一种适用于低空影像的数字表面模型自动获取方法

无人飞行器系统获取的低空影像数据往往倾角大、像幅小且重叠度不规则,同时在灰度与比例尺上可能不一致.针对其特点,提出了一种适用于低空影像的数字表面模型自动获取方法.首先,采用影像水平纠正、构建金字塔、Wallis滤波以及Harris特征提取等方法对低空影像进行匹配预处理;然后,对经预处理的多级影像采取由粗到精的匹配,再基于低空影像高重叠度的特点进行三视检核以剔除误匹配点;最后采用近邻内插生成规则格网的数字表面模型.试验表明,该方法有效可行,生成的数字表面模型产品精度较高,对于改进现有的生产流程具有一定的实际意义.     

Classification of 24 New Ordinary Chondrites from the Grove Mountains, Antarctica

Petrography and mineral chemistry of 24 ordinary chondrites from the Grove Mountains, Antarctica, have been studied in order to identify their chemical-petrographic types. These samples were selected from a total of 4448 Grove Mountains (GRV) meteorites collected during the 19th Chinese Antarctic Research Expedition so as to make an estimation of the large GRV meteorite collection. The chemical-petrographic types of these meteorites are presented below: 1 H3,2 H4, 4 H5, 2 H6, 1 L4, 7 L5, 5 L6, 1 LL4 and 1 LL6. The new data weaken the previous report that unequilibrated ordinary chondrites are unusually abundant in the Grove Mountains region. However, this work confirms significant differences in distribution patterns of chemical-petrographic types between the Grove Mountains and other     

The unification of RBLs with XBLs

Many astronomers have discussed the property of BL Lacertae objects, including the variation of spectrum, the correlation of multi-wave bands and the property of polarization, which could give good information for studying intrinsic correlation of components and position of BL Lacertae objects. In the paper, we investigated the properties of RBLs and XBLs and RBLs/XBLs (these objects can also be found by radio survey as by X-ray survey). Firstly, we collected the light curve of 28 BL Lacertae objects, and gained their short timescales by Structure Function (SF). Secondly, we analyzed the distribution of the short timescales of some BL Lacertae objects, including 28 objects’ timescales calculated by SF, as well as the distribution of the redshift and the black hole mass and the flux densities of the multi-wavebands (radio, near-infrared, optical and Gamma-ray). Based on statistical analysis, the result of the paper support the unification model of RBLs and XBLs.     

Variability Study of the SX Phoenicis Star BL Camelopardalis

New time-series photometric observations of BL Cam in the V band and white light were made during 2005 to 2007 at the Xinglong Station of China. The frequency analysis confirms two closely separated frequencies, 25.181 d-1 and 25.571 d-1, but the frequency of 31-32 d-1 reported in the literature was not detected in the new data. New times of maximum light were determined from both our light curves and those available on Internet, allowing a more comprehensive study of the O - C diagram, together with the times of maximum light in the literature. A new interpretation, including the period increasing before 1988 and decreasing since 1992 of BL Cam and the light-time effect in a binary system, looks plausible.     

Formation of Transient Coronal Holes during the Eruption of a Quiescent Filament and its Overlying Sigmoid

By using Hα, He I 10830, EUV and soft X-ray (SXR) data, we examined a filament eruption that occurred on a quiet-sun region near the center of the solar disk on 2006 January 12, which disturbed a sigmoid overlying the filament channel observed by the GOES-12 SXR Imager (SXI), and led to the eruption of the sigmoid. The event was associated with a partial halo coronal mass ejection (CME) observed by the Large Angle and Spectrometric Coronagraphs (LASCO) on board the Solar and Heliospheric Observatory (SOHO), and resulted in the formation of two flare-like ribbons, post-eruption coronal loops, and two transient coronal holes (TCHs), but there were no significantly recorded GOES or Hα flares corresponding to the eruption. The two TCHs were dominated by opposite magnetic polarities and were located on the two ends of the eruptive sigmoid. They showed similar locations and shapes in He Ⅰ 10830, EUV and SXR observations. During the early eruption phase, brightenings first appeared on the locations of the two subsequent TCHs, which could be clearly identified on He Ⅰ 10830, EUV and SXR images. This eruption could be explained by the magnetic flux rope model, and the two TCHs were likely to be the feet of the flux rope.     

异地异构天文数据资源的统一访问

天文观测数据资源具有时间跨度大,数据量大,存储、管理分散,管理工具驳杂等特点.如何提供给天文学家一个统一访问这些异地存放的异构数据资源的方案,是虚拟天文台的一个重要研究课题.本文提出了一种基于网格的解决方案.我们基于OGSA-DAI技术实现了对天文星表数据,图像数据和光谱数据的封装(DataNode).我们设计的虚拟天文台数据访问服务(VO-DAS)实现了对DataNode的自动资源发现以及异地异构数据库的联合访问.这将使天体的多波段交叉证认成为可能.VO-DAS支持国际虚拟天文台联盟(IVOA)的各项相关标准,使得它具有良好的互操作性.它的对外接口简单实用,可以针对不同需求的天文数据用户发展出多种网格应用产品.通过在两个科学范例中应用VO-DAS服务,证明了它的可行性.     

基于Albedo-NDVI特征空间的玛曲县荒漠化时空动态监测

开展荒漠化时空动态监测是荒漠化防治的一项重要基础工作。以地处青藏高原东北缘的甘肃省玛曲县为例,以该县2001年、2005年、2010年的TM影像和2015年的HJ-1影像为数据来源,利用Albedo-NDVI特征空间法,从整体到局部,分别对该县全区域及其黄河沿岸地区不同尺度区域近15年的土地荒漠化进行了监测和时空动态分析。研究结果表明：Albedo-NDVI特征空间法能便捷、有效、精确地对荒漠化信息进行提取和分级,有利于荒漠化的定量分析与监测;玛曲县近15年来实施的生态恢复工程效果显著,该县荒漠化状况有所改善,荒漠化土地的面积持续减小,程度不断降低,主要发生“轻度荒漠化土地向非荒漠化土地”的转移;但是由于沙源丰富、人口密集以及过度放牧等原因,玛曲县黄河沿岸5 km带状区域荒漠化以“非荒漠化土地向轻度荒漠化土地”转移为主,荒漠化状况较全县整体水平严重,并且仍有不断恶化的趋势。     

中阿尔金南缘志留纪高压泥质片麻岩的发现及其构造地质意义

在中阿尔金南缘西段尤努斯萨依北部原划长城系巴什库尔干岩群中首次发现一套高压泥质片麻岩。根据岩相学观察和矿物化学成分可识别出其四期矿物共生组合:早期为石榴子石+多硅白云母+单斜辉石(?)+斜长石+黑云母+石英+金红石+钛铁矿;第二期为石榴子石+蓝晶石+钾长石+斜长石+黑云母+石英+金红石+钛铁矿;第三期为石榴子石+夕线石+钾长石+斜长石+黑云母+石英+金红石+钛铁矿;晚期为石榴子石+夕线石+斜长石+黑云母+石英+钛铁矿。依据矿物内部一致性热力学数据,基于THERMOCALC 3. 40程序平台,计算出P-T视剖面图,并结合矿物等值线、矿物对温压计等计算,依次确定四期变质温压条件为15. 8～18. 3kbar/646～729℃、10. 30～12. 30kbar/781～821℃、8. 50～9. 60kbar/812～838℃和4. 65～5. 70kbar/698～725℃。上述四期变质阶段共同构成一个早期降压升温后降压降温的顺时针型演化的P-T轨迹,指示出与陆壳俯冲-折返相关的变质地质事件。利用LA-ICP-MS进行的锆石原位微区U-Pb定年和微量元素分析结果表明,该岩石记录了432. 0±2. 7Ma、401. 4±2. 5Ma和381. 1±2. 4Ma三期变质年龄,可能分别代表了该岩石早期高压、中期高压麻粒岩相-麻粒岩相和后期角闪岩相变质阶段的时代。该高压岩石出露于中阿尔金地块西段南缘长城系巴什库尔干岩群之中,与南侧以断裂带分隔的赋存于阿尔金岩群之中的南阿尔金高压-超高压岩石出露的构造位置明显不同,其峰期变质时代(～432Ma)亦明显不同于南阿尔金高压-超高压岩石的峰期变质时代(～500Ma)。因此,该高压岩石与南阿尔金高压-超高压岩石显然不能构成同一条变质岩带。结合区域地质背景和前人关于柴北缘陆壳属性高压-超高压岩石峰期变质时代(～430Ma)的研究成果综合分析,本文初步认为该高压岩石可能是柴北缘高压-超高压变质岩带的西延或是被中新生代以来阿尔金复杂多期次走滑断裂系迁移而就位于中阿尔金南缘的部分柴北缘高压-超高压变质岩片/岩块。     

1979-2016年我国东北地区空中水汽状况及变化趋势分析

水汽是形成云和降水的物质基础,与全球水分循环和能量平衡密切相关,对天气和气候具有重要影响。基于NCEP/NCAR月值再分析资料,综合分析我国东北地区上空不同高度层位比湿的气候学特征和长期趋势变化,同时分析了整层积分水汽通量的季节变化。结果表明：东北地区空中水汽集中分布于500 hPa以下,1979年至20世纪末低层比湿呈增加趋势,2000年后转为缓慢下降,但2012年以来波动回升。此外,东北地区比湿及水汽通量季节差异明显,夏季水汽含量最多,冬季最少,秋季多于春季;东北地区水汽含量最大值出现于7月,最低值出现在每年12月至次年1月。水汽来源受东亚季风系统影响明显,夏季水汽源地主要为南海,渤海和黄海对东北地区夏季水汽也有一定贡献;其他季节水汽主要来源于西风带输送。     

中东地区阿普特阶Shuaiba组碳酸盐岩沉积体系特征及模式探究

中东地区主力产油层系Shuaiba组的勘探及研究逐渐以地层岩性圈闭为主,笔者通过总结Bab盆地阿普特阶Shuaiba组沉积相类型,多油田地层格架及空间展布特征的对比,为系统恢复Shuaiba组沉积演化过程及模式提供地质依据。研究表明,阿普特阶Shuaiba组共发育开阔台地、台地边缘、台缘斜坡及盆地相4种沉积相单元和6种亚相类型,各相带单元受控于四个三级层序且沿Bab盆地周缘呈带状展布。开阔台地一侧,主要沉积了第二个三级层序对应的Lower Shuaiba地层;台地边缘往Bab台内盆地区域,则以第三和第四个三级层序对应的Upper Shuaiba地层为主。Shuaiba组生物礁、滩建造集中发育在第二个三级层序的高位域阶段,滩间海、缓坡及盆地相受控于海进和低位体系域。阿普特阶Shuaiba台地边缘生物建隆、台内浅滩在空间上相互叠置并成带展布,符合弱镶边型缓坡台地沉积模式,该类型台地具备深水陆棚性质的非常宽缓的斜坡,且缓坡往盆地一侧发育一个镶边台地边缘。