基于Plücker直线的机载LiDAR点云与航空影像的配准

机载LiDAR点云与航空影像的配准是地物提取的关键。本文提出了基于Plücker直线的机载LiDAR点云与航空影像的配准模型。基于三维线空间线变换Plücker直线方程,确定点云和影像中的同名直线间的相对位姿关系,建立Plücker直线共面条件方程,通过影像上的Plücker直线在三维线空间中的螺旋运动,实现像点到其对应LiDAR点的坐标变换。结果表明,Plücker直线共面条件配准模型简洁,将旋转和平移统一处理,避免了两者间的耦合误差,提高了配准精度,为获取高质量的地球三维空间信息提供了技术支持。     

SN 1994W: an interacting supernova or two interacting shells?

We present a multi-epoch quantitative spectroscopic analysis of the Type IIn supernova (Type IIn SN) 1994W, an event interpreted by Chugai et al. as stemming from the interaction between the ejecta of a SN and a  0.4 M_⊙  circumstellar shell ejected 1.5 yr before core collapse. During the brightening phase, our models suggest that the source of optical radiation is not unique, perhaps associated with an inner optically thick cold dense shell and outer optically thin shocked material. During the fading phase, our models support a single source of radiation, an hydrogen-rich optically thick layer with a near-constant temperature of ∼7000 K that recedes from a radius of  4.3 × 10¹⁵  at a peak to  2.3 × 10¹⁵ cm  40 d later. We reproduce the hybrid narrow-core broad-wing line profile shapes of SN 1994W at all times, invoking an optically thick photosphere exclusively (i.e. without any external optically thick shell). In SN 1994W, slow expansion makes scattering with thermal electrons a key escape mechanism for photons trapped in optically thick line cores, and allows the resulting broad incoherent electron-scattering wings to be seen around narrow-line cores. In SNe with larger expansion velocities, the thermal broadening due to incoherent scattering is masked by the broad profile and the dominant frequency redshift occasioned by bulk motions. Given the absence of broad lines at all times and the very low ⁵⁶Ni yields, we speculate whether SN 1994W could have resulted from an interaction between two ejected shells without core collapse. The high conversion efficiency of kinetic to thermal energy may not require a SN-like energy budget for SN1994W.     

地面高精度磁测在印尼滨海型磁铁矿应用

综合运用低纬度化极与建立模型正演等数据处理手段进行隐伏矿体预测,发现与成矿有关的磁异常,显示良好成矿前景。钻孔证实有工业矿体。     

一个罕见的铀钨矿物组合

本文首次报导钨锰矿和铀矿物在空间上叠生的现象。这种叠生现象出现在一种很特别类型的矿床中，与传统的铀钨伴生理论有悖，这种铀、钨叠生矿化不仅具有重要的经济价值，而且也会拓展铀、乌伴生理论的研究。     

滇西耿马四排山地区地质新认识

滇西耿马四排山地区弄巴组（原南皮可组上部）盛产化石抱粉，通过５０多块样品的分析，获得了晚泥盆世末（Ｒｅｔｉｓｐｏｒａｌｅｐｉｄｏｐｈｙｔａ）叶至早石炭世早期（Ｇｒａｎｄｉｓｐｏｒａｓｐｉｃｕｌｉｆｅｒａ）孢粉组合。它们可以与西欧同期孢粉进行对比，并能部分地与澳大利亚同期孢粉对比。因原南皮河组岩性复杂，已经被刘本培等（１９９３）改为南皮河群。本文对原南皮河组上部地层进行了研究并命名为弄巴组，其时代为晚泥盆世末至早石炭世。通过抱粉相分析和野外沉积标志的观察以及对孢粉比较学的研究，从而获得了对该套地层沉积相和植物古地理方面的新认识。     

THE GREATER MIDDLE EAST AND REFORM IN THE BUSH ADMINISTRATION'S IDEOLOGICAL IMAGINATION

ABSTRACT. In pursuit of its foreign‐policy goals, the administration of President George W. Bush has attempted a dramatic reshaping of the vision of the Middle East in the American mind. References to the “new” or “greater” Middle East now include countries far outside traditional concepts of the region, including those in West Africa, Southeast Asia, and Central Asia. The administration argues that this region is defined not by cultural (Arab) or religious (Islam) characteristics but by a lack of democracy; hence a grand strategy is needed to execute reform. This article examines current U.S. efforts to achieve reform in the region, the components of the ideological construction of the New Middle East, the perceived role of Iraq, Turkey's potential role as a “model” for the region, and responses from the region to current U.S.‐led reform efforts.     

机载W波段毫米波辐射计扫描成像研究

通过机载试验 ,本文进行了W波段毫米波辐射计 (RADW92 )扫描成像研究 ,取得了黄河、渭河部分水域的微波辐射图像。试验结果表明 ,RADW92基本满足星载应用的要求。文中分析了影响图像质量的各种误差因素 ,并且提出了相应的解决方案。RADW92工作的中心频率为 92GHz ,带宽 2GHz ,积分时间 6 0ms ,系统灵敏度 0 6K ,线性度 0 999,天线为卡塞格伦 (Cassegrain)天线     

On the ore-forming conditions and ore-forming model of the superlarge multimetal deposit in Shizhuyuan

Eight favorable ore-forming conditions for the Shizhuyuan W-multimetal deposit are proposed. They are: (i) the geochemistry background special enriching the volatile and W and Sn ore-forming elements; (ii) the existence of melt-fluid system very rich in volatile and ore-forming elements; (iii) supply of sufficient ore-forming material and volatile multi-source; (iv) the infiltration and convection water source and driving force partly supplied by the Jurassic reservoir basin; (v) favorable tectonic conditions; (vi) ore-bearing greisen and vein superimposed in the pre-existing skarn rocks; (vii) favorable ore-transport and ore-concentration strata condition; (viii) there were a set of favorable ore-forming structures in Shizuyuan area; (ix) the orebody has good ore-reserve condition. Finally, ore-forming models are proposed. The paper is one of the achievements on the research related to the Climbing Project “The basic related to searching for the superlarge deposits supported by the State Science and Technology Commission. This research is also granted by the National Natural Science Foundation of China (Grant No. 49572134).     

The high-velocity molecular stream in W51B: a ring structure with compact H ii regions

We present ¹³ CO J  = 1 − 0 line observations of the H  ii region complex W51B located in the high-velocity (HV) stream. These observations reveal a filamentary and clumpy structure in the molecular gas. The mean local standard of rest (LSR) velocity ∼ + 65 km s⁻¹ of the molecular gas in this region is greater than the maximum velocities allowed by kinematic Galactic rotation curves. The size and mass of the molecular clouds are ∼ 48 × 17 pc² and ∼ 2.4 × 10⁵ M⊙ respectively. In a position–velocity diagram, molecular gas in the southern part comprises a redshifted ring structure with v _LSR=+ 60 to +73 km s⁻¹. The velocity gradient of this ring is ∼ 0.5 km s⁻¹ pc⁻¹, and the mass is ∼ 6.2 × 10⁴ M⊙. If we assume that the ring is expanding with a uniform velocity, the expansion velocity, radius and kinetic energy are ∼ 7 km s⁻¹, ∼ 13 pc and ∼ 3.0 × 10 ⁴⁹ erg respectively. The kinetic energy and mass spectrum of the ring could be explained by an expanding cylindrical cloud with a centrally condensed mass distribution. The locations of two compact H  ii regions, G49.0−0.3 and G48.9−0.3, coincide with the two molecular clumps in this ring. We discuss star formation, and the mechanism that produced the ring structure.