利用地震面波和重力资料联合反演地壳—上地幔三维密度结构的方法探讨

本文探讨了利用地震面波和重力资料联合反演地壳－地幔三维密度结构的反演问题。首先建立了地震面波和重力资料的观测方程,然后应用广义线性反线理论给出了反演问题的解。模型试验结果表明,与单纯面波反演的结果相比,联合反演的解在分析率和方差两个方面都有改善,当加入扰动重力数据时,在０－３００ｋｍ深度范围内联合反演的结果明显好于单纯面波反演的结果。     

GPS网与地面网的坐标连接

本文对坐标系统的转换以及坐标的拟合推估进行了论述。     

三层BP网隐层节点数确定方法的研究

对确定三层BP网络隐层节点数的理论依据和现有做法进行了研究,提出了一种三层BP网络隐层节点数的双向确定法     

数字化地图印刷一种随机挂网计算模型

基于彩色图像像素3刺激值与相应网点面积率之间的α幂修正的Neugebauer方程,建立由常规的调幅网为基础的调频挂网计算模型,以此实现分色胶片随机挂网     

内核地球模型的形变场和地球参考系

讨论了内核地球模型的形变场（ 位移、速度） 和地球参考系的确立, 为内核地球动力学的研究提供了依据。     

深基静载试验与沉降观测

用深基静载试验成果,确定地基土承载力标准值并估算高层建筑的沉降量。通过建筑物沉降观测,对试验成果进行分析和评价,认为用此种方法确定地基承载力标准值,可直接用于工程设计。     

Long-term behavior and statistical characterization of BeiDou signal-in-space errors

GPS Solutions - We derive orbit and clock errors for BeiDou satellites from March 1, 2013, to September 30, 2016 by comparing broadcast ephemerides with the precise ephemerides produced by Wuhan...     

Improving BDS integer ambiguity resolution using satellite-induced code bias correction for precise orbit determination

GPS Solutions - Successful resolution of integer ambiguity over long baselines is a key to improve the accuracy of precise orbit determination for global navigation satellite system satellites. The...     

Enhanced orbit determination for BeiDou satellites with FengYun-3C onboard GNSS data

GPS Solutions - A key limitation for precise orbit determination of BeiDou satellites, particularly for satellites in geostationary orbit (GEO), is the relative weak geometry of ground stations....     

Lookback time as a test for f(R) gravity in the Palatini approach

We use the recently released data of lookback time (LT)-redshift relation, the cosmic microwave background shift parameter and the baryon acoustic oscillation measurements to constrain cosmological parameters of f (R) gravity in the Palatini formalism by considering the f (R) form of type (a) f (R) = R β/Rn and (b) f (R) = R + α ln R β. Under the assumption of a Friedmann-Robertson-Walker universe, we achieved the best fitting results of the free parameters (Ωm0, n) for (a) and (Ωm0, α) for (b). We find tha...