Seismology of stellar envelopes: probing the outer layers of a star through the scattering of acoustic waves

The outer layers of Sun-like stars are regions of rapid spatial variation which modulate the p-mode frequencies by partially reflecting the constituent acoustic waves. With the accuracy that has been achieved by current solar observations, and that is expected from imminent stellar observations, this modulation can be observed from the spectra of the low-degree modes. We present a new and simple theoretical calculation to determine the leading terms in an asymptotic expansion of the outer phase of these modes, which is determined by the structure of the surface layers of the star. Our procedure is to compare the stellar envelope with a plane-parallel polytropic envelope, which we regard as a smooth reference background state. Then we can isolate a seismic signature of the acoustic phase and relate it to the stratification of the outer layers of the convection zone. One can thereby constrain theories of convection that are used to construct the convection zones of the Sun and Sun-like stars. The accuracy of the diagnostic is tested in the solar case by comparing the predicted outer phase with an exact numerical calculation.     

Defect properties of albite

Knowledge of the defect properties of Lunar and Mercurian minerals has recently become important, with the advent of models which attempt to explain the formation of the thin exosphere of these celestial bodies. Here, we have calculated the formation energies of sodium and oxygen vacancies in the mineral albite (NaAlSi₃O₈), as well as the Schottky defect energy for the removal of a Na₂O unit. We have employed both the supercell and Mott–Littleton approaches, using Kohn–Sham density functional theory and classical interatomic potential methods. As well as reporting the defect energies and structures, we comment upon the relative merits of the methods used.     

An Analysis on Limit Load for Corroded Submarine Pipelines

1 .Introduction Submarine pipelines are one of the safest and the least environmentally disruptive means for ma-rine gas or oil transport . With the development of exploitation of submarine oil or gas ,the safety ofsubmarine pipelines has becomethe major …     

一种提高教育版VirtuoZoNT的影像处理能力的方法

现有的教育版数字摄影测量软件VirtuoZoNT3.6仅能处理扫描孔径大于0.1mm的影像,针对这一瓶颈问题,本文从数字影像的内定向公式入手,分析得到了影像扫描孔径与框标理论坐标之间的关系。通过修改参数文件可使教育版VirtuoZoNT具备处理扫描孔径小于0.1mm影像的能力,同时通过转换数据格式可使其处理其他不同类型的影像数据。     

晚新生代亚洲干旱气候发展与全球变冷联系的风尘沉积证据

在干旱气候背景下常常有风尘物质的释放和传输,风尘沉积被认为是干旱环境变化良好的地质记录。在亚洲中部和中国北方,大面积的干旱区被沙漠戈壁覆盖,这些地区是粉尘物质的重要源地,释放的风尘物质影响局地和区域环境,并通过参与生物地球化学循环等影响更大空间尺度的气候变化。因此,亚洲中部干旱气候的形成和演化以及发展趋势一直受到重视。长期以来,关于晚新生代亚洲中部干旱气候发展的驱动机制至少有两种解释:一是青藏高原的隆升控制着亚洲中部的干旱化过程,随着高原的阶段性隆升亚洲干旱气候逐步增强;二是晚新生代全球变冷直接驱动着亚洲变干,全球变冷是主导因素。中国黄土高原及其周边地区堆积的黄土-红粘土序列是指示亚洲干旱化过程良好的地质记录,通过对新获得的风尘堆积记录的分析,发现在晚新生代中国风尘堆积的时空演化与全球变冷有较好的对应,全球变冷可以促使亚洲中部干旱气候发展并加强粉尘活动,而青藏高原隆升的幅度和时间还不清楚,进而认为是全球变冷而不是青藏高原隆升直接驱动亚洲内陆的阶段性变干。基于这些结果,我们认为以前关于青藏高原隆升影响全球气候的结论可能高估了青藏高原在地球环境演化中的作用,关于高原隆升直接驱动亚洲干旱化的结论还需要检验。     

浅谈局域网的内部安全管理

自上个世纪70年代初出现局域网,局域网已普及到国民经济的各个部门,也同样成为测绘行业各类数字测绘产品的生产服务平台.如何搞好局域网的内部管理,确保网络安全运行,成为一个亟待解决的课题.根据多年来网络管理的亲身经历,本人认为事故大多都间接地来自于内部安全管理上的疏忽和漏洞.     

Neutron irradiation and post-irradiation annealing of rutile (TiO2−x ): effect on hydrogen incorporation and optical absorption

Neutron irradiation and post-irradiation annealing under oxidising and reducing conditions have been used to investigate H incorporation in, and the optical properties of, reduced (TiO_2−x ) rutile. Optical absorption in rutile is mainly due to a Ti³⁺ Ti⁴⁺ intervalence charge transfer effect. The main mechanism for H incorporation in rutile involves interstitial H not coupled to other defects, which has important implications for the rate of H diffusion, and possibly also on the electrical properties of rutile. Additional minor OH absorption bands in IR spectra indicate that a small amount of interstitial H is coupled to defects such as Ti³⁺ on the main octahedral site, and indicates that more than one H incorporation mechanism may operate. Concentration of oxygen vacancies has a controlling influence on the H affinity of rutile.     

框标与影像叠置时的自适应内定向算法

虽然自动内定向在过去的几年是研究的热点问题，但是针对P31这类近景相机的影像进行自动内定向还存在一些问题，主要原因在于P31影像的框标叠置在景物上。认为自动内定向可以看做一个全局影像匹配问题，分两步进行。首先，用模板匹配和Hough变换在影像上提取可能的框标点，然后用软对应和确定性退火结合仿射变换得到惟一的框标位置。试验和结果分析说明，利用本文方法，可以惟一确定框标，并发现严重的粗差。同时提出自动确定最小的框标搜索区域的方法。     

分层重力图像方法及其应用

分层重力图像方法是依据三维地震波速的层析成像结果，通过速度与密度相关关系，转换得到分层的密度结构模型，计算并给出各分层在地表的重力异常分布图像．以中国大陆为例，给出其不同深度的7个分层的重力异常图像和不同分层叠加的综合（或总合）重力异常分布图像．经过与实测的中国布格重力异常资料对比分析，结果表明两者的重力场特征相当一致；分层重力图像的结果能较好地反映地下不同深度的物质分布．