福建仙游园庄地区南园组新层型剖面的建立 及时代的重新厘定

在福建省闽侯县鹅宅-南园村层型剖面所划分的南园组被证实为早白垩世石帽山群后,原鹅宅-南园村割面已失去层型剖面的意义.通过125万周宁县幅、福州市幅、莆田市幅、泉州市幅的区域地质调查和系统研究,在福建省仙游县园庄建立了南园组的新层型剖面,重新厘定了南园组的地层层序和岩石组合,根据地层叠覆关系、同位素测年和古生物资料的系统研究结果,将南园组的时代重新厘定为晚侏罗世-早白垩世初期.     

三维地震属性参数在煤层厚度预测中的应用

依托“西部煤炭资源高精度三维地震勘探技术”项目工程,对晋城某矿南翼大巷东南区5m×5m×1ms的三维地震数据体,采用三维地震属性参数预测煤层厚度及其变化规律：沿3煤层、15煤层10ms时窗提取地震属性42种,根据钻孔资料,计算出煤厚与地震属性相关系数;从中优选出相关系数大于0．35的地震属性,其中3煤层9个、15煤层10个;然后进行地震属性互相关分析,优选出与3煤、15煤层厚度相关系数较大的4种属性,建立预测煤厚的BP神经网络模型,分别选取3煤层12个、15煤层4个实测数据作为学习训练和测试样本,以钻孔地震属性作为学习样本,对网络进行训练,最终获得全区煤层厚度。经与预留钻孔成果资料对比,预测精度较高,结果可用。     

Integrated chronostratigraphy of Proterozoic-Cambrian boundary beds in the western Anabar region, northern Siberia

Carbonate-rich sedimentary rocks of the western Anabar region, northern Siberia, preserve an exceptional record of evolutionary and biogeochemical events near the Proterozoic/Cambrian boundary. Sedimentologically, the boundary succession can be divided into three sequences representing successive episodes of late transgressive to early highstand deposition; four parasequences are recognized in the sequence corresponding lithostratigraphically to the Manykal Formation. Small shelly fossils are abundant and include many taxa that also occur in standard sections of southeastern Siberia. Despite this coincidence of faunal elements, biostratigraphic correlations between the two regions have been controversial because numerous species that first appear at or immediately above the basal Tommotian boundary in southeastern sections have first appearances scattered through more than thirty metres of section in the western Anabar. Carbon- and Sr-isotopic data on petrographically and geochemically screened samples collected at one- to two-metre intervals in a section along the Kotuikan River, favour correlation of the Staraya Reckha Formation and most of the overlying Manykai Formation with sub-Tommotian carbonates in southeastern Siberia. In contrast, isotopic data suggest that the uppermost Manykai Formation and the basal 26 m of the unconformably overlying Medvezhya Formation may have no equivalent in the southeast; they appear to provide a sedimentary and palaeontological record of an evolutionarily significant time interval represented in southeastern Siberia only by the sub-Tommotian unconformity. Correlations with radiometrically dated horizons in the Olenek and Kharaulakh regions of northern Siberia suggest that this interval lasted approximately three to six million years, during which essentially all 'basal Tommotian' small shelly fossils evolved.     

Origin of the hydrocarbon component of carbonaceous chondrites: the star-meteorite connection

We report the results of an experiment that produced a residue which closely matches the hydrocarbon component of the Murchison carbonaceous chondrite. This experiment suggests that the parent material of the meteoritic component originated as polycyclic aromatic hydrocarbon species in carbon stars during their later stages of evolution. The experiments also indicate that the pathway from those formation sites to eventual incorporation into the meteorite parent body involved hydrogenation in a plasma in the solar nebula or in H II regions prior to the solar nebula. This model is consistent with what is known about the meteoritic hydrocarbon component including deuterium abundance, the observation of cosmic infrared emission bands best attributed to polycyclic aromatic hydrocarbon molecules, and the inherent stability of these molecules that allows their formation in stars and subsequent survival in the interstellar medium.     

Plasma processing of interstellar PAHs into solar system kerogen

Processes resulting in the formation of hydrocarbons of carbonaceous chondrites and the identity of the interstellar molecular precursors involved are an objective of investigations into the origin of the solar system and perhaps even life on earth. We have combined the resources and experience of an astronomer and physicists doing laboratory simulations with those of a chemical expert in the analysis of meteoritic hydrocarbons, in a project that investigated the conversion of polycyclic aromatic hydrocarbons (PAHs) formed in stellar atmospheres into alkanes found in meteorites. Plasma hydrogenation has been found in the University of Alabama at Birmingham Astrophysics Laboratory to produce from the precursor PAH naphthalene, a new material having an IR absorption spectrum (Lee, W. and Wdowiak, T.J., Astrophys. J. 417, L49-L51, 1993) remarkably similar to that obtained at Arizona State University of the benzene-methanol extract of the Murchison meteorite (Cronin, J.R. and Pizzarello, S., Geochim. Cosmochim. Acta 54, 2859-2868, 1990). There are astrophysical and meteoritic arguments for PAH species from extra-solar sources being incorporated into the solar nebula, where plasma hydrogenation is highly plausible. Conversion of PAHs into alkanes could also have occurred in the interstellar medium. The synthesis of laboratory analogs of meteoritic hydrocarbons through plasma hydrogenation of PAH species is underway, as is chemical analysis of those analogs. The objective is to clarify this heretofore uninvestigated process and to understand its role during the origin of the solar system as a mechanism of production of hydrocarbon species now found in meteorites. Results have been obtained in the form of time-of-flight spectroscopy and chemical analysis of the lab analog prepared from naphthalene.     

用非线性稳健回归作清江隔河岩工程溢坝始期预报

清江隔河岩水利枢纽工程是国家"七五"重点工程之一.在县城西十公里处.第一次达标洪水(≥3500立方米/秒)的日期(称溢坝始期)的预报,对工程进度及安全影响很大.非线性稳健回归在[1]中作了介绍.我们的主要工作是:非线性因子的普查;系数α的确定;系数β的求算及最优变量的选择.一、数据的处理为与我站1960年-1990年资料对应,取同期隔河岩溢坝始期(简称始期)资料,以距     

Results of TV imaging of Phobos (Experiment VSK-Fregat)

From February to March 1989 the Phobos 2 spacecraft took 37 TV images of Phobos at a distance of 190-1100 km. These images complement Mariner-9 and Viking data by providing higher-resolution coverage of a large region West of the crater Stickney (40-160 degrees W) and by providing disk-resolved measurements of surface brightness at a greater range of wavelengths and additional phase angles. These images have supported updated mapping and characterization of large craters and grooves, and have provided additional observations of craters' and grooves' bright rims. Variations in surface visible/near-infrared color ratio of almost a factor of 2 have been recognized; these variations appear to be associated with the ejecta of specific large impact craters. Updated determinations of satellite mass and volume allow calculation of a more accurate value of bulk density, 1.90 +/- 0.1 g cm-3. This is significantly lower than the density of meteoritic analogs to Phobos' surface, suggesting a porous interior perhaps containing interstitial ice.     

山东省玲珑金矿田深部资源第二富集带的研究和预测

开展构造变形岩相形迹地质方法填图，确立矿田NEE、NE和NNE三组方向的构造蚀变矿化带的成矿和控矿的构造分布模型，用构造校正方法 测算玲珑－焦家式金矿典型矿田的成矿深度。玲珑金矿田四期成矿的深度分别约为3 454.97 m（213 Ma），1 914.42 m（100.28 Ma），1 090.97 m（80.67 Ma）和720.55 m（71.86 Ma）。在地物化资料基础上开展综合预测，预测了3组方向构造蚀变矿化带深部第二富集带的赋存深度、富集金矿的概量。胶东金矿深部存在第二富集带已被地勘部门和矿山近10年的深部地质勘查工程所证实。胶东金矿深部第二富集带揭露数百吨新增储量的事实还表明，中国东部燕山期构造岩浆作用有关的金属矿，主要和燕山期基底逐渐上隆及反钟向区域压剪的大地构造环境有关，其大型矿山深部发育深部第二资源富集带的现象可能是普遍的。     

拉斯维加斯谷地下水开采引起的地面沉降和地裂缝

美国西南干旱半干旱地区人口增长非常快。水不仅要满足基本的需求（饮用水、污水系统等），而且还要维持乡村潮湿地区生活方式的改变（郊区的草地、高尔夫球场、庭院的游泳池等）。这些水的使用，既能满足供水系统所在区域地表水供水的需求，又可以满足最基本的地下水开采。然而，地下水的开采对沉积含水层有不利的影响，这些含水层是特有的沙漠区地下水流域的承载。这些影响包括含水层不同程度的压实、旧断层的重新复活、地表的裂缝，还能对人为的基础设施有相当大的影响。