中亚低涡背景下南疆西部两次强冰雹环境场对比分析

利用常规资料、14:00加密探空、NCEP1°×1°再分析资料,对比分析2013年6月18日和2014年6月23日南疆西部两次强冰雹环境场及物理机制,表明两次冰雹环境场有相同之处:在环流经向度较大的中亚低涡背景下,前期有明显降水,傍晚前后由中亚低涡后部西北气流下产生,高空干冷平流、低层暖湿环境、较大的垂直温度递减率及低层辐合线或切变线为冰雹天气提供了强不稳定层结和动力触发条件,为冷平流强迫类型。但两次冰雹中亚低涡位置、强度、物理机制变化等有所不同:"6·18"中亚低涡压至南疆西部,低涡强,西北风大,而"6·23"中亚低涡在巴尔喀什湖附近,位置偏北,低涡较弱,西北风较小;"6·18"偏西北气流、风(垂直)切变、强回波伸展高度、层结不稳定、水汽及动力等变化均较"6·23"明显偏强;"6·18"的0℃层和-20℃层的高度均比"6·23"的低300~400 m;"6·18"低层南疆盆地偏东风日变化明显,即傍晚到夜间增强,山前东西风辐合促使上升运动发展,并有明显的中尺度垂直环流圈,而"6·23"低层为西北风风速辐合及与偏东风的切变。     

天山山区水汽和云水含量的空间分布特征

利用欧洲数值预报中心(ECMWF)发布的第一代全球分辨率ERA-Interim再分析数据,分析了1979～2014年天山山区水汽含量和云水含量的空间分布特征。结果显示：(1)水汽含量的高值中心出现在伊犁河谷地区,中心值域在10—11kg m-2之间,低值区位于天山中部的巴音布鲁克附近,中心值域在5—6kg m-2之间;夏季水汽含量最丰富,在8—11kg m-2之间。(2)云液水含量的高值区出现在博格达山北坡,而云冰水含量的高值区在西天山海拔较高的托木尔峰地区,低值区均在伊犁河谷等海拔低的地区;夏季云液水含量、云冰水含量均呈减少趋势,云冰水含量较云液水减少的更为明显,下降速率为0.28kg kg-1/10a;(3)垂直分布上,云液水含量在600hpa左右的高空出现高值区,中心最大值为10kg kg-1;云冰水含量的高值区则出现在500hpa左右的高空,为11kg kg-1;在对流层大气中云冰水含量值远大于云液水,且云冰水发展的高度较云液水更高。     

青藏高原片麻岩穹窿与找矿前景

片麻岩穹窿是研究俯冲-折返和碰撞-折返造山过程的重要窗口。已查明的大量青藏高原片麻岩穹窿(群)分布在古特提斯和新特提斯大洋俯冲-折返以及地体碰撞-折返过程中。松潘-甘孜造山带中雅江甲基卡片(麻)岩穹窿的三叠纪变质片岩的含矿伟晶岩脉中发现了超大型锂矿床,揭示片(麻)岩穹窿构造与同构造花岗岩、含矿伟晶岩脉以及大型印支滑脱带在时空和成因上有天然联系,为片麻岩穹窿的找矿前景提供了范例。     

东天山哈密地区早二叠世花岗岩体及镁铁质包体的年代学, 岩石地球化学特征及其构造意义

花岗岩中包体是区域构造与深部过程研究结合的良好窗口,对研究花岗岩的成因和壳-幔相互作用有非常重要的意义。东天山南山口黑云母二长花岗岩中广泛发育镁铁质包体。主量元素组成上,寄主花岗岩岩具有中酸性、准铝质、富碱、富钾等特征;镁铁质包体则偏基性、贫钾。微量和稀土元素组成上,富集Rb、K、Th、U,贫Sr、P、Nb、Ta、Ti,且Zr、Hf含量相对较高,具中-强的铕负异常(0.46~0.57)。镁铁质包体与寄主岩具有相似的微量元素特征,但相对富集Sr、P,贫Zr、Hf,铕负异常中等或不明显(0.80~0.93)。闪长质包体属于同源包体,为寄主花岗岩同源母岩浆经结晶分异形成的早期产物。运用LA-ICP-MS锆石U-Pb定年技术,该南山口岩体暗色镁铁质微粒包体与寄主黑云母二长花岗岩的锆石U-Pb年龄分别为298.2±2.0Ma和294.0±2.7Ma,包体与寄主岩样品具有相似的Hf同位素组成,暗示其母岩浆来自新元古代晚期和早古生代亏损地幔中分离的新生地壳。该高钾钙碱性的花岗岩及其包体可能形成于东天山后碰撞背景下的板片断离后引起软流圈上涌,底侵体带来的热能使得新元古代晚期和早古生代的新生地壳发生部分熔融。     

Geochemical fractionation of Ni,Cu and Pb in the deep sea sediments from the Central Indian Ocean Basin: An insight into the mechanism of metal enrichment in sediment

Metal speciation study in combination with major element chemistry of deep sea sediments provided possible metal enrichment pathways in sediments collected from environmentally different locations of Central Indian Ocean Basin (CIB). Metal speciation study suggests that Fe–Mn oxyhydroxide phase was the major binding phase for Ni, Cu and Pb in the sediments. The second highest concentrations of all these metals were present within the structure of the sediments. Easily reducible oxide phase (within the Fe–Mn oxyhydroxide binding phases) was the major host for all the three metals in the studied sediments. Major element chemistry of these sediments revealed that there was an increased tendency of Cu and Ni to get incorporated into the deep sea sediment via the non-terrigenous Mn-oxyhydroxide fraction, whereas, Pb gets incorporated mostly via amorphous Fe-hydroxides into the sediment from the CIB. This is the first attempt to provide an insight into the mechanism of metal enrichment in sediment that host vast manganese nodule.     

Delineation and assessment of Central Indian Suture through lineament extraction approach using Remote Sensing and Geographic Information System

Lineament extraction approach allowed mapping of larger number of lineaments in a classical manner in tectonic and structural studies. In the present study, various techniques were adopted to extract lineaments using Landsat ETM+ images. To remove the biasness of the images, some pre-processing techniques like stream ordering, band differencing, colour texturing were employed to enhance the edges of the structural features. Extracted lineaments and its distribution and orientation were mapped using ArcGIS Spatial analyst tool. Results of the study showed maximum number of lineaments were oriented in the ENE–SWS direction with 63° overall inclination. Accuracy assessment and validation were made with respect to visual interpretation and overlaying the lineament on Digital Topographic Model as well as with respect to an existing geological lineament map of the study site. The result of accuracy assessment indicates higher compatibility of Central Indian Suture with the geological map of the study area.     

Possible spatial variability in the Selwyn Block of Central Victoria: evidence from Late Devonian felsic igneous rocks

The Neoproterozoic to Cambrian Selwyn Block in Central Victoria forms the mainly unexposed basement to the Paleozoic metasediments, granitic rocks and felsic volcanic complexes of the Melbourne Zone of the Lachlan Orogen. The Late Devonian felsic rocks are largely products of partial melting of the Selwyn Block, and their chemistry implies that their sources were most probably arc-related andesite, dacite, volcaniclastic greywackes and some pelites. When plotted against the median longitudes of the plutons and volcanic complexes, the average values for ⁸⁷Sr/⁸⁶Sr_t and ?Nd_t (at 370 Ma) reveal broad trends interpreted to reflect possible compositional and/or age structure in the Selwyn Block. Assuming that the trends are real, from W to E, I-type sources are progressively less crustally evolved, probably younging eastward. The S-type sources show no trend in ?Nd_t, suggesting that there was efficient sediment mixing. The ⁸⁷Sr/⁸⁶Sr_t values, however, become more evolved eastward (opposite in sense to the apparent variation in the I-type sources). This is interpreted as the original Selwyn Block sediments having been more pelitic eastward, perhaps suggesting a deepening of the basin in this direction, as well as structurally upward in the succession. The opposite senses of variation highlights the spatial separation of the S- and I-type sources and suggest that the granitic magmas here are unlikely to represent any sort of mixing continuum.     

月球东海盆地综合解析与撞击初始条件的研究

东海是月球上最年轻的多环撞击盆地,关于其形成机制的研究很多,但成果大都基于正撞击的机制提出的,虽然有部分学者提出东海是斜撞击的,但缺乏具体撞击参数。本文通过多源数据融合,综合分析LRO影像数据、LOLA地形数据、M~3高光谱数据和IIM高光谱数据,对东海地区的地貌特征、物质成分进行了较为系统的解译,发现在东海中央熔融区存在一条与东海撞击方向垂直的中央隆起区域(中央隆起线),其也是中央熔融区粗糙部分与光滑部分的分界线,结合撞击坑成坑理论,认为其可能是撞击过程冲击波作用引起的堆叠作用形成的。同时利用GRAIL数据及对该地区的重力异常的成因进行了分析,认为异常是由于压强、温度及岩石粘度的改变引起局部莫霍面抬升和中央熔融物的形成而出现的,进而估算出熔融物占盆地内物质的25%,约为1.1×10~6km~3。同时,对GRAIL数据的剖面分析结果也支持了本文的斜撞击理论。最后,综合多方面的信息和撞击理论获取东海盆地构造分布图,并根据中央隆起线、溅射物及线性构造的分布特征等,提出东海盆地理论上是由一直径在50~100km的撞击体以10~30km/s的速度自东偏北约20°~30°方向以20°~30°的角度斜撞击月表而形成的。这可为研究更早期的月球撞击坑提供理论参考。     

早古生代古亚洲洋俯冲记录:来自东天山卡拉塔格高镁安山岩的年代学、地球化学证据

吐哈盆地南缘荒草坡群大柳沟组火山岩出露于大草滩断裂以北的彩霞山、土屋铜矿北和卡拉塔格地区。该组火山岩主要为基性、中酸性熔岩及火山碎屑岩组合。LA-ICP MS锆石U-Pb分析获得安山岩和英安岩的年龄分别为434.8±3.8Ma和438.4±4.9Ma,表明大柳沟组火山岩形成于早志留世。安山岩Si O2含量为54.35%~60.70%;Al2O3含量为11.8%~16.3%,Mg O含量为4.94%~8.27%,Ti O2含量为0.38%~0.52%,Na2O和K2O的含量分别为0.50%~3.83%和0.08%~1.26%,铝饱和指数(A/CNK)为0.77~1.37,低ΣREE(43×10-6~70×10-6),为具有亏损源区特征的高镁安山岩。英安岩较安山岩Si O2含量高(63.74%~75.35%),具有相似的Al2O3(12.3%~16.0%%)和Ti O2(0.32%~0.52%)含量;Na2O和K2O含量分别为2.01%~5.53%和0.16%~2.19%,ΣREE含量较安山岩略高(61×10-6~84×10-6),铝饱和指数(A/CNK)为0.77~5.74。安山岩和英安岩均轻重稀土分异明显,具有中等的Eu负异常;富集大离子亲石元素(LILE),亏损高场强元素(HFSE),具有明显的Nb-Ta-Ti负异常。相似的岩石地球化学特征表明安山岩和英安岩可能为同源岩浆,英安岩是安山质岩浆经过角闪石等矿物结晶分异作用形成的,安山岩的母岩岩浆很可能来自亏损大洋岩石圈地幔。基于该组岩石组合、地球化学特征和区域地质资料,推测研究区高镁安山岩可能形成于洋内弧环境,这表明东天山吐哈盆地南缘卡拉塔格地区在早古生代已经存在古亚洲洋的俯冲。     

西准噶尔玛依勒地区枕状玄武岩年代学、地球化学及岩石成因

通过对造山带内洋岛玄武岩的时代及地球化学性质研究,不仅可以进行古海山/大洋高原的识别,而且还可以进行古洋盆演化及古构造格局恢复。笔者等最新在西准噶尔玛依勒山北侧识别出一套枕状玄武岩,其与火山碎屑岩、硅质岩共生。枕状玄武岩斜长石微晶普遍发育中空骸晶结构,是在水下熔岩急剧萃冷条件下迅速结晶的产物。通过LA-ICP-MS锆石U-Pb测年,获得枕状玄武岩206Pb/238U加权平均年龄为437.2±2.2Ma,该年龄的获得填补了志留纪碱性玄武岩的空白。岩石地球化学分析结果显示,玛依勒枕状玄武岩为碱性玄武岩系列,岩石具有中等Si O2(44.89%~47.81%),高Ti O2(3.28%~4.12%)及P2O5(0.50%~0.70%),低Mg O(3.49%~6.79%),轻、重稀土元素分异较为明显((La/Yb)N=5.5~7.3),无明显Eu异常(Eu/Eu*=0.96~1.06),相对富集Rb、Th、U,亏损Ba、K、Sr,没有明显Nb、Ta负异常,这些地球化学特征与洋岛玄武岩(OIB)极其相似。微量元素含量及反映源区性质的比值表明,枕状玄武岩来源于富集地幔源区,主要组成为尖晶石和石榴石二辉橄榄岩,并发生了5%±的部分熔融,其形成于大洋板内与地幔柱有关的海山/大洋岛屿环境。结合前人研究,认为西准噶尔乃至古亚洲洋在中古生代洋内俯冲的同时,大洋板内可能存在地幔柱活动。