基于GIS的北京城市形态研究

经典的城市形态理论包括同心圆理论、扇形理论和多核心理论.利用2002年北京市土地利用图,采用GIS缓冲区分析的方法,分析了北京市各功能用地的方向特征和圈层特征.结果表明:北京市的土地利用体现了明显的圈层特征,同时各类功能用地在各方向的分布又明显受到了河流、交通干道和工业区等地理要素的影响.北京没有形成城市总体规划的多中心布局,第一道绿化隔离地区中绿地面积没有明显高出其他地区,基本上已经失去了中心城区和边缘集团隔离开的功能.总体上,北京城市空间形态主要是同心圆和扇形的结合,更接近同心圆理论和扇形理论的混合形式.     

地质和岩土工程光纤传感监测技术综述

光纤传感器与常规传感器相比具有很大的优越性,已经成为地质和岩土工程监测领域中的研究热点。本文介绍了光纤传感监测系统的种类、基本测量原理和目前国内外的研究发展状况,并对各种传感技术的性能和特点进行了比较,指出了光纤传感监测技术应用于地质和岩土工程监测尚需研究的相关课题。     

Multiple Volcanic Episodes of Flood Basalts Caused by Underplating

Most Large igneous provinces (LIPs) are emplaced within <10 Ma, with a main pulse of the magmatism in<1 Ma[1]. For example, the Siberian Traps [2] and the Deccan Traps [3] were probably erupted within one million years. Many events, such as the Columbia River event, feature a single pulse of magmatism, followed by a protrac-ted period of magmatism at a much lower rate that is linked to a plume tail[4].     

OBE理念下GIS空间分析课程思政教学设计与实践

以成果导向教育(Outcome Based Education,OBE)和课程思政理念为指导进行课程设计与实践,是地理信息科学专业应用型人才培养的发展趋势.围绕专业人才培养目标和课程教学目标,以反向设计为原则,结合专业毕业要求,确定课程学习成果,然后以成果为导向,设计实施教学改革,将思政元素有机融入专业教学中,培养学生综合素养.地理信息系统(Geographic Information System,GIS)方向的课程《GIS空间分析》是地理信息科学专业核心课程,探索和实施成果导向下的课程思政教学目标的达成,围绕教学目标进行有效的教学设计,结合课程内容从理论知识和实践操作两个层面进行课程思政教学融入设计,提出课程思政融入专业课教学的典型案例和实施路径,包括制定课程目标、确定学习成果、探索和实施新型教学方式、优化课程考核和评价方式等方面.     

Infinitesimal orbits around lagrange points in the elliptic,restricted three-body problem

This study presents a method of obtaining asymptotic approximations for motions near a Lagrange point in the planar, elliptic, restricted three-body problem by using a von Zeipel-type method. The calculations are carried out for a second-order escape solution in the proximity of the equilateral Lagrange point, L ₄, where the primaries' orbital eccentricity is taken as the small parameter .     

The acceleration of minor ion species in the solar wind

This paper provides a comprehensive analysis of the dynamics of the flow of minor ion species in the solar wind under the combined influences of gravity, Coulomb friction (with protons), rotational forces (arising from the Sun's rotation and the interplanetary spiral magnetic field) and wave forces (induced in the minor ion flow by Alfvén waves propagating in the solar wind). It is assumed that the solar wind can be considered as a proton-electron plasma which is, to a first approximation, unaffected by the presence of minor ions. In the dense hot region near the Sun Coulomb friction accelerates minor ions outwards against the gravitational force, part of which is cancelled by the charge-separation electric field. Once the initial acceleration has been achieved, wave and rotational forces assist Coulomb friction in further increasing the minor ion speed so that it becomes comparable with, or perhaps even exceeds, the solar wind speed. A characteristic feature of the non-resonant wave force is that it tends to bring the minor ion flow into an equilibrium where the radial speed matches the Alfvén speed relative to the solar wind speed, whereas Coulomb friction and rotational forces tend to bring the flow into an equilibrium where the radial speed of the minor ions equals the solar wind speed. Therefore, provided that there is sufficient wave energy and Coulomb friction is weak, the minor ion speed can be trapped between these two speeds. This inteststing result is in qualitative agreement with observational findings to the effect that the differential flow speed between helium ions and protons is controlled by the ratio of the solar wind expansion time to the ion-proton collision time. If the thermal speeds of the protons and minor ions are small compared to the Alfvén speed, two stable equilibrium speeds can exist because the rapid decrease in the Coulomb cross-section with increasing differential flow speed allows the non-resonant wave force to balance Coulomb friction at more than one ion speed. However, it must be emphasized that resonant wave acceleration and/or strong ion partial pressure gradients are required to achieve radial speeds of minor ions in excess of the proton speed, since, as is shown in Section 4, the non-resonant wave acceleration on protons and minor ions are identical when their radial speeds are the same, with the result that, in the solar wind, non-resonant wave acceleration tends (asymptotically) to equalize minor ion and proton speeds.     

Observations of the structure and evolution of solar flares with a soft X-ray telescope

132 soft X-ray flare events have been observed with The Aerospace Corporation/Marshall Space Flight Center S-056 X-ray telescope that was part of the ATM complement of instruments aboard Skylab. Analyses of these data are reported in this paper. The observations are summarized and a detailed discussion of the X-ray flare structures is presented. The data indicated that soft X-rays emitted by a flare come primarily from an intense well-defined core surrounded by a region of fainter, more diffuse emission. Loop structures are found to constitute a fundamental characteristic of flare cores and arcades of loops are found to play a more important role in the flare phenomena than previously thought. Size distributions of these core features are presented and a classification scheme describing the brightest flare X-ray features is proposed. The data show no correlations between the size of core features and: (1) the peak X-ray intensity, as indicated by detectors on the SOLRAD satellite; (2) the rise time of the X-ray flare event, or (3) the presence of a nonthermal X-ray component. An analysis of flare evolution indicates evidence for preliminary heating and energy release prior to the main phase of the flare. Core features are found to be remarkably stable and retain their shape throughout a flare. Most changes in the overall configuration seem to be the result of the appearance, disappearance or change in brightness of individual features, rather than the restructuring or re-orientation of these features. Brief comparisons with several theories are presented.     

我国高寒草甸植被生产力及其影响因子

生物量是重要的植物群落数量特征，直接反映生态系统生产者的物质生产量，是生态系统生产力的重要体现。高寒草甸广泛分布于青藏高原，是高寒生态系统的主要植被类型。回顾了高寒草甸生物量的研究成果。高寒草甸生物量呈典型的金字塔式垂直分布格局，地上生物量主要集中于0—10cm的冠层，地下生物量也集中分布于0—10cm的土层内。增温和多雨会降低生物量，叶面积和物种丰富度与地上生物量成正相关关系，氮素的增加有助于植被生物量的增长，而放牧率与生物量成显著负相关。