北天山巴音沟蛇绿岩形成于早石炭世:来自辉长岩LA-ICPMS锆石U-Pb年龄的证据

北天山巴音沟蛇绿岩中堆晶辉长岩的LA-ICPMS锆石U-Pb测年结果确定:巴音沟蛇绿岩中辉长岩形成的同位素地质年代为344.0±3.4Ma。表明巴音沟蛇绿岩所代表的洋盆形成于早石炭世。综合前人天山石炭纪蛇绿岩及构造演化的研究成果,笔者认为巴音沟蛇绿岩是大陆板内强烈拉张的产物。     

Evaluation of directional normalization methods for Landsat TM/ETM+ over primary Amazonian lowland forests

Biodiversity mapping in extensive tropical forest areas poses a major challenge for the interpretation of Landsat images, because floristically clearly distinct forest types may show little difference in reflectance. In such cases, the effects of the bidirectional reflection distribution function (BRDF) can be sufficiently strong to cause erroneous image interpretation and classification. Since the opening of the Landsat archive in 2008, several BRDF normalization methods for Landsat have been developed. The simplest of these consist of an empirical view angle normalization, whereas more complex approaches apply the semi-empirical Ross–Li BRDF model and the MODIS MCD43-series of products to normalize directional Landsat reflectance to standard view and solar angles. Here we quantify the effect of surface anisotropy on Landsat TM/ETM+ images over old-growth Amazonian forests, and evaluate five angular normalization approaches. Even for the narrow swath of the Landsat sensors, we observed directional effects in all spectral bands. Those normalization methods that are based on removing the surface reflectance gradient as observed in each image were adequate to normalize TM/ETM+ imagery to nadir viewing, but were less suitable for multitemporal analysis when the solar vector varied strongly among images. Approaches based on the MODIS BRDF model parameters successfully reduced directional effects in the visible bands, but removed only half of the systematic errors in the infrared bands. The best results were obtained when the semi-empirical BRDF model was calibrated using pairs of Landsat observation. This method produces a single set of BRDF parameters, which can then be used to operationally normalize Landsat TM/ETM+ imagery over Amazonian forests to nadir viewing and a standard solar configuration.     

北祁连西段祁青构造混杂岩中的单颗粒锆石U-Pb年龄及其地质意义

在北祁连西段三岔口等6幅1∶5万区域地质调查中,对祁青构造混杂岩进行了调查研究,通过LA-ICPMS法单颗粒锆石U-Pb同位素测年,获得206Pb/238U表面加权平均年龄494±15Ma,相当于中寒武世,故将该混杂岩解体,部分归为中寒武世黑刺沟组。     

湖南七宝山矿床石英斑岩锆石U-Pb定年及Hf同位素地球化学

湖南浏阳七宝山铜多金属矿床位于钦杭成矿带西南段,是湘东北规模最大的铜多金属矿床,矿区内的石英斑岩对成矿贡献非常大。石英斑岩内锆石具有典型岩浆期锆石特征,LA-ICP-MS U-Pb定年结果为154.8依1.8 Ma,代表其形成年龄,属晚侏罗世岩浆活动产物。岩浆期锆石的176Hf/177Hf=0.282120~0.282539,对应的εHf(t)值均为负值,集中在-19.8~-4.9,计算的亏损地幔模式年龄(tDM1)集中在1001~1596 Ma,平均地壳模式年龄(tDM2)集中于1519~2450 Ma,表明石英斑岩的岩浆源区具有明显壳源特征,来自于古元古代至中元古代地壳的部分熔融。结合岩石学研究,七宝山矿区内石英斑岩体成因可能是在华南地块受到伊泽奈奇(Izanagi)板块向西北俯冲的影响下,古元古代至中元古代地壳部分熔融形成岩浆,而后岩石圈拆沉和软流圈物质上涌进入岩浆发生不均匀混合在晚侏罗世上侵形成的。     

湘南荷花坪锡多金属矿床成矿年代研究

荷花坪锡多金属矿床是本世纪初在南岭中段湘南地区新发现的一个大型矿床,区内的锡多金属矿化产在王仙岭岩体东南内、外接触带,已发现有Ⅰ、Ⅱ、Ⅲ和Ⅳ号4个主要锡多金属矿体。其中,Ⅰ、Ⅱ和Ⅳ号矿体由早期矽卡岩型和晚期蚀变碎裂岩型矿石组成,Ⅲ号矿体则由独立产出的蚀变碎裂岩型矿石组成,且包含有部分碎裂花岗斑岩。以往研究已对Ⅳ号矿体中的矽卡岩型矿石和Ⅲ号矿体中含矿斑岩脉分别采用辉钼矿Re-Os法和锆石SHRIMP U-Pb法进行了测年,获得的年龄分别为224.0±1.9Ma和142±2Ma。本文补充了晚期蚀变碎裂岩型矿石的~(40)Ar/~(39)Ar测年,结果显示,Ⅱ号矿体中蚀变碎裂岩型矿石白云母样品和石英样品的坪年龄分别为151.88±1.58Ma和155.39±7.04Ma;Ⅳ号矿体中蚀变碎裂岩型矿石石英样品的坪年龄为156.94±1.64Ma。结合前人研究资料综合分析,认为荷花坪矿区存在印支晚期(224Ma)、燕山早期(151~156Ma)和燕山晚期(142Ma)三期成矿作用,分别与区内印支期中粗粒含电气石黑云母花岗岩、燕山早期中粗粒黑云母花岗岩和燕山晚期花岗斑岩脉有关,不同期成岩、成矿作用的构造环境均为岩石圈的拉张伸展。湘南地区印支期(205~224Ma)基性岩浆活动及荷花坪矿床印支期成岩、成矿过程中均有幔源物质的参与,它们共同指示南岭地区中生代构造体制的转换或岩石圈伸展减薄可能始于印支主期(230~244Ma)之后的224Ma左右,即晚三叠世。     

冀北赤城二堡子片麻状角闪二长岩的锆石SIMS U-Pb年龄及其地质意义

运用岩相学研究理论和元素地球化学研究理论,针对冀北赤城二堡子片麻状角闪二长岩,进行岩相学(4件样品)和地球化学分析(4件样品),结果表明:角闪二长岩的矿物成分为斜长石(30%~35%)、碱性长石(25%~30%)、角闪石(15%~20%)、石英(10%~15%)和黑云母(5%~10%)等。岩石中w(SiO2)介于60.16%~62.16%之间,w(K2O+Na2O)为8.56%~8.82%,稀土总量较高(ΣREE为246.30×10-6~317.76×10-6),(La/Yb)N值为28.18~42.79,具有轻稀土富集、重稀土亏损的分配模式,Eu异常(Eu/Eu*值为0.90~1.03)及Ce异常(Ce/Ce*值为0.91~0.98)均不明显,富集大离子亲石元素(如Ba,Rb,Sr和Th等)及轻稀土元素(如La,Ce和Nd等),亏损高场强元素(如Nb,Ta,Zr和Hf等)。角闪二长岩的锆石SIMS U-Pb年龄为243.1Ma±1.8 Ma,锆石的Th/U比值为0.709~1.258,表明其形成于三叠纪,应该是中生代印支期岩浆作用的产物,这是赤城地区确定的第二个印支期中酸性侵入岩体,其形成可能与赤城-崇礼断裂带在印支期重新活动有关。赤城印支期角闪二长岩体的确定表明赤城、崇礼地区存在印支期(~239Ma^243Ma)岩浆-变质-构造热事件,这对于冀北大地构造演化特征的确定具有重要的指示意义。     

Source mechanism and source parameters of May 28, 1998 earthquake,Egypt

On May 28, 1998, a moderate size earthquake of mb 5.5 occurred offshore the northwestern part of Egypt (latitude 31.45°N and longitude 27.64°E). It was widely felt in the northern part of Egypt. Being the largest well-recorded event in the area for which seismic data from the global digital network are available, it provides an excellent opportunity to study the tectonic process and present day stress field occurring along the offshore Egyptian coast. The source parameters of this event are determined using three different techniques: modeling of surface wave spectral amplitudes, regional waveform inversion, and teleseismic body waveform inversion. The results show a high-angle reverse fault mechanism generally trending NNW–SSE. The P-axis trends ENE–WSW consistently with the prevailed compression stress along the southeastern Hellenic arc and southwestern part of the Cyprean arc. This unexpected mechanism is most probably related to a positive inversion of the NW trending offshore normal faults and confirms an extension of the back thrusting effects towards the African margin. The estimated focal depth ranges from 22 to 25 km, indicating a lower crustal origin earthquake owing to deep-seated tectonics. The source time function indicates a single source with rise time and total rupture duration of 2 and 5 s, respectively. The seismic moment (M _o) and the moment magnitude (M _w) determined by the three techniques are 1.03 × 10¹⁷ Nm, 5.28; 1.24 × 10¹⁷ Nm, 5.33; and 1.68 × 10¹⁷ Nm, 5.42; respectively. The calculated fault radius, stress drop, and the average dislocation assuming a circular fault model are 7.2 km, 0.63 Mpa, and 0.11 m, respectively.     

Estimation of abl Parameters Using the Vertical Velocity Measurements of an Acoustic Sounder

The friction velocity, the surface heat flux and the height of the Atmospheric Boundary Layer (ABL) are important parameters. In this work, vertical velocity variance ( _w ² ) and wind velocity structure parameter (C _v ² ) profiles estimated by acoustic sounder measurements are used, along with similarity relations, to estimate these parameters in the unstable Atmospheric Boundary Layer and the friction velocity in the stable one. The data were collected by two acoustic sounders with different height range and resolution under various atmospheric conditions (stability) and at two experimental sites in different terrain. The C _v ² profiles are estimated using gate difference of the vertical velocity measurements and the assumption of local isotropy. The vertical velocity data are corrected for the significant effects of noisy measurements and sampling volume averaging on the _w ² and C _v ² estimations using original techniques that are presented in this work. The results of the similarity method using acoustic sounder data are compared against estimates of the corresponding atmospheric parameters obtained from direct measurements. The comparison confirms the ability of the method to provide reasonably accurate estimates of these parameters especially in the middle of the day.     

Possible impact melt and debris flows at Tooting Crater, Mars

Candidate examples of impact melt flows and debris flows have been identified at Tooting crater, an extremely young (<2 Myr), 29 km diameter impact crater in Amazonis Planitia, Mars. Using HiRISE and CTX images, and stereo-derived digital elevation models derived from these images, we have studied the rim and interior wall of Tooting crater to document the morphology and topography of several flow features in order to constrain the potential flow formation mechanisms. Four flow types have been identified; including possible impact melt sheets and three types of debris flows. The flow features are all located within 2 km of the rim crest on the southern rim or lie on the southern interior wall of the crater ∼1500 m below the rim crest. Extensive structural failure has modified the northern half of the crater inner wall and we interpret this to have resulted in the destruction of any impact melt emplaced, as well as volatile-rich wall rock. The impact melt flows are fractured on the meter to decameter scale, have ridged, leveed lobes and flow fronts, and cover an area >6 km × 5 km on the southern rim. The debris flows are found on both the inner wall and rim of the crater, are ∼1-2 km in length, and vary from a few tens of meters to >300 m in width. These flows exhibit varying morphologies, from a channelized, leveed flow with arcuate ridges in the channel, to a rubbly flow with a central channel but no obvious levees. The flows indicate that water existed within the target rocks at the time of crater formation, and that both melt and fluidized sediment was generated during this event.     

锡林浩特东部早白垩世白音高老组岩石地球化学特征、LA-MC-ICP-MS锆石U-Pb年龄及地质意义

锡林浩特东部白音高老组火山岩主要由石泡流纹岩、珍珠岩、碎斑熔岩、流纹质熔结凝灰岩等组成。LA-MC-ICP-MS锆石U-Pb定年显示,火山岩形成于134 Ma~139 Ma之间的早白垩世。岩石地球化学研究表明:该组火山岩具有高硅、高钾、高Fe OT/Mg O比值(4.88~19.09),贫镁、钙特征,属高钾钙-碱性岩系;稀土元素表现为稀土总量较高(∑REE=82.02~436.61)、轻重稀土分馏明显(LaN/YbN=2.23~20.74)、属轻稀土富集型(LRE/HRE=2.71~11.87)、Eu负异常显著(δEu=0.06~0.42);微量元素特征表现为大离子亲石元素(LILE)Rb、Th、U、K相对较为富集,高场强元素(HFSE)Nb、Ta相对亏损,而Ba、Sr、Zr、Ti强烈亏损,与A2型花岗岩特征相似。其岩浆来源为典型的壳源岩浆系列,是陆壳岩石部分熔融的产物,形成于造山后的张性构造环境。