suffering from huge lost by devastating earthquakes, such as Tangshan earthquake. The attenuation (Q_P and Q_S) of the surficial Quaternary sediment has not been studied at natural seismic frequency (1?10 Hz), which is crucial to earthquake hazards study. Borehole seismic records of micro earthquake provide us a good way to study the velocity and attenuation of the surficial structure (0?500 m). We found that there are two pulses well separated with simple waveforms on borehole seismic records from the 2006 M_W4.9 Wen'an earthquake sequence. Then we performed waveform modeling with generalized ray theory (GRT) to confirm that the two pulses are direct wave and surface reflected wave, and found that the average v_P and v_S of the top 300 m in this region are about 1.8 km/s and 0.42 km/s, leading to high v_P/v_S ratio of 4.3. We also modeled surface reflected wave with propagating matrix method to constrain QS and the near surface velocity structure. Our modeling indicates that Q_S is at least 30, or probably up to 100, much larger than the typically assumed extremely low Q (~10), but consistent with Q_S modeling in Mississippi embayment. Also, the velocity gradient just beneath the free surface (0?50 m) is very large and velocity increases gradually at larger depth. Our modeling demonstrates the importance of borehole seismic records in resolving shallow velocity and attenuation structure, and hence may help in earthquake hazard simulation.     

Estimation of orographically induced wave drag in the stable boundary layer during the CASES-99 experimental campaign

This paper addresses the quantification of gravity wave drag due to small hills in the stable boundary layer. A single column atmospheric model is used to forecast wind and temperature profiles in the boundary layer. Next, these profiles are used to calculate vertical profiles of gravity wave drag. Climatology of wave drag magnitude and “wave drag events” is presented for the CASES-99 experimental campaign. It is found that gravity wave drag events occur for several relatively calm nights, and that the wave drag is then of equivalent magnitude as the turbulent drag. We also illustrate that wave drag events modify the wind speed sufficiently to substantially change the surface sensible heat flux.