Reconstructing the landing trajectory of the CE-3 lunar probe by using images from the landing camera

An accurate determination of the landing trajectory of Chang'e-3(CE-3)is significant for verifying orbital control strategy, optimizing orbital planning, accurately determining the landing site of CE-3 and analyzing the geological background of the landing site. Due to complexities involved in the landing process, there are some differences between the planned trajectory and the actual trajectory of CE-3. The landing camera on CE-3 recorded a sequence of the landing process with a frequency of 10 frames per second. These images recorded by the landing camera and high-resolution images of the lunar surface are utilized to calculate the position of the probe, so as to reconstruct its precise trajectory. This paper proposes using the method of trajectory reconstruction by Single Image Space Resection to make a detailed study of the hovering stage at a height of 100 m above the lunar surface. Analysis of the data shows that the closer CE-3 came to the lunar surface, the higher the spatial resolution of images that were acquired became, and the more accurately the horizontal and vertical position of CE-3 could be determined. The horizontal and vertical accuracies were7.09 m and 4.27 m respectively during the hovering stage at a height of 100.02 m. The reconstructed trajectory can reflect the change in CE-3's position during the powered descent process. A slight movement in CE-3 during the hovering stage is also clearly demonstrated. These results will provide a basis for analysis of orbit control strategy,and it will be conducive to adjustment and optimization of orbit control strategy in follow-up missions.     

Data preprocessing and preliminary results of the Moon-based Ultraviolet Telescope on the CE-3 lander

The Moon-based Ultraviolet Telescope(MUVT) is one of the payloads on the Chang'e-3(CE-3) lunar lander. Because of the advantages of having no atmospheric disturbances and the slow rotation of the Moon, we can make long-term continuous observations of a series of important celestial objects in the near ultraviolet band(245～340 nm), and perform a sky survey of selected areas, which cannot be completed on Earth. We can find characteristic changes in celestial brightness with time by analyzing image data from the MUVT, and deduce the radiation mechanism and physical properties of these celestial objects after comparing with a physical model. In order to explain the scientific purposes of MUVT, this article analyzes the preprocessing of MUVT image data and makes a preliminary evaluation of data quality. The results demonstrate that the methods used for data collection and preprocessing are effective, and the Level 2A and 2B image data satisfy the requirements of follow-up scientific researches.     

Scientific data products and the data pre-processing subsystem of the Chang'e-3 mission

The Chang'e-3(CE-3) mission is China's first exploration mission on the surface of the Moon that uses a lander and a rover. Eight instruments that form the scientific payloads have the following objectives:(1) investigate the morphological features and geological structures at the landing site;(2) integrated in-situ analysis of minerals and chemical compositions;(3) integrated exploration of the structure of the lunar interior;(4) exploration of the lunar-terrestrial space environment, lunar surface environment and acquire Moon-based ultraviolet astronomical observations. The Ground Research and Application System(GRAS) is in charge of data acquisition and pre-processing, management of the payload in orbit, and managing the data products and their applications. The Data Pre-processing Subsystem(DPS) is a part of GRAS.The task of DPS is the pre-processing of raw data from the eight instruments that are part of CE-3, including channel processing, unpacking, package sorting, calibration and correction, identification of geographical location, calculation of probe azimuth angle, probe zenith angle, solar azimuth angle, and solar zenith angle and so on, and conducting quality checks. These processes produce Level 0, Level 1 and Level 2data. The computing platform of this subsystem is comprised of a high-performance computing cluster, including a real-time subsystem used for processing Level 0 data and a post-time subsystem for generating Level 1 and Level 2 data. This paper describes the CE-3 data pre-processing method, the data pre-processing subsystem, data classification, data validity and data products that are used for scientific studies.     

基于BFGS法融合InSAR和GPS技术监测地表三维形变

虽然InSAR技术具有高精度、大范围和高空间分辨率等优点,但只能监测雷达视线方向上的一维地表形变;而GPS技术虽可以监测地表的三维形变,但其空间分辨率很低.本文针对融合InSAR和GPS技术监测地表高空间分辨率三维形变展开研究.首先证明了简单的局部最优化迭代算法就能求得综合InSAR和GPS监测地表形变速率的能量函数模型的全局最优估值.随后提出了利用BFGS局部最优算法反演最优的地表三维形变速率.该方法既能避免全局最优化算法计算复杂且难以收敛的问题,又能克服传统的解析法中数值计算不稳定的缺点.最后,通过模拟实验和美国南加州真实数据实验表明,该方法能够得到高精度的地表三维形变速率场.而且当观测或插值误差导致解析法误差较大时,BFGS方法仍能得到高精度、稳定的全局最优解.     

SAR偏移量跟踪技术估计天山南依内里切克冰川运动

流动性是冰川的一个主要特征,监测其流速变化可以为冰川物质平衡和冰川灾害研究提供重要信息.本文研究利用2007-2008年的7景ALOS/PALSAR影像和偏移量跟踪技术提取亚洲最大的山岳冰川之一--南伊内里切克冰川的运动场.ALOS/PALSAR影像的时间连续性和南伊内里切克冰川的冰碛覆盖为SAR偏移量跟踪技术获取连续的冰川表面流速提供了基础,然而冰川积累区降雪、附加冰带消融、陡坡区域裂缝发育等客观事件的发生对速度的获取仍有局部影响.尽管如此,本文仍得到了整个冰川不同季节的平面运动场,并且在所有6个时间段内观测到的运动场非常吻合.详细地分析揭示南伊内里切克冰川运动具备以下规律:流速由轴部向两侧递减,由源头向下至雪线处运动速度逐渐增加,然后再向末端逐渐递减;流速大小和坡度大小呈非线性正相关,坡度从1°突变至16°时,冰川运动加速会导致裂缝发育;夏季受冰川湖影响,尾部分支流速能激增至96 cm/d;暖季速度会高于寒季5～10 cm/d.该冰川的冰舌主体日平均速度为20～50 cm/d,局部最高速度可以达到65 cm/d.在冰舌上提取了一些样点的速度作统计,结果显示各个时段中所有样点的平均速度最高可达33.3 cm/d,最低可至27.9 cm/d.冰舌部分的速度和2004年的数据相比下降了约5 cm/d.     

地基观测的夜侧极光对行星际激波的响应

行星际激波与地球磁层相互作用通常会导致日侧极光活动增强,随后沿着极光卵的晨昏两侧向夜侧扩展的激波极光.行星际激波也可能直接导致夜侧扇区极光活动增强,甚至沉降粒子能通量的数量级可以与典型亚暴相比拟.本文首次利用我国南极中山站和北极黄河站连续多年积累的极光观测数据,对行星际激波与地球磁层相互作用期间地面台站在夜侧扇区(18—06MLT)观测的极光响应进行了分析.对18个极光观测事件的分析结果表明:行星际激波与磁层相互作用可以在夜侧触发极光爆发和极光微弱增强或静态无变化事件;太阳风-磁层能量耦合的效率以及磁层空间的稳定性决定着行星际激波能否触发极光爆发.     

Coesite-bearing eclogite breccia: implication for coseismic ultrahigh-pressure metamorphism and the rate of the process

A coesite-bearing eclogite breccia is reported here for the first time at Yangkou in the Chinese Su–Lu ultrahigh-pressure (UHP) metamorphic belt. It is thrusted over a coesite-bearing coronitic eclogite and is gradational to a foliated eclogite at the contact. The coronitic eclogite is characterized by garnet coronas between fine-grained high-pressure mineral aggregates forming pseudomorphs after plagioclase, ilmenite, biotite, and pyroxene in a gabbroic protolith. The breccia consists of fine-grained cataclastic eclogite fragments (garnet + omphacite + coesite/quartz ± phengite ± kyanite) and a coarser-grained matrix schist (garnet + quartz + phengite + kyanite). The foliated eclogite consists of intercalating bands of the cataclastic eclogite and a schist similar to the fragments and the matrix, respectively, in the breccia. The igneous fabric of the eclogitized gabbro is increasingly obliterated from the coronitic eclogite through the foliated eclogite to the breccia. Micropoikilitic amoeboid garnet containing numerous inclusions of omphacite and other high-pressure minerals is characteristic of eclogite facies pseudotachylytes and suggests flash melting and rapid crystallization. In the breccia and foliated eclogite, quartz + K-feldspar ± albite aggregates are included in garnet or form strings cutting across the cataclasites. In some aggregates, quartz grains are cemented by K-feldspar and vesicular albite, also implying crystallization from melts in a rapid cooling and decompression process from the UHP condition. The field context, the locally preserved igneous fabric in the breccia, the similar whole-rock compositions, as well as the complementary mineral assemblages in the fragments and the matrix with respect to the coronitic eclogite, suggest that the breccia was formed by cataclasis and segregation of minerals in a former coronitic eclogite in response to a sudden pressure release. Intergranular coesite is found only in the eclogite cataclasites and may have survived via the rapid cooling event, as coesite converts to quartz completely in a few years when being cooled slowly at lower pressures. Such rate information is incompatible with the presumed deep subduction/exhumation process but implies transient UHP metamorphism coeval with the seismic event.     

大地水准面异常在湖南地区的地球物理解释

以湖南地区为例,利用超高阶地球重力位模型EGM2008计算了研究区的重力大地水准面,并采用棱柱体公式和球体公式相结合的方法分别进行了完全地形改正和Airy-Heiskanen局部均衡改正,得到布格大地水准面和均衡大地水准面.对三种大地水准面进行不同波长分量的分离处理,得到包含不同深度异常信息的剩余大地水准面,并结合其他地球物理资料对研究区进行了详细的地球物理解释.结果表明,剩余重力大地水准面可以有效地反映出研究区内的深部构造特征,如深大断裂带分布、构造块体位置、上地幔密度横向分布等,但对地壳内异常结构反映不明显;研究区岩石圈密度变化相对平缓,厚度由东向西增加;根据剩余均衡大地水准面及研究区Airy局部均衡莫霍面,可以大致推测出研究区的莫霍面起伏形态以及均衡状态,可作为一种有用的参考信息.     

基于实时精密单点定位技术的暴雨短临预报

提出了一种将实时精密单点定位(Precise Point Positioning, PPP)技术用于暴雨短临预报的新方法.该方法首先基于GPS连续运行参考站网(Continuously Operating Reference Stations, CORS)实时估计的精密卫星钟差完成PPP解算,再以实时获取的对流层延迟(Zenith Tropospheric Delay, ZTD)及其增量变化为依据进行暴雨短临预报.研究结果表明:一般雷暴天气来临之前的2~6 h,ZTD增量表现为先后突破±5 mm/5 min,且后续记录到的实际降水量大小与ZTD维持在高水平阶段的时间长短有较好的对应关系;就热带气旋而言,在强风作用下,ZTD增量变化表现的异常活跃和复杂,规律性较弱,但对短临预报强降雨仍有一定的指示作用.     

Experimental Studies of Sound Attenuation in Seabed Sediments on Column Sample Length Scale

Seabed sediment microstructure has an influence on its acousto-physical properties, and the properties in a length of the sediment column reflect an aspect of the macroscopic behavior of the microstructure. An original measurement method of the sound attenuation within small distance cross sections in a sediment column, and the corresponding approach in data processing to attain an attenuation factor are detailed in the paper. This method was used to measure the compressional wave in series of points with a small distance in the sediment column, and it is shown that exponential attenuation is a type of compressional wave attenuation model for a sediment column in its full length. It indicates that there are various models of compressional wave attenuation in seabed sediments in the South China Sea after comparison of data from other literature. The method of measuring sound attenuation satisfies the sampling space interval in the acoustical forward and inverse problems in seabed sediments, and the original method provides a new approach for finding out sound attenuation mechanism in seabed sediments on small length scale.