山东桩海地区中生界碎屑岩储层特征及其控制因素

采用岩芯观察、薄片鉴定、扫描电镜分析及X-衍射分析等手段,对桩海地区中生界碎屑岩储层的成岩作用、储集空间和控制因素进行了研究。结果表明,桩海地区中生界碎屑岩储层经历了强烈的压实压溶作用和胶结交代作用、多期次的溶解作用和裂缝形成作用;成岩作用阶段可划分为早成岩B,中成岩A1,A2 和中成岩B期。储集空间以溶解孔隙和裂缝为主,裂缝主要有构造裂缝、压实裂缝和解理裂缝;溶解孔隙主要有长石溶解孔隙和碳酸盐胶结物溶解孔隙,其成因主要与大气降水溶解作用和沙河街组、东营组有机质演化过程中形成的有机酸溶解作用有关。桩海地区中生界碎屑岩储层的控制因素主要有沉积作用、成岩作用和构造作用。沉积作用控制了碎屑岩杂基、分选、磨圆等结构特征,进而控制了原生孔隙结构,为后期溶解作用的形成奠定了基础。断层和不整合面作为流体运移通道为溶解作用提供酸性介质,断层和不整合的规模越大对碎屑岩储层物性的控制作用越明显,距离断层和不整合面越近的储层物性越好。溶解作用受沉积作用和构造作用的控制,在原始孔隙结构好、压实作用和早期胶结作用弱以及裂缝发育的地区,溶解作用强烈、次生孔隙发育、储层物性好。在沉积作用、成岩作用和构造作用的综合控制下,中生界顶底及内部不整合面附近发育多个次生孔隙发育带,中生界顶部处于中成岩A1 亚期的储层次生孔隙最发育。     

农业资源信息标准参考模型研究

为满足全社会对农业资源信息共享的迫切需求,使农业资源信息标准化的工作在统一的框架下进行,借鉴国际地理信息标准制定的思路,初步提出了农业资源信息标准化的技术框架--农业资源信息标准参考模型。该标准参考模型是由指导标准、通用标准、专用标准和领域标准等三个部分组成。本文重点阐述了5个指导标准、4类通用标准的标准组成和要点,提出依据基础标准制定专用标准作为农业资源信息较低层次标准制定的重要原则与方法。农业资源信息标准参考模型对于以信息的积累与服务为主的行业信息标准化具有普遍的指导意义。     

S－闭空间上的函数

研究了当Ｘ为Ｓ－闭空间时，Ｃ（Ｘ）的子集Ｆ为紧的充要条件，从而扩充了著名的Ａｓｃｏｌｉ定理。     

星载铷原子频率标准的可靠性研究

星载原子频率标准在许多空间系统中担当着重要的角色,其性能和可靠性对这些系统的功能有重要的影响。介绍了广泛使用的星载铷原子频率标准的基本工作原理,分析了影响其可靠性的各种因素,并探讨了提高其可靠性的基本途径。     

太阳软X射线观测进展

太阳软x射线观测在太阳物理的研究中，特别在日冕结构、磁场和日冕等离子体活动等物理现象的研究中起着重要的作用。太阳软x射线观测主要有光谱和成像观测两种．随着观测技术、方法和内容的发展，太阳软x射线观测揭示了太阳物理的许多重要的科学现象，并在预报、监测空间天气变化，预警空间灾变天气等方面也有着重要的应用．     

高轨空间碎片的观测模拟

对高轨空间碎片进行了观测模拟。在观测模拟中，分别选取南京和云南两个观测站；采用2种跟踪方式：跟踪恒星和跟踪卫星；对于同一地理经度上的同步卫星进行了观测；提供了发现新目标的方法；并给出了新目标的初轨。这为我国空间碎片的数据库的建立作了有益的尝试，对于卫星和航天器的飞行安全具有特别重要的意义。     

TOWARDS AN INTEGRATED SCIENTIFIC AND SOCIAL CASE FOR HUMAN SPACE EXPLORATION

I will argue that an ambitious programme of human space exploration, involving a return to the Moon, and eventually human missions to Mars, will add greatly to human knowledge. Gathering such knowledge is the primary aim of science, but science’s compartmentalisation into isolated academic disciplines tends to obscure the overall strength of the scientific case. Any consideration of the scientific arguments for human space exploration must therefore take a holistic view, and integrate the potential benefits over the entire spectrum of human knowledge. Moreover, science is only one thread in a much larger overall case for human space exploration. Other threads include economic, industrial, educational, geopolitical and cultural benefits. Any responsibly formulated public space policy must weigh all of these factors before deciding whether or not an investment in human space activities is scientifically and socially desirable.     

The science behind the vision for U.S. space exploration: the value of a human–robotic partnership

The Vision for U.S. Space Exploration offers new opportunities for aggressively increasing the pace of scientific discoveries across the Solar System by empowering an on-site partnership between humans and robotics, enhanced by new technology-enabled capabilities. In particular, the early emphasis of this new Vision will be on development of new scientific activities on the Moon, and later on Mars. Integration of in situ traditional science activities with creative new types of applied scientific research on the Moon and Mars is a key ingredient in the US Vision. The Apollo era record of achievement involving human exploration is particularly informative, as it demonstrates the accelerated pace of scientific discovery and understanding that resulted from human “on site” activities, however briefly, on planetary surfaces. An example of how integrated human and robotic exploration can enable breakthrough science on the planet Mars is provided in order to illustrate these points. The scientific opportunities associated with the Vision for US Space Exploration are many, and with the incorporation of human-based capabilities on the Moon and Mars, an accelerated pace of discovery and understanding will be possible.     

非线性相对运动下空间碎片碰撞概率计算的研究

空间目标碰撞概率的计算是航天器进行空间碎片预警和规避机动的基础.为了简化计算,目前国内外在计算碰撞概率问题过程中大多基于线性相对运动的条件,将三维碰撞概率计算积分问题简化为位置误差概率密度函数在圆域内的二维积分问题.但是当空间目标相对运动速度较小时,这种线性运动条件不再成立,就需要在真实的非线性相对运动状态下重新考虑碰...     

On Relativistic Equations of Motion of an Earth Satellite

For numerical integration of the geocentric equations of motion of Earth satellites in the general relativity framework one may choose now between rather simple equations involving in their relativistic dynamical part only the Earth-induced terms and very complicated equations taking into account the relativistic third-body action. However, it is possible quite easily to take into account the relativistic indirect third-body perturbations and to neglect much lesser direct third-body perturbations. Such approach is based on the use of the Newtonian third-body perturbations in geocentric variables with expressing them in the relativistic manner in terms of the barycentric arguments. Together with it, to extend the known results for the spheroid model of the Earth, the Earth-induced terms are treated in great detail by including the non-spin part of the Earth vector-potential and the Earth triaxial non-sphericity.This revised version was published online in October 2005 with corrections to the Cover Date.