改进的GNSS/水准点优化选择的逐步剔除法          下载免费PDF全文

崔家武  张兴福  周波阳  杜向锋  魏德宏 《武汉大学学报(信息科学版)》2019,44(10):1505-1510

GNSS/水准联测点的合理选择对GNSS高程拟合至关重要，剔除法是一种较好的优化选点方法，传统的剔除法是以高程异常拟合误差最小为目标函数进行优化选点，可能会出现选点不均匀情况。鉴于此，提出根据GNSS/水准点生成的泰森多边形面积大小进行优化选点，并在此基础上对传统优化选点的方法进行改进，即同时考虑高程异常拟合误差大小及由泰森法生成的多边形面积大小进行优化选点（称为综合法）。以1~3次多项式拟合模型为研究对象，实验结果表明，GNSS/水准点优化选择的综合法可在改善点分布的同时获得稳定性好、精度较高的高程异常拟合结果。  相似文献   

Study of Adsorption Isotherm Curves of Amino Acids on the Kaolinite     

刘效兰  张正斌 《海洋通报(英文版)》2002,4(1):52-60

This paper studies the adsorption isotherm curves of four amino acids (glyucine,aspartic acid,glutamic acid and lysine)and the effects of existences of different concentrations of Cu(Ⅱ) on them.Both the adsorption isotherm of the amino acids on the kaolinite and that when the copper ion Cu(Ⅱ） exists belong to the Langmuir type.The slopes of these adsorption isotherm increase with the increasing concentrations of Cu(Ⅱ） added.It can be explained in terms of formation of the type(Ⅰ） ternary surface complexes in these systems.The regular pattern of the effects of copper ion Cu(Ⅱ) on the adsorption isotherm of amino acids on the kaolinite is identical with that of its effects on the exchange and adsorption percentage E(%)-pH on the kaolinite in the same system.  相似文献   

南海北部藻类粒级结构及色素成分对浮游植物吸收系数的影响   总被引：2，自引：0，他引：2       下载免费PDF全文

王桂芬  曹文熙  许大志  杨跃忠 《海洋学报》2007,29(1):38-48

在珠江口、广东沿岸及南海北部三个航次生物-光学数据的基础上,研究了色素打包效应和色素成分的变化对浮游植物吸收系数的影响,结果表明,两种因素对吸收系数都有较大的贡献,但在不同的水体它们的影响程度各有不同.对网采浮游植物含量较高的珠江口和广东沿岸的水体而言,色素打包效应较强,对675 nm处比吸收系数的贡献平均分别为40%和20%;对微型浮游植物占主导地位的南海北部航次的水体,打包效应较弱,对675 nm处比吸收系数的影响平均仅为6%.采用多元线性回归的方法对吸收光谱进行分析,发现除叶绿素a之外的辅助色素对吸收系数的贡献主要表现在蓝绿光波段,三个航次440 nm波长处对总吸收的贡献平均分别为44%,43%和53%,其中对珠江口和广东沿岸航次的水体主要是光合类胡萝卜素的吸收贡献,而对南海北部航次的水体除了光合类胡萝卜素以外还要受到光保护类胡萝卜素的影响.由于河口、近岸和外海水体藻类粒级结构和辅助色素成分对浮游植物吸收系数的贡献有明显的差异,在南海北部水体建立比较精确的生物光学模型时,需考虑藻类粒级结构及色素成分对浮游植物吸收系数的影响.  相似文献   

南海北部水体叶绿素a浓度反演的生物光学模型   总被引：2，自引：0，他引：2  

许大志  曹文熙  王桂芬 《热带海洋学报》2007,26(2):15-21

利用2003年至2005年秋季在南海多个航次的现场观测数据,研究了南海北部海区遥感反射率的变化,并分析了用于全球海洋叶绿素a浓度反演的OC2和OC4模型在本海区的适用性。结果表明,在南海北部海域,OC2和OC4模型高估了叶绿素a浓度,高估范围一般约在80%—200%之间,其中最高可达640%,即OC2和OC4模型并不适用于南海海域。在此基础上,根据现场实测的表观光学数据,利用遥感反射率比值(Rrs(433)/Rrs(555))与叶绿素a浓度的关系建立了两套能够精确反演南海北部海域叶绿素a浓度的本地化经验算法———算法1和算法2,并利用其对南海北部海域的叶绿素a浓度进行反演。结果表明,由本地化模型反演得到的叶绿素a浓度与实测的叶绿素a浓度具有较好的相关关系,其平均相对偏差分别为51%和53%,相关系数为0.75。  相似文献   

船体辐射对气温测量的影响及其在通量计算中造成的误差     

张庆荣  王昭正 《热带海洋》1990,9(3):84-90

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山东紫露草对诱变剂的过敏性     

马德修方宗熙  周汝伦侯家龙陈登勤  戴继勋 《山东海洋学院学报》1981,11(4):47-52

美国产紫露草(Tradescantia paludosa)的微核(MCN)技术用于监测环境污染物已是熟知的有效手段，山东紫露草即毛萼紫露草(Tradescantia reflexa)对环境污染物的敏感性如何，未见报道。本实验的目的在探测这两种植物的染色体对环境污染  相似文献   

VR-GIS技术在高压输电线选线中的应用研究——以康定-崇州500kv送电线路为例     

仇文侠  何政伟  许辉熙  赵银兵  姜兰  张怡  李喆 《测绘科学》2008,33(6):202-203,225

VR-GIS技术是一门新兴技术,已经在很多领域得到广泛应用。本文基于ERDAS、ArcGIS、MapGIS等遥感和GIS专业软件,将VR-GIS技术应用到高压输电线选线中,制作康定-崇州500kv送电线路(大杠～沙坪段)走廊带的三维景观飞行模拟系统,再现研究区真实地形、地貌,使工作人员沉浸于虚拟环境中,为其分析和处理问题提供方便,解决因自然环境恶劣造成的外业调查困难等问题。  相似文献   

Fault Characteristics in Longmen Mountain Thrust Belt,Western Sichuan Foreland Basin,China   总被引：1，自引：0，他引：1  

万桂梅  汤良杰  杨克明  金文正  吕志洲  余一欣 《中国地质大学学报(英文版)》2008,19(6):611-624

Through field geological survey,the authors found that abundant thrust faults developed in the Longmen (龙门) Mountain thrust belt.These faults can be divided into thrust faults and strike-slip faults according to their formation mechanisms and characteristics.Furthermore,these faults can be graded into primary fault,secondary fault,third-level fault,and fourth-level fault according to their scale and role in the tectonic evolution of Longmen Mountain thrust belt.Each thrust fault is composed of several secondary faults,such as Qingchuan (青川)-Maowen (茂汶) fault zone is composed of Qiaozhuang (乔庄) fault,Qingxi (青溪) fault,Maowen fault,Ganyanggou (赶羊沟) fault,etc..The Longmen Mountain thrust belt experienced early Indosinian movement,Anxian (安县) movement,Yanshan (燕山)movement,and Himalayan movement,and the faults formed gradually from north to south.  相似文献   

坚守在客户身边的彩虹——记客户服务中心成立半周年     

北京理正软件设计研究院-客户服务中心 《中国勘察设计》2008,(9)

北京理正是勘察设计行业中唯一一家能提供全面信息化技术服务的大型软件企业,十几年来始终致力于为设计企业提供全方位服务,CAD辅助设计软件、设计院管理信息系统、协同设计软件这三大系列六十多种软件产品几乎覆盖了设计院信息化建设需求的方方面面.  相似文献   

Evolutionary status of the pre-protostellar core L1498     

Kuiper TB  Langer WD  Velusamy T 《The Astrophysical journal》1996,468(2):761-773

L1498 is a classic example of a dense cold pre-protostellar core. To study the evolutionary status, the structure, dynamics, and chemical properties of this core we have obtained high spatial and high spectral resolution observations of molecules tracing densities of 10(3)-10(5) cm-3. We observed CCS, NH3, C3H2, and HC7N with NASA's DSN 70 m antennas. We also present large-scale maps of C18O and 13CO observed with the AT&T 7 m antenna. For the high spatial resolution maps of selected regions within the core we used the VLA for CCS at 22 GHz, and the Owens Valley Radio Observatory (OVRO) MMA for CCS at 94 GHz and CS (2-1). The 22 GHz CCS emission marks a high-density [n(H2) > 10(4) cm -3] core, which is elongated with a major axis along the SE-NW direction. NH3 and C3H2 emissions are located inside the boundary of the CCS emission. C18O emission traces a lower density gas extending beyond the CCS boundary. Along the major axis of the dense core, CCS, NH3 and C3H2 emission show evidence of limb brightening. The observations are consistent with a chemically differentiated onion-shell structure for the L1498 core, with NH3 in the inner and CCS in the outer parts of the core. The high angular resolution (9"-12") spectral line maps obtained by combining NASA Goldstone 70 m and VLA data resolve the CCS 22 GHz emission in the southeast and northwest boundaries into arclike enhancements, supporting the picture that CCS emission originates in a shell outside the NH3 emitting region. Interferometric maps of CCS at 94 GHz and CS at 98 GHz show that their emitting regions contain several small-scale dense condensations. We suggest that the differences between the CCS, CS, C3H2, and NH3 emission are caused by a time-dependent effect as the core evolves slowly. We interpret the chemical and physical properties of L1498 in terms of a quasi-static (or slowly contracting) dense core in which the outer envelope is still growing. The growth rate of the core is determined by the density increase in the CCS shell resulting from the accretion of the outer low-density gas traced by C18O. We conclude that L1498 could become unstable to rapid collapse to form a protostar in less than 5 x 10(6) yr.  相似文献