Comparison of USGS and DLR topographic models of Comet Borrelly and photometric applications

Stereo analysis of images obtained during the 2001 flyby of Comet Borrelly by NASA's Deep Space 1 (DS1) probe allows us to quantify the shape and photometric behavior of the nucleus. The shape is complex, with planar facets corresponding to the dark, mottled regions of the surface whereas the bright, smooth regions are convexly curved. The photometric as well as textural differences between these regions can be explained in terms of topography (roughness) at and below the image resolution, without invoking significant variations in single-particle properties; the material on Borrelly's surface could be quite uniform. A statistical comparison of the digital elevation models (DEMs) produced from the three highest-resolution images independently at the USGS and DLR shows that their difference standard deviation is 120 m, consistent with a matching error of 0.20 pixel (similar to reported matching accuracies for many other stereo datasets). The DEMs also show some systematic differences attributable to manual versus automatic matching. Disk-resolved photometric modeling of the nucleus using the DEM shows that bright, smooth terrains on Borrelly are similar in roughness (Hapke roughness θ=20°) to C-type asteroid Mathilde but slightly brighter and more backscattering (single-scattering albedo w=0.056, Henyey-Greenstein phase parameter g=−0.32). The dark, mottled terrain is photometrically consistent with the same particles but with roughnesses as large as 60°. Intrinsically darker material is inconsistent with the phase behavior of these regions. Many local radiance variations are clearly related to topography, and others are consistent with a topographic explanation; one need not invoke albedo variations greater than a few tens of percent to explain the appearance of Borrelly.     

Hubble Space Telescope observations of the nucleus fragment 73P/Schwassmann-Wachmann 3-C

The investigation of fragmented comets provides information on the physical properties and internal structure of cometary nuclei, as well as insights into the mechanisms responsible for cometary breakups. The Jupiter-family Comet 73P/Schwassmann-Wachmann 3 (73P/SW3) fragmented non-tidally into at least four components, and probably more, in the autumn of 1995. Fragment C was detected with the Wide Field Planetary Camera 2 (WFPC2) of the Hubble Space Telescope (HST) on 26 November 2001 when it was 3.26 AU from the Sun and 2.34 AU from the Earth. The high spatial resolution of the HST allowed us to separate the signal of the fragment from that of its coma, and to determine its R magnitude in the Johnson-Kron-Cousins photometric system from four images taken with the F675W filter. Assuming a spherical body with a geometric albedo of 0.04 and a linear phase coefficient of 0.04 mag deg⁻¹ for the R band, we derived an effective radius of . The pre-breakup radius of the original nucleus was estimated to be 1.1 km, which implies that the volume of fragment C is ∼25% of the total volume of the pre-breakup nucleus. The limited temporal coverage of our observations preclude deriving an accurate shape or rotational period; our measurements are consistent with a rather spherical body but an elongated shape cannot be excluded. Fragment C was very active despite its rather large heliocentric distance, with an estimated dust production rate of (∼130 metric tons day⁻¹). A very large fraction of the surface area of fragment C must have been sublimating to sustain such a high level of activity. Fragment C may be recovered at its next return in 2006, if it does not experience further fragmentation.     

河北平原曲流河沉积特征及其模式

本文研究了河流沉积构造、结构、石英颗粒表面特征和沉积相特征,并提出组成曲流点坝标志的两个重要要素及沉积模式。有助于认识古代岩相中点坝层序和对此模式。     

New Trends in Numerical Simulation of the Motion of Small Bodies of the Solar System

A brief survey of the results obtained by the authors in the development and investigation of the algorithms of numerical simulation of the motion of solar system small bodies is given. New approaches to the construction of the algorithms of high-accuracy numerical simulation of the dynamics of small bodies and the methods of the determination of the domain of their possible motions are presented.     

俄罗斯利用外资的轨迹

俄罗斯利用外资的轨迹与中国不同,本文通过对外资增长速度与资本,部门及空间结构变化趋势,分析了俄罗斯利用外资的基本特点。     

广东外商投资结构变化研究

９０年代以来,广东省外商投资的结构发生了四大变化,一是尽管外资继续以亚洲资本为主,但欧美外资稳步增长;二是以合作经营、“三来一补”和对外借款方式的投资减少,外商独资、合资经营投资比重上升并居于主导地位;三是流向制造业的外资大幅度增长,商服、房地产投资稳中有降;皲是外资在空间上向边缘地区扩散转移。针对外资的结构变化趋势,提出未来的引资对策：（１）保持亚洲外商稳定增长,大力开发欧美资本市场,实施全球引     

长江三角洲地区可持续发展的态势与对策

长江三角洲自20世纪90年代以来经济发展非常迅速, 在全国的地位不断上升, 且其产业结构也在逐步改善。外商投资在该区异常活跃, 投资规模越来越大, 2003年实际利用外资占全国的比例已达45.55%。该地区还是我国区域经济合作发展实施进程较快、力度较大、政府重视程度较高的地区。但长江三角洲在发展中仍存在不少问题, 如引进外资的整体层次不高、耕地流失严重且建设用地的集约化程度较低、能源缺口较大、交通运输紧张及生态环境恶化等。长江三角洲地区目前虽然出现了这些问题, 但不能由此而限制它的发展, 要充分利用长江三角洲有利的区位优势, 走可持续发展道路, 在发展中解决问题。具体应该做到要切实明确长江三角洲在全国区域经济分工中的地位, 在提高产业发展层次的同时, 不可放松对劳动密集型产业的发展, 并以科学发展观为指导, 加强土地资源和能源的管理, 加速环境保护和生态修复工作的进程。     

国外休闲制约研究的特征与展望——基于《Journal of Leisure Research》、《Leisure Sciences》、《Journal of Park and Recreation Administration》期刊

选取国外三大休闲权威期刊《Journal of Leisure Research》（1992—2014年）、《Leisure Sciences》（1998—2014年）、《Journal of Park and Recreation Administration》（2001—2014年）共130篇休闲制约研究论文,通过文献统计和文献分析法,从研究方法、研究内容及发展趋势三方面,分析国外休闲制约研究的基本特征。研究认为：国外休闲制约研究方法以定量研究方法为主,定性研究方法日益受到重视;国外学者重点关注休闲制约因素、休闲制约协商、女性休闲制约、种族人群休闲制约和青少年休闲制约等内容,同时强调内在机制研究和模型构建。此外,关注社会文化制约因素,加强跨学科研究和时间纵向研究,重视中国文化背景下的休闲制约研究对世界休闲制约研究的独特贡献以及跨文化合作的必要性是未来研究的重要方向。     

玲南金矿床矿体地质特征及深部资源前景

玲南金矿床位于玲珑金矿田内,由招远-平度断裂带北段的破头青断裂带控制,是一超大型的蚀变岩型金矿床。目前钻探控制最大深度接近2 000m,主矿体控制最大斜深约2 200m,矿体沿倾向仍未封闭,预测深部仍有较好的资源前景。     

莱州市土山-东宋铁矿地质特征

通过近几年的地质找矿工作,莱州市土山—东宋地区发现了中型变质沉积铁矿床。矿床产于古元古代粉子山群小宋组二段底部的含铁岩系。矿石工业类型为需选弱磁性铁矿石,主要成因类型为磁铁黑云片岩型、磁铁变粒岩型。矿床范围内共划分了5个矿段40个矿体。该文以此为基础,对矿区地质特征进行分析研究,以期促进山东省铁矿地质勘查工作的开展。