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991.
Cooling rate (CR) effects on the intensity of thermoremanent magnetization has been documented for archaeomagnetic materials, where cooling in laboratory conditions is generally much faster compared to natural cooling rates. Since the latter condition also applies to many volcanic rocks, we have investigated in this study the influences of the CR on the determination of absolute paleointensity using recent basaltic rocks. We used magnetically and thermally stable samples mainly containing Ti-poor pseudo-singledomain titanomagnetites (the most widely used material for Thellier paleointensity experiments). These samples previously succeed in retrieving the strength of laboratory field intensities with the Coe’s version of the Thellier method in a simulated paleointensity experiment using similar cooling rates. Our experimental results indicate that the cooling rate effects produce systematic and significant overestimates of the absolute intensity up to 70%. The effect can be much larger than predicted by Neél theory for non-interacting single-domain grains.  相似文献   
992.
A numerical model (two horizontal dimensions, vertically integrated) is used to investigate the generation of long ocean waves, ranging from 20 min to almost 2 h, at Buenos Aires continental shelf. The domain includes the Río de la Plata estuary and the continental shelf together and extends from 33.5° to 40.5°S latitude, and from 51° to 63°W longitude. Sea-level oscillations are modeled by forcing with passage of atmospheric cold fronts and atmospheric gravity waves. Both forcing mechanisms, which have been present during high activity lapses of long ocean waves, are mathematically implemented. After several numerical simulations, it is concluded that the pressure and wind fields associated to cold fronts do not generate long ocean waves in the area, though they do produce disturbances with periods longer than the tidal ones. On the other hand, it is so concluded that atmospheric gravity waves are an effective mechanism to force long ocean waves. Results obtained show that generation of long ocean waves is highly sensitive depending on the propagation direction and the phase speed of the atmospheric gravity waves. The long ocean wave event detected during the large-amplitude gravity-wave event of 13 October 1985 is successfully simulated. Finally, all our results suggest that atmospheric gravity waves are a highly effective mechanism forcing for the generation of long ocean waves in Buenos Aires coastal waters.  相似文献   
993.
Accurate modeling of storage of carbon dioxide (CO2) in heterogeneous aquifers requires experiments of the capillary pressure as function of temperature and pressure. We present a method with which static drainage and imbibition capillary pressures can be measured continuously as a function of saturation at various temperature (T) and pressure (P) conditions. The measurements are carried out at (TP) conditions of practical interest. Static conditions can be assumed as small injection rates are applied. The capillary pressure curves are obtained for the unconsolidated sand–distilled water–CO2 system. The experimental results show a decrease of drainage and imbibition capillary pressure for increasing CO2 pressures and pronounced dissolution rate effects for gaseous CO2. Significant capillary pressure fluctuations and negative values during imbibition are observed at near critical conditions. The measurement procedure is validated by a numerical model that simulates the experiments.  相似文献   
994.
A series of 88 Vulcanian explosions occurred at the Soufrière Hills volcano, Montserrat, between August and October, 1997. Conduit conditions conducive to creating these and other Vulcanian explosions were explored via analysis of eruptive products and one-dimensional numerical modeling of magma ascent through a cylindrical conduit. The number densities and textures of plagioclase microlites were documented for twenty-three samples from the events. The natural samples all show very high number densities of microlites, and > 50% by number of microlites have areas < 20 μm2. Pre-explosion conduit conditions and decompression history have been inferred from these data by comparison with experimental decompressions of similar groundmass compositions. Our comparisons suggest quench pressures < 30 MPa (origin depths < 2 km) and multiple rapid decompressions of > 13.75 MPa each during ascent from chamber to surface. Values are consistent with field studies of the same events and statistical analysis of explosion time-series data. The microlite volume number density trend with depth reveals an apparent transition from growth-dominated crystallization to nucleation-dominated crystallization at pressures of ∼ 7 MPa and lower. A concurrent sharp increase in bulk density marks the onset of significant open-system degassing, apparently due to a large increase in system permeability above ∼ 70% vesicularity. This open-system degassing results in a dense plug which eventually seals the conduit and forms conditions favorable to Vulcanian explosions. The corresponding inferred depth of overpressure at 250–700 m, near the base of the dense plug, is consistent with depth to center of pressure estimated from deformation measurements. Here we also illustrate that one-dimensional models representing ascent of a degassing, crystal-rich magma are broadly consistent with conduit profiles constructed via our petrologic analysis. The comparison between models and petrologic data suggests that the dense conduit plug forms as a result of high overpressure and open-system degassing through conduit walls.  相似文献   
995.
The ratio of 87Sr/86Sr was measured from different water samples of thermal/mineral (hot spring as well as crater lake) and meteoric origins, in order to specify the location and to verify the detailed model of a volcano-hydrothermal system beneath Zao volcano. The ratio showed a trimodal distribution for the case of thermal/mineral water: 0.7052–0.7053 (Type A, Zao hot spring), 0.7039–0.7043 (Type B, Okama crater lake and Shin-funkiko hot spring), and 0.7070–0.7073 (Type C, Gaga, Aone, and Togatta hot springs), respectively. However, in comparison, the ratio was found to be higher for meteoric waters (0.7077–0.7079). The water from the central volcanic edifice (Type B) was found to be similar to that of nearby volcanic rocks in their Sr isotopic ratio. This indicates that the Sr in water was derived from shallow volcanic rocks. The 87Sr/86Sr ratio for water from the Zao hot spring (Type A) was intermediate between those of the pre-Tertiary granitic and the Quaternary volcanic rocks, thus suggesting that the water had reacted with both volcanic and granitic rocks. The location of the vapor–liquid separation was determined as the boundary of the pre-Tertiary granitic and the Quaternary volcanic rocks by comparing the results of this strontium isotopic study with those of Kiyosu and Kurahashi [Kiyosu, Y., Kurahashi, M., 1984. Isotopic geochemistry of acid thermal waters and volcanic gases from Zao volcano in Japan. J. Volcanol. Geotherm. Res. 21, 313–331.].  相似文献   
996.
根据1993年我国28个台站地面及高空气象要素资料,拟合出这28个台站所在地区整层大气可降水量同地面湿度参量(地面水汽压、地面露点)关系的经验表达式,并且在此基础上,通过引进地理纬度ψ和海拔高度H两个参量,将经验系数参数化,建立起由地面湿度参量计算整层大气可降水量的经验计算模式.另外还拟合出这些地区整层大气有效水汽含量同可降水量关系的经验表达式,提出一个先由地面湿度参量计算整层大气可降水量,再由此计算出整层大气有效水汽含量的方法.  相似文献   
997.
岩石磁性与低温流体成矿作用关系探讨   总被引:4,自引:0,他引:4  
大量研究表明 ,低温流体通过改变岩石中磁性矿物的组成而改变了岩石的磁化率和剩磁等磁性参数 ,利用岩石磁学和古地磁学的方法能够帮助区分不同时期和类型的流体事件。笔者认为流体对围岩的影响受岩石组织类型的控制 ,通过研究岩石组织类型可望了解磁性矿物转变和重磁化的机制。文章通过金矿围岩地球化学和磁性参数对比的实例分析 ,提出岩石组织内部磁场也可能对流体的成矿作用发生重要影响。流体在萃取围岩中有用元素或发生成矿物质聚集的同时也可能导致新的磁性矿物形成。在此过程中 ,磁性矿物的晶体生长以化学剩磁的方式记录下环境磁场 ,由此可以研究流体运移轨迹。  相似文献   
998.
断裂构造研究进展对工程地质学的启示   总被引:4,自引:0,他引:4  
在长期地质作用下形成的岩体和岩体结构是工程地质学研究的基本内容,它们的形成和演化主要受控于构造作用,而系统地解析体所经历的构造作用是认知岩体结构,抽象和概括岩体工程地质模型的突破口,因此,重视和应用现代构造地质学研究的新理论,新方法必将会对岩体工程地质学研究起着重要的指导意义。本文系统总结了与工程地质研究相关的现代构造地质学理论和思维观的研究进展,在此基础上分析了这些理论方法对工程地质工作的启示和指导意义,希望起到抛砖引玉的作用。  相似文献   
999.
吉林集安金厂沟矿田岩石化学及地球化学特征   总被引:2,自引:0,他引:2  
金厂沟矿田以金矿床为主,矿体与矿化点分布于燕山期中酸性杂岩体的内外接触带上。岩石化学及地球化学特征表明集安变质岩系遭受中级变质,含有较高的金等金属成矿元素; 中酸性杂岩体是地幔熔浆与壳源物质混杂形成,各成矿物质为幔源,同时汲取壳源,金来源于变质岩系和中酸性岩浆岩。  相似文献   
1000.
吉东火山岩型金矿地质特征及流体包裹体研究   总被引:1,自引:0,他引:1  
通过对主要金矿床的流体包裹体 ,S、C、H和O同位素特征研究分析 ,认为金成矿的物化环境 :温度为 15 6~ 2 84℃、压力小于 6 6 0× 10 5Pa (深度不超过 2km) ;成矿流体具有富含H2 O、SO2 - 4、Cl- 和高K+的特点 ,是岩浆热液和大气降水的混合流体 ;成矿物质主要来源于火山 次火山岩  相似文献   
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