结构体整体变形量提取算法

以往利用三维激光扫描提取变形量都是基于DEM模型进行变形量的提取。该方法提取的是一维变形量,没有考虑不同方向的变形量。针对此,对基于K-最邻近点搜索的ICP算法进行改进;并基于局部匹配的方法,提取结构体的整体变形量,包括变形的方向和大小。首先,对ICP算法中最邻近点搜索容易出现重复的地方进行了修改,构建了改进的K-最邻近点搜索的ICP算法。其次,利用该算法对采集的两期点云进行全局配准,并将配准后的结构体点云进行归一化处理。最后,利用该算法对结构体点云进行局部匹配,从而可以得到结构体的整体变形量,包括3个旋转向量和3个平移向量。通过实例,验证了该方法在结构体变形提取中的有效性。     

An analysis of subaerial beach rotation and influences of environmental forcing adjacent to the proposed Swansea Bay Tidal Lagoon

Beach Profiles surveys and gale climate data were utilised to assess medium timescale beach rotation at four beaches located along the shores of a crenulated embayment within Swansea Bay, Southwest Wales. The proposed Tidal Lagoon is located within this Bay. Results identified a 7 year (1998–2005) record of cyclic summer/winter rotation and a 14 year (1999–2013) record of annual rotation within the subaerial zone on all four assessed beaches. In the absence of headlands to trap sediment it is asserted that the driving force for beach rotation is the presence of Swansea Dockland/Tawe dredged channel complex, Port Talbot Harbour and the Neath dredged channel which form surrogate headlands essentially creating four separate beach systems through restricting sediment by-pass. Seasonal averaged wind and wave variables showed differing correlation with volume changes and cross-correlation results showed that volume variation lagged behind forcing variables by up to six months (i.e. the resolution of the data). This was confirmed by the annually averaged results which showed only subtle correlation. Here volume change in most cases lagged forcing variables by less than one year. Based on correlations, wind direction variability follows closely with volume changes but wind speed, wave period and height are generally opposite. Initial results suggest that the proposed Swansea Bay Tidal Lagoon, located between sediment cells and surrogate headlands, would have little negative effect on subaerial coastal processes. These datasets will be used as a benchmark for monitoring prior to, during and post construction, with results being used to update and inform subsequent strategies.     

FY-2E扫描辐射计云图受月球干扰的影响

针对2012年3—12月FY-2E气象卫星云图出现4次明显的白色亮带异常状况,分析4个红外通道白色亮带出现的原因和影响机理。根据异常白色亮带出现的时间、亮带区域内的内容及亮带过后数据序列的特点,确定是月球出现在卫星视场外左侧临近区域引起的异常情况。以FY-2E气象卫星观测模式分析月球干扰云图的机理和过程,月球通过直流恢复导致云图中出现白色亮带,基于FY-2E气象卫星工作参数定量计算月球干扰云图的准确时间,确认在2012年3月—2013年1月FY-2E气象卫星共有12次受到月球干扰,而业务系统仅发现4次。根据异常数据分析干扰时间的计算精度,确认卫星的电子学随机误差和月球天平动是引起计算精度的重要原因。重新发现的异常云图显示了对月球干扰现象分析的合理性以及对干扰事件过程的计算准确性,有助于数据用户对FY-2E气象卫星云图的准确认识与应用。     

FY-3A/MWHS冷空测值受月球影响分析及修正

为解决月球对风云三号卫星微波湿度计在轨实时辐射定标的影响问题,该文根据风云三号卫星微波湿度计在轨实时观测数据分析,通过多项式拟合分析技术,建立修正模型,消除月球影响,得到合理的辐射定标结果。风云三号卫星微波湿度计在轨实测数据分析表明:月球对风云三号卫星微波湿度计在轨辐射定标结果影响最严重时一天内可干扰4~5条轨道,每条轨道有近100个扫描周期受到污染。月球影响致使冷空定标观测数据跳升1000个计数值,如果不进行污染滤除会造成对地观测亮温下降约20 K,导致辐射资料无法同化进入数值天气预报模式。通过与同类载荷的交叉比对分析,修正月球影响后,风云三号卫星微波湿度计在轨实时辐射定标结果精度与在轨测试结果相当。     

论月球不对称的演化

月球形成初期有一个固体内核,表层是岩浆“海洋”重力分异,冷却固结形成月壳,由于同步自转,其一侧总是向着地球,在地球引力场作用下,使固体内核向地球一侧移动,月壳表层轻的物质向背地球一侧漂浮,所以月亮背地球一侧１５０公里,向地球一侧仅有６０公里,这种演化机制使大部分月海分布在向地球一侧。     

河西走廊地块古生代地层古地磁初步研究

古地磁初步研究结果表明,早古生代阶段,河西走廊过渡带与阿拉善地块古纬度接近,且漂移过程中形影相随,说明其间并无洋盆相隔。志留纪末,河西走廊过渡带与阿拉善地块拼接,但二者磁极位置与古方位均有差异,可能表明走廊过渡带相对于阿拉善地块同时作了顺时针旋转。泥盆纪时,两地块古纬度一致,但古方位不同,可能反映在碰撞拼合后二者间仍有相对的旋转运动。二叠纪时,二块体的空间位置及其配置关系已与现状接近。     

利用信息融合进行月球卫星自主导航

研究了绕月卫星自主导航方法,提出了由星敏感器、紫外月球敏感器和测高仪组成的多源信息组合导航方案。将Unscented Kalman滤波(UKF)应用于非线性导航系统,采用信息融合技术设计了相关的联邦滤波算法,实现了系统的信息互补,完成了卫星轨道的最优估计。利用数学仿真对这种导航系统的有效性进行了验证,并与基于扩展Kal man滤波(EKF)的信息融合算法进行了比较。仿真结果表明,所提出的UKF融合算法具有良好的稳定性,可进一步提高导航系统的精度。     

一种基于扫描线填充算法的分块影像旋转的实现方法

针对分块影像旋转时的效率问题,提出了一种基于扫描线填充算法的实现方法,详细说明了实现步骤,并举例进行了验证。     

Matching the frequency spectrum of pre-main sequence stars by means of standard and rotating models

We applied the aton evolutionary code to the computation of detailed grids of standard (non-rotating) and rotating pre-main sequence (PMS) models and computed their adiabatic oscillation spectra, with the aim of exploring the seismic properties of young stars. As, until now, only a few frequencies have been determined for ∼40 PMS stars, the way of approaching the interpretation of the oscillations is not unique. We adopt a method similar to the matching mode method by Guenther and Brown making use, when necessary, also of our rotating evolutionary code to compute the models for PMS stars. The method is described by a preliminary application to the frequency spectrum of two PMS stars (85 and 278) in the young open cluster NGC 6530. For the Star 85, we confirm with self-consistent rotating models, previous interpretation of the data, attributing three close frequencies to the mode   n = 4, l = 1  and   m = 0  , +1 and −1. For the Star 278, we find a different fit for the frequencies, corresponding to a model within the original error box of the star, and dispute the possibility that this star has a T _eff much cooler that the red boundary of the radial instability strip.     

大气对地球自转季节性变化的贡献

采用１９７９－１９９５年期间新的大气角动量资料,研究了大气在季节性时间尺度上对日长变化和极移的贡献。结果表明,考虑了风和大气压的贡献后,大气在周年和半年时间尺度上对日长变化的贡献分别可达９５％和８８％。同时还给出了大气对极移激发的定量结果,其中,大气的周年尺度上对极移Ｘ分同的贡献为１６％,对Ｙ分量的贡献为４３％;在半年尺度上海洋的贡献,才能进上步解决地球自转激发的问题。