榴辉岩的化学分类

以山东荣成地区的榴辉岩为例,把榴辉岩分为镁一榴辉岩、铁一榴辉岩和钙一榴辉岩三类。三类榴辉岩的岩石化学,主要造岩矿物成分都有明显差别,石榴石分别是镁铝榴石、铁铝榴石和钙铝榴石。绿辉石的硬玉分子也有不同。三类榴辉岩的化学成分限制是Mg-榴辉岩MgO>10%,石榴石以镁铝榴分子占优势,Fe-榴辉岩的MgO<10,石榴石以铁铝榴石分子占优势。Ca-榴辉岩CaO>19%,石榴石以钙铝榴石分子优势。     

吉林省地质灾害类型及防治对策探讨

本文针对吉林省的地质灾害类型及各类地质灾害的成因，分布及其危害进行了论述。对其防治对策进行了探讨，提出了切合本省实际的五项防治措施。     

天津盛夏降水趋势与初夏华北高压的统计分析

根据初夏(6月)的天气气候演变，预测盛夏(7～8月)的短期气候趋势，一直是急需解决的难题。文章揭示了自1958年以来天津盛夏降水趋势与初夏时节临近地区上空的环流特征之间的统计关系。结果表明，初夏华北高压强时盛夏天津降水偏少，反之盛夏天津降水偏多，不仅逐年的对应关系显著，而且变化趋势相反，转折时期也一致。初步解释了20世纪70年代以前天津(华北)盛夏多雨和80年代至今天津(华北)少雨的物理原因。以此为主要根据建立了初夏对于盛夏天津降水的短期气候预测方法，1998～2003年连续6年预报正确。     

北京连续降雪过程分析

该文对2002年12月份北京出现的1841年以来历史上最长的连续6天的降雪天气进行了合成分析和诊断分析。北半球合成环流形势显示，连续降雪发生在东亚稳定的纬向环流形势下，其上游地区强大经向环流和阻塞高压使中纬度东亚和西太平洋纬向环流得以维持。东亚合成环流的垂直结构表明，连续降雪期间华北地区始终处于锋区中，并存在低空辐合、高空辐散的散度场垂直分布结构。卫星水汽云图显示出有水汽通道向河套倒槽云系输送水汽。华北地区的诊断分析表明，地面和边界层中山东地区分裂高压南侧向北回流的偏南气流是造成降雪的主要水汽通道。变形场的流场结构使水汽在北京附近辐合。垂直剖面展现了华北回流降雪天气近地面层的浅薄的冷空气垫，和暖湿空气回流在冷空气垫上的爬升，并在其上形成一个浅薄的饱和层。     

青藏高原影响亚洲夏季气候研究的最新进展

文中回顾了近 10a来吴国雄等在青藏高原影响亚洲夏季气候研究方面的最新进展。通过分析东西风交界面的演变证明 ,由于青藏高原的春季加热 ,亚洲季风区对流层低层冬季盛行偏东风转变为夏季偏西南风最早发生在孟加拉湾东部 ,与其相伴随的激烈对流降水出现在其东面。因此孟加拉湾东部至中印半岛西部是亚洲季风最早爆发的地区。同时也指出盛夏伊朗高原和青藏高原加热所激发的同相环流嵌套在欧亚大陆尺度的热力环流中 ,从而加强了东亚的夏季风 ,加剧了中西亚的干旱 ;并通过其所激发的波动对夏季东亚的气候格局产生重要影响。文中还比较了夏季南亚高压的伊朗模态和青藏模态性质的异同及其对亚洲夏季降水异常分布的不同影响。     

喜马拉雅中段高压麻粒岩变质作用、地球化学与年代学

研究的高压麻粒岩发现于西藏亚东以北约40公里的(Zherger-La)、出露在藏南拆离系(STDS)主构造面下盘的高喜马拉雅结晶岩系中,是继喜马拉雅东西构造结的Nanga Barbat、Namjag Barwa和喜马拉雅中段Khatra & Marina地区、定结地区发现的榴辉岩或高压麻粒岩之后,在青藏高原上新近发现的高压麻粒岩.该麻粒岩呈岩片被包裹于花岗质片麻岩中.麻粒岩记录了两期变质作用,早期矿物组合为Grt+Cpx+Pl+Qz,属麻粒岩相变质产物,矿物成分分析显示早期矿物组合达到了平衡,并且没有表现成分扩散;后期矿物组合为Hbl+Pl+Bio或Opx+Pl,指示了较高温但相对压力较低的麻粒岩相退变变质作用,矿物成分分析和结构显示了退变作用没有达到变质平衡.显微结构可以观察到多组变质反应Grt+Cpx+Qtz=Opx+Pl,Grt+Qtz=Opx+Pl,Grt+Cpx+L=Hbl+Pl+Bio+Mt,和Cpx+L=Hbl+Mt.根据矿物平衡关系,利用Grt-Cpx温度计和Grt-Cpx-Pl-Qz压力计估算的早期变质作用温压为T=780～850℃,P=12～15kbar,相对应的地温梯度16℃～18℃/km.借用Hbl-Pl温度计和A1tot in Hbl压力计估算的晚期变质作用温压为T=730～760℃;P=4～6kbar,相当的地温梯度为38℃～50℃/km.变质作用P-T演化呈等温降压轨迹,指示麻粒岩地体从增厚(或俯冲)地壳到减薄增温(或部分熔融)地壳,进而被快速剥露地表的构造过程.初步的地球化学结果表明高压麻粒岩原岩可能相当于大陆拉斑玄武岩.麻粒岩锆石SHRIMP年代学有两组相对集中的年龄分别为98±5 Ma(5 spots)和17.0±0.3 Ma(13 spots).高压麻粒岩的两期变质作用的温度都在700℃以上,略高于锆石U-Pb同位素体系计时封闭温度,推断17 Ma是高压麻粒岩变质后发生折返,随高喜马拉雅结晶岩系剥露冷却的年龄;98.4Ma的测年结果被推测是高压麻粒岩原岩形成的年龄.在喜马拉雅山,高压麻粒岩记录了类似增厚地壳到减薄地壳的转变一方面可能是地壳深部作用机制的转变,另一方面,这种机制与喜马拉雅南坡巨大的降雨量和去顶作用有密切关系,意义重大.     

High-pressure experimental growth of diamond using C–K2CO3–KCl as an analogue for Cl-bearing carbonate fluid

High-pressure, high-temperature diamond growth experiments have been conducted in the system C–K₂CO₃–KCl at 1050–1420 °C, 7.0–7.7 GPa. KCl is of interest because of the strong effect of halogens on the phase relations of carbonate-rich systems [Geophys. Res. Lett. 30 (2003) 1022] and because of the occurrence of KCl coexisting with alkali silicate–carbonate fluids in natural-coated diamond [Geochim. Cosmochim. Acta 64 (2000) 717]. We have used system C–K₂CO₃–KCl as an analogue for these mantle fluids in diamond growth experiments. The presence of KCl reduces the potassium carbonate liquidus to ≤1000 °C at 7.7 GPa, allowing it to act as a solvent catalyst for diamond growth at temperatures below the continental geotherm. This is a reduction on the minimum diamond growth temperature reported in the alkali-carbonate–C–O–H system [Lithos 60 (2002) 145]. Diamond growth using carbonate solvent catalysts is characterised by a relatively long induction period. However, the addition of KCl also reduced the period for diamond growth in carbonate to 5 min; no such induction period appears to be necessary. It is suggested that KCl destabilises carbonate, allowing greater solubility and diffusion of carbon.     

Experimental and theoretical study of stability of dense hydrous magnesium silicates in the deep upper mantle

Fluid-undersaturated experiments were conducted to determine the phase relations in the simplified peridotite system MgO-SiO₂-H₂O (MSH) at 11.0-14.5 GPa and 800-1400 °C. Stability relations of dense hydrous magnesium silicates (DHMSs) under fluid-undersaturated conditions were experimentally examined. From the fluid-absent experimental results, we retrieved thermodynamic data for clinohumite, phase A, phase E, and hydrous wadsleyite, consistent with the published data set for dry mantle minerals. With this new data set, we have calculated phase equilibria in the MSH system including dehydration reactions. The dehydration reactions calculated with lower water activities of 0.68-0.60 match the fluid-present experiments of this study above 11.0 GPa and 1000 °C, indicating that considerable amounts of silicate component were dissolved into the fluid phase. The calculated phase equilibria illustrate the stability of the post-antigorite phase A-bearing assemblages. In the cold subducting slab peridotite, phase A + enstatite assemblage survives into the transition zone, whereas phase A + forsterite + enstatite assemblage forms hydrous wadsleyite at a much shallower depth of about 360-km. The slab is subducted with no dehydration reactions occurring when entering the transition zone. The phase equilibria also show the high temperature stability of phase E. Phase E is stable up to 1200 °C at 13.5 GPa, a plausible condition in the mantle of relatively low temperature, i.e., beneath subduction zones. Phase E is a possible water reservoir in the mantle as well as wadsleyite and ringwoodite.     

Polymorphic phase transition in Superhydrous Phase B

We synthesized superhydrous phase B (shy-B) at 22 GPa and two different temperatures: 1200°C (LT) and 1400°C (HT) using a multi-anvil apparatus. The samples were investigated by transmission electron microscopy (TEM), single crystal X-ray diffraction, Raman and IR spectroscopy. The IR spectra were collected on polycrystalline thin-films and single crystals using synchrotron radiation, as well as a conventional IR source at ambient conditions and in situ at various pressures (up to 15 GPa) and temperatures (down to −180°C). Our studies show that shy-B exists in two polymorphic forms. As expected from crystal chemistry, the LT polymorph crystallizes in a lower symmetry space group (Pnn2), whereas the HT polymorph assumes a higher symmetry space group (Pnnm). TEM shows that both modifications consist of nearly perfect crystals with almost no lattice defects or inclusions of additional phases. IR spectra taken on polycrystalline thin films exhibit just one symmetric OH band and 29 lattice modes for the HT polymorph in contrast to two intense but asymmetric OH stretching bands and at least 48 lattice modes for the LT sample. The IR spectra differ not only in the number of bands, but also in the response of the bands to changes in pressure. The pressure derivatives for the IR bands are higher for the HT polymorph indicating that the high symmetry form is more compressible than the low symmetry form. Polarized, low-temperature single-crystal IR spectra indicate that in the LT-polymorph extensive ordering occurs not only at the Mg sites but also at the hydrogen sites.     

Nine thousand years of upper montane soil/vegetation dynamics from the summit of Caratuva Peak,Southern Brazil

Biodiversity loss, climate change, and increased freshwater consumption are some of the main environmental problems on Earth. Mountain ecosystems can reduce these threats by providing several positive influences, such as the maintenance of biodiversity, water regulation, and carbon storage, amongst others. The knowledge of the history of these environments and their response to climate change is very important for management, conservation, and environmental monitoring programs. The genesis of the soil organic matter of the current upper montane vegetation remains unclear and seems to be quite variable depending on location. Some upper montane sites in the very extensive coastal Sea Mountain Range present considerable organic matter from the late Pleistocene and other from only the Holocene. Our study was carried out on three soil profiles (two cores in grassland and one in forest) on the Caratuva Peak of the Serra do Ibitiraquire (a sub-range of Sea Mountain Range – Serra do Mar) in Southern Brazil. The δ¹³C isotopic analyses of organic matter in soil horizons were conducted to detect whether C₃ or C₄ plants dominated the past communities. Complementarily, we performed a pollen analysis and ¹⁴C dating of the humin fraction to obtain the age of the studied horizons. Except for a short and probably drier period (between 6000 and 4500 cal yr BP), C₃ plants, including ombrophilous grasses and trees, have dominated the highlands of the Caratuva Peak (Pico Caratuva), as well as the other uppermost summits of the Serra do Ibitiraquire, since around 9000 cal yr BP. The Caratuva region represents a landscape of high altitude grasslands (campos de altitude altomontanos or campos altomontanos) and upper montane rain/cloud forests with soils that most likely contain some organic matter from the late Pleistocene, as has been reported in Southern and Southeastern Brazil for other sites. However, our results indicate that the studied deposits (near the summit) are from the early to late Holocene, when somewhat wetter and warmer conditions (since around 9000 cal yr BP) enabled a stronger colonization of the ridge of Pico Caratuva by mainly C₃ plants, especially grassland species. However, at the same time, even near the summit, the soil core from the forest site already presented the current physiognomy (or a shrubby/elfin or successional forest), indicating that the colonization of the neighboring uppermost saddles and valleys were probably populated mainly by upper montane forest species.