Geochemistry and Petrogenesis of Late Ediacaran Rare-metalAlbite Granites of the Arabian-Nubian Shield

The Abu Dabbab albite granite(ADAG), in the central Eastern Desert of Egypt, hosts the most significant rare metal ore deposit in the northern part of the Neoproterozoic Arabian-Nubian Shield. Here, we report detailed field,petrographic, mineralogical and geochemical investigation of the ADAG, an isolated stock-like granitic body with sharp intrusive contacts against metamorphic country rocks, probably emplaced at about 600 Ma. The fine-grained porphyritic upper unit is a preserved remnant of the shallowly-emplaced apex of the magma chamber, whereas the medium-grained lower unit crystallized at deeper levels under subvolcanic conditions. The peraluminous leucocratic ADAG shares common geochemical characteristics with post-collisional intraplate A-type magmas. In addition to the conspicuous enrichment in Na2 O, the ADAG is remarkable for its anomalous concentrations of Ta, Nb, Li, Hf, Ga, Sn, Zn and heavy rare-earth elements. Nb-Ta minerals in the ADAG are mixed with Fe-Mn oxides, forming black patches that increase in abundance toward of the base of the intrusion. Columbite-tantalite, cassiterite and wolframite are the most important ore minerals.Pronounced negative Eu anomalies(Eu/Eu* = 0.10–0.24) reflect extreme magmatic fractionation and perhaps the effects of late fluid-rock interaction. The ADAG was most likely generated by partial melting of the juvenile middle crust of the ANS as the geotherm was elevated by erosional uplift following lithospheric delamination and it was emplaced at the intersection of lineations of structural weakness. Although formation of the ADAG and its primary enrichment in rare metals are essentially due to magmatic processes, late-stage metasomatism caused limited redistribution of rare metals. Fluid-driven subsolidus modification was limited to the apex of the magma chamber and drove development of greisen, amazonite, and quartz veins along fracture systems.     

1961—1987年与1988—2014年辽宁省气候区划界线变化及可能气候成因

基于同一区划方法、指标体系,使用1961—2014年辽宁省52站气象观测资料,分析辽宁省气温、气候区划指标、范围及界线的变动特征。结果表明：辽宁省年均气温在1988年发生一次突变,突变后气温开始显著上升;≥10 ℃积温日数比较显著地响应气温突变,而干燥指数、7月平均气温变化不显著。在空间分布上区划指标值均存在不同程度的变化。① 全省≥10 ℃积温日数均出现增加,但在中西部地区显著增加;② 在盘锦-抚顺一线以北（南）,气候总体呈不显著变湿（干）趋势;③ 7月平均气温呈缓慢上升趋势。区划范围及界线位置出现更加显著地变化：① 暖温带范围主要向北向东扩展,中温带向东收缩;② 半湿润区范围主要向北向西扩展,半干旱区向西北方向收缩,湿润区范围基本不变;③ Tb范围显著向北向东扩展,Ta范围向北向东收缩。在此基础上分析了气候格局变化的可能气候成因,发现突变后≥10 ℃积温日数期间500 hPa高度场增加与4月和10月东亚冬季风减弱,4—10月东北冷涡持续天数增加和7月500 hPa高度场增加,可能分别是温度带,Tb区、Ta区和半湿润区、半干旱区变化的原因。     

培育密度和投饵量对长牡蛎壳黑选育品系幼虫生长存活及附着变态的影响

为探究长牡蛎(Crassostrea gigas)壳黑选育品系规模化繁育适宜的培育密度和投饵量,本研究以长牡蛎野生群体幼虫为对照组,分析了不同培育密度(3、7和15个/mL)和不同初始投饵量(0.4、0.8和1.6×10~3cells·ind^-1·d^-1)对长牡蛎壳黑选育品系幼虫生长、存活及附着的影响。研究显示,培育密度和投饵量对长牡蛎幼虫的生长速率、存活率和附着率有显著交互作用(P<0.05)。在培育密度3和7个/mL实验组,长牡蛎幼虫生长速率随投饵量增加而显著增大(P<0.05),并在培育密度7个/mL、投饵量1.6×10~3cells·ind^-1·d^-1实验组达到最大值。而在培育密度15个/mL实验组,投饵量增加对长牡蛎幼虫的生长速率无显著影响(P> 0.05)。且在培育密度15个/mL、投饵量1.6×10~3cells·ind^-1·d^-1实验组长牡蛎壳黑品系幼虫存活率和附着率最低。但在培育密度15个/mL实验组长牡蛎壳黑选育品系幼虫的壳高始终高于野生群体幼虫。且除投饵量0.4×10~3cells·ind^-1·d^-1实验组外,长牡蛎壳黑选育品系幼虫生长速率、存活率和附着率均高于野生群体幼虫。研究结果表明,长牡蛎壳黑选育品系幼虫最适培育条件为培育密度7个/mL、投饵量1.6×10~3cells·ind^-1·d^-1,增加投饵量可促进长牡蛎幼虫生长,但过高的培育密度会与投饵量产生拮抗作用,抑制幼虫生长,不利于幼虫存活和附着。与长牡蛎野生群体相比,壳黑选育品系幼虫能适应更高的培育密度环境,在饵料充足的条件下,其幼虫的生长、存活及附着性状均优于野生群体。     

Structural Setting and Kinematic Analysis of the Halaban Region,Eastern Arabian Shield,Saudi Arabia

The vorticity analysis technique was applied to measure the different lithological units,such as schist,metagranite and metavolcano-sedimentary rocks,which are present in the Halaban region.This work aims to interpret the relationship between the different lithologies and the tectonic setting,in order to elucidate the nature of kinematic analysis in the Halaban region.The kinematic analyses were applied to feldspar porphyroclasts,quartz and hornblende for twentysix samples.The kinematic vorticity number (W_m) for deformed rocks in the study area ranged from～0.6 to 0.9.The direction of the long axes for finite strain data (X axes) revealed a WNW trend with shallow dipping.The direction of the short axes for finite strain data (Z axes) were represented by vertical with associated horizontal foliation.The results of the kinematic vorticity and strain analyses are characterized by simple shear with different degrees of deformation in the Halaban region.Furthermore,our finite strain data shows no significant volume change during deformation.The subhorizontal foliation was synchronized with thrusting and deformation.Furthermore,throughout the overlying nappes,the same attitudes of tectonic contacts are observable,the nappes in the orogens being formed from simple shear deformation.     

大陆岩石圈研究进展

从地震学、地球化学、岩石学等不同学科的角度,对大陆岩石圈研究进展做了简要介绍。不同学科的最新研究成果表明,岩石圈在热状态、化学成分和力学行为等方面具有高度非均匀性。这不仅表现为岩石圈性质和结构随深度的变化,而且还反映在不同时代、大陆与海洋以及克拉通和造山带岩石圈结构特征的显著差异上。性质和结构的差异体现了岩石圈形成和长期演化过程的复杂性。我们认为,不同岩石圈块体之间、岩石圈与深部对流地幔之间普遍存在着相互作用。这种相互作用被认为是稳定克拉通岩石圈遭受改造甚至破坏的深部机制,同时还是地球深、浅部物质交换的重要方式,因而显著影响着地球深部的对流和地表的构造过程。值得注意的是,由于岩石圈本身定义的模糊性及其厚度的不确定性,地震活动与岩石圈强度之间的关系以及大陆岩石圈演化的规律性等问题仍有待于进一步的研究和探索。     

New Cases of Superflares on Slowly Rotating Solar-type Stars and Large Amplitude Superflares in G-and M-type Main Sequence Stars

In our previous work, we searched for superflares on different types of stars while focusing on G-type dwarfs using entire Kepler data to study statistical properties of the occurrence rate of superflares. Using these new data, as a byproduct, we found 14 cases of superflare detection on 13 slowly rotating Sun-like stars with rotation periods of24.5–44 days. This result supports the earlier conclusion by others that the Sun may possibly undergo a surprise superflare. Moreover, we found 12 and se...     

无人机载线阵摆扫CCD影像几何校正

针对无人机载线阵CCD传感器摆扫成像的技术特点,利用GPS/INS组合导航系统提供的导航遥测数据,对无人机载的线阵摆扫CCD影像建立了严格的成像模型,并设计了详细的几何校正流程。实验结果证实采用文中的成像模型和几何校正流程,可获得正确、高精度地理编码的线阵摆扫CCD正射影像。     

青藏高原东缘构造演化的SHRIMP锆石U-Pb年代学框架

青藏高原东缘一直被普遍认为是一个吸收印度—欧亚大陆碰撞变形的调节带。本文所获得的最新SHRIMP锆石U-Pb测年结果显示:青藏高原东缘具有更加复杂的地质历史。测年结果表明,高原东缘最古老的前寒武纪结晶基底形成于古元古代(2401~1912Ma)。这一古老基底首先受到中元古代构造热事件(1361~1040Ma)的影响,随后受到新元古代与弧岩浆活动有关构造热事件(791~817Ma)的强烈改造。松潘—甘孜复理石杂岩的基底是亲洋壳型的,形成于晚新元古代的大陆裂解作用(681~655Ma)。高原东缘的前寒武纪微地块可能是由这次裂解作用从扬子或青藏地块拉裂出去形成的。这些微陆块先增生拼贴于东冈瓦纳大陆、然后又从中裂离,并最终卷入高原东缘的特提斯构造演化过程中。伴随东冈瓦纳大陆裂解,高原东缘古特提斯洋于石炭纪至二叠纪早期拉开(328~292Ma),经早中生代弧-陆碰撞作用闭合(224~213Ma)。中侏罗世这一地区发育显著的构造岩浆活动(175Ma),但其动力学背景仍不十分清楚。晚白垩世岩浆活动(97Ma)可能是印度板块初始俯冲阶段的产物。新生代岩浆作用(18Ma)与陆-陆碰导致的大规模走滑断层作用所引起的同熔作用有关。