辽宁鞍本—抚顺地区新太古代含铁建造层位对比及形成时代讨论     

卢崇海  张耀华  奚锐  李季  关树野  张爽  邢德和  谢鑫竹 《化工矿产地质》2013,(4):193-200

辽宁鞍本—抚顺地区太古宙变质层状岩系,前人分别建立了太古宙鞍山群井家沟组、石棚子组、通什村组、红透山组、樱桃园组、大峪沟组和茨沟组等地层单位,这些地层单位均呈规模大小不等的包体状、孤岛状等形态赋存于太古宙变质深成岩中,各组之间大部分孤立存在,无底无顶,相互间接触关系不清,是否属于同一时期形成的产物,长期一来存在着较多的争议。通过对各岩组原岩恢复、层序对比、含铁建造、变质作用等特点和以往及近期获得高精度测年数据的分析研究,把辽宁鞍本—抚顺地区太古宙层状岩系厘定为新太古代井家沟岩组、红透山岩组、茨沟岩组和樱桃园岩组等四个构造岩石地层单位,形成时间在27²5亿a左右,为新太古代中晚期产物。  相似文献   

基于磁通负反馈结构的高灵敏度感应式磁场传感器研制   总被引：5，自引：2，他引：3       下载免费PDF全文

朱万华  底青云  刘雷松  闫彬  刘凯  方广有 《地球物理学报》2013,56(11):3683-3689

感应式磁场传感器广泛应用于地球物理电磁勘探仪器,但也是阻碍我国地球物理电磁勘探仪器装备研发和推广应用的瓶颈技术.在我国SinoProbe计划中"地面电磁探测(SEP)系统"项目支持下,我们研制出用于大地电磁测深(the Magnetotellurics MT)方法的高灵敏度磁场传感器.研制过程中,采用磁通负反馈技术,增强传感器系统工作稳定性;采用斩波稳零放大电路技术,有效降低低频1/f噪声对传感器灵敏度的影响;采用高磁导率合金材料,增加磁场传感器的灵敏度.最终,MT磁场传感器工作频率范围为1 m√HZ ~1 k√HZ ,噪声水平0.1 √HZ 时为1.5 pT/√HZ ;1 √HZ 时为0.15 pT/√HZ ;10 √HZ 时为0.03 pT/√HZ ;长度96 cm,重量≤6 kg.理论和测试结果表明:与同类产品比较,本文研制的感应式磁场传感器在≥10 √HZ 时,平均噪声水平从150 fT/√HZ ,下降至30 fT/√HZ ,噪声水平更优,测量精度更高,能够更好地满足MT方法的需求.  相似文献   

新疆吐尔库班套蛇绿混杂岩的发现及其地质意义   总被引：4，自引：0，他引：4       下载免费PDF全文

王玉往  王京彬  王莉娟  龙灵利  唐萍芝  廖震  张会琼 《地学前缘》2011,18(3):151-165

蛇绿岩作为残留洋壳的良好记录,对于研究古板块构造及其演化具有重要意义。新发现的吐尔库班套蛇绿混杂岩位于新疆阿尔泰布尔津南部,主要由超镁铁岩、辉长岩、辉绿岩、玄武岩、复理石建造等构成。其中辉长岩和片麻状花岗岩的锆石U Pb年龄在363～355 Ma,指示蛇绿岩的形成、洋壳俯冲时代在晚泥盆世晚期。岩石地球化学特征表明,该蛇绿岩套的镁铁超镁铁岩和玄武岩属低碱、低钛、富镁的拉斑玄武岩系列,具有较典型的幔源岩石特征,玄武岩形成于类似洋中脊的构造环境。混杂岩带中的片麻状花岗岩属于钠质的低钾岩石系列,形成于火山弧或同碰撞构造环境,亦为洋壳俯冲的结果。吐尔库班套蛇绿岩与科克森套、乔夏哈拉、布尔根蛇绿岩一起构成了沿额尔齐斯分布的蛇绿混杂岩带,构成了分割西伯利亚板块和哈萨克斯坦-准噶尔板块的斋桑-科克森套-南蒙古缝合带。  相似文献   

新疆沙冬青叶片蛋白质的双向电泳技术研究   总被引：1，自引：1，他引：0  

鲁春芳  尹林克 《中国沙漠》2011,31(1):96-100

提取新疆沙冬青叶片中蛋白质受到脂类、酚类等次生代谢产物的干扰,针对这种现象,进行了组分提取优化方法和双向电泳技术的改进。实验分析表明,用乙醚淋洗完整叶片,50 mmol·L-1 Tris-HCl缓冲液,上样量240 μg（7 cm胶条）,考马斯亮蓝染色等方法可很大程度增加提取可溶性蛋白含量,结合丙酮-三氯乙酸的沉降,可较完整地提取蛋白质组。  相似文献   

Mineral chemistry of a Cenozoic igneous complex,the Urumieh–Dokhtar magmatic belt,Iran: Petrological implications for the plutonic rocks          下载免费PDF全文

Maryam Honarmand  Nematollah Rashidnejad Omran  Franz Neubauer  Ghasem Nabatian  Mohammad Hashem Emami  Manfred Bernroider  Jamshid Ahmadian  Mohammad Ebrahimi  Xiaoming Liu 《Island Arc》2016,25(2):137-153

The Niyasar plutonic complex, one of the Cenozoic magmatic assemblages in the Urumieh‐Dokhtar magmatic belt, was the subject of detailed petrographic and mineralogical investigations. The Niyasar magmatic complex is composed of Eocene to Oligocene mafic rocks and Miocene granitoids. Eleven samples, representing the major rock units in the Niyasar magmatic complex and contact aureole were chosen for mineral chemical studies and for estimation of the pressure, temperature, and oxygen fugacity conditions of mineral crystallization during emplacement of various magmatic bodies. The analyzed samples are composed of varying proportions of quartz, plagioclase, K‐feldspar, hornblende, biotite, titanite, magnetite, apatite, zircon, garnet, and clinopyroxene. Application of the Al‐in‐hornblende barometer indicates pressures of around 0.2 to 0.4 kbar for the Eocene–Oligocene mafic bodies and around 0.5 to 1.7 kbar for the Miocene granitoids. Hornblende‐plagioclase thermometry yields relatively low temperatures (661–780 °C), which probably reflect late stage re‐equilibration of these minerals. The assemblage titanite–magnetite–quartz as well as hornblende composition were used to constrain the oxygen fugacity and H₂O content during the crystallization of the parent magmas in the Miocene plutons. The results show that the Miocene granitoids crystallized from magmas with relatively high oxygen fugacity and high H₂O content (~5 wt% H₂O). The Miocene granitoids show similar range of oxygen fugacity, H₂O contents and mineral chemical compositions, which indicate a common source for their magmas. Although the crystallization pressures of the Miocene plutons discriminate various categories of plutonic bodies emplaced at depths of about 5.7–6.5 km (Marfioun pluton), about 4.2 km (Ghalhar pluton) and 1.9–2.3 km (Poudalg pluton), they were later uplifted to the same level by vertical displacement of faults. The emplacement depths of the Niyasar plutons suggest that the central part of the Urumieh‐Dokhtar magmatic belt has experienced an uplift rate of ca. 0.25–0.4 mm/yr from the Miocene onwards.  相似文献   

Contributions of slab fluid and sediment melt components to magmatism in the Mariana Arc–Trough system: Evidence from geochemical compositions and Sr,Nd, and noble gas isotope systematics          下载免费PDF全文

Yasuo Ikeda  Keisuke Nagao  Teruaki Ishii  Daisuke Matsumoto  Robert J. Stern  Hiroo Kagami  Makoto Arima  Sherman H. Bloomer 《Island Arc》2016,25(4):253-273

This study presents new major and trace element, mineral, and Sr, Nd, and noble gas isotope geochemical analyses of basalts, gabbro, and clinopyroxenite from the Mariana Arc (Central Islands and Southern Seamount provinces) including the forearc, and the Mariana Trough (Central Graben and Spreading Ridge). Mantle source compositions beneath the Mariana Arc and the Mariana Trough indicate a mantle source that is depleted in high field strength elements relative to MORB (mid‐oceanic ridge basalt). Samples from the Mariana Arc, characterized by high ratios of Ba/Th, U/Th, ⁸⁴Kr/⁴He and ¹³²Xe/⁴He, are explained by addition of fluid from the subducted slab to the mantle wedge. Correlations of noble gas data, as well as large ion lithophile elements, indicate that heavy noble gases (Ar, Kr, and Xe) provide evidence for fluid fluxing into the mantle wedge. On the other hand, major elements and Sr, Nd, He, and Ne isotopic data of basalts from the Mariana Trough are geochemically indistinguishable from MORB. Correlations of ³He/⁴He and ⁴⁰Ar/³⁶Ar in the Mariana Trough samples are explained by mixing between MORB and atmosphere. One sample from the Central Graben indicates extreme enrichment in ²⁰Ne/²²Ne and ²¹Ne/²²Ne, suggesting incorporation of solar‐type Ne in the magma source. Excess ¹²⁹Xe is also observed in this sample suggesting primordial noble gases in the mantle source. The Mariana Trough basalts indicate that both fluid and sediment components contributed to the basalts, with slab‐derived fluids dominating beneath the Spreading Ridge, and that sediment melts, characterized by high La/Sm and relatively low U/Th and Zr/Nb, dominate in the source region of basalts from the Central Graben.  相似文献   

Geochemical characteristics of deposits from the 2011 Tohoku‐oki tsunami at Hasunuma,Kujukuri coastal plain,Japan          下载免费PDF全文

Tetsuya Shinozaki  Yuki Sawai  Junko Hara  Minoru Ikehara  Dan Matsumoto  Koichiro Tanigawa 《Island Arc》2016,25(5):350-368

We examined the geochemical characteristics and temporal changes of deposits associated with the 2011 Tohoku‐oki tsunami. Stable carbon isotope ratios, biomarkers, and water‐leachable ions were measured in a sandy tsunami deposit and associated soils sampled at Hasunuma, Kujukuri coastal plain, Japan, in 2011 and 2014. At this site, the 2011 tsunami formed a 10–30 cm ‐thick layer of very fine to medium sand. The tsunami deposit was organic‐poor, and no samples contained any detectable biomarkers of either terrigenous or marine origin. In the underlying soil, we identified hydrocarbons and sterols derived from terrestrial plants, but detected no biomarkers of marine origin. In the samples collected in 2011, concentrations of tsunami‐derived water‐leachable ions were highest in the soil immediately beneath the tsunami deposit and then decreased gradually with depth. Because of its finer texture and higher organic content, the soil has a higher water‐holding capacity than the sandy tsunami deposit. This distribution suggests that ions derived from the tsunami quickly penetrated the sand layer and became concentrated in the underlying soil. In the samples collected in 2014, concentrations of water‐leachable ions were very low in both soil and sand. We attribute the decrease in ion concentrations to post‐tsunami rainfall, seepage, and seasonal changes in groundwater level. Although water‐leachable ions derived from seawater were concentrated in the soil beneath the tsunami deposit following the tsunami inundation, they were not retained for more than a few years. To elucidate the behavior of geochemical characteristics associated with tsunamis, further research on organic‐rich muddy deposits (muddy tsunami deposits and soils beneath sandy tsunami deposits) as well as sandy tsunami deposits is required.  相似文献   

Correlating biostratigraphy and palaeoceanographic changes during late Quaternary at cold seeps with gas hydrate‐free areas of the Japan Sea using foraminifera paleoecology          下载免费PDF全文

Mahsa Saeidi Ortakand  Shiro Hasegawa  Ryo Matsumoto  Hiroki Matsuda 《Island Arc》2016,25(1):55-71

Late Quaternary foraminifera assemblages have been examined in two sediment cores (MD179‐3296 and MD179‐3317) from cold seep areas in the eastern margin of the Japan Sea, off Joetsu, Niigata Prefecture. Foraminifera assemblages in core MD179‐3296, which was located at the center of a pockmark on the Umitake Spur, show no evidence of methane flux and, especially in its upper portion, share the same paleo‐environmental history as other free gas hydrate areas of the Japan Sea. In comparison, in the core MD179‐3317 at the center of a pockmark at Joetsu Knoll, foraminiferal distributions were strongly affected by methane activities and, in the main part of the core, were deposited under local conditions. Three horizons were identified in this core, which are characterized by the high abundance value of Thalmannammina parkerae and might be related to methane flux due to sea level fall especially through late marine isotope stage (MIS) 3 and MIS 2.  相似文献   

CCD and photon-counting photometric observations of asteroids carried out at Padova and Catania observatories     

D. Gandolfi  M. Cigna  C. Blanco 《Planetary and Space Science》2009,57(1):1-1507

We present the results of observational campaigns of asteroids performed at Asiago Station of Padova Astronomical Observatory and at M.G. Fracastoro Station of Catania Astrophysical Observatory, as part of the large research programme on Solar System minor bodies undertaken since 1979 at the Physics and Astronomy Department of Catania University. Photometric observations of six Main-Belt asteroids (27 Euterpe, 173 Ino, 182 Elsa, 539 Pamina, 849 Ara, and 984 Gretia), one Hungaria (1727 Mette), and two Near-Earth Objects (3199 Nefertiti and 2004 UE) are reported. The first determination of the synodic rotational period of 2004 UE was obtained. For 182 Elsa and 1727 Mette the derived synodic period of 80.23±0.08 and , respectively, represents a significant improvement on the previously published values. For 182 Elsa the first determination of the H-G magnitude relation is also presented.  相似文献   

南极中山站电离层的极区特征   总被引：9，自引：1，他引：8       下载免费PDF全文

沈长寿  资民筠  王劲松  刘顺林  徐寄遥 《地球物理学报》2005,48(1):1-6

本文利用1996年的电离层数字测高仪DPS-4所测的f0F2、f0E以及美国NOAA和DMSP卫星观测估算的半球功率指数和午夜极光区赤道侧边界纬度等资料,考察中山站电离层的极区特征。结果表明,在太阳和地磁宁静环境下,冬季极夜磁正午中山站处于极隙区中心时,电离层内的电离密度达全天的最大值;上、下午各有数小时间隔位极光带内时,高能粒子的电离作用也很重要;夜间进入极差区后,电子密度则很低。夏季极昼时,太阳EUV辐射的电离效应使电离层电离密度比冬季值大许多,而且,日变化的最大值时间也提前了1~2h,强磁扰时,极隙区和极光带均向低纬侧移动;中山站上空的电子密度会大幅度下降。在中等扰动环境下情况要加复杂：磁正午前后极隙区内软粒子沉降的电离强度有所减小,而上、下午极光区的高能粒子电离则有较大增加。  相似文献