A method and results of color calibration for the Chang'e-3 terrain camera and panoramic camera

The terrain camera(TCAM) and panoramic camera(PCAM) are two of the major scientific payloads installed on the lander and rover of the Chang'e 3 mission respectively. They both use a Bayer color filter array covering CMOS sensor to capture color images of the Moon's surface. RGB values of the original images are related to these two kinds of cameras. There is an obvious color difference compared with human visual perception. This paper follows standards published by the International Commission on Illumination to establish a color correction model, designs the ground calibration experiment and obtains the color correction coefficient. The image quality has been significantly improved and there is no obvious color difference in the corrected images. Ground experimental results show that:(1) Compared with uncorrected images, the average color difference of TCAM is 4.30, which has been reduced by 62.1%.(2) The average color differences of the left and right cameras in PCAM are 4.14 and 4.16, which have been reduced by 68.3% and 67.6% respectively.     

Data processing for the Active Particle-induced X-ray Spectrometer and initial scientific results from Chang'e-3 mission

The Active Particle-induced X-ray Spectrometer(APXS) is an important payload mounted on the Yutu rover, which is part of the Chang'e-3 mission. The scientific objective of APXS is to perform in-situ analysis of the chemical composition of lunar soil and rock samples. The radioactive sources,55 Fe and109Cd, decay and produce α-particles and X-rays. When X-rays and α-particles interact with atoms in the surface material, they knock electrons out of their orbits, which release energy by emitting X-rays that can be measured by a silicon drift detector(SDD). The elements and their concentrations can be determined by analyzing their peak energies and intensities. APXS has analyzed both the calibration target and lunar soil once during the first lunar day and again during the second lunar day. The total detection time lasted about 266 min and more than 2000 frames of data records have been acquired. APXS has three operating modes: calibration mode, distance sensing mode and detection mode. In detection mode, work distance can be calculated from the X-ray counting rate collected by SDD. Correction for the effect of temperature has been performed to convert the channel number for each spectrum to X-ray energy. Dead time correction is used to eliminate the systematic error in quantifying the activity of an X-ray pulse in a sample and derive the real count rate. We report APXS data and initial results during the first and second lunar days for the Yutu rover. In this study, we analyze the data from the calibration target and lunar soil on the first lunar day. Seven major elements, including Mg, Al, Si, K, Ca, Ti and Fe, have been identified. Comparing the peak areas and ratios of calibration basalt and lunar soil the landing site was found to be depleted in K, and have lower Mg and Al but higher Ca, Ti, and Fe. In the future,we will obtain the elemental concentrations of lunar soil at the Chang'e-3 landing site using APXS data.     

地磁活动K指数自动计算FMI方法的改进

将Kp指数与国际地磁学与高空物理学协会(International Association of Geomagnetism and Aeronomy,下文简称IAGA)推荐的FMI方法(V1.0)计算的K值对比分析后发现,二者的差值在中国区域内出现"不同台站之间K1~K8两头离散、K值整体高出K_p约0.5个单位、个别日期S_R计算错误、相邻日期S_R频繁出现跨天台阶"现象.针对这些现象,分析了可能产生的原因,并对原FMI算法进行了四处改进.用改进后的FMI算法计算了全球8个台站、中国5个台站在2003-2005年和2009年共4年的K指数数据,并将计算结果分别与Kp指数以及这些台站用其他方法计算的K值进行一致性比较,发现改进后的计算结果与二者更为接近,说明本文对FMI方法的改进是有效的.     

LAMOST Medium-Resolution Spectral Survey of Galactic Nebulae(LAMOST MRS-N):An overview of scientific goals and survey plan

Since Sep.2018,LAMOST has started the medium-resolution(R～7500) spectral survey(MRS).We proposed the spectral survey of Galactic nebulae,including H Ⅱ regions,HH objects,supernova remnants,planetary nebulae and the special stars with MRS(LAMOST MRS-N).LAMOST MRS-N covers about 1700 square degrees of the northern Galactic plane within 40°l215° and-5° b5°.In this 5-year survey,we plan to observe about 500 thousand nebulae spectra.According to the commissioning observations,the nebulae spectra can provide precise radial velocity with uncertainty less than 1 km s~(-1).These high-precision spectral data are of great significance to our understanding of star formation and evolution.     

四川省生态旅游发展的层次与阶段

生态旅游是一项新的旅游活动、一项新的产业,是社会经济发展到一定阶段的产物。生态旅游的开发是一个循序渐进的过程,产业的发展存在着初级阶段、发展阶段和成熟阶段。结合四川社会经济发展水平和生态旅游资源分布规律,四川生态旅游形式应具有一定的时空特征,表现为时间上的阶段性和空间上的差异性,即在同一时期的不同地区或同一地区的不同发展阶段同时存在三种形式的生态旅游:泛生态旅游、准生态旅游、纯生态旅游。     

基于影象融合的干旱区城镇居民地信息提取研究

针对TM多波段图象中城镇居民地与裸地光谱特征相似难以准确提取城镇居民地信息的问题,利用雷达图象对居民地信息的敏感性,采用HIS变换方法,融合了2003年西安地区的Landsat TM和Radarsat SAR影象,并对融合影象做二类监督分类提取出城镇居民地信息,结果显示与TM图象监督分类相比,融合后的图象能很好地消除裸地对城镇居民地提取影响,其精度可达到84.21%,大大高于由TM多光谱影象监督分类所得到的精度71.79%,为提取干旱区城镇居民地信息提供一种新方法。     

山东荣成月湖潮汐汊道系统的沉积物平衡问题——兼论人类活动的影响

在月湖进行了沉积物采样和潮汐水文观测,分析计算了表层沉积物类型、泥沙输运率、现代沉积速率,讨论了月湖的沉积物平衡。结果显示,月湖的沉积速率较快。按目前的数据和资料估算,月湖每年的沉积通量约为(1.8~2.3)×10⁴ t,而正常情况下的沉积物供应量每年只有(0.5~1.2)×10⁴ t。研究表明,人类活动还改变了月湖的物理与生态过程。由于土地利用的方式及其强度发生了变化,月湖汇水盆地的侵蚀量大为增加,侵蚀模数可能远大于400 t/(km²·a),从而使流域侵蚀量大大超出了正常范围,加剧了月湖的淤积。     

日本沼虾(Macrobrachium nipponensis)池养越冬抱卵亲虾表型性状对个体繁殖力的影响效应

采用多元分析方法定量研究了日本沼虾池养越冬抱卵亲虾体重(BW)、净重(NW)、体长(BL)、头胸甲长(CL)、胸宽(CW)、胸高(CH)、腹节长(AL)、额剑长(RL)、尾节长(TL)等11项表型性状对其个体繁殖力的影响效应。结果表明:(1)实验对象所测各表型性状间均呈极显著相关(P<0.01),它们在对个体繁殖力各评价指标的影响上具较好的区分度;(2)影响个体绝对繁殖力(FJ)、体重相对繁殖力(FW)和体长相对繁殖力(FL)的关键表型性状及其直接作用强弱排序分别为BW>BL>CH>RL>AL>NW,BW>CL>RL>CH>TL>NW和BW>CL>CH>RL>NW,相关指数依次为0.810、0.621和0.798,其中BW-NW组合和CH-RL组合分别为决定个体繁殖力的核心变量和公共从属变量;(3)适用于估算个体繁殖力的回归方程分别为:FJ=5087.802BW-6599.877NW+200.927CH+114.774RL+211.878BL-154.965AL-6266.840,FW=1140.538BW-2018.663NW+85.217CH+70.852RL+78.694CL+74.623TL-1152.576,FL=105.453BW-134.613NW+4.307CH+2.709RL+3.623CL-61.737;(4)W(♀)=0.029BL+0.065CL+0.121CW+0.105CH-2.448可精确估算其净重值。     

Late Jurassic I-type rhyolites from the Duobuza region,north-central Tibet: evidence for the occurrence of juvenile lower crust and crustal growth in the Southern Qiangtang Terrane

ABSTRACT

Previous studies of the Southern Qiangtang (SQ) Terrane in Tibet have shown significant growth of continental crust during the late Mesozoic (ca. 170–120 Ma) through underplating of mantle-derived melts beneath ancient lower crust. However, the mechanism of crustal growth remains defective during the Late Jurassic. In this contribution, we report new zircon U–Pb ages, whole-rock major and trace element concentrations, and zircon Hf isotopic compositions of Late Jurassic rhyolites from the Duobuza area in the SQ Terrane. Zircon LA–ICP–MS U–Pb dating yields concordant ages and weighted mean ²⁰⁶Pb/²³⁸U ages of 151–149 Ma, indicating that the rhyolites were erupted during the Late Jurassic. The rhyolite samples yield high SiO₂ (69.1–73.4 wt.%) and Na₂O (3.82–6.49 wt.%) concentrations, high values of the differentiation index (95.4–98.5), moderate Al₂O₃ (13.1–15.5 wt.%) and K₂O (2.55–3.26 wt.%) concentrations, and relatively low TiO₂ (0.34–0.44 wt.%), MgO (0.14–0.67 wt.%), and MnO (0.01–0.10 wt.%) concentrations and Mg# values (8.9–33.5). They are enriched in Rb, Th, Ba, and Pb, depleted in Nb, Ta, Sr, Ti, and P, and yield negative Eu anomalies. These characteristics suggest that the Duobuza rhyolites represent medium- to high-K calc-alkaline, highly fractionated I-type granitoids. Variations in major and trace element concentrations indicate that the rhyolites underwent significant fractionation of Fe–Ti oxides, plagioclase, K-feldspar, hornblende, biotite, and apatite. The samples yield positive zircon ε_Hf(t) values (+0.08 to +10.9) and young T^CD _M model ages (816–386 Ma), indicating that they were generated through partial melting of juvenile lower crust of the SQ Terrane. These data are distinct from those of Late Jurassic intermediate–felsic plutons in the SQ Terrane that generally yield negative ε_Hf(t) values and ancient T_C ^DM model ages. We suggest that the occurrence of the Duobuza rhyolites is the significant witness. The presence of juvenile lower crust beneath the SQ Terrane during the Late Jurassic (ca. 150 Ma) rather than during the Early Cretaceous (ca. 120Ma). The transition from ancient to juvenile lower crust has already began in the SQ Terrane during the Late Jurassic.     

建立潮汐汊道P-A关系的沉积动力学方法

在均衡状态下，潮汐汉道系统的纳潮量(P)与口门面积(A)之间存在着较稳定的关系，通常用幂函数形式来表达。计算P-A关系的传统O’Brien方法因其统计性质无法给出单一潮汐汉道的P-A关系。根据沉积动力学原理，每个潮汐汉道的P-A关系都受涨落潮历时、断面平均流速、口门形态、纳潮量、淡水径流量、沿岸毛输沙量和沉积物粒度等因素的控制，对上述因素的每一种组合，都有对应的均衡态P-A关系。作者在前人工作的基础上，尝试着建立了计算单一潮汐汊道P-A关系的沉积动力学方法，并以山东半岛月湖为算例对该方法的应用进行了讨论。结果表明，均衡态潮汐汉道的P-A关系的指数n稳定在1．15左右，而系统C的变化较大。