Measuring the Fundamental Parameters of Hot Hydrogen－Rich White Dwarfs

This review considers the observations of hot, hydrogen-rich white dwarf stars, with particular reference to measurements of temperature, surface gravity and composition. Spectroscopic data from a variety of wavelength ranges are required for this work and, in particular, the important contributions from optical, ultraviolet and extreme ultraviolet studies are discussed. Using the values of Tefr and log g determined for an individual white dwarf, estimates of mass and radius might be derived from the theoretical mass-radius relation. The issue of the accuracy of the theoretical mass-radius calculations and the prospects for making empirical tests using observational data are outlined.     

基于无人机影像的面向对象建筑物结构分级提取方法研究

为提高遥感影像建筑物结构识别精度,综合利用光谱、形状、空间、纹理和数字表面模型(DSM)建立了建筑物结构分级提取方法。基于研究区无人机高分辨率影像,采用面向对象的影像分析策略,首先进行多尺度分割,以最佳分割与合并指数提取影像中建筑物目标;然后分别采用规则、训练样本与DSM方法对建筑物结构进行分类;最后将3种分类方法进行融合,对比分析了单一方法和融合分类方法的建筑物结构分类精度。结果表明:基于规则+样本+DSM的半监督建筑物结构分类方法错分率、漏检率与Kappa系数最优。     

内蒙古高原小叶锦鸡儿(Caragana microphylla)灌丛沙丘:形态特征及表面气流

小叶锦鸡儿灌丛沙丘是内蒙古高原阴山北麓农牧交错带的主要风沙堆积类型.野外调查表明灌丛沙丘在该区主要分布在耕地、冲积扇下风侧和村落周围等人类活动频繁的地段.根据对耕地、冲积扇下风侧典型样地灌丛沙丘形态参数的详细测量和沙丘及丘间地气流的系统观测结果,发现灌丛沙丘覆盖度及风沙沉积量顺风向减小,近地面气流空气动力学粗糙度顺风向减小;在沙丘单体,风速廓线由迎风坡经丘顶至背风坡趋于复杂.在沙丘形态诸参数中,沙丘高度与水平尺度之间存在良好的幂函数相关,表明在目前风况和沙源环境中该区灌丛沙丘处在加积增高阶段,但其速率小于水平扩展.该区灌丛沙丘的规模主要受上风侧可供沙源有效性和灌丛生长状况的控制,灌丛沙丘的出现是该区土壤风蚀和土地退化的主要标志.     

低渗透储层微流动机理及应用进展综述

低渗透储层具有孔喉细小、孔隙结构复杂、比表面积大,黏土矿物类型丰富等特点,这些特点致使流体在低渗透储层中流动会产生强烈的微流动效应。微流动效应主要包括稀薄效应和不连续效应、表面优势效应、低雷诺数多流态效应、多尺度多相态效应等,这些特殊效应将影响描述流体流动的微分方程及边界状态。孔隙结构特征、黏土矿物产状、润湿性、岩石矿物荷电性等是低渗透储层微流动的影响因素,通过控制这些因素,可以改变流体在低渗透储层中的流动特征,从而控制油、气、水产量。目前已经形成了界面修饰技术、电化学驱油等采油新技术。以微流动机理为基础,结合孔隙结构特征,找出影响低渗透储层流体流动的主控因素,采用具有针对性的开采技术将成为高效开发低渗透油气资源的有效途径。     

呼伦贝尔沙质源区铅同位素分布特征及其示踪意义的初步研究

呼伦贝尔沙质草原风蚀坑发育于宽单峰中能风况环境,是该区主要风沙地貌类型.对碟形坑表面气流的观测结果显示,气流进入风蚀坑后,在入风口扩散,风速开始降低至坑底达到最低;在坑后缘出风口汇集形成急流,风速剧增至坑后积沙顶部风速达到最高值.风蚀坑后缘在风沙流的磨蚀作用下后退,风蚀坑顺风向扩展,同时此处较大的剪切风速和输沙率使大量来自坑内的沙物质沉积到坑后草地上呈扇状蔓延.呼伦贝尔沙质草原风蚀坑在来自西北、西和西南方向风的交替作用下,向东南、东和东北方向扩展而生成.随着风蚀坑深度和水平尺度的增加,最终可能沿强风能方向或合成输沙方向扩展成为大型的槽形坑.     

Polarimetric entropy of the ocean surface with a two-scale scattering model

The relationships among an ocean wave spectrum,a fully polarimetric coherence matrix,and radar parameters are deduced with an electromagnetic wave theory.Furthermore,the relationship between the polarimetric entropy and ocean wave spectrum is established based on the definition of entropy and a twoscale scattering model of the ocean surface.It is the first time that the polarimetric entropy of the ocean surface is presented in theory.Meanwhile,the relationships among the fully polarimetric entropy and the parameters related to radar and ocean are discussed.The study is the basis of further monitoring targets on the ocean surface and deriving oceanic information with the entropy from the ocean surface.The contrast enhancement between human-made targets and the ocean surface with the entropy is presented with quad-pol airborne synthetic aperture radar（AIRSAR） data.     

WaMoS Ⅱ测波雷达应用及对比分析

利用大万山海洋环境监测站WaMoS Ⅱ雷达测量的数据与同步SZF遥测波浪浮标、SLC9-2型直读式海流计的数据分别进行了对比分析。结果表明WaMoS Ⅱ测波雷达获取的有效波高、波峰周期、表面流速、流向等海洋物理要素的变化趋势与SZF遥测波浪浮标获取的波浪数据及SLC9-2型直读式海流计测到的海流数据有较好的一致性。其中,2012年6月16—22日雷达和遥测波浪浮标对比结果为:波高、周期的相关系数分别为0.71,0.38,平均相对误差分别为23.3%,12.5%。6月28—29日的对比结果为:流速、流向的相关系数分别为0.83,0.89,平均相对误差分别为14.5%,4.1%。其中,WaMoS Ⅱ系统测量的有效波高值需通过对比分析进行校准,本文利用的对比分析数据时间序列较短,但经校准后,有效波高值的相关性仍可升至0.75。     

热带气旋风场非对称性对表面海浪场的影响

用WAVEWATCHIII海浪模拟了5个不同风场结构的热带气旋下海浪平均要素和海浪方向谱来研究其对风场非对称性的响应。结果表明热带气旋诱发的海浪场对风场的非对称性很敏感。随着风场非对称性加强,有效波高除了左前象限增加以外在其他所有象限内都减小,且有效波高场的非对称性增强,并且非对称轴逆时针旋转,同时,有效波高最大值的位置向前移动。风场的非对称性对其他平均要素也有影响,尤其在左后象限最明显,例如平均波长,平均波向,波峰方向等。风场的非对称性对海浪谱的多峰性以及主导波的频率和传播方向都有很重要的影响。     

Simulation and causes of eastern Antarctica surface cooling related to ozone depletion during austral summer in FGOALS-s2

Two parallel sets of numerical experiments （an ozone-hole simulation and a non-ozone-hole simulation） were performed to investigate the effect of ozone depletion on surface temperature change using the second spectral version of the Flexible Global Ocean-Atmosphere-Land System model （FGOALS-s2）, focusing on the eastern Antarctica （EA） continent in austral summer. First, we evaluated the ability of the model to simulate the EA surface cooling, and found the model can successfully reproduce the cooling trend of the EA surface, as well as the circulation change circling the South Pole in the past 30 years. Second, we compared the two experiments and discovered that the ozone depletion causes the cooling trend and strengthens the circumpolar westerly flow. We further investigated the causes of the EA surface cooling associated with the ozone hole and found two major contributors. The first is the ozone-hole direct radiation effect （DRE） upon the surface that happens because the decrease of the downward longwave （LW） radiation overcomes the increase of the downward shortwave （SW） radiation under clear sky. The second is the cloud radiation effect （CRE） induced by ozone depletion, which happens because the decreased downward SW radiation overcomes the increased downward LW radiation in the case of increased cloud. Although the CRE is theoretically opposite to the DRE, their final net effect makes comparable contributions to the EA surface cooling. Compared with the surface radiation budget, the surface heat flux budgets have a much smaller contribution. We additionally note that the CRE is basically ascribed to the circulation change.