Activity and kinematics of members of the TW Hydrae association

We present high-resolution echelle spectroscopy of 20 stars in 16 systems catalogued as members of the TW Hydrae association, and 16 stars identified as possible new members. We have calibrated the range of coronal and chromospheric activity expected for such young stars as a function of spectral type by combining our observations with literature data for field and open cluster stars. We also compute space motions for TWA members and candidate members with proper motion measurements, using two techniques to estimate distances to stars lacking direct trigonometric parallax measurements. The mean space motion of the four TWA members with known parallaxes is  ( U , V , W : −10.0, −17.8, −4.6) km s⁻¹  . 14 of the candidates have properties inconsistent with cluster membership; the remaining two are potential new members, although further observations are required to confirm this possibility.     

The SFR and IMF of the galactic disk

There is a long term dynamical heating of stellar populations with age observed in the age – velocity dispersion – relation (AVR). This effect allows a determination of the star formation history SFR(t) from local kinematical data of main sequence stars. Using a self-consistent disk model for the vertical structure of the disk, we find from the kinematics of the stars in the solar neighbourhood that the SFR shows a moderate star burst about 10 Gyr ago followed by a continuous decline to the present day value consistent with the observed number of OB stars. The gravitational potential of the gas component and of the Dark Matter Halo is included and the effect of chemical enrichment, finite lifetime of the stars and mass loss of the stellar component are taken into account. The scale heights for main sequence stars together with the SFR is then used to determine constistently the IMF from the observed local luminosity function. The main new result is that the power law break in the present day mass function (PDMF) around 1 M _⊙ is entirely due to evolutionary effects of the disk and does not appear in the IMF. This revised version was published online in August 2006 with corrections to the Cover Date.     

CPⅢ测量数据处理系统开发若干关键技术研究

本文首先介绍了无砟轨道的相关内容,指出CPⅢ测量数据处理是整个建设中的关键,提出系统开发的总体目标与要求且设计了系统总体结构,详细阐述了系统开发中涉及的关键技术与基本理论,文中最后结合具体工程实例验证系统开发成果。     

遥感技术在地质找矿中的应用及发展前景

遥感技术作为矿产勘查的一种手段应用于找矿,并取得了一定成就.遥感技术的直接应用是蚀变遥感信息的提取,遥感技术的间接应用包括地质构造信息、植被的光谱特征及矿床改造信息等方面.遥感找矿具有很大的发展前景的领域主要有:高光谱数据、数据融合技术、3S的紧密结合、计算机技术的发展.     

翁牛特旗--库伦旗一带严重缺水区的地质环境及找水途径

翁牛特旗--库伦旗一带为西辽河平原周边的严重缺水区.通过分析研究区地下水形成的地质环境,认为降水量、地形地貌、岩性构造和地下水循环是造成研究区严重缺水的主要因素,地层岩性和新构造运动是影响地下水富集的决定性因素.指出要加强含水层的岩性和构造、基岩区的断裂性质和产状的研究,并提出在基岩区、低山丘陵区寻找构造裂隙水和断裂带脉状水是解决研究区严重缺水的较好途径.     

湘西南区氧化锰矿成矿规律及找矿方向

湘西南区氧化锰矿以锰帽型氧化锰矿为主，赋矿地层为震旦系下统湘锰组。其特点是含锰点多，分布面广，矿体在地壳贫化，往下３～７ｍ开始富集，氧化深度４０ｍ左右。     

西昌盆地油气化探普查效果及下一步找油气方向

为了配合国家加快油气资源勘查步伐，四川石油管理局将西昌盆地作为下一步勘探重点地区，由于西昌盆地属勘探新区，各种地质、构造情况复杂，首先在该区实施了油气化探普查，油气化探普查结果证实了西昌盆地中部地区为油气泄漏特征，这与七坝1井结果吻合，同时发现了三个重点区域，指出盆地西部为下一步工作的重点地区，为下一步地震勘探指明找油气方向。     

海洋自主航行器多海湾区域完全遍历路径规划

海洋自主航行器在对海底地形测绘和水文信息搜集过程中,简单锯齿形完全遍历路径规划算法对多海湾海底地形探测易出现重复区域和遗漏区域的问题。本文提出了遗漏海湾和重复海湾及其进入点、退出点和门户的路径规划环境表达概念,并将其应用在基于行为的锯齿形完全遍历路径规划改进算法中,有效地减少了海洋自主航行器全覆盖地形测绘的重复区域和遗漏区域。在网格化定常流场海域内,对某一阻力特性已知的自主水下机器人进行了完全遍历路径规划仿真,验证了基于重复和遗漏海湾搜索行为的完全遍历路径规划算法的遍历性和不重复性,并降低了区域全覆盖地形测绘任务的耗能。最终,通过小型无人艇湖试验证了算法在完全遍历路径规划中的节能性和实用性。