辽宁营口—盖县地区早元古代辽河群构造世代

营口—盖县地区早元古代辽河群经历了三个世代的构造变形。第一世代为枢纽近南北向的具轴面片理的平卧层理褶皱;第二世代为与第一世代近共轴的具轴面褶劈理的近水平直立片理褶皱;第三世代则为东西向的倾竖片理褶皱。     

Source Fault Model of the 1771 Yaeyama Tsunami, Southern Ryukyu Islands, Japan, Inferred from Numerical Simulation

The 1771 Yaeyama tsunami is successfully reproduced using a simple faulting model without submarine landslide. The Yaeyama tsunami (M 7.4), which struck the southern Ryukyu Islands of Japan, produced unusually high tsunami amplitudes on the southeastern coast of Ishigaki Island and caused significant damage, including 12,000 casualties. Previous tsunami source models for this event have included both seismological faults and submarine landslides. However, no evidence of landslides in the source has been obtained, despite marine surveying of the area. The seismological fault model proposed in this study, describing a fault to the east of Ishigaki Island, successfully reproduces the distribution of tsunami runup on the southern coast of the Ryukyu Islands. The unusual runup heights are found through the numerical simulation attributable to a concentration of tsunami energy toward the southeastern coast of Ishigaki Island by the effect of the shelf to the east. Thus, the unusual runup heights observed on the southeastern coast of Ishigaki Island can be adequately explained by a seismological fault model with wave-ray bending on the adjacent shelf.     

Relative contributions of runoff and sediment from sources within a road prism and implications for total sediment delivery

This study examines runoff and sediment generation rates within the road prism on unsealed road segments in the Cuttagee Creek catchment near Bermagui in New South Wales, Australia. A large (600 m²) rainfall simulator was used to measure runoff and sediment yields from each of the potential sediment and runoff sources and pathways. These included the road surface, table‐drain, upslope contributing area and cutslope face, and the entire road segment as measured at the drain outlet. Experiments were conducted on two major types of road (ridge‐top and cut‐and‐fill) of varying traffic usage and maintenance standard for two 30‐minute simulations of increasing rainfall intensity. From the range of possible sources within the road prism, the road surface produced the dominant source of excess runoff and sediment at each site with limited contributions from the table‐drain, cutslope face or contributing hillslope. Sediment generation varied significantly with road usage and traffic intensity. Road usage was strongly related to the amount of loose available sediment as measured prior to the experiments. Table‐drains acted primarily as sediment traps during the low rainfall event but changes in sediment concentration within the drains were observed as runoff volumes increased during the higher rainfall event of 110 mm h^?1, releasing sediment previously stored in litter and organic dams. The experiments demonstrate the potential roles of various features of the road prism in the generation and movement of sediment and water. Copyright © 2006 John Wiley & Sons, Ltd.     

中国南方海相层系埋藏史类型与生烃演化模式

在漫长的地质历史中,中国南方海相层系经历了多旋回构造运动与强烈后期改造。印支运动以来,多期沉降与隆升及其地区差异性表现产生了"早降晚抬"和"早抬晚降"两大类6种形式的埋藏演化史类型。受埋藏史类型控制,南方各地区不同层系烃源岩的生烃演化史存在明显差异性。按生烃过程是否连续及成熟演化明显暂停前是否已达到或超过生烃高峰期,将南方海相烃源岩的生烃演化过程归纳为连续生烃模式、二次生烃模式和晚期生烃模式等3种类型。     

氢化物发生-原子荧光光谱法测定地球化学样品中痕量铋

样品经王水溶解后,加入KMnO4溶液氧化,草酸除去过量KMnO4后的体系,直接用氢化物发生原子荧光光谱法测定地质样品中痕量Bi。方法使Au、Pd、As、Sb、Se、Te等元素的允许量大为提高,减少了不同测定体系中共存元素对Bi测定的干扰。方法的检出限(6s)为0.042μg/g,精密度(RSD,n=12)为1.88%~5.57%。经国家一级地质标准物质验证,测定值与标准值吻合。     

Imaging and power generation strategies for chandrayaan-1

The Chandrayaan-1 mission proposes to put a 550 kg lunarcraft into Geostationary Transfer Orbit (GTO) using the Polar Satellite Launch Vehicle (PSLV) which will subsequently be transferred into a 100 km circular lunar polar orbit for imaging purposes. In this paper, we describe certain aspects of mission strategies which will allow optimum power generation and imaging of the lunar surface. The lunar orbit considered is circular and polar and therefore nearly perpendicular to the ecliptic plane. Unlike an Earth orbiting remote sensing satellite, the orbit plane of lunar orbiter is inertially fixed as a consequence of the very small oblateness of the Moon. The Earth rotates around the Sun once a year, resulting in an apparent motion of Sun around this orbit in a year. Two extreme situations can be identified concerning the solar illumination of the lunar orbit, noon/midnight orbit, where the Sun vector is parallel to the spacecraft orbit plane and dawn/dusk orbit, where the Sun vector is perpendicular to the spacecraft orbit plane. This scenario directly affects the solar panel configuration. In case the solar panels are not canted, during the noon/midnight orbit, 100% power is generated, whereas during the dawn/dusk orbit, zero power is generated. Hence for optimum power generation, canting of the panels is essential. Detailed analysis was carried out to fix optimum canting and also determine a strategy to maintain optimum power generation throughout the year. The analysis led to the strategy of 180‡ yaw rotation at noon/midnight orbits and flipping the solar panel by 180‡ at dawn/dusk orbits. This also resulted in the negative pitch face of the lunarcraft to be an anti-sun panel, which is very useful for thermal design, and further to meet cooling requirements of the spectrometers. In principle the Moon’s surface can be imaged in 28 days, because the orbit chosen and the payload swath provide adequate overlap. However, in reality it is not possible to complete the imaging in 28 days due to various mission constraints like maximum duration of imaging allowed keeping in view the SSR sizing and payloads data input rate, time required for downlinking the payload data, data compression requirements and visibility of the lunarcraft for the Bangalore DSN. In each cycle, all the latitudes are swept. Due to the constraints mentioned, only 60‡ latitude arc coverage is possible in each orbit. As Bangalore DSN is the only station, half of the orbits in a day are not available. The longitudinal gaps because of non-visibility are covered in the next cycle by Bangalore DSN. Hence, in the firstprime imaging season, only 25% of the prime imaging zones are covered, and an additional threeprime imaging seasons are required for a full coverage of the Moon in two years. Strategy is also planned to cover X-ray payload coverage considering swath and orbit shift.     

The evolution characteristics and fractionation mechanism of carbon isotopes in the process of "multi-stage hydrocarbon generation"

The Jiyang Sag and the Liaohe Basin are the two important areas where immature oil resources are distributed in China. From these two areas immature-low mature to mature oil samples were collected for carbon isotopic analysis. The extracts of source rocks are dominant in the Jiyang Sag while crude oils are dominant in the Liaohe Basin. The maturity index, R., for source rocks varies from 0.25%(immature) to 0.65% (mature). Studies have shown that within this range of R. values the extracts of source rocks and crude oils, as well as their fraction components, have experienced observable carbon isotope fractionation. The carbon isotopic values tend to increase with burial depth, the oils become from immature-low mature to mature, and the rules of evolution of oils show a three-stage evolution pattern, i. e. ,light→heavy→light→heavy oils. Such variation trend seems to be related to the occurrence of two hydrocarbon-generating processes and the main hydrocarbon-forming materials being correspondingly non-hydrocarbons and possessing MAB characteristics, lower thermodynamic effects and other factors. In the process towards the mature stage, with increasing thermodynamic effects, the thermal degradation of kerogens into oil has become the leading factor, and correspondingly the bond-breaking ratio of 12 C-13C also increases,making the relatively 12C-rich materials at the low mature stage evolve again towards 13C enrichment.     

Comparison of two approaches for generation of daily rainfall data

There has been extensive research on the problem of stochastically generating daily rainfall sequences for use in water management applications. Srikanthan and McMahon [Australia Water Resources Council, Canberra, 1985] proposed a transition probability matrix (TPM) model that performs better for Australian rainfall than many alternative models, particularly where long records (say 100 years) are available. Boughton [Report 99/9, CRC for Catchment Hydrology, Monash University, Melbourne, 21pp, 1999] incorporated an empirical adjustment into the TPM model that allows the model to reproduce the observed variability in the annual rainfall. More recently, Harrold et al. [Water Resour Res 39(10, 12):1300, 1343, 2003a,b] proposed nonparametric models for the generation of daily rainfall occurrences and rainfall amounts on wet days. By conditioning on short, medium and long-term characteristics, this approach is also able to preserve the variability in annual rainfall. In this study, the above two approaches were used to generate daily rainfall data for Sydney and Melbourne, and the results evaluated. Both approaches preserved most of the daily, monthly and annual characteristics that were compared, with the nonparametric approach providing marginally better performance at the cost of greater model complexity. The nonparametric approach was also able to preserve the variability and persistence in the annual number of wet days.     

琼东南盆地崖 13-1气田气源区圈定与成藏运聚模式

琼东南盆地崖 13 -1气田成藏运聚模式一直存在不同的认识.应用生烃动力学、碳同位素动力学及流体包裹体方法对该气田有效气源区、气藏充注时间和运聚效率等进行了研究.结果表明, 崖 13 -1气藏成藏时间较晚,天然气主成藏期出现在 2 Ma以后;有效气源区是崖南凹陷斜坡带崖城组,现埋深范围 4 000～ 5 500 m; 天然气为累积聚集气,目前天然气仍在有效的充注阶段.在此基础上,提出了崖 13 1气田天然气成藏运聚模式.此研究方法及建立起的成藏模式对于莺-琼盆地天然气勘探具有重要指导意义.     

天然矿物低温催化脂肪酸酯生烃反应动力学研究

选择十八烷酸甲酯为模型化合物,以 10种天然矿物为载体,通过动力学方法考察了天然矿物对脂肪酸酯生烃反应的催化作用.结果表明,地质低温条件下天然矿物对脂肪酸酯生烃反应具有催化作用.矿物的催化作用主要体现在对反应活化能和指前因子的影响上.粘土、碳酸盐和金属元素对于脂肪酸酯生烃反应具有不同的催化作用,碳酸盐矿物相对于粘土矿物使生烃反应的活化能降低,过渡金属化合物矿物存在时,催化反应活化能介于碳酸盐和粘土矿物之间.天然矿物的存在能够升高或降低反应指前因子.