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891.
本文探讨了附加系统参数平差法在带有测距系统误差的导线网中的应用,说明了当系统误差比较显著时.采用附加系统参数平差法的可行性、必要性及其优越性。  相似文献   
892.
The analysis of the time and space distribution of specular (reflecting) points in bistatic altimetry between GPS and CHAMP satellites or SAC-C (taken as examples) is extended from Wagner and Klokočník (2003 J. Geod 77: 128–138). We demonstrate a significantly higher number and density of reflecting points in bistatic altimetry in comparison with traditional monostatic altimetry. After an outline of our older accuracy assessment for the vertical position of the reflecting point, we add a new independent derivation and compare both approaches. We account for orbit errors of both the transmitters (GPS) and receiver (CHAMP) satellites, and the measurement (delay) error. We found that the accuracy of the vertical position of the reflecting point decreases only slowly with increasing off-nadir angle and that the orbit errors must be accounted for if decimeter and better accuracy is required. In this paper, we do not study errors such as state of the ocean, technical parameters of the receiving system, and atmospheric corrections.  相似文献   
893.
Low-low satellite-to-satellite tracking (ll-SST) range-rate observations have been predicted by two methods: one based on a linear perturbation theory in combination with the Hill equations, and one based on solving the equations of motion of two low-flying satellites by numerical integration. The two methods produce almost equivalent Fourier spectra of the range-rate observations after properly taking into account a few resonant terms. For a typical GRACE-type configuration, where the two satellites trail each other at a distance of 300 km at an altitude of 460 km, and in the presence of the EGM96 gravity field model, complete to spherical harmonic degree and order 70, the agreement between the Fourier spectra is about 1 mm/s compared to a root-mean-square (RMS) value of more than 220 mm/s for the range-rate signal. The discrepancy of 1 mm/s can be reduced significantly when not taking into account perturbations caused by the J2 term. Excluding the J2 term, the agreement between the two methods improves to 0.4 mm/s compared to a RMS value of 6 mm/s for the range-rate signal. These values are 0.01 and 2.3 mm/s when ignoring the spectrum for frequencies below two cycles per orbital revolution, reducing the discrepancy even further to about 0.5% of the signal. The selected linear perturbation theory is thus capable of modeling gravity field induced range-rate observations with very high precision for a large part of the spectrum.  相似文献   
894.
Some theory problems affecting parameter estimation are discussed in this paper. Influence and transformation between errors of stochastic and functional models is pointed out as well. For choosing the best adjustment model, a formula, which is different from the literatures existing methods, for estimating and identifying the model error, is proposed. On the basis of the proposed formula, an effective approach of selecting the best model of adjustment system is given. Project supported by the Open Research Fund Program of the Key Laboratory of Geospace Environment and Geodesy, Ministry of Education, Wuhan University (No. 905276031-04-10).  相似文献   
895.
The satellite missions CHAMP, GRACE, and GOCE mark the beginning of a new era in gravity field determination and modeling. They provide unique models of the global stationary gravity field and its variation in time. Due to inevitable measurement errors, sophisticated pre-processing steps have to be applied before further use of the satellite measurements. In the framework of the GOCE mission, this includes outlier detection, absolute calibration and validation of the SGG (satellite gravity gradiometry) measurements, and removal of temporal effects. In general, outliers are defined as observations that appear to be inconsistent with the remainder of the data set. One goal is to evaluate the effect of additive, innovative and bulk outliers on the estimates of the spherical harmonic coefficients. It can be shown that even a small number of undetected outliers (<0.2 of all data points) can have an adverse effect on the coefficient estimates. Consequently, concepts for the identification and removal of outliers have to be developed. Novel outlier detection algorithms are derived and statistical methods are presented that may be used for this purpose. The methods aim at high outlier identification rates as well as small failure rates. A combined algorithm, based on wavelets and a statistical method, shows best performance with an identification rate of about 99%. To further reduce the influence of undetected outliers, an outlier detection algorithm is implemented inside the gravity field solver (the Quick-Look Gravity Field Analysis tool was used). This results in spherical harmonic coefficient estimates that are of similar quality to those obtained without outliers in the input data.  相似文献   
896.
The response of the Earth’s crust to the direct effect of lunisolar gravitational forcing is known as the body tide. The body tide is superimposed by surface-loading forces due to the pressure of the periodically varying ocean tide acting on the Earth, called ocean tide loading (OTL). Both body tide and OTL can be decomposed into components of the same frequency known as tidal parameters. However, OTL is more complicated than body tides because of the dynamic effects of the ocean. Estimating OTL requires a model of the ocean tides and knowledge of the elastic properties of the solid Earth. Thus, synthetic tide parameters (amplitude factors and phase leads) have been developed here on a world-wide grid for gravity and positional displacements. The body tide contributions were added to the oceanic contribution to provide the Earth tide response. The accuracy and reliability of the synthetic tidal parameters have been estimated by comparing observed gravity and vertical-displacement tide parameters with those interpolated from our synthetic model, which shows good agreement. Tests also indicate that the synthetic tide parameters provide realistic gravimetric and displacements for practical use in tidal prediction.  相似文献   
897.
为解决城市边界层中大气O3浓度的预报问题,选用一种简明有效的光化学反应方案建立光化学模式, 并与大气平流扩散的箱格预报模型进行了嵌套,从而将大气化学过程引入到城市空气污染数值预报系统 (CAPPS) 中。同时,根据实际需要研究了VOC (Volatile Organic Compounds) 浓度及NOx源排放量等参数缺测时,根据前期监测浓度采用遗传算法反演未知参数的具体方法。利用2001年9月8~17日在北京舞蹈学院监测的O3、NOx资料及相应的气象数据,用改进后的CAPPS模式进行了单箱预报试验。预报试验结果表明,嵌套后的模式对O3浓度的变化具备一定的预报能力。  相似文献   
898.
利用中国东部1990~2000年旬平均土壤湿度、降水和气温观测资料,通过对0~50 cm层次土壤湿度进行旋转主分量分析 (REOF),重点分析了淮河流域土壤湿度的时空分布特征, 并初步研究了土壤湿度与前期、同期和后期不同时段降水与气温的关系。发现春季以30 cm为界,30 cm以上各层土壤湿度异常的第一旋转空间模态十分相似, 其大值中心主要位于淮河流域,而30 cm以下 (30~50 cm) 各层的第二旋转空间模态与之亦十分类似, 因此称该模态为“淮河型”,而夏季和秋季虽然该模态也很显著, 但特征不如春季突出。该模态在各层次土壤中具有明显的持续性特征,均存在40旬左右的显著周期;并与前期和同期降水(气温)呈显著正 (负) 相关关系,与约半年后的降水 (气温) 呈负 (正) 相关关系。  相似文献   
899.
通过遥感技术与地面测定相结合的方法,对北京城市热岛现状作观测研究,得到北京城市地面的温度分布特点。使用北京大学城市边界层模式从气象观点就“楔形绿地”规划对北京城市气候的影响进行研究和评价,模式通过对城市地表复杂性和多样性的特征进行细致描述,建立了一个细致模拟城市特点的城市边界层能量平衡模式,并用此能量平衡模式得到的地面温度作为下边界条件,中尺度气象模式MM5做初始场和侧边界条件,建立一个最小分辨率为500 m的城市边界层模式系统,来研究城市边界层在中尺度背景场作用下的精细结构。通过个例模拟,模式能够较准确地模拟城市边界层的风温场分布情况,可以用来对楔形绿地规划进行模拟试验。通过对规划后的气象场在特定的气象条件下进行模拟,结果显示,建造大型的楔形绿地后,绿地区域及绿地周围约1 km以内的地区温度有所降低,降低的程度由规划前后的地表类型改变的剧烈程度、风速大小及与绿地的距离决定,但是这种规划方案却会因城市的下风方向的风速减小而导致通风不畅。  相似文献   
900.
对自20世纪80年代以来的大气热力学发展进行了综合评述, 阐述了如城市热岛效应、全球增暖等非传统大气热力学问题; 基于大气非平衡态热力学的非线性理论, 提出应发展突显热力学作用的数值模式, 并阐述其必要性和可能性。  相似文献   
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