钝顶螺旋藻的硝酸还原酶与氢酶之间的电子竞争   总被引：2，自引：0，他引：2  

张慧苗  顾天青 《海洋与湖沼》1996,27(2):203-206

于1994年6－11月，运用生物化学方法以钝项螺旋藻为材料制备整体细胞和无细胞提取物。测定表明，整体细胞硝酸还原酶与氢酶活性的相互关系和无细胞提取物氢酶与硝酸还原酶的（对还原甲基紫精）Km值，分别为2．299×10－7mol／L和1．098×10－7mol／L；证实在硝酸还原酶与氢酶之间存在着电子竞争。  相似文献   

����GPS˫Ƶ�ز���λ����Ԫ��������VTEC     

林剑  吴云  周义炎  施顺英  邢乐林 《大地测量与地球动力学》2007,27(5):68-71

?????????μ?????????????????????vertical total electron content??VTEC????????,???????????????????????????????VTEC?????????????????????????VTEC??IGS??International GNSS Service??????VTEC?????仯??????￡????????????????????????????????γ???仯???ɡ?  相似文献   

Evaluating microbial chemical choices: The ocean chemistry basis for the competition between use of O2 or NO3− as an electron acceptor     

《Deep Sea Research Part I: Oceanographic Research Papers》2014

  相似文献   

石榴石钇(Y)元素电子探针分析及应用——以佛子岭石榴云母片岩为例SCIEI北大核心CSCD     

王娟  张妍  宋传中  石永红  侯振辉  王智慧  彭春蕾 《岩石学报》2022,38(3):619-638

石榴石是最重要的造岩矿物之一,通常能够保留早期的矿物结构和物质并记录较为晚期的变形和变质反应。石榴石钇(Y)元素环带特征丰富、复杂,不同的环带特征通常暗示不同的形成环境或经历了不同的变质事件,是变质演化历史研究的重要媒介之一。以往的研究中,多以LA-ICP-MS作为石榴石Y元素的主要分析手段,EPMA主要用于主量元素的分析。但是,LA-ICP-MS的束斑尺寸(44μm)和基底效应较EPMA(0~5μm)大,当石榴石颗粒小、包体和裂隙发育或成分环带以微区尺寸内存在较大变化时,大束斑更容易覆盖某些特殊信息。通过对石榴石Y元素测试参数的调试和标样验证,最终确定峰位测试时长和背景测试时长分别为140s和70s,并进行了PHA谱峰干扰剥离,降低检测限至54×10^(-6)。本文将通过对比佛子岭石榴云母片岩(LD025)4颗石榴石的EPMA主、微量原位分析(Ca、Mg、Mn、Fe、Y、Al、Si、Cr、Ti、Na)和LA-ICP-MS石榴石Y元素分析结果,论证EPMA分析Y元素的可行性。石榴石X-ray Mapping和主量成分剖面揭示该4颗石榴石均为生长环带,Mn呈钟形分带,Y与X Sps呈强烈正相关性,与X Grs、X Alm、X Prp相关性不清晰。EPMA和LA-ICP-MS分析结果显示Y含量曲线在核部和幔部具有良好的一致性,Grt1~Grt3中Y均表现出自核部(500×10^(-6)~1200×10^(-6))向幔部(200×10^(-6)~500×10^(-6))逐渐降低,极边部Y含量低(20×10^(-6)~200×10^(-6))且变化复杂;Grt4中Y含量差异相对较小(180×10^(-6)~450×10^(-6)),仅在边部出现不同程度的升降。因EPMA对于Y元素含量较低(<200×10^(-6))时灵敏度不够或者LA-ICP-MS束斑尺寸大容易掩盖边部窄带成分真实变化等原因,二者在边部Y元素差异较大。分别对EPMA和LA-ICP-MS的分析结果应用Grt-Xtm温度计和Grt单矿物压力计获得的变质PT结果显示Grt1~Grt3(核-幔-边)和Grt4(核-边)均记录较为完整、统一的温压演化过程。M1→M2→M3的变质温压变化分别为T=530~544℃、P=0.78~0.82GPa→T=577~616℃、P=0.89~0.98GPa→T=631~661℃、P=1.01~1.07GPa,表现为顺时针演化型式,M1至M3反映的是一个“暖俯冲”过程。根据温度评价结果,Grt1~Grt3(1.2~1.4mm,自形程度高)形成时间应早于Grt4(0.8mm,自形程度低)。由此可知,大颗粒的石榴石Y元素含量及变化特征通常更容易揭示相对完整的变质演化历史。本次研究为变泥质岩演化历史、变质温压评价等研究提供了不同视角和思路,结合EPMA主量(矿物成分、X-ray mapping、BSE分析)和微量元素(Y等)分析能够更加精准、全面地解读地质信息。  相似文献   

纳米比亚湖山铀矿载铀矿物研究     

徐楷  李光来  王仁波  刘晓东  张怀峰  张雄杰  邬斌 《地质论评》2023,69(Z1):209-212

  相似文献   

西藏帮布勒矽卡岩型铅锌矿床闪锌矿化学成分特征及其地质意义     

王永强  王勇  唐菊兴  贺传凯  王海勇  闫鹏刚  冯翼鹏 《地球学报》2023,44(3):485-497

帮布勒矿床是近年来在西藏冈底斯—念青唐古拉多金属成矿带西段新发现的大型矽卡岩型Pb-Zn矿床。闪锌矿作为该矿床的主要矿石矿物之一,其矿相学特征及化学组分对于揭示成矿物理化学条件和流体演化过程具有重要意义。本文选取帮布勒矿床近端及远端矽卡岩中不同世代闪锌矿开展详细的显微结构观察和电子探针成分研究。结果表明,帮布勒矿床闪锌矿可划分为2个世代:第Ⅰ世代闪锌矿主要产于近端矽卡岩,呈暗红色-棕红色,常与乳滴状黄铜矿共生,并交代他形磁铁矿、磁黄铁矿,Fe元素含量较高(部分闪锌矿Fe含量>10%),Zn/Fe值<10;第Ⅱ世代闪锌矿可进一步分为两类:第一类(Ⅱa)闪锌矿在近端及远端矽卡岩中均有发育,呈棕黄色,充填于辉石、石榴子石等矽卡岩矿物间及其裂隙中;第二类(Ⅱb)闪锌矿主要产于远端矽卡岩中,呈黄色-浅黄色,与方铅矿和石英共生,第Ⅱ世代闪锌矿相比于第Ⅰ世代闪锌矿Fe、Mn含量明显偏低,Zn含量较高。闪锌矿Fe元素温度计估算结果显示,从第Ⅰ世代至第Ⅱ世代成矿温度逐渐降低,分别为160～314℃、138～157℃,与闪锌矿Zn/Fe比值指示结果一致。综上证据,本文认为帮布勒矿床早期成矿流体...  相似文献   

Geochronological constraints on uranium mineralization within the Hüttenberg siderite deposit (Eastern Alps,Austria)     

《Chemie der Erde / Geochemistry》2021,81(1):125678

A small-scale hydrothermal uranium mineralization hosted within the siderite deposit at Hüttenberg (Eastern Alps, Austria) was re-investigated using modern scanning electron microscope (SEM) and microprobe (EMPA) methods. The uranium mineralization comprises brannerite, coffinite and uraninite, and is spatially associated with Fe-, Ni- and Co-arsenides (loellingite, rammelsbergite, safflorite), bismuth and bismuthinite, as well as rare accessory silver-bearing minerals and gold locally. The U-bearing fluids also carried P, Y and REEs, which precipitated as xenotime and P–Y coffinite. The uranium mineralization paragenetically postdates the metasomatic formation of the host siderite ore.Uraninite allows for precise single spot EMPA ages to be calculated (±2 Ma) due to its high radiogenic lead content. There is an excellent internal consistency in the uraninite data with calculated dates ranging between 77 and 84 Ma. We interpret that these record the crystallization age of the uraninite, and that any influences of lead loss or common Pb are minimal. Brannerite was also analyzed but U-total Pb microprobe data scatter (c.30–80 Ma) with evidence of lead loss, particularly in altered domains. It does, however, provide a minimum constraint on the timing of mineralization that is consistent with the crystallization age of the uraninite. Coffinite proved completely unsuitable for U-total Pb geochronology due to extreme lead loss. However, hydrothermal xenotime yields a U-total Pb age of 78 ± 5 Ma, consistent with the uraninite age. Therefore, the U-total Pb geochronological data support a late Cretaceous age for the U-mineralization of c. 80 Ma. Considering this timing constraint together with other geological and indirect thermochronological aspects, we conclude that the siderite deposit of Hüttenberg is older and formed at c. 90−80 Ma.  相似文献   

Characterisation of deformation and flow mechanics around porphyroclasts in a calcite marble ultramylonite by means of EBSD analysis   总被引：1，自引：0，他引：1  

Michel Bestmann  David J. Prior  Bernhard Grasemann 《Tectonophysics》2006,413(3-4):185-200

This paper studies the flow heterogeneity around porphyroclasts associated with greenschist facies deformation of a calcite marble shear zone. Microstructural data from electron backscatter diffraction analyses (EBSD) are used to constrain the flow mechanics of this dominantly non-coaxial type of deformation. The microstructure of the undisturbed ultramylonite (grain-size range 5–100 μm, mean 40 μm) is interpreted to represent steady-state (time-independent) flow conditions with flow planes parallel to the shear zone boundary. Single calcite porphyroclasts (grain-size 1–3 mm) caused flow perturbation in the fine-grained marble ultramylonite. It is the shape, in particular, of these rigid porphyroclasts that controls their rotational behaviour during deformation and, therefore, the development of specific flow fabrics. The flow planes around elongated-rhomboidal, stable porphyroclasts change the orientation to become roughly parallel to the porphyroclast margin, whereas the geometry of flow planes around nearly equant, rotating porphyroclasts describes a δ-type flow pattern. We infer that to some extent decoupling at the clast–matrix interface has occurred to guarantee a stable orientation of elongated porphyroclasts, but was not sufficient to reduce the rotation rate of equant clasts to zero. According to the flow deflection, the general crystallographic preferred orientation (CPO) with its single c-axis maximum perpendicular to the flow plane is rotated about an axis which is (sub)parallel to the kinematic rotation axis of the shear zone. Ultramylonite microstructures, CPOs and misorientation data are best explained by the dual operation of grain-size-insensitive (dislocation creep with recovery and recrystallization) and grain-size-sensitive (diffusion creep) mechanisms. The limited grain-size reduction around porphyroclasts suggests that the grain-size-insensitive mechanisms controlled rheology.  相似文献   

TandEM: Titan and Enceladus mission   总被引：1，自引：0，他引：1  

《Experimental Astronomy》2009,23(3):893-946

TandEM was proposed as an L-class (large) mission in response to ESA’s Cosmic Vision 2015–2025 Call, and accepted for further studies, with the goal of exploring Titan and Enceladus. The mission concept is to perform in situ investigations of two worlds tied together by location and properties, whose remarkable natures have been partly revealed by the ongoing Cassini–Huygens mission. These bodies still hold mysteries requiring a complete exploration using a variety of vehicles and instruments. TandEM is an ambitious mission because its targets are two of the most exciting and challenging bodies in the Solar System. It is designed to build on but exceed the scientific and technological accomplishments of the Cassini–Huygens mission, exploring Titan and Enceladus in ways that are not currently possible (full close-up and in situ coverage over long periods of time). In the current mission architecture, TandEM proposes to deliver two medium-sized spacecraft to the Saturnian system. One spacecraft would be an orbiter with a large host of instruments which would perform several Enceladus flybys and deliver penetrators to its surface before going into a dedicated orbit around Titan alone, while the other spacecraft would carry the Titan in situ investigation components, i.e. a hot-air balloon (Montgolfière) and possibly several landing probes to be delivered through the atmosphere.  相似文献   

太阳射电尖峰爆与电子回旋共振吸收     

俞雪华  徐民健 《天文学报》1995,36(4):359-366

本文采用等离子体动力学方法，研究了日冕条件下磁化非相对论热等离子体对太阳射电辐射产生的电子回旋共振吸收，并在辐射频率等于电子回旋谐波频率时求得ｎ≥２谐波吸收率的近似表示式，以及其对等离子体温度，出射角度和谐波数的变化规律，在应用部分，讨论了电子回旋共振吸收对于太阳射电尖峰爆发的影响，认为目前观测到的尖峰爆，大多数高能电子束来自日冕的内层。  相似文献