频率域电磁测深中磁场水平分量新的计算方法     

汤井田  何继善 《物探化探计算技术》1993,15(1):64-68

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遥感技术与美国的人口普查     

H.A.莫罗——琼斯  J.F.沃特金斯  林珲 《地理科学进展》1985,4(3):37-43

引言 D.布鲁金尼的论文《可用空间时代技术进行更精确的人口普查》提出了一些有趣的问题。我们为能够在《摄影测量工程和遥感》杂志上看到这篇有关遥感在社会科学领城内的应用的论文而高兴。我们认为只有了解人口普查数据的多种用途之后,再来检验那些改进人口普查的方法才是合适的,众所周知,每十年一次的人口普查数据的精度和完备性并不是没有缺点的。无疑地,许多人口普查人员将首先承认,每次由点数  相似文献   

伪随机码调制的CW半导体激光雷达试制报告     

肖弟权  何建新  邱万智 《成都信息工程学院学报》1993,(4)

本文报告一种用半导体激光器作光源,用子脉冲宽度100ns,长度为511的周期伪随机码对半导体激光器的输出作幅度调制;APD作光电检测器,高速数字信号处理器TMS320C25作信号处理的激光雷达组成方案和试作样机的实验结果。  相似文献   

矿床地球化学模型的建立及其找矿效果探讨—以团结沟金矿为例     

魏仪方  何高文 《长春地质学院学报》1992,23(4):393-399

当今矿床学研究中的热点问题之一是矿床模型研究。矿床建模的理论与方法，矿床模型的定量化是目前矿床模型研究中亟待解决和完善的问题。从典型矿床入手，首先建立易于实现定理化的矿床地球化学模型，将有助于打破矿床模型研究的僵局。团结沟金矿床地球化学模型的建立是一个初步尝试。矿床地球化学模型能迅速转化为找矿模型，为找矿预测提供简捷有效的途径。  相似文献   

MONITORING THE DIFFUSION OF SUSPENDED SEDIMENTS AND STABILITY OF TIDAL RADIAL SAND RIDGES AREA USING MULTI-SATELLITE REMOTE SENSING DATA     

黄海军  何宜军 《中国海洋湖沼学报》2001,19(4):361-367

Nine Landsat TM tapes and images and MSS images, 10 NOAA tapes and images and 1 SAR image from 1973 to 1997 were used to analyse the diffusion of suspended sediments and the change of tidal radial sand ridges in the northern part of the Changjiang River delta, the South Yellow Sea. The results showed that the diffusion of suspended sediments was controlled by the tide, net current, and submarine topography in this area. The distribution of suspended sediments had close relationship with thesubmarine topography. The old Huanghe River delta and the Changjiang River comprise the main sediment supply for the formation of radial sand ridges, whose evolution can be divided into three stages since the Huangbe River changed its course and flowed northward into the Bohai Sea.  相似文献   

11颗类星体光谱(英文)     

陈建生  P.A.Shaver  I.J.Danziger 《中国天文和天体物理学报》1985,(4)

对天区0112-35的UKST物端棱镜底片上的11个类星体候选者进行了光谱观测,证实为类星体,给出了它们的红移值、证认图及光谱图。11个类星体中有6个属于角距小于4角分的3对类星体;1个类星体-星系对。  相似文献   

美国地貌学情况综述     

J.E.科斯塔  云浦 《地理科学进展》1985,4(2):29-33

我们根据地貌工作者和第四纪地质学工作的人数、专业团体会员人数及其有关出版物等情况对美国地貌学家的活动状况做一个综述。美国的地貌学出现于19世纪末期。当时的地质学和地理学还紧密联系在一起的。当地理学成为一个独立学科时,其成员主要是自然地理学家和学过地质学的地貌学工作者。在本世纪30年代期间,地理学家们反对环境决定论的模式,地貌学的重要性有所下降。  相似文献   

国家自然科学基金海洋科学项目基础资料数据库管理系统的设计     

许启望  何广顺 《海洋通报》1995,14(6):68-71

介绍了以ＦｏｘＰｒｏ为软件开发平台的国家自然科学基金海洋科学项目基础资料数据库管理系统的设计。该系统包括国家自然科学基金支持的海洋各分支学科项目的基础信息，如资料、人员、获奖情况等。并提供了查询和统计分析等功能，为管理部门管理和有效地利用海洋科学基金项目的基础资料提供了科学手段。  相似文献   

Heterodyne spectroscopy of the 158 micron C II line in M42     

Boreiko RT  Betz AL  Zmuidzinas J 《The Astrophysical journal》1988,325(2):L47-L51

We have obtained velocity-resolved spectra of the 12C II 157.8 microns 2P3/2-2P1/2 fine structure line in the M42 region of Orion. Observations at 0.8 km s-1 resolution with a laser heterodyne spectrometer show multiple velocity components in some locations, with typical linewidths of 3-5 km s-1. Spectra of theta 1C and BN-KL also show weak emission from the F = 2-1 hyperfine component of the equivalent 13C II line. From the observed 12C II/13C II line intensity ratios, we deduce that the 12C II emission is optically thick with tau approximately 5 at both positions. Excitation temperatures of 128 K and 90 K, together with column densities of approximately 1 x 10(19) cm-2 and approximately 4 x 10(18) cm-2, are derived for theta 1C and BN-KL, respectively.  相似文献   

Variations in the HCN/HNC abundance ratio in the Orion molecular cloud     

Goldsmith PF  Irvine WM  Hjalmarson A  Elldér J 《The Astrophysical journal》1986,310(1):383-391

We have used observations of the rare isotopes of HCN and HNC to determine the relative abundance of these two chemical isomers along the central ridge of the Orion molecular cloud. The abundance ratio [HCN]/[HNC] decreases by more than an order of magnitude from the relatively warm plateau and hot core sources toward the KL nebula to the colder, more quiescent clouds to the north and south. Even in the cooler regions, however, the ratio is an order of magnitude larger than that found in previous investigations of cold dark clouds. We determine the kinetic temperature in the regions we have studied from new observations of methylacetylene (CH3CCH), together with other recent estimates of the gas temperature near KL. The results suggest that the warmer portions of the cloud are dominated by different chemical pathways than those in the general interstellar cloud material.  相似文献