冬季EC 2m温度预报在贵州毕节地区的检验分析

利用毕节市8个国家站02时、14时气温实况数据,分别计算2016-2018年冬季(12月、1月、2月)EC细网格2 m温度预报的准确率、平均绝对误差、绝对误差,检验在升温、平稳、降温3类天气过程中温度预报效果,为模式温度预报订正提供参考依据。结果表明:02时的预报平均准确率比14时高约10%;除赫章站以外,其余站点准确率在60%~80%之间,有一定预报参考意义;3类天气过程中,平稳、降温天气中温度预报效果明显优于升温天气;升温天气过程中02、14时温度预报大多偏低0~4℃,降温天气过程中02时温度预报总体偏低0~4℃,14时偏高0~4℃。     

BCC_CSM1.1(m) 模式对热带太平洋潜热通量的评估

利用1979—2005年OAFlux (Objectively Analyzed air-sea Fluxes) 观测资料以及CMIP5的15个耦合模式的模拟结果,评估了BCC_CSM1.1(m) 模式对热带太平洋年平均潜热通量气候态和变化趋势的模拟能力,并分析造成趋势偏差的可能原因。结果表明:BCC_CSM1.1(m) 模式模拟热带太平洋年平均潜热通量气候态在各纬度上差异较大, 其中在赤道的模拟能力较佳,而在10°N和8°S附近模拟偏差较大;BCC_CSM1.1(m) 模式对热带太平洋年平均潜热通量趋势的模拟能力一般,造成趋势偏差的主要原因是该模式低估了风速对潜热通量的局地贡献以及它对风速的非局地贡献的模拟存在较大偏差。此外,该模式未能较好地模拟出风速对全球变暖响应。因此,BCC_CSM1.1(m) 模式对热带太平洋年平均潜热通量趋势模拟的改进需加强其对风速模拟的改进。     

Mid-IR (8–13 μm) images of the 21 μm,carbon rich proto-planetary nebulae

We present 9.7 and 11.8 m narrow band (/=10%) images of three carbon (C-) rich proto-planetary nebulae with an unusual 21 m feature: IRAS 07134+ 1005, IRAS 22272+5435, and IRAS 04296+3429. The images were taken at UKIRT using the Berkeley/IGPP/LEA mid-IR camera. All three objects have a bipolar shape adding to the existing evidence that C-rich PPNe are by nature bipolar. Furthermore, we find the same bipolar morphology in a previous study of the C-rich, young planetary nebula, IRAS 21282+5050. We believe these four objects form an evolutionary sequence which links the C-rich asymptotic giant branch (AGB) stars with the C-rich planetary nebulae (PNe). From this evolutionary sequence, we conclude that bipolarity in C-rich PNe begins on the AGB and that the dynamical ages of these PPNe are in fair agreement with theoretical ages for a 0.6 M hydrogen burning core star.     

m序列生成结构分析

详细分析了m序列的生成结构；利用r级带有某些特定反馈的移位寄存器状态变换矩阵，特征多项式及母函数，提出了几个判定r级带有某些特定反馈的移位寄存器输出的序列为m序列的条件。     

基于曙光3000计算环境的寒旱区资源环境数据平台建设

通过对寒区旱区资源环境研究中已积累的大量特色数据、应用模式和程序的分析,对分布式网络环境中的数据采集与管理、应用模式和程序的移植集成、应用程序与数据的交互访问等技术进行了讨论,提出建立由数据中心、中间件服务、应用服务、一站式管理组成的数据平台是提高数据利用效率,方便实现数据与应用集成,提高科研效率的一种有效途径之一.对数据平台建设的主要思路及实现技术进行了详细讨论,并在实验基础上,初步建立了基于曙光3000高性能计算环境的寒区旱区资源环境数据平台,为以后的数据网格建设做了一定的技术准备.     

m序列在水声通信中应用

针对在水声通信中使用m序列作为编码形式的扩频通信系统进行研究.分析扩频码的产生和序列特点,给出的声线搜索、信息解码的具体方法.对其中相关运算提出了快速算法,解决了运算中的瓶颈问题,极大地提高了运算速度,并对长序列的快速相关进行了初步探索.     

High-resolution remote sensing mapping of global land water

Land water, one of the important components of land cover, is the indispensable and important basic information for climate change studies, ecological environment assessment, macro-control analysis, etc. This article describes the overall study on land water in the program of global land cover remote sensing mapping. Through collection and processing of Landsat TM/ETM+, China’s HJ-1 satellite image, etc., the program achieves an effective overlay of global multi-spectral image of 30 m resolution for two base years, namely, 2000 and 2010, with the image rectification accuracy meeting the requirements of 1:200000 mapping and the error in registration of images for the two periods being controlled within 1 pixel. The indexes were designed and selected reasonably based on spectral features and geometric shapes of water on the scale of 30 m resolution, the water information was extracted in an elaborate way by combining a simple and easy operation through pixel-based classification method with a comprehensive utilization of various rules and knowledge through the object-oriented classification method, and finally the classification results were further optimized and improved by the human-computer interaction, thus realizing high-resolution remote sensing mapping of global water. The completed global land water data results, including Global Land 30-water 2000 and Global Land 30-water 2010, are the classification results featuring the highest resolution on a global scale, and the overall accuracy of self-assessment is 96%. These data are the important basic data for developing relevant studies, such as analyzing spatial distribution pattern of global land water, revealing regional difference, studying space-time fluctuation law, and diagnosing health of ecological environment.     

行星会合指数变化与太阳绕太阳系质心运转的周期

本文创建了行星会合指数(K)运动学方程,通过定义的行星会合指数可以指代行星会合与相背离的程度,进而发现太阳(S)绕太阳系质心(C)运动的轨迹、形态变化特征.对该运动学方程构建的图像分析发现,太阳绕太阳系质心转动有近半程时间,太阳系质心是处于太阳本体之内.以质量为权重求出了行星系质心运日运动的恒星周期,从而获得了太阳绕太阳系质心运转的真正周期为21.8192年(约22年),并得到了太阳绕太阳系质心运动的轨迹.     

共面闭合断续节理岩体强度特性直剪试验研究

通过直剪试验条件下的模型试验,研究了不同节理连通率、节理排列方式、正应力条件下同时包含闭合节理和岩桥的剪切面的变形和强度特性及其相应的变化规律,初步探讨了节理、岩桥变形和破坏机理。