Effects of Kerr space–time on spectral features from X-ray illuminated accretion discs

We performed detailed calculations of the relativistic effects acting on both the reflection continuum and the iron line from accretion discs around rotating black holes. Fully relativistic transfer of both illuminating and reprocessed photons has been considered in Kerr space–time. We calculated overall spectra, line profiles and integral quantities, and present their dependences on the black hole angular momentum. We show that the observed EW of the lines is substantially enlarged when the black hole rotates rapidly and/or the source of illumination is near above the hole. Therefore, such calculations provide a way to distinguish between different models of the central source.     

西藏罗布莎铬铁矿区高海拔巨厚覆盖层钻探技术

西藏罗布莎铬铁矿区海拔高、覆盖层厚、地质条件复杂,岩层破碎、裂隙发育,局部岩层水溶、水蚀、水敏,存在地层漏失、缩径等钻探难题。本文总结了该区28个中深钻孔施工经验,包括：钻孔结构、钻进工艺、冲洗液、护壁堵漏技术、复杂情况采取的技术措施等,取得了较好的效果,各项指标满足设计要求,岩（矿）心采取率达到90%以上,台月效率555 m,各项质量指标均符合设计要求。     

Shock metamorphism on the moon

Shock metamorphism of the lunar samples is discussed. All types of lunar glasses formed by various-size collision-type impact are found as impact glass, ropy glass and agglutinates. The agglutinates bonded by crystal and glassy materials contain hydrogen and helium from the solar wind components. Lunar shocked minerals of plagioclase and silica show anomalous compositions and densities. There are typical two formation processes on planetary materials formed by shock events; that is (1) shocked quartz formed by silica-rich target rocks (esp. on evolved planets of the Earth and Mars), and (2) shocked silica with minor Al contents formed from plagioclase-rich primordial crusts of the Moon. The both shocked silica grows to coarse-grain normal crystals after high-temperature metamorphism which cannot distinguish the original main formation event of impact process.     

Statistical evaluation of methods for the calculation of static formation temperatures in geothermal and oil wells using an extension of the error propagation theory

The feasibility of using the more sophisticated weighted least-squares (WLS) model, as opposed to the traditional ordinary least-squares (OLS), in linear regressions of BHT data to estimate the static formation temperatures (SFT) was investigated. The most commonly used analytical methods (line-source; spherical and radial heat flow; and cylindrical heat source) were applied. Error propagation equations were derived to calculate errors in the time function of each method. These errors were combined with the BHT measurement errors to compute weighting factors for applying the WLS. Intercept uncertainties were estimated for all regressions using sets of synthetic and actual borehole logs taken from geothermal and oil applications. SFT computed with the spherical and radial heat flow method were generally greater than those from the other two methods.     

使用流体压差法建立根缘油气藏动态平衡

根缘油气藏(深盆油气藏) 是紧临源岩存在的烃类聚集, 是在高勘探程度下所发现的油气藏类型.由于它在成藏机理及存在方式上的特殊性, 常规意义上所采用的动力平衡方程不再适合于对其成藏平衡作用过程的分析.结合根缘油气藏地质特征及其演化特点, 采用对连续油气柱上升力的分解分析方法, 讨论了流体压差的平衡问题, 建立了位于源岩上部的根缘油气藏的动力平衡方程.      

鲁西大汶口地区全新世临沂组沉积物粒度分布特征及地质意义

出露于大汶口盆地的临沂组为一套第四系松散堆积物,上部以土黄色、灰黄色含砂质粉砂、粉砂质粘土为主,下部为砂砾石层,是大汶口盆地内河流演化过程中的沉积响应和物质记录。通过对临沂组进行研究,可以反演大汶口盆地第四纪以来的沉积区水动力环境、物质运移方式和沉积环境。该文在区域地质调查工作的基础上,结合粒度分析频率曲线、概率累积曲线、粒度参数和沉积物宏观特征,对临沂组的沉积相、沉积环境和沉积韵律进行了研究。研究表明,大汶口地区临沂组下部为河床亚相边滩沉积微相,上部为河漫亚相河漫滩沉积微相,经历了由简单高能→复杂中能-中低能→简单中低能→复杂中低能的水动力沉积环境变化。另外依据岩石组合特征,将其划分为4个明显的沉积韵律和1个不明显的沉积韵律组。