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11.
Phase equilibria simulations were performed on naturally quenchedbasaltic glasses to determine crystallization conditions priorto eruption of magmas at the Mid-Atlantic Ridge (MAR) east ofAscension Island (7–11°S). The results indicate thatmid-ocean ridge basalt (MORB) magmas beneath different segmentsof the MAR have crystallized over a wide range of pressures(100–900 MPa). However, each segment seems to have a specificcrystallization history. Nearly isobaric crystallization conditions(100–300 MPa) were obtained for the geochemically enrichedMORB magmas of the central segments, whereas normal (N)-MORBmagmas of the bounding segments are characterized by polybariccrystallization conditions (200–900 MPa). In addition,our results demonstrate close to anhydrous crystallization conditionsof N-MORBs, whereas geochemically enriched MORBs were successfullymodeled in the presence of 0·4–1 wt% H2O in theparental melts. These estimates are in agreement with direct(Fourier transform IR) measurements of H2O abundances in basalticglasses and melt inclusions for selected samples. Water contentsdetermined in the parental melts are in the range 0·04–0·09and 0·30–0·55 wt% H2O for depleted and enrichedMORBs, respectively. Our results are in general agreement (within±200 MPa) with previous approaches used to evaluate pressureestimates in MORB. However, the determination of pre-eruptiveconditions of MORBs, including temperature and water contentin addition to pressure, requires the improvement of magma crystallizationmodels to simulate liquid lines of descent in the presence ofsmall amounts of water. KEY WORDS: MORB; Mid-Atlantic Ridge; depth of crystallization; water abundances; phase equilibria calculations; cotectic crystallization; pressure estimates; polybaric fractionation  相似文献   
12.
The character of convergence along the Arabian–Iranian plate boundary changes radically eastward from the Zagros ranges to the Makran region. This appears to be due to collision of continental crust in the west, in contrast to subduction of oceanic crust in the east. The Makran subduction zone with a length of about 900 km display progressively older and highly deformed sedimentary units northward from the coast, together with an increase in elevation of the ranges. North of the Makran ranges are large subsiding basins, flanked to the north by active volcanoes. Based on 2D seismic reflection data obtained in this study, the main structural provinces and elements in the Gulf of Oman include: (i) the structural elements on the northeastern part of the Arabian Plate and, (ii) the Offshore Makran Accretionary Complex. Based on detailed analysis of these data on the northeastern part of the Arabian Plate five structural provinces and elements—the Musendam High, the Musendam Peneplain, the Musendam Slope, the Dibba Zone, and the Abyssal Plain have been identified. Further, the Offshore Makran Accretionary Complex shown is to consist Accretionary Prism and the For-Arc Basin, while the Accretionary Prism has been subdivided into the Accretionary Wedge and the Accreted/Colored Mélange. Lastly, it is important to note that the Makran subduction zone lacks the trench. The identification of these structural elements should help in better understanding the seismicity of the Makran region in general and the subduction zone in particular. The 1945 magnitude 8.1 tsunamigenic earthquake of the Makran and some other historical events are illustrative of the coastal region’s vulnerability to future tsunami in the area, and such data should be of value to the developing Indian Ocean Tsunami Warning System.  相似文献   
13.
中祁连东段什川杂岩基的岩石化学特征及年代学研究   总被引:5,自引:4,他引:1  
祁连造山带被托菜南山-了高山构造带及宗务隆山-贵得构造带分为北祁连、中祁连及南祁连构造带。什川岩基位于中祁连构造带东部,由闪长岩、斜长花岗岩、二长花岗岩组成;对二长花岗岩进行U-Pb单颗粒锆石微区LA-ICP-MS同位素测定,获得444.6Ma及414.3Ma两组加权平均年龄,前者代表岩石的形成年龄,后者代表构造热事件年龄。二长花岗岩主量元素W(SiO_2)=68.66%~80.77%,w(K_2O)/w(Na_2O)>1和A/CNK介于0.95~1.21间,总体为钾质钙碱性过铝质花岗岩。岩石富集LILE元素(K、Th、Rb、Ba等),亏损HFSE元素(Ta、Nb、Y等);稀土元素总量较高(∑REE多介于109.05×10~(-6)~322.66×10~(-6)),轻重稀土强烈分馏(∑LREE/∑HREE介于7.92~31.68),稀土元素分配模式为轻稀土富集型,具中等-强Eu负异常(δEu=0.26~0.58)。岩石矿物组合及岩石地球化学特征共同表明,什川岩基为中上地壳泥砂质岩石部分熔融而成,形成温度较低,为加厚地壳拆沉熔融成因。这为祁连造山带构造演化及其深部动力学机制研究提供了新的资料。  相似文献   
14.
黑龙江省金厂金矿床J0矿体流体地球化学研究   总被引:7,自引:6,他引:1  
黑龙江省东宁县金厂金矿床是最新发现的特大型金矿床,目前探获黄金资源量86吨,它位于中亚造山带东端的吉黑成矿带,是与中生代中酸性岩浆活动有关的复杂成矿系统,矿化类型可能包括了斑岩型、爆破角砾岩型、浅成低温热液型.研究表明,高丽沟J0号矿体为爆破角砾岩型,热液成矿过程经历了早、中、晚3个阶段,分别形成以石英-黄铁矿、多金属硫化物-石英和碳酸盐为代表的矿物组合,中阶段矿物含自然金最多,次为早阶段矿物.初始成矿流体系统为高温、高盐度、高氧逸度、富CO2的岩浆热液;经减压沸腾,CO2等挥发分大量逸出,流体温度、盐度和氧逸度下降,导致大量金属硫化物及自然金快速沉淀;大气降水混入导致晚阶段流体低温、低盐度、贫CO2,对成矿贡献甚微.总体而言,成矿流体盐度高(11.70%~37.81%NaCl.eq),成矿作用发生在中-高温(238.3~425.7℃)的浅成环境(深633m~2736m).岩浆-流体成矿系统富CO2应发育于大陆碰撞造山带的伸展构造背景,而非大洋板块俯冲诱发的岩浆弧背景.  相似文献   
15.
南印度洋SST与南亚季风环流年代际变化的研究   总被引:2,自引:0,他引:2  
利用美国NCEP全球大气再分析资料和JONES全球海表面温度异常(SSTA)资料,分析了南印度洋SSTA和南亚季风环流年代际变化的特征。研究发现,无论是南印度洋副热带海水辐合区的SST还是赤道以北非洲西海岸附近上升运动海区的SST的长期变化趋势,除了准3-5年的变化以外,还存在着明显的年代际的变化。对于全球最显著南亚季风环流的分析表明,南亚季风环流也存在明显的年代际时间尺度的变化。与南太平洋SST的年代际变化相比,南印度洋SST的变化周期要相对短一些。通过分析南半球冷空气年代际活动的特征发现,冷空气与南印度洋SST年代际时间尺度的变化具有密切的联系。  相似文献   
16.
Mud volcanoes, mud cones, and mud ridges have been identified on the inner portion of the crestal area, and possibly on the inner escarpment, of the Mediterranean Ridge accretionary complex. Four areas containing one or more mud diapirs have been investigated through bathymetric profiling, single channel seismic reflection profiling, heat flow measurements, and coring. A sequence of events is identified in the evolution of the mud diapirs: initially the expulsion on the seafloor of gasrich mud produces a seafloor depression outlined in the seismic record by downward dip of the host sediment reflectors towards the mud conduit; subsequent eruptions of fluid mud may create a flat topped mud volcano with step-like profile; finally, the intrusion of viscous mud produces a mud cone.The origin of the diapirs is deep within the Mediterranean Ridge. Although a minimum depth of about 400 m below the seafloor has been computed from the hydrostatic balance between the diapiric sediments and the host sediments, a maximum depth, suggested by geometric considerations, ranges between 5.3 and 7 km. The presence of thermogenic gas in the diapiric sediments suggests a better constrained origin depth of at least 2.2 km.The heat flow measured within the Olimpi mud diapir field and along a transect orthogonal to the diapiric field is low, ranging between 16 ± 5 and 41 ± 6 mW m–2. Due to the presence of gas, the thermal conductivity of the diapiric sediments is lower than that of the host hemipelagic oozes (0.6–0.9 and 1.0–1.15 W m–1 K–1 respectively).We consider the distribution of mud diapirs to be controlled by the presence of tectonic features such as reverse faults or thrusts (inner escarpment) that develop where the thickness of the Late Miocene evaporites appears to be minimum. An upward migration through time of the position of the décollement within the stratigraphic column from the Upper Oligocene (diapiric sediments) to the Upper Miocene (present position) is identified.  相似文献   
17.
The Agulhas Ridge is a prominent topographic feature that parallels the Agulhas-Falkland Fracture Zone (AFFZ). Seismic reflection and wide angle/refraction data have led to the classification of this feature as a transverse ridge. Changes in spreading rate and direction associated with ridge jumps, combined with asymmetric spreading within the Agulhas Basin, modified the stress field across the fracture zone. Moreover, passing the Agulhas Ridge’s location between 80 and 69 Ma, the Bouvet and Shona Hotspots may have supplied excess material to this part of the AFFZ thus altering the ridge’s structure. The low crustal velocities and overthickened crust of the northern Agulhas Ridge segment indicate a possible continental affinity that suggests it may be formed by a small continental sliver, which was severed off the Maurice Ewing Bank during the opening of the South Atlantic. In early Oligocene times the Agulhas Ridge was tectono-magmatically reactivated, as documented by the presence of basement highs disturbing and disrupting the sedimentary column in the Cape Basin. We consider the Discovery Hotspot, which distributes plume material southwards across the AAFZ, as a source for the magmatic material.  相似文献   
18.
中太平洋铁锰结壳铅同位素研究   总被引:5,自引:0,他引:5  
已有研究表明大洋中溶解的铅(Pb)来源于陆源物质,但是,对Pb进入大洋的途径争议很大。为此分析了取自中太平洋两块铁锰结壳样品的Pb同位素组成,获得了整个新生代的中太平洋Pb同位素演化历史。结果表明这两块结壳的Pb同位素随时间的演化曲线与中北太平洋沉积物岩心LL44-GPC3中风成碎屑的Pb同位素演化曲线相似。证实该区深水中的天然溶解铅主要来自风成粉尘,并且50Ma之前中太平洋中溶解Pb同位素组成主要取决于源自美洲的风成粉尘的输入,40Ma之后主要取决于源自亚洲的风成粉尘的输入。  相似文献   
19.
A 140 km long wide-angle seismic profile has been acquired by use of 6 Ocean Bottom Seismographs across the Jan Mayen Ridge, North Atlantic. The profile was acquired twice; once with a traditionally tuned standard source and secondly with a somewhat smaller source tuned on the first bubble pulse. Analysis of the frequency content of the data reveals that the single-bubble source within the 10-15 Hz frequency range generates a signal with a level about 5 db above that of the standard source. These differences can partly be related to differences in airgun depth. The higher output level for these frequencies enables the single-bubble source to resolve intra-crustal structures with a higher degree of certainty, when compared to the data acquired by use of the standard source array. The standard source seems to generate slightly more energy for frequencies around 6 Hz, probably due to the use of a large 1200 in/sup3 gun in this array. These low frequencies a re of importance for mapping of lower crustal and upper mantle structures, and it is recommended that this is taken into account when seismic sources for mapping of deep crustal and upper mantle structures are designed.  相似文献   
20.
根据作者在印度洋东部海域的延绳钓生产实践,对渔获的大眼金枪鱼群体的群体构成、摄食、繁殖等基本生物学特征进行了初步探讨.结果表明,渔获群体由纯重10~115kg、叉长80~195cm个体组成,纯重与叉长关系式w=2.000×10-5×L2.969;渔获物以3~5龄个体为主,雄性个体所占比例明显高于雌性个体,且随年龄增长雄性个体所占比例逐步提高.鱼群在该海域产卵期较长,不同年龄组性腺发育节律有明显差异.  相似文献   
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