Age and emplacement of late-Variscan granites of the western Bohemian Massif with main focus on the Hauzenberg granitoids (European Variscides, Germany)

The Variscan Hauzenberg pluton consists of granite and granodiorite that intruded late- to postkinematically into HT-metamorphic rocks of the Moldanubian unit at the southwestern margin of the Bohemian Massif (Passauer Wald). U–Pb dating of zircon single-grains and monazite fractions, separated from medium- to coarse-grained biotite-muscovite granite (Hauzenberg granite II), yielded concordant ages of 320 ± 3 and 329 ± 7 Ma, interpreted as emplacement age. Zircons extracted from the younger Hauzenberg granodiorite yielded a ²⁰⁷Pb–²⁰⁶Pb mean age of 318.6 ± 4.1 Ma. The Hauzenberg granite I has not been dated. The pressure during solidification of the Hauzenberg granite II was estimated at 4.6 ± 0.6 kbar using phengite barometry on magmatic muscovite, corresponding to an emplacement depth of 16-18 km. The new data are compatible with pre-existing cooling ages of biotite and muscovite which indicate the Hauzenberg pluton to have cooled below T = 250–400 °C in Upper Carboniferous times. A compilation of age data from magmatic and metamorphic rocks of the western margin of the Bohemian Massif suggests a west- to northwestward shift of magmatism and HT/LP metamorphism with time. Both processes started at > 325 Ma within the South Bohemian Pluton and magmatism ceased at ca. 310 Ma in the Bavarian Oberpfalz. The slight different timing of HT metamorphism in northern Austria and the Bavarian Forest is interpreted as being the result of partial delamination of mantle lithosphere or removal of the thermal boundary layer.     

Magma–host interactions during differentiation and emplacement of a shallow-level, zoned granitic pluton (Tarçouate pluton, Morocco): implications for magma emplacement

The Tarçouate pluton (Anti-Atlas, Morocco) is an inversely zoned laccolith emplaced 583 Ma ago into low-grade metasediments, with the following succession: leucocratic granites, biotite–granodiorites (±monzodiorites), hornblende–granodiorites (±monzodiorites) and monzodiorites syn-plutonic dykes. These rocks form two distinct, chemically coherent, units:

(1) A main unit consists of layered (572<59 wt.%) and homogeneous (632<67%) hornblende–granodiorites, biotite–granodiorites (672<72%) and aplites (702<76%). All these rocks are metaluminous to peraluminous and display fractionated HREE depleted patterns (La/Yb_N=14–61; Yb_N=0.7–6.8). Initial ⁸⁷Sr/⁸⁶Sr ratios (0.7072 to 0.7080) increase, whereas _Nd(t) values (−1.7 to −2.8) decrease from the hornblende– to the biotite–granodiorites. Monzodiorites occur as mafic microgranular enclaves or syn-plutonic dykes.

(2) A subordinate unit consists of leucocratic, distinctly peraluminous, muscovite-bearing granites (722<75%) occurring at the northern edge of the pluton and as dykes in the surrounding schists towards the top of the pluton. These rocks are free of monzodioritic enclaves. They display less fractionated patterns with higher HREE contents (La/Yb_N=2–19; Yb_N=11–18), a distinct _Nd(t) value (−11.8) and a ⁸⁷Sr/⁸⁶Sr initial ratio (0.7480) within those of the surrounding schists (0.7393–0.7819).

Magma–host interactions are closely related to differentiation and occurred at different levels, but mainly before emplacement. Field relationships and petrogenetic modelling show that the bt–granodiorites formed at levels deeper than the level of emplacement, by fractional crystallisation (0.65

These data preclude any significant material transfer process for the emplacement of the Tarçouate pluton, but rather suggest assembly of successive pulses of variably differentiated crystal-poor magmas. These shallow level granitic plutons can be considered as an end-member of magma emplacement with minimum interactions with the country rocks.     

Late Paleozoic granitoids of western Transbaikalia: magma sources and stages of formation

Geochemical and geochronological studies of the main types of granitoids of the Angara-Vitim batholith (AVB) and granites of the Zaza complex in western Transbaikalia were carried out. U-Pb (SHRIMP-II) and Rb-Sr dating yielded the age of autochthonous gneiss-granites of the Zelenaya Griva massif (325.3±2.8 Ma), quartz syenites of the Khangintui pluton (302.3±3.7 Ma) and intruding leucogranites of the Zaza complex (294.4±1 Ma), monzonites of the Khasurta massif (283.7±5.3 Ma), and quartz monzonites of the Romanovka massif (278.5±2.4 Ma). The U-Pb and Rb-Sr dates show that the Late Paleozoic magmatism in western Transbaikalia proceeded in two stages: (1) 340–320 Ma, when predominantly mesocratic granites of the Barguzin complex, including autochthonous ones, formed, and (2) 310–270 Ma, when most AVB granitoids formed. We suggest that at the early stage, crustal peraluminous granites formed in collision geodynamic setting. At the late (main) stage, magmatism occurred in postorogenic-extension setting and was accompanied by the formation of several geochemical types of granitoids: (1) typical intrusive mesocratic granites of the Barguzin complex, similar to those produced at the first stage; (2) melanocratic granitoids (monzonitoids, quartz syenites), which were earlier dated to the early stage of the AVB evolution; (3) leucocratic medium-alkali (peraluminous) granites of the Zaza intrusive complex; and (4) some alkali-granite and syenite intrusions accompanied by alkaline mafic rocks. The diversity of granitoids that formed at the late stage of magmatism was due to the heterogeneous composition of crust protoliths and different degrees of mantle-magma participation in their formation.     

青藏高原新生代地壳变形对同碰撞岩浆侵位的制约

同碰撞岩浆作用是青藏高原新生代构造-岩浆活动的一种重要形式，各种类型岩浆岩广泛分布于高原内不同的构造单元中，其中有的来自地幔，不过规模都不大，它们是如何穿过异常厚的地壳侵位到近地表或喷出地表，这还是个未解之谜。根据构造分析，这些岩浆岩均侵位于新生代向斜构造中，例如侵入于高原东南边缘的楚雄复向斜、兰坪．思茅复向斜和老君山向斜的碱性岩，侵入于高原南缘的北喜马拉雅拉轨岗日向斜的片麻状花岗岩以及喷出于高原北部巴颜喀拉和雁石坪复向斜的安山-玄武岩。文中通过一个力学模式，说明这些岩浆岩的侵位受控于地壳应力场特征，即：向斜构造的下部承受的是张应力，地壳发生减薄和张裂，下地壳或上地幔熔融物质以此为通道发生向上的侵位。不过，因向斜顶部地壳承受的是挤压应力，地壳发生挤压缩短，所以只有少量岩浆能侵位到近地表并发生变形。与此相反，背斜构造的下部地壳产生的是挤压应力，阻止了下伏地壳内岩浆的侵入。因此，岩浆的侵位一般不会沿背斜发生。这一力学机制解释了为什么青藏高原规模很小的同碰撞岩浆能穿过异常厚的地壳沿一系列向斜构造侵位到近地表或喷出地表的原因。     

Microstructural evidence for magma confluence and reusage of magma pathways: implications for magma hybridization,Karakoram Shear Zone in NW India

In the Karakoram Shear Zone, Ladakh, NW India, Miocene leucogranitic dykes form an extensive, varied and complex network, linking an anatectic terrane exposed in the Pangong Range, with leucogranites of the Karakoram Batholith. Mineral paragenesis of the heterogeneous anatectic source rocks suggests melting has resulted from water influx into rocks at upper amphibolite facies conditions, and microstructures suggest anatexis was contemporaneous with shearing. The network is characterized by continuous and interconnected dykes, with only rare cross‐cutting relationships, forming swarms and chaotic injection complexes where magmatic rocks cover up to 50% of the outcrop area. Despite this volume of magma, the system did not lose continuity, suggesting that it did not flow en masse and that the magma network was not all liquid simultaneously. Leucogranites in this network, including leucosomes in migmatites, carry an isotopic signature intermediate between the two main anatectic rocks in the source, suggesting efficient homogenization of the magmatic products. Here, we describe a number of microscopic features of these magmatic rocks which suggests that several pulses of magma used the same pathways giving rise to textural and chemical disequilibrium features. These include: (i) narrow, tortuous corridors of fine‐grained minerals cutting across or lining the boundaries of larger grains, interpreted to be remnants of magma‐filled cracks cutting across a pre‐existing magmatic rock; (ii) corrosion of early formed grains at the contact with fine‐grained material; (iii) compositional zoning of early formed plagioclase and K‐feldspar grains and quartz overgrowths documented by cathodoluminescence imaging; (iv) incipient development of rapakivi and anti‐rapakivi textures, and (iv) different crystallographic preferred orientation of early formed quartz and fine‐grained quartz. Mapping of the fine‐grained corridors interpreted to represent late melt channels reveal an interlinked network broadly following the S‐C fabric defined by pre‐existing magmatic grains. We conclude that early formed dykes provided a pathway exploited intermittently or continuously by new magma batches. New influxes of magma opened narrow channels and migrated through a microscopic network following predominantly grain boundaries along an S‐C fabric related to syn‐magmatic shearing. A mixed isotopic signature resulted not from the mixing of magmas, but from the micro‐scale interaction between new magma batches and previously crystallized magmatic rocks, through local equilibration.     

Preferred orientation of plagioclase—neutron diffraction and U-stage data

Pole figures of anorthosite mylonite (An 65) from San Juan Bautista, California, were determined with neutron diffraction using a 23 position sensitive detector. This novel technique enables us to deconvolute the complex diffraction spectrum of this triclinic mineral into fifteen separate peaks hkl which are measured simultaneously. All pole figures display strong preferred orientation with complicated triclinic distributions from which it appears that (001) poles are concentrated normal to the schistosity plane of the specimen. The triclinic mineral is well suited to discuss some fundamental issues of texture representation. If crystals are measured individually (e.g., on the U-stage), positive and negative ends of directions can be unequivocally identified and the whole sphere, rather than a hemisphere, is necessary to represent the distribution of positive axes. This is illustrated for a plagioclase-rich amphibolite from Ornö Huvud, Sweden.     

Analogue study of particle segregation in pyroclastic density currents, with implications for the emplacement mechanisms of large ignimbrites

Abstract Analogue flume experiments were conducted to investigate the transport and sedimentation behaviour of turbulent pyroclastic density currents. The experimental currents were scaled approximately to the natural environment in three ways: (1) they were fully turbulent; (2) they had a very wide range of particle sizes and associated Rouse numbers (the ratio of particle settling velocity to effective turbulent eddy velocity in the current); and (3) they contained particles of two different densities. Two sets of surge‐type experiments were conducted in a 5 m long, water‐filled lock‐exchange flume at five different volumetric particle concentrations from 0·6% to 23%. In one set (one‐component experiments), the currents contained just dense particles; in the other set (two‐component experiments), they contained both light and dense particles in equal volume proportions. In both sets of experiments, the population of each component had a log‐normal size distribution. In the two‐component experiments, the size range of the light particle population was selected in order to be in hydrodynamic equivalence with that of the dense particles. Dense particles were normally graded, both vertically and downstream, in the deposits from both sets of experiments. The mass loading (normalized to the initial mass of the suspension) and grain size of the dense component in the deposits decreased with distance from the reservoir and were insensitive to initial total particle concentration in the currents. On the other hand, in the two‐component experiments, the light particles were extremely sensitive to concentration. They were deposited in hydrodynamic equivalence with the dense particles from dilute currents, but were segregated efficiently at concentrations higher than a few per cent. With increasing particle concentration, the large, light particles were carried progressively further down the flume because of buoyancy effects. Deposits from the high‐concentration currents exhibited reverse vertical grading of the large, light particles. Efficient segregation of the light component was observed even if the bulk density of the current was less than that of the light particles. In both sets of experiments, marked inflexions in the rate of downstream decline in mass loading and maximum grain size of the dense component can be attributed to the presence of two different particle settling regimes in the flow: (1) particles with Rouse numbers >2·5, which did not respond to the turbulence and settled rapidly; and (2) particles with Rouse numbers <2·5, which followed the turbulent eddies and settled slowly. The results are applied to the transport and sedimentation dynamics of pyroclastic density currents that generate large, widespread ignimbrites. Field data fail to reveal significant departures from aerodynamic equivalence between pumice and lithic clasts in three such ignimbrites: the particulate loads of some large ignimbrites are transported principally in turbulent suspensions of low concentration. In some ignimbrites, the well‐developed inflexions in curves of maximum lithic (ML) size vs. distance can be attributed to the existence of distinct high and low Rouse number particle settling regimes that mark the transition from an overcharged state to one in which the residual particulate load is transported more effectively by turbulence.     

一个新的花岗岩成因分类:基于变质岩深熔作用理论与大数据的证据

花岗岩目前的ISMA分类不是一个系统的分类,花岗岩分类可能需要从花岗岩的起源来考虑。花岗岩源自变质岩,可能是来自地幔或玄武质岩浆底侵带来的热导致的下地壳底部发生部分熔融的熔体形成的。因此,花岗岩与变质岩源岩有成因联系和因果关系,变质岩为母,花岗岩为子。根据埃达克岩与残留相平衡的理论,埃达克岩形成于斜长石消失线之上。那么,出现在石榴石出现线之上的是什么花岗岩呢?出现在石榴石出现线之下的又是什么花岗岩呢?本文即尝试从这个思路来探讨花岗岩的分类,并采用大数据方法予以佐证,得到的初步结果可以将花岗岩分为3类:(1)位于斜长石消失线之上的为高Sr低Y型花岗岩(高压,代表加厚的地壳);(2)位于斜长石消失线与石榴石出现线之间的为低Sr低Y类型花岗岩(中压,代表正常厚度的地壳);(3)位于石榴石出现线之下的为高Y型花岗岩(低压,代表减薄的地壳)。大数据研究的结果支持上述分类,给出的地球化学标志大体是:Sr含量为400×10^-6,Y含量为(20~35)×10^-6。     

REE geochemistry and isotopic data of Archean silicic volcanics and granitoids from the Pilbara Block,Western Australia: implications for the early crustal evolution

Eighteen silicic volcanic rocks of the Warrawoona Group and ten associated plutonic rocks from the Pilbara Block, Western Australia, have been chosen for geochemical and isotopic studies. Silicic volcanics of the UNSB (Upper member of North Star Basalt) are dated at 3.56—3.57

, by both the Rb-Sr and the Sm-Nd methods. The respective 1 (initial isotopic composition) values are 0.7005 ± 5 (Sr) and 0.50810 ± 39 (Nd). This age is consistent with the stratigraphic interpretation that the TalgaTalga Subgroup, in which the North Star Basalt occupies the lowermost position, is overlain by the Duffer Formation, whose age was earlier established at 3.45

by the zircon U-Pb method. The new Rb-Sr data on six silicic lava samples from the Duffer Formation yield an isochron of 3.23 ± 0.28 (2v). Though imprecise, this age agrees with the zircon age within error limits. Rb-Sr ages of 2.3–2.4.

obtained for the ‘Panorama’ rocks and the Wyman Formation do not correspond to their initial eruption ages. Chemical arguments suggest that these ages represent the time of metasomatism associated with the widespread thermal event in this region about 2.3–2.4

ago.Geochemically, most of these analyzed rocks (volcanic and plutonic) are of tonalite-trondhjemitegranodiorite (TTG) composition, a typical feature found in many other Archean terrains. They generally show fractionated REE patterns, except the Panorama Formation rocks. Furthermore, the Wyman Formation rhyolites and the post-tectonic adamellites show significant negative Eu anomalies, suggesting a similar mode of magma generation and a probable genetic link. Theoretical considerations suggest that most of these TTG rocks could have been generated by partial melting of amphibolitic or basaltic sources, followed by fractional crystallization.Although the Archean granitic gneisses often possess mantle-like I_sr values, the trace element data indicate that they could not have been derived by direct melting of upper mantle materials. The immediate tectonic implication is that in any Archean terrain, the formation of Na-rich continental crust of TTG suite must be preceded by the presence of basaltic crust. The occurrence of this basaltic crust is a matter of controversy. Such crust might have been totally destroyed by repeated melting processes, or its remnants are now represented by some of the mafic-ultramafic enclaves within the tonalite-trondhjemite batholiths.     

幔源岩浆在地壳中分层侵位的控制因素：二维热-力学模拟

幔源岩浆在地壳内的上升和聚集样式不仅依赖于岩浆自身的性质, 还取决于围岩的强度和热状态。已有数值和物理模型大多关注岩浆自身物性对其上升过程的影响, 而对围岩流变强度或热状态如何影响岩浆的上升和聚集过程的研究相对薄弱, 尤其是周期性的幔源岩浆在壳内分层侵位的受控因素仍然不清楚。本文利用二维热-力学数值模拟方法, 通过发展多期岩浆脉冲和岩墙生成算法, 研究了岩浆从深部地幔上升至地壳内部侵位的动力学过程, 系统测试了地壳(围岩)地温梯度(上、下地壳的地温梯度分别以G_UC和G_LC表示)和地壳强度对岩浆上升过程和聚集样式的影响。模拟结果表明: (1)地壳地温梯度对岩浆的侵位深度有重要影响, 岩浆侵入冷地壳(G_UC=G_LC=12.5K/km), 岩浆主体在岩石圈深度聚集, 地表的相对高差小于140m;岩浆侵入温地壳(G_UC=G_LC=15K/km)在下地壳底部聚集形成岩浆房, 上升至上、下地壳界面, 岩浆房上方的地表地形呈现中心拗陷两翼隆起的形态, 地表最大高程可达3km; 岩浆侵入热地壳(G_UC=G_LC=17.5K/km)仅在下地壳底部聚集形成岩浆房, 地形演化特征与温地壳背景的情况类似, 但最大高程小于1.5km。(2)在同等地壳地温梯度条件下, 上、下地壳的相对强度决定了岩浆的聚集样式: 下地壳的强度越弱, 岩浆更易在下地壳聚集形成岩浆房; 上地壳的强度越弱, 岩浆更易在地表喷发。进一步分析表明: 岩浆的聚集样式受地壳地温梯度与地壳流变分层性的共同控制, 地壳越热且流变强度分层性越显著则越有利于岩浆在地壳中的多层级侵位; 每一期岩浆脉冲的供给均会导致岩浆房内部的超压值骤增。我们的模拟结果对理解火山喷发前壳内岩浆的赋存状态及岩浆活动区的地形演化具有启示意义。

     

花岗岩混合成因研究及大陆动力学意义

岩相学特别是同位素地球化学研究显示,很多花岗岩并非起源于单一物源,而可能是壳、幔物质的三源（元）混合产物,也可能是三源（元）混合产物,如长英质上地壳物质、基性下地壳物质、幔源基性物质或陆壳、洋壳、地幔物质。因而,用花岗岩推断下地壳物质组成特性有时不一定可靠,但花岗岩混合成因研究却有可能提供有关地壳结构、生长演化以及地壳、洋壳、地幔三者相互作用关系的信息,进而可能成为探索大陆动力学的一条新途径。     

P-V equation of state of portlandite, Ca(OH)2, from powder neutron diffraction data

 A high pressure neutron powder diffraction study of portlandite [Ca(OH)₂] has been performed at ISIS facility (U.K.); nine spectra have been collected increasing the pressure by steps, up to 10.9 GPa, by means of a Paris-Edinburgh cell installed on the POLARIS diffractometer. The tensorial formalism of the lagrangian finite strain theory and the Birch-Murnaghan equation of state have been used to determine, independently, two values of the bulk modulus of portlandite, obtaining K ₀=38.3(±1.1) GPa [linear incompressibilities: K _0a=188.4(±9.9), K _0c=64.5(±2.5) GPa] and K ₀=34.2(±1.4) GPa, respectively. The present results comply with values from previous measurements by X-ray diffraction [K ₀=37.8(±1.8) GPa] and Brillouin spectroscopy [K ₀=31.7(±2.5) GPa]. Reasonably, Ca(OH)₂ has revealed to be bulkly softer than Mg(OH)₂ [K ₀=41(±2), K _0a=313, K _0c=57 GPa]. The Ca(OH)₂ linear incompressibility values reflect the nature of forces acting to stabilize the (001) layer structure and, further, prove that the replacement Ca/Mg mainly affects the elastic properties in the (001) plane, rather than along the [001] direction. Data from a full refinement of the structure at room pressure are reported. Received January 12, 1996/Revised, accepted June 15, 1996     

Mesozoic high-Ba–Sr granitoids from North China: geochemical characteristics and geological implications

Abstract Mesozoic magmatism occurred extensively in the North China block (NCB) and the Dabie–Sulu orogen (DSO) post-dating the North–South China collision, resulting in abundant intrusive and volcanic rocks ranging from basic to acidic compositions. The intermediate-acidic intrusive rocks can be grouped into two types, namely high-Ba–Sr granitoids and low-Ba–Sr granitoids that both have distinct geochemical characteristics. The high-Ba–Sr granitoids are similar in most of the incompatible trace element systematics to the associated basic rocks, which probably originated from melting of subcontinental lithospheric mantle, indicating significant mantle contributions to them. Geochemical similarities are observed between the basic rocks from the NCB and DSO, implying a regional-scale magma-generating mechanism and that mantle enrichment beneath the DSO was independent from the Triassic deep continental subduction in the region. We therefore interpret that the Mesozoic magmatism resulted from delamination of the ancient lithospheric mantle beneath the eastern part of North China.     

新疆拜城县波孜果尔A型花岗岩类矿物学特征及岩浆形成的温度条件

新疆拜城县波孜果尔A型花岗岩类为富含铌、钽、锆等有用元素的含矿岩体。通过偏光显微镜、电子探针(EPMA)化学成分分析、电子探针背散射(BSE)对波孜果尔A型花岗岩类的矿物学特征进行了研究,并对岩浆形成的温度条件与构造背景进行了讨论。结果表明,波孜果尔A型花岗岩类包括霓石钠闪石英碱性长石正长岩、霓石钠闪碱性长石花岗岩、黑云母碱性长石正长岩3种岩石类型。主要造岩矿物包括石英、钠长石、钾长石、霓石、钠铁闪石和铁叶云母。副矿物包括锆石、烧绿石、钍石、萤石、独居石、氟碳铈镧矿、磷钇矿等。岩浆平均温度832~839℃,形成于非造山的板内构造环境,且具高温、无水、低氧逸度的成岩特点。     

不同来源两个系列Li-F花岗岩的同位素组成区别

根据地质和地球化学特点,特别是同位素组成,将Li-F花岗岩划分为浅源南岭系列(系列Ⅰ)和深源长江系列(系列Ⅱ).系列Ⅰ的δO18＞10‰,ISr＞0.7100,εNd(t)＜-6,在207Pb/204Pb-206Pb204Pb铅同位素构造图上位于上地壳线附近;系列Ⅱ的δ18O＜10‰,ISr＜0.7100,εNd(t)＞-6,在207Pb/204Pb-206Pb/204铅同位素构造图上位于地幔线与造山带线之间.说明浅源南岭系列Li-F花岗岩物质来源比较浅,以上地壳(再循环地壳)物质为主,而深源长江系列Li-F花岗岩物质来源比较深,以地幔、下地壳和造山带(原生地壳)物质为主.     

Phase transformations and inherited lattice preferred orientations: implications for seismic properties

In phase transitions via either the martensitic (diffusionless shear) or nucleation and growth mechanism a specific orientation relationship may exist between the two phases. In cases where the orientation relationship is known, the lattice preferred orientation (LPO) inherited by the new phase may be calculated from the LPO of the old phase. The method of calculation is presented in a form suitable for the spherical harmonic method of texture analysis using the orientation distribution function (ODF). Examples are presented for the -β-quartz, calcite-aragonite, orthopyroxene-clinopyroxene and olivine-spinel transformations.

The seismic properties of the transformed and untransformed phases are calculated from the ODF and the single crystal elastic constants. In particular the -β quartz transformation is considered in detail. The quartz polycrystal is very anisotropic in the alpha field (V_p anisotropy coefficient, A = 8.1%) and almost isotropic in the β-field (A = 2.1%). The transition is accompanied by V_p velocity increase of 0.6 km/s. In the other example discussed, olivine-β-spinel, there is also a decrease in V_p anisotropy coefficient from 11.1% (olivine) to 4.0% (β-spinel). The estimate of the volume fraction of olivine at the 400 km discontinuity (associated with this phase transition) is shown to depend on the direction of wave propagation.     

Late Proterozoic older granitoids from the North Eastern desert of Egypt: petrogenesis and geodynamic implications

Major, trace, and REE data for three localities of calc?Calkaline older granitoid rocks exposed in the north Eastern Desert of Egypt are presented. These rocks were selected to cover wide compositional spectrum of the Egyptian older granitoid varieties. They are petrographically represented by granodiorite, tonalite, quartz?Cdiorite, and quartz?Cmonzodiorite. The rocks are comparable with the peraluminous, unfractionated calc?Calkaline suites and fall within the volcanic arc and I-type granite fields. So, they can be regarded as belonging to the volcanic arc collision stage (665?C614?Ma). The granitoids are geochemically similar to other rocks recorded from continental margin arc-systems being exhibit light-REE enriched patterns with variable but chiefly positive Eu anomaly. The latter has reverse relationship with the ??REE, which was attributed to the fractionation of hornblende during partial melting. These patterns are comparable with models involving partial melting of amphibolitic source. This source must represent basalts, gabbros, or volcanics of an island arc system that were transformed to the level of the island arc crust during continental growth where the P?CT conditions are suitable for partial melting. Thus, it is plausible that the studied rocks were derived by partial melting of LREE-enriched, garnet-free, and amphibole-bearing (i.e., hydrated) mafic source. Wadi Milaha granitoids are consistent with the derivation by a high degree of partial melting (30?C40%) of amphibolite protolith in the deep crust. However, the two other localities (Wadi Umm Anab and West Gharib) are matching with 20?C30% partial melting. Within each locality, variation in rock types from granodiorite to tonalite is said to be dominated by variable degree of restite separation during magma ascent. The high water and volatile contents in Wadi Milaha granitoids allowed higher degree of partial melting (30?C40%). Moreover, the lower volatile contents in the other two localities (Wadi Umm Anab and West Gharib) gave lower degrees of partial melting (20?C30%). These processes may resemble important geodynamic features of the Arabo-Nubian Shield evolution in the north Eastern Desert of Egypt.     

Geochemistry of lavas from Mohns Ridge,Norwegian-Greenland Sea: implications for melting conditions and magma sources near Jan Mayen

 Mohns Ridge lavas between 71 and 72°30′N (∼360 km) have heterogeneous compositions varying between alkali basalts and incompatible-element-depleted tholeiites. On a large scale there is a continuity of incompatible element and isotopic compositions between the alkali basalts from the island Jan Mayen and Mohns Ridge tholeiites. The variation in isotopes suggests a heterogeneous mantle which appears to be tapped preferentially by low degree melts (∼5%) close to Jan Mayen but also shows its signature much further north on Mohns Ridge. Three lava types with different incompatible element compositions [e.g. chondrite-normalized (La/Sm)_N<1 to >2] occur in the area at 72°N and were generated from this heterogeneous mantle. The relatively depleted tholeiitic melts were mixed with a small degree melt from an enriched source. The elements Ba, Rb and K of the enriched melt were probably buffered in the mantle by residual amphibole or phlogopite. That such a residual phase is stable in this region of oceanic mantle suggests both high water contents and low mantle temperatures, at odds with a hotspot origin for Jan Mayen. Instead we suggest that the melting may be induced by the lowered solidus temperature of a “wet” mantle. Mohns MORB (mid ocean ridge basalt) and Jan Mayen area alkali basalts have high contents of Ba and Rb compared to other incompatible elements (e.g. Ba/La >10). These ratios reflect the signature of the mantle source. Ratios of Ce/Pb and Rb/Cs are normal MORB mantle ratios of 25 and 80, respectively, thus the enrichments of Ba and Rb are not indicative of a sedimentary component added to the mantle source but were probably generated by the influence of a metasomatizing fluid, as supported by the presence of hydrous phases during the petrogenesis of the alkali basalts. Geophysical and petrological models suggest that Jan Mayen is not the product of hotspot activity above a mantle plume, and suggest instead that it owes its existence to the unique juxtaposition of a continental fragment, a fracture zone and a spreading axis in this part of the North Atlantic. Received: 3 May 1995 / Accepted: 6 November 1995     

Lattice-preferred orientation of olivine found in diamond-bearing garnet peridotites in Finsch,South Africa and implications for seismic anisotropy

Seismic anisotropy in the upper mantle provides important constraints on mantle dynamics, continental evolution and global tectonics and is believed to be produced by the flow-induced lattice-preferred orientation (LPO) of olivine. Recent experimental studies at high pressure and temperature have suggested that the LPO of olivine is affected by pressure in addition to water and stress. However, there has been no report yet for the pressure-induced LPO of natural olivine because samples from the deep upper mantle are rare and often unsuitable for study due to ambiguous foliation and lineation. Here we show evidence of the pressure-induced LPO of natural olivine in diamond-bearing garnet peridotites from Finsch, South Africa. We found that the [010] axes of olivine are aligned subnormal to foliation and that the [001] axes are aligned subparallel to lineation, which is known as B-type LPO of olivine. The equilibrium pressure of the samples, as estimated using geobarometer, was greater than 4 GPa, indicating that the samples originated from a depth greater than ∼120 km. In addition, FTIR spectroscopy of the olivine showed that the samples are dry, with a water content of less than 90 ± 20 ppm H/Si (5.5 ± 1.2 ppm wt. H₂O). These data suggest that the samples are the first natural examples of olivine displaying B-type LPOs produced due to high pressure under dry condition. Our data indicate that the trench-parallel seismic anisotropy observed in many subduction zones in and below subducting slabs at depths greater than ∼90 km under dry condition may be attributed to the pressure-induced olivine fabrics (B-type LPO) and may be interpreted as the entrainment of the sub-lithospheric mantle in the direction of subduction rather than anomalous trench-parallel flow.