我国低钛月海型模拟月壤初始物质选择的地球化学依据

以Apollo14月壤样品和美国JSC-1模拟月壤的地球化学特征为基础,结合我国低钛玄武岩火山的分布,对我国不同地区新生代玄武岩的化学成分、年龄、储量等方面进行对比分析结果表明,滇西北金沙江地区和吉林辉南红旗林场-四海地区的玄武质火山喷发物的化学成分与Apollo14月壤样品和美国JSC-1模拟月壤相似,比较适合用于我国低钛月海玄武岩模拟月壤研制的初始物质。野外地质调查发现,吉林省辉南县金川镇红旗林场—四海一带产出的玄武质火山渣为距今1600 a的该玄武质火山岩的喷发物,其储量大、质地纯、粒度均匀,而且比滇西北金沙江地区最近一期的玄武质火山渣新鲜,最适合作为我国低钛月海玄武岩模拟月壤研制的初始物质。     

NEAR-FAULT DISPLACEMENT AND DEFORMATION OBTAINED FROM ONE-KILOMETER-LONG FAULT-CROSSING BASELINE MEASUREMENTS-A PRELIMINARY EXPERIMENT AT 2 SITES ON THE EASTERN BOUNDARY OF THE SICHUAN-YUNNAN BLOCK

The current and conventional fault-crossing short baseline measurement has a relatively high precision, but its measurement arrays usually fail to or cannot completely span major active fault zones due to the short length of the baselines, which are only tens to 100 meters. GNSS measurement has relatively low resolution on near-fault deformation and hence is not suitable for monitoring those faults with low motion and deformation rates, due to sparse stations and relatively low accuracy of the GNSS observation. We recently built up two experimental sites on the eastern boundary of the active Sichuan-Yunnan block, one crossing the Daqing section of the Zemuhe Fault and the other crossing the Longshu section of the Zhaotong Fault, aiming to test the measurement of near-fault motion and deformation by using fault-crossing arrays of one-kilometer-long baselines. In this paper, from a three-year-long data set we firstly introduce the selection of the sites and the methods of the measurement. We then calculate and analyze the near-field displacement and strain of the two sites by using three hypothetical models, the rigid body, elastic and composed models, proposed by previous researchers. In the rigid body model, we assume that an observed fault is located between two rigid blocks and the observed variances in baseline lengths result from the relative motion of the blocks. In the elastic model, we assume that a fault deforms uniformly within the fault zone over which a baseline array spans, and in the array baselines in different directions may play roles as strainmeters whose observations allow us to calculate three components of near-fault horizontal strain. In the composed model, we assume that both displacement and strain are accumulated within the fault zone that a baseline array spans, and both contribute to the observed variances in baseline lengths. Our results show that, from the rigid body model, variations in horizontal fault-parallel displacement component of the Zemuhe Fault at the Daqing site fluctuate within 3mm without obvious tendencies. The displacement variation in the fault-normal component keeps dropping in 2015 and 2016 with a cumulative decrease of 6mm, reflecting transverse horizontal compression, and it turns to rise slightly(suggesting extension)in 2017. From the elastic model, the variation in horizontal fault-normal strain component of the fault at Daqing shows mainly compression, with an annual variation close to 10^-5, and variations in the other two strain components are at the order of 10^-6. For the Longshu Fault, the rigid-body displacement of the fault varies totally within a few millimeters, but shows a dextral strike-slip tendency that is consistent with the fault motion known from geological investigation, and the observed dextral-slip rate is about 0.7mm/a on average. The fault-parallel strain component of the Longshu Fault is compressional within 2×10^-6, and the fault-normal strain component is mainly extensional. Restricted by the assumption of rigid-body model, we have to ignore homolateral deformation on either side of an observed fault and attribute such deformation to the fault displacement, resulting in an upper limit estimate of the fault displacement. The elastic model emphasizes more the deformation on an observed fault zone and may give us information about localizations of near-fault strain. The results of the two sites from the composed model suggest that it needs caution when using this model due to that big uncertainty would be introduced in solving relevant equations. Level surveying has also been carried out at the meantime at the two sites. The leveling series of the Daqing site fluctuates within 4mm and shows no tendency, meaning little vertical component of fault motion has been observed at this site; while, from the rigid-body model, the fault-normal motion shows transverse-horizontal compression of up to 6mm, indicating that the motion of the Zemuhe Fault at Daqing is dominantly horizontal. The leveling series of the Longshu site shows a variation with amplitude comparable with that observed from the baseline series here, suggesting a minor component of thrust faulting; while the baseline series of the same site do not present tendencies of fault-normal displacement. Since the steep-dip faults at the two sites are dominantly strike-slip in geological time scale, we ignore probable vertical movement temporarily. In addition, lengths of homolateral baselines on either side of the faults change somewhat over time, and this makes us consider the existence of minor faults on either side of the main faults. These probable minor faults may not reach to the surface and have not been identified through geological mapping; they might result in the observed variances in lengths of homolateral baselines, fortunately such variations are small relative to those in fault-crossing baselines. In summary, the fault-crossing measurement using arrays with one-kilometer-long baselines provides us information about near-fault movement and strain, and has a slightly higher resolution relative to current GNSS observation at similar time and space scales, and therefore this geodetic technology will be used until GNSS networks with dense near-fault stations are available in the future.     

PG激变星候选天体的光变曲线

我们于1989年用北京天文台兴隆观测站的60/90/180厘米施密特望远镜及Thomson红敏CCD对14个PG候选激变变星进行光度观测.其光变曲线特性表明:PG0027+260,PG0818+513,和PC1030+590为激变食变星,PG1341—079 是一个可能的激变食变星,PG1551+719为SU UM_a型矮新星,此外还有6个天体的光变曲线有激变星特有的闪变特征.因此PG样本中,激变变星的成功率为79％.PG1030+590的轨道周期为3~h279,PG1717+413的闪变变幅在二个月内有明显变化,它与本身的亮度无明显相关,说明闪变变幅的变化可能是亮斑的局部效应.     

青藏高原多年冻土微生物的培养和计数

以青藏高原腹地北麓河流域的两个6m钻孔为对象,对多年冻土中保存的微生物进行初步培养和总数测定,并分析了微生物与土壤环境之间的关系.结果表明,两个钻孔中可以培养的微生物数目在3.6×10⁶～5.0×10²之间;随着深度增加,冻土年代递增,可以培养的数目显著减少.表层冻土属于季节冻土,可培养的微生物种群较多.总的土壤微生物数目(包括可以培养和不能培养的微生物)随深度递减,两个孔在3.8×10⁹～1.0×10⁷之间.相关性分析表明,土壤中可以培养的微生物以及总的微生物与土壤的pH值、电导率、总有机质和全氮没有显著的相关关系,而与土壤深度关系密切.两个钻孔间的地表植被虽然差异明显,但从可培养的微生物数量和土壤微生物总数比较看来,两孔间没有明显的不同.     

浅谈地理国情普查项目中控制点库的制作

数字正射影像数据是地理国情普查中主要的调查数据源,同时也是普查成果数据的重要组成部分。而控制点作为数字正射影像制作的基础数据也是普查成果中必不可少的一部分。本文就国情普查成果中影像控制点的采集与整理进行了探讨。     

雅鲁藏布江蛇绿岩中地幔柱型岩浆作用——来自氦、氩同位素的证据

雅鲁藏布江蛇绿岩的氦、氩同位素组成分别是：蛇绿岩中变质橄榄岩的^3He/^4He比值为1．104-3．384Ra,平均为2．383Ra;玄武岩的He同位素组成比较均一,^3He/^4He平均值为5．359 Ra;辉绿岩的^3He／^4He比值变化较大,为1—5Ra。由于各岩石样品有不同程度的蚀变,造成放射性成因He的加入,因此大多数样品He同位素组成比低于亏损地幔大洋中脊玄武岩的值(MORB≈8Ra),不能真实反映源区特征。而采自吉定的辉绿岩样品^3He/^4He比值平均高达31．57Ra,与夏威夷发现的热点地幔源区的样品比值接近;分步加热法进一步测试,其高比值的He是在低温区段释放的。这种高^3He/^4He比值He的捕获,表明雅鲁藏布江蛇绿岩形成时存在地幔柱型富集地幔岩浆作用。     

新疆西准噶尔红山岩体及其中闪长质岩墙的时代——来自锆石LA-ICP-MS定年的证据

作为一种特殊产状的岩浆岩,岩墙保存有岩浆活动和地球动力学背景等方面的重要信息。为了研究和探讨西准噶尔乃至中亚地区古生代晚期的地球动力学环境,我们对西准噶尔地区侵入花岗岩的暗色岩墙开展了卫星遥感影像解译、地表地质调查和相关室内研究工作。研究发现,新疆西准噶尔红山花岗岩体中发育大量环状和非环状闪长岩岩墙。环状岩墙从中心到外围,岩墙宽度逐渐变窄,矿物粒度也逐渐变细;非环状岩墙切割环状岩墙,宽度和矿物粒度都没有明显变化。为了确定这些岩墙的形成时代,对3个环状岩墙样品、2个非环状岩墙和1个花岗岩样品进行了锆石LA-ICP-MSU-Pb定年,得到环状岩墙的年龄为:304±1Ma、302±1Ma、303±1Ma;非环状岩墙的年龄为:302±1Ma、302±1Ma;花岗岩的年龄为304±1Ma。结合不同类型岩墙及其与岩体的穿切关系,确定红山岩体的形成时代为304Ma左右,环状岩墙的形成时代为303Ma左右,非环状岩墙的形成时代为302Ma左右。这一年代学研究成果揭示出西准噶尔地区在石炭纪末期发育不同类型的岩浆活动,闪长质岩墙所占据的裂隙是在石炭纪末期形成的;为从岩浆活动和由这些岩墙所占据的裂隙研究,探讨该区古生代晚期的地球动力学环境,提供了有力的时间约束。     

江苏省里下河(兴化-泰州)地区浅表沉积物特征及古地理环境演变

里下河地区浅部沉积物多为全新世中、晚期堆积,多数地区缺失全新世早期沉积。沉积物以淤泥质亚粘土、亚粘土、亚砂土,粉砂质淤泥、淤泥质粉砂、淤泥及泥炭为特征。沉积前的古地貌为四周高、中间低的碟形盆地。古气候经历了温湿—暖湿—温湿—温干的变化过程。区内曾有两次海侵,第一次海侵发生在全新世早中期,范围几乎遍及全区;第二次海侵发生在全新世晚期,规模小、范围窄、时间短,为海水沿江河倒灌、回溯形起。该区古环境自全新世以来经历了浅水海湾—古泻湖—湖沼地及平原的演变过程,最终形成现今河湖稠密的低凹平原。     

江苏启东地区发现浅层天然气气源层与晚更新世末期古土壤层——据江苏1:5万余东镇等七幅区调

江苏东南部启东地区开展的1∶5万区域地质调查工作已经完成野外工作验收,通过整理分析新获取的地质资料,发现工作区内"下切河谷"地区地表下46~59 m处普遍存在棕黄色、灰绿色、灰黑色"硬黏土层",厚度2~10 m不等;局部地区钻孔岩心剖面在本层顶部表现为明显的古土壤层,见根痕构造、钙质结核等暴露成土特征,其下部可见灰黑色富有机质、植物碎屑的粉砂质黏土层。古土壤层的发现证明了本区在末次盛冰期并不完全为下切河谷地区,更新了前人对测区晚更新世末期沉积地层的认识;而厚度0.5~2 m不等的富有机质、植物碎屑的粉砂质黏土层为本区浅层天然气提供了气源。