云南三江口地区超基性岩岩石化学及成因   总被引：1，自引：0，他引：1  

俞赛赢  杨仕潘 《云南地质》2005,24(1):83-88

三江口地区超基性岩按岩石类型可分六种,岩石的m/f值小于6 5,属铁质超基性岩,呈包体状产于下二叠统木星土岩组(P1mx.)及上二叠统洛吉组(P2lj)中,与其为同源异相产物,形成于板块裂陷环境。岩浆活动时期大致为晚古生代 早三叠世早期,可能代表古特提斯形成的早期阶段。成果为进一步研究和恢复该区古构造格局提供重要依据。  相似文献   

矿产开发与环境保护   总被引：4，自引：0，他引：4  

郭真 《吉林地质》1997,16(2):11-16

通过国内多个矿区实例，较系统地叙述了矿产资源开发导致的生态环境破坏和污染状况。表明矿产开发中对环境污染的途径包括河流、土壤、等。最后简要介绍了国内、国外几种对采矿污染比较有效的防治措施。  相似文献   

Viscosity of peridotite liquid up to 13 GPa: Implications for magma ocean viscosities     

Christian Liebske  Bettina Schmickler  Hidenori Terasaki  Brent T. Poe  Akio Suzuki  Ken-ichi Funakoshi  Ryota Ando  David C. Rubie 《Earth and Planetary Science Letters》2005,240(3-4):589-604

The viscosity of synthetic peridotite liquid has been investigated at high pressures using in-situ falling sphere viscometry by combining a multi-anvil technique with synchrotron radiation. We used a newly designed capsule containing a small recessed reservoir outside of the hot spot of the heater, in which a viscosity marker sphere is embedded in a forsterite + enstatite mixture having a higher solidus temperature than the peridotite. This experimental setup prevents spheres from falling before a stable temperature above the liquidus is established and thus avoids difficulties in evaluating viscosities from velocities of spheres falling through a partially molten sample.

Experiments have been performed between 2.8 and 13 GPa at temperatures ranging from 2043 to 2523 K. Measured viscosities range from 0.019 (± 0.004) to 0.13 (± 0.02) Pa s. At constant temperature, viscosity increases with increasing pressure up to  8.5 GPa but then decreases between  8.5 and 13 GPa. The change in the pressure dependence of viscosity is likely associated with structural changes of the liquid that occur upon compression. By combining our results with recently published 0.1 MPa peridotite liquid viscosities [D.B. Dingwell, C. Courtial, D. Giordano, A. Nichols, Viscosity of peridotite liquid, Earth Planet. Sci. Lett. 226 (2004) 127–138.], the experimental data can be described by a non-Arrhenian, empirical Vogel-Fulcher-Tamman equation, which has been modified by adding a term to account for the observed pressure dependence of viscosity. This equation reproduces measured viscosities to within 0.08 log₁₀-units on average. We use this model to calculate viscosities of a peridotitic magma ocean along a liquid adiabat to a depth of  400 km and discuss possible effects on viscosity at greater pressures and temperatures than experimentally investigated.  相似文献   

再论察尔汗盐湖达布逊二级补给系统S3盐层晶间卤水分异问题          下载免费PDF全文

徐少康 《盐湖研究》1995,3(4):23-33

本湖Ｓ３盐层晶间卤水（简称晶卤）分异的成因是一个与钾盐矿床的成因及最佳开发密切相关的基本理论问题。文献［１－２］提出了晶卤分异成因新观点（阶段性淡化说）的基本理论框架。继文献［３］之后，本文对晶卤分异的又一复杂地区进行了深入解剖，为阶段性淡化说再次提供大量事实依据，具有一定的理论和经济意义。  相似文献   

暖温带地理景观中土壤硒的分异特征   总被引：17，自引：0，他引：17  

侯少范  李德珠等 《地理学报》1992,47(1):31-39

本文按垂直自然带谱研究了暖温带地理景观中山地草旬土、山地棕壤、山地淋溶褐土和潮土中硒的分异特征。结果表明：（1）硒在土剖面上的分异，除受生物富集的影响外，淋溶和粘人作用强烈地制约着硒在剖面上的迁移；（2）不同机械组分中的硒含量以粘粒中最高，呈明显的粘粒＞细粉粒＞中粉粒＞砂粒序列。因此，成土过程中，不同机械组分以及次生或们生矿物和垂直运动和自然分选作用对土壤硒的地理分异具有非常重要的作用。（3）易于淋溶失的有机态或钙结合的硒对所研究的土壤表层硒的贡献都大于50％。提出淋溶作用是我国低硒带形成的主要外营力。  相似文献   

青藏高原地理环境研究进展   总被引：27，自引：4，他引：23  

郑度  李炳元 《地理科学》1999,19(4):295-302

经三纪青藏地区曾二次隆升与夷平,３,４Ｍａ以来经历了高原强烈隆起,现代季风形成,高原山地抬升、进入冰冻圈,环境剧烈波劝,高原内部干旱化及全新世环境波动变化等古寺理演化阶段。  相似文献   

以高斯理论为基础计算弯曲钻孔节点空间坐标   总被引：1，自引：0，他引：1  

朱学立  燕长海  胡安国  李荣成 《物探化探计算技术》2007,29(6):545-549

为了拟合出更加接近钻孔实际的曲线,结合钻孔测斜实际,以严密的高斯理论为基础,给出了以钻孔天顶角和倾角为参数的弯曲钻孔的参数方程。并在此基础上,推出了钻孔曲线各点的计算公式,更准确地描述了钻孔的实际情况,为后续工作剖面图的绘制和储量计算提供了基础。这里使用高斯和折线法作为一个实例,对比计算了赤土店铅锌矿区ZK13002钻孔。计算结果表明:在钻孔曲线形状、累计弧长、插值点特征等多个方面的高斯法都优于折线法,而因算法的改变引起的工作量又是很小的。  相似文献   

制冷控制系统研制与探析     

吴鹏  郑勇  路杰 《大地测量与地球动力学》2011,31(Z1):157-160

根据实际应用研制制冷控制系统,该系统采用温度测量、PID控制及PWM脉宽调制等技术实现了对目标对象的制冷处理,具有一定的应用价值。  相似文献   

Internal structure of Europa and Callisto     

O.L. Kuskov  V.A. Kronrod 《Icarus》2005,177(2):550-569

Models of the internal structure of completely differentiated Europa and partially differentiated Callisto have been constructed on the basis of Galileo gravity measurements, geochemical constraints on composition of ordinary and carbonaceous chondrites, and thermodynamic data on the equations of state of water, high-pressure ices, and meteoritic material. We assume thermal and mechanical equilibrium for the interiors of the satellites. A geophysically and geochemically permissible thickness of Europa's outer water-ice shell lies between 105 and 160 km (6.2-9.2% of total mass). Our results show that the bulk composition of the rock-iron core of Europa may be described by material approaching the L/LL-type chondrites in composition, but cannot be correlated either with the material of CI chondrites or H chondrites. For Europa's L/LL-chondritic models, core radii are estimated to be 470-640 km (5.3-12.5% of total mass). The allowed thickness of Europa's H₂O layer ranges from 115±10 km for a differentiated L/LL-type chondritic mantle with a crust to 135±10 km for an undifferentiated mantle. We show that Callisto must only be partially differentiated into an outer ice-I layer, a water ocean, a rock-ice mantle, and a rock-iron core (mixture of anhydrous silicates and/or hydrous silicates + FeFeS alloy). We accept that the composition of the rock-iron material of Callisto is similar to the bulk composition of L/LL-type chondritic material containing up to 10-15% of iron and iron sulfide. Assuming conductive heat transfer through the ice-I crust [Ruiz, 2001. The stability against freezing of an internal liquid-water ocean on Gallisto. Nature, 412, 409-411], heat flows were estimated and the possibility of the existence of a water ocean in Callisto was evaluated. The liquid phase is stable (not freezing) beneath the ice crust, if the heat flow is between 3.3 and 3.7 mW m⁻², which corresponds to the heat flow from radiogenic sources. The thickness of the ice-I crust is 135-150 km, and that of the underlying water layer, 120-180 km. The results of modeling support the hypothesis that Callisto may have an internal liquid-water ocean. The allowed total (maximum) thickness of the outer water-ice shell is up to 270-315 km. Rock-iron core radii, depending on the presence or absence of hydrous silicates, do not exceed 500-700 km, the thickness of an intermediate ice-rock mantle is not less than 1400 km, and its density is in the range of 1960-2500 kg m⁻³. The surface temperature of Callisto is expected to be 100-112 K. The total amount of H₂O in Callisto is found to be 49-55 wt%. The correspondence between the density and moment of inertia values for bulk ice-free Io, rock-iron core of ice-poor Europa, and rock-iron cores of Ganymede and Callisto shows that their bulk compositions may be, in general, similar and may be described by the composition close to a material of the L/LL-type chondrites with the (Fe_tot/Si) weight ratios ranging from 0.9 to 1.3. Planetesimals composed of these types of ordinary chondrites could be considered as analogues of building material for the rock-iron cores of the Galilean satellites. Similarity of bulk composition of the rock-iron cores of the inner and outer satellites implies the absence of iron-silicon fractionation in the protojovian nebula.  相似文献   

The intermediate step in fractionation trends of mildly alkaline volcanic suites: An experimental insight from the Pavin trachyandesite (Massif Central,France)     

《Comptes Rendus Geoscience》2019,351(8):525-539

We examined magma storage conditions and eruptive dynamics for the trachyandesite (~58 wt% SiO₂, 9–10 wt% alkalis) of the Pavin monogenetic volcano, a maar-like explosive crater belonging to a small group of youngest volcanoes in the Massif Central. By confronting the natural samples to experimental products, we constrained pre-eruptive conditions around 950–975 °C, 150–200 MPa (~5.5–7.0 km in depth), NNO+1.5, and 4.5–5.5 wt% melt H₂O. There is petrological evidence of magma crystallization in the conduit up to shallow levels (~50 MPa; 2 km in depth) before fragmentation into pumice clasts in the last kilometre of ascent. The experiments highlight the role of biotite and of crystallization pressure in defining separate compositional trends of residual liquids, i.e. alkaline (trachytes) versus sub-alkaline (dacite-rhyolite).  相似文献