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991.
Petrology of ultrahigh-pressure eclogites from the ZK703 drillhole in the Donghai, eastern China 总被引:25,自引:0,他引:25
The 558-m-deep ZK703 drillhole located near Donghai in the southern part of the Sulu ultrahigh-pressure metamorphic belt, eastern China, penetrates alternating layers of eclogites, gneisses, jadeite quartzites, garnet peridotites, phengite–quartz schists, and kyanite quartzites. The preservation of ultrahigh-pressure metamorphic minerals and their relics, together with the contact relationship and protolith types of the various rocks indicates that these are metamorphic supracrustal rocks and mafic-ultramafic rock assemblages that have experienced in-situ ultrahigh-pressure metamorphism. The eclogites can be divided into five types based on accessory minerals: rutile eclogite, phengite eclogite, kyanite–phengite eclogite, quartz eclogite, and common eclogite with rare minor minerals. Rutile eclogite forms a thick layer in the drillhole that contains sufficient rutile for potential mining. Two retrograde assemblages are observed in the eclogites: the first stage is characterized by the formation of sodic plagioclase+amphibole symplectite or symplectitic coronas after omphacite and garnet, plagioclase+biotite after garnet or phengite, and plagioclase coronas after kyanite; the second stage involved total replacement of omphacite and garnet by amphibole+albite+epidote+quartz. Peak metamorphic P–T conditions of the eclogites were around 32 to 40 kbar and 720°C to 880°C. The retrograde P–T path of the eclogites is characterized by rapidly decreasing pressure with slightly decreasing temperature. Micro-textures and compositional variations in symplectitic minerals suggest that the decompression breakdown of ultrahigh-pressure minerals is a domainal equilibrium reaction or disequilibrium reaction. The composition of the original minerals and the diffusion rate of elements involved in these reactions controlled the symplectitic mineral compositions. 相似文献
992.
《International Geology Review》2012,54(12):1528-1556
ABSTRACTThe intra-continental orogeny and tectonic evolution of the Mesozoic Yanshan fold-thrust belt (YFTB) in the northern North China Craton (NCC) have been strongly debated. Here, we focus on the Shangyi basin, located in the centre of the YFTB. An integrated analysis of sedimentary facies, palaeocurrents, clast compositions, and detrital zircon dating of sediments was adopted to determine the palaeogeography, provenance, basin evolution, and intra-continental orogenic process. The Shangyi basin comprises the well-exposed Early–early Middle Jurassic Xiahuayuan Formation and the Longmen Formation, and the Late Jurassic–Early Cretaceous Tuchengzi Formation. Based on the 18 measured sections, five facies associations – including alluvial fan, fluvial, delta, lacustrine, and eolian facies – have been identified and described in detail. The onset of the Shangyi basin was filled with fluvial, deltaic, and lacustrine deposits controlled by the normal fault bounding the northern basin, corresponding to the pre-orogeny. In the Middle Jurassic, the cobble–boulder conglomerates of alluvial fan, as molasse deposits, were compatible with the syn-orogeny of the Yanshan movement, which played a critical role in northern North China and even East Asia. After the depositional break in the Middle–Late Jurassic, the Shangyi basin, controlled by the normal fault present in the north of the basin, re-subsided and quickly expanded southward with thick sedimentation, which is correlative with the post-orogeny. Combined with A-type granites, metamorphic core complexes, mafic dikes, and rift basins of the Late Jurassic–early Early Cretaceous present in the northern NCC and Mongolia, significant extension was widespread in the northern NCC and even in northeast Asia. Moreover, vertical changes of provenance indicate that the Taihang Mountain and the Inner Mongolia palaeo-uplift (IMPU) present at the west and north of the basin, respectively, experienced uplift twice in the Middle–Late Jurassic and Early Cretaceous, resulting in a regional depositional break. 相似文献
993.
For the dynamics of general-relativistic adiabatic fluids a reduced Hamiltonian formalism is presented. For slowly moving fluids an approximation scheme is defined. The first steps of the scheme are worked out explicitly. Radiation damping and emission, and backscattering are discussed. The usefulness of the formalism for numerical relativity is pointed out. 相似文献
994.
日球边界射电辐射是太阳系最强的射电辐射现象,辐射功率至少达1013 W,能够提供日球边界附近高能电子束和背景磁等离子体结构的重要物理信息.自1983年旅行者号卫星首次探测到日球边界射电辐射后,其便受到研究者们的广泛持续关注.日球边界射电辐射大致有两类:辐射频率相对较高的瞬时辐射或称漂移辐射以及辐射频率相对较低的持续辐射或称非漂移辐射.通常两类辐射都从大约2 kHz开始,漂移辐射具有向高频率漂移的特征,频漂率约为1–3 kHz/yr,频率范围1.8–3.6 kHz,持续时间较短大致100–300 d;非漂移辐射没有明显的频率漂移,频率范围1.8–2.6 kHz,持续时间较长大致3 yr.目前普遍认为日球边界射电辐射与激波有关.介绍了该射电辐射可能的辐射产生源区、辐射物理机制以及与辐射相关的激波来源,并且讨论了尚存在的科学问题以及展望了未来可以进一步开展的研究. 相似文献
995.
R.A. Laing 《Monthly notices of the Royal Astronomical Society》2002,329(2):417-422
We derive expressions for the total and linearly polarized synchrotron emissivity of an element of plasma containing relativistic particles and disordered magnetic field that has been sheared or compressed along three independent directions. Our treatment follows that given by Matthews & Scheuer in the special case of a power-law electron energy spectrum. We show that the emissivity integrals depend on a single parameter, making it straightforward to generate one-dimensional look-up tables. We also demonstrate that our formulae give identical results to those in the literature in special cases. 相似文献
996.
997.
We present the results of spectral modeling of 17 Trojan asteroids. The surface composition of this group of objects (located just beyond the main belt, trapped in Jupiter's stable Lagrange points) remains uncertain due to an absence of diagnostic absorption features in their spectra. We quantitatively analyze spectra of these objects covering the range 0.3-4.0 μm using the formulation for scattering in a particulate medium developed by Hapke. Since the widest spectral range possible is desired to provide the most robust results, recently measured near-IR spectra are combined with previously published visible and near-IR data. These composite spectra are converted to and modeled in terms of geometric albedo to provide the additional constraint of the absolute brightness of the asteroids. It is important that this modeling is performed for a large number of objects, and results are derived based on trends among best-fit models. Under this rigorous examination, we find that it is unlikely that the red spectral slope is a result of organics on the surfaces, due mainly to the lack of absorptions in the L-band. Instead, anhydrous silicates adequately describe the spectral characteristics of this group of objects. A significant fraction of carbonaceous material is also likely present, but is not responsible for the red spectral slope in these models. Also, using these models, we estimate that these surfaces contain at most a few wt% of H2O ice and no more than 10-30 wt% of hydrated silicates. 相似文献
998.
短波辐射研究概述 总被引:1,自引:0,他引:1
王延慧 《沙漠与绿洲气象(新疆气象)》2013,7(2):68-73
主要阐述太阳短波辐射研究在陆面过程及陆气相互研究中的重要性,全面回顾了有关短波辐射的研究成果,结合目前在陆面过程领域具有代表性的短波辐射研究方案,指出当前在这一领域研究中有待于解决的问题和发展趋势,为进一步研究太阳短波辐射状况和特征提供科学依据. 相似文献
999.
黑龙江争光金矿床隐爆角砾岩特征及其地质意义 总被引:2,自引:0,他引:2
黑龙江争光金矿床位于大兴安岭东北缘的多宝山矿集区,矿体主要呈脉状产于燕山期闪长岩体与中奥陶统多宝山组的内外接触带上,受断裂构造控制明显。在野外地质调查过程中,发现了3个隐爆角砾岩体(J-1、J-2、J-3),角砾岩体从中心向外侧有较显著的岩石类型分带,中心为热液隐爆角砾岩,向外角砾增大,逐渐过渡为震碎角砾岩。根据胶结物的不同和穿插关系可将其分为四期,最早期为硅质胶结,中期为绿泥石胶结,其次为矿质胶结,最后为灰黑色安山质胶结,其中第二期和第三期隐爆作用与矿化关系密切。通过对隐爆角砾岩地质特征的研究,结果表明在Ⅱ号矿带绿泥石胶结隐爆角砾岩体深部具有寻找与矿质胶结隐爆角砾岩有关金铜矿化体的潜力,这对争光金矿床深部及外围找矿具有一定的指导意义。 相似文献
1000.
近二十年来,蒙古南戈壁成矿带在寻找大宗金属矿产方面取得丰硕成果,发现了欧玉陶勒盖和查干苏布尔加等与古亚洲洋晚泥盆世岛弧演化有关的大型斑岩型矿床。研究表明:1)欧玉陶勒盖—查干苏布尔加地区在法门期弧岩浆与矿化作用之后,经历了短暂的抬升和剥蚀过程,随后被石炭纪火山-沉积岩所覆盖。两个矿床皆被埋藏于法门期(D_3)—杜内期(C_1)不整合面之下;2)矿床现今出露于石炭纪—二叠纪岩体包围的"天窗"中,矿体能否保存与其上覆岩层遭受的剥蚀程度有关;3)近EW向展布的蒙古南戈壁成矿带在欧玉陶勒盖—查干苏布尔加地区受三叠纪—早白垩世准巴彦断裂左旋走滑运动的影响,局部转变为NE走向,向东可延伸至中国境内东乌旗一带。因此,在中国内蒙古东乌旗地区开展的找矿勘查工作应重点关注法门期(D_3)—杜内期(C_1)不整合之下的晚泥盆世侵入体及其围岩,并在成矿远景区进行相应的区域构造解析研究。 相似文献