地闪回击的微秒级辐射场特征及近地面连接过程分析

利用１μｓ时间分辨率的慢天线电场变化仪在甘肃中川地区雷暴过程中测量得到的大量地闪辐射波形地地闪回击辐射场特征及回击的慢前沿过程进行分析,发现１８次正地闪和８５次负地闪产在周前沿过程上升时间为１９．２μｓ和９．４μｓ,８４次负地闪继后回击的前沿过程为４．３ μｓ。ＹＹ ＵＤＡ Ｏ ３．１μ;     

大气湍流对天基遥感系统地面分辨率的影响

分辨率是所有光学成像系统最重要的技术指标之一。当成像系统与待成像目标之间存在大气湍流时,后者便会在不同程度上影响图像分辨率。天基光学遥感更加关心大气湍流对目标地面分辨率的影响。从大气湍流相干长度和到达角起伏两个角度,通过详细的公式推导和数值计算,分别讨论天基光学遥感系统成像过程中湍流对图像地面分辨率的影响。结果表明,地面分辨率0.5 m以上的甚高分辨率遥感成像需要考虑大气湍流因素。     

风场反演中距离圈上速度退模糊方法研究

在深入分析速度模糊的特点后,根据在距离圈上不模糊点到模糊点的不连续性,以及对模糊跳变处风速差和最大不模糊速度间关系的判定,从零方位开始在距离圈上逐点进行速度模糊的判定,并引入模糊标记的形式以确定退模糊处理的区间.然后通过实例分析,证明了方法的可用性和正确性.最后利用经过该方法处理的低仰角基本速度资料成功反演了雷达风场.     

区域一体化与制度距离作用下的中国企业跨境并购

在区域一体化蓬勃发展的背景下,研究企业跨境并购有助于更好地理解资本在区域间的流动。论文基于BVD-Zephyr数据库统计的2003—2017年中国企业跨境并购数据,分析了交易双方是否签订区域一体化协定和彼此间的制度距离对跨境并购成功率和交易金额的影响。通过Heckman两阶段回归,研究发现：① 区域一体化能够促进中国企业达成跨境并购交易,但不能提升交易金额;② 中国企业与正式制度距离远,即法律、规制层面差异大的国家内企业完成跨境并购的可能性更高,但正式制度距离的存在不利于交易规模扩大;③ 非正式制度距离与交易完成呈负相关关系,即文化层面上的差异过大不利于中国企业完成跨境并购。然而交易一旦完成,非正式制度距离大的贸易双方交易金额更高。此外,论文还认为,随着区域一体化进程的深化,内部成员国之间正式制度距离会衰减,其对交易规模的阻碍作用也会被削弱。     

非量测数码相机单像空间后方交会的辅助分步像主距与像主点的简单测定

近年来,非量测的中、高端普通数码相机越来越多的应用到航空、近景等摄影测量领域[3]。影响摄影测量成果精度的重要因素之一是相机的技术参数,因此相机技术参数的检校是保证成果质量能否满足精度要求的关键问题之一。本文着重讲述了在以单像空间后方交会为基础的相机检校中,受制于实践环境,当控制场各控制点的几何分布通常被布置离一个平面不大的范围内,则会使未知数的解极不稳定,甚至有不定解得可能。为防止出现错解以及不定解,先通过试验场检校给出像主距f和像主点(x0,y0)初始值,从而避免上述情况发生,文中给出了方法、原理及实践数据、结果。     

健康视角下城市建成环境对老年人日常步行活动的影响研究

“健康老龄化”背景下,促进身体活动是提升老年人健康水平的重要方式,也是当前多学科交叉研究的热点。依托南京市居民身体活动调查数据,选择老年人日常生活中最普遍且有益健康的步行活动作为研究主题,探究建成环境的影响,以期为相关理论与实践提供有益探索。研究表明：① 老年人日常步行空间范围可作为步行所涉及建成环境边界,不同类型的主要活动场所则可识别建成环境要素需求差异。② 日常生活所涉及的公共开放空间、商业及公共服务设施的密集性,以及主观建成环境感知对老年人交通性/休闲性步行活动具有显著影响。③ 基于老年人日常步行活动习惯及建成环境对步行活动的影响,可从有效供给日常步行生活空间、积极引导健康生活方式方面提出相应规划策略。     

Testing the stereoscopic precision of a large-format digital camera

The use of large-format digital cameras in aerial photogrammetry is leading to great improvements in photogrammetric production. Since they were first introduced about 10 years ago, the technological community has been testing and investigating the conditions under which this major change can be consolidated. But a certain (and understandable) bias may be noticed in the efforts that developers, researchers and clients are undertaking. Almost all of the efforts aim at checking the quality of automated measurements and very little attention has been directed to stereoscopic measurements by human operators, which, nevertheless, still represent an important task that needs to be carried out in the production chain. This paper presents the results from a number of tests (13 operators from a variety of enterprises) performed to check the stereoscopic precision of Vexcel UltraCamD camera images compared with Leica RC30 film images. The main conclusion to be drawn from the empirical data is that stereoscopic precision does not depend on the type of camera.     

Velocity Distance of the Open Cluster M11

On the reasonable hypothesis that the internal motions of member stars of a cluster are random and isotropic, a method which can be used to estimate the velocity distance of the cluster and its uncertainty is developed. The velocity distance so determined is an absolute distance estimate, and is completely independent of the (widely used) luminosity distance, which is a relative distance estimate. Using the published high-accuracy observational data of radial velocities and proper motions of the stars in the open cluster M11 region, we have determined the distance of M11 to be 1.89 ± 0.52kpc. This is in quite good agreement with the published luminosity distances of the cluster. We briefly discuss the problems concerned, including the sources of errors in the method and its applicable range.     

船舶监控系统中航迹线动态绘制算法应用研究

在船舶监控系统中应用3S技术，实现了船只航迹线的动态绘制，系统能够根据船只航行方向动态显示航行轨迹，程序开发过程中涉及到偏转角度算法和距离插值两个核心算法。实践表明，这两个算法的合理应用，在航迹线可视化表现方面取得了良好的效果。     

Cepheid parallaxes and the Hubble constant

Revised Hipparcos parallaxes for classical Cepheids are analysed together with 10 Hubble Space Telescope ( HST )-based parallaxes. In a reddening-free V , I relation we find that the coefficient of log  P is the same within the uncertainties in our Galaxy as in the Large Magellanic Cloud (LMC), contrary to some previous suggestions. Cepheids in the inner region of NGC 4258 with near solar metallicities confirm this result. We obtain a zero-point for the reddening-free relation and apply it to the Cepheids in galaxies used by Sandage et al. to calibrate the absolute magnitudes of Type Ia supernova (SNIa) and to derive the Hubble constant. We revise their result for H ₀ from 62 to 70 ± 5 km s⁻¹ Mpc⁻¹. The Freedman et al. value is revised from 72 to 76 ± 8 km s⁻¹ Mpc⁻¹. These results are insensitive to Cepheid metallicity corrections. The Cepheids in the inner region of NGC 4258 yield a modulus of 29.22 ± 0.03 (int.) compared with a maser-based modulus of 29.29 ± 0.15. Distance moduli for the LMC, uncorrected for any metallicity effects, are 18.52 ± 0.03 from a reddening-free relation in V , I ; 18.47 ± 0.03 from a period–luminosity relation at K ; 18.45 ± 0.04 from a period–luminosity–colour relation in J , K . Adopting a metallicity correction in V , I from Macri et al. leads to a true LMC modulus of 18.39 ± 0.05.