采用调零天线阵测向解GNSS姿态仪的整周模糊度

由多个单元天线组成的GNSS调零天线阵通常用于在大功率干扰信号来波方向上形成天线波束方向图零点,以此来抗压制性干扰。采用此调零天线阵所自然形成的二维短基线,按照电子侦察中多基线干涉仪测向原理,通过短基线的相位差测量值来解GNSS姿态仪长基线的相位差模糊,从而实现了GNSS姿态仪的整周模糊度的实时解算。该方法通过GNSS姿态仪与调零天线阵的组合应用,不仅提高了解模糊的性能,而且增强了整个系统抗干扰反欺骗的能力,从而为GNSS姿态仪和调零天线的拓展应用提供了重要参考。      

密山市及周边地区放蜂的气候资源—不利的气象条件分析

在文献[1]的基础上，进一步对密山市及其周边地区放蜂中对密源植物及蜂群活动不利或能造成灾害和损失的天气与气候条件，包括负积温值，日最低温度＜7℃的日数，大风，冰雹，雷暴等进行了统计分析与评价，为蜂农提供放蜂的科学依据。     

西北太平洋热带云团发展与两类El Nio事件的联系

利用1982—2009年全球热带云团数据集、NCEP/NCAR再分析资料和英国Hadley中心海温资料,并引入热带云团生成率(Genesis Productivity,GP)来分析EP(Eastern Pacific)El Nio和CP(Central Pacific)El Nio事件与西北太平洋热带云团发展的相关性。研究表明,1)夏秋两季GP与Nio3指数在东南区(SE)均为显著正相关,在西南区(SW)仅秋季呈显著正相关;GP与EMI(El Nio Modoki Index)指数在夏季SE区域为显著正相关,在秋季南中国海(South China Sea,SCS)区呈负相关。2)在EP El Nio年,夏季SE区域的GP增大与低层涡度、高层散度以及低层相对湿度的相对增大一致。夏季SW区域与秋季SE区域的GP增大与有利的高低空配置相关,La Nia年则与之相反。3)在CP El Nio年,夏季SE区域的GP增大伴随着低层涡度和高层散度的增加,同时与充足的水汽及弱风切变相吻合;而秋季SCS区域的GP下降源于正涡度带、正散度带以及水汽带的东移。     

WRF模式制备的气象驱动数据在新疆喀依尔特斯河流域的验证

随着寒区水文模拟研究的深入,空间分布式模型的快速发展,迫切需求高分辨率的气象驱动数据.研究基于WRF模式动力降尺度和Micromet统计降尺度方法,制备了阿尔泰山额尔齐斯河源区喀依尔特斯河流域春季1 km分辨率气象驱动数据,并利用地面观测资料从小时尺度上对其进行了验证,为该流域春季分布式融雪径流模型做充分准备.结果表明:小时尺度上2 m气温、2 m相对湿度、10 m风速、地表接收的短波辐射和长波辐射的平均绝对误差MBE分别为0.43℃、-2.9%、3.7 m·s~(-1)、28.2 W·m~(-2)和-36.2 W·m~(-2),其平均均方根误差RMSE分别为3.81℃、18.2%、4.8 m·s~(-1)、163.5W·m~(-2)和52 W·m~(-2),与实测对比拟合的R~2分别为0.84、0.32、0.03、0.7和0.3.在小时尺度上,2 m温度和地表接收短波辐射的模拟结果比较理想,可以用于高时间分辨率水文模拟.     

山东省棚户区改造项目资金财政监管平台设计与应用

针对目前棚户区改造项目贷款审批和资金发放难于监管的特点,本文重点研究了将地理信息、遥感等技术应用于棚户区改造项目管理和资金监管,建立了时空数据一体化管理和项目动态监管模型,通过项目地理位置上报、历史影像对比、地理信息辅助审核等技术解决了棚改项目资金重复申报的问题和资金发放监管不到位的问题,依托于天地图山东丰富的地图数据资源,研发了山东省棚户区改造项目资金财政监管平台,建立了棚改项目上报、初审、现审、放款、监管、支付的一整套管理流程,实现全省棚改项目的空间化和实时监督管理。     

基于 JavaScript 的地理事件可视分析框架设计

随着互联网的飞速发展,网络环境下地理信息的可视化表达成为研究的热点。在JavaScript技术和可视分析技术研究基础上,对互联网中地理事件可视分析框架进行设计,目的是探索网络环境下,地理事件可视化的表达方式和可行性分析,搭建适合互联网的地理事件可视分析框架,为基于Web的地理信息可视分析系统的实现打下基础。     

The dust distribution within the inner coma of comet P/Halley 1982i: encounter by Giotto's impact detectors

Analysis of the data from Giotto's Dust Impact Detection System experiment (DIDSY) is presented. These data represent measurement of the size of dust grains incident on the Giotto dust shield along its trajectory through the coma of comet P/Halley on 1986 March 13/14. First detection occurred at some 287000 km distance from the nucleus on the inbound leg; the majority of the DIDSY subsystems remained operational after closest approach (604 km) yielding the last detection at about 202000 km from the nucleus. In order to improve the data coverage (and especially for the smallest grains, to approximately 10(-19) kg particle mass), data from the PIA instrument has been combined with DIDSY data. Flux profiles are presented for the various mass channels showing, to a first approximation, a 1/R2 flux dependence, where R is the distance of the detection point from the cometary nucleus, although significant differences are noted. Deviations from this dependence are observed, particularly close to the nucleus. From the flux profiles, mass and geometrical area distributions for the dust grains are derived for the trajectory through the coma. Groundbased CCD imaging of the dust continuum in the inner coma at the time of encounter is also used to derive the area of grains intercepted by Giotto. The results are consistent with the area functions derived by Giotto data and the low albedo of the grains deduced from infrared emission. For the close encounter period (-5 min to +5 min), the cumulative mass distribution function has been investigated, initially in 20 second periods; there is strong evidence from the data for a steepening of the index of the mass distribution for masses greater than 10(-13) kg during passage through dust jets which is not within the error limits of statistical uncertainty. The fluences for dust grains along the entire trajectory is calculated; it is found that extrapolation of the spectrum determined at intermediate masses (cumulative mass index alpha = 0.85) is not able to account for the spacecraft deceleration as observed by the Giotto Radio Science Experiment and by ESOC tracking operations. Data at large masses (>10(-8) kg) recently analysed from the DIDSY data set show clear evidence of a decrease in the mass distribution index at these masses within the coma, and it is shown that such a value of the mass index can provide sufficient mass for consistency with the observed deceleration. The total particulate mass output from the nucleus of comet P/Halley at the time of encounter would be dependent on the maximum mass emitted if this change in slope observed in the coma were also applicable to the emission from the nucleus; this matter is discussed in the text. The flux time profiles have been converted through a simple approach to modeling of the particle trajectories to yield an indication of nucleus surface activity. There is indication of an enhancement in flux at t approximately -29 s corresponding to crossing of the dawn terminator, but the flux detected prior to crossing of the dawn terminator is shown to be higher than predicted by simple modelling. Further enhancements corresponding to jet activity are detected around +190 s and +270 s.     

珠江口盆地东部海域天然气水合物成藏气源特征探讨

通过钻探,在珠江口盆地东部海域获取了天然气水合物实物样品,在5个取心站位目标层段进行了保压取心,获取了水合物岩心释放气样品,同时在13个层段获取了水合物分解气体样品。钻探取心的5个站位都在航次现场选择层段制备了顶空气样品。所有气体均进行了气体组成与同位素分析,结果表明:水合物气体组成以甲烷占绝对优势,甲烷含量96.5%～99.8%;乙烷含量极少,为(175～554)×10~(-6),未检测出C_(2+)以上烃类气体。水合物气体甲烷碳-氢同位素分析测试结果表明,δ~(13)C_(1 )为-68.4‰～-71.2‰,δDC_1为-182‰～-184‰,据此判识水合物气体成因类型为生物成因气。水合物气源成因类型与水合物产出形态没有直接关系,多种产出类型的水合物可能与储层发育及形态特征有密切联系。主要气源位于1000m以内的浅地层中,主要以侧向运移方式运移至稳定域有利部位形成水合物。