岩石物理岩石孔喉结构特征对核磁T2谱影响的数值模拟

We built a three-dimensional irregular network model which can adequately describe reservoir rock pore-throat structures. We carried out numerical simulations to study the NMR T2 distribution of water-saturated rocks. The results indicate that there is a good correlation between T2 distribution and the pore radius frequency histogram. The total T2 distribution can be partitioned into pore body and pore throat parts. The effect of parameters including throat radius, pore-throat ratio, and coordination number of the micro- pore structure on the T2 distribution can be evaluated individually. The result indicates that： 1 ） with the increase of the pore throat radius, the T2 distribution moves toward longer relaxation times and its peak intensity increases; 2） with the increase of the pore-throat ratio, the T2 distribution moves towards longer T2 with the peak intensity increasing and the overlap between pore body T2 and pore throat T2 decreasing; 3） With the increase of connectivity, the short T2 component increases and peak signal intensity decreases slightly.     

基于岩石物理转换模型的苏里格致密砂岩储层测井评价与产能预测

苏里格地区致密砂岩储层勘探开发难度很大,测井解释遇到了储层参数计算和产能预测不准确的问题.本文针对这些难点,基于已有的转换模型,推导并验证了T₂-I和T₂-K_r转换模型,提出了采用转换模型应用于测井综合解释和产能预测的方法.基于实验数据设定孔径大于1 μm的孔隙为大孔,中孔孔径在1 μm和0.03 μm之间,小孔孔径为0.03 μm以下.并建立了不同孔径范围模型中关键参数α与核磁参数T_2lm的关系,这为转换模型在测井解释中的应用提供了必要条件.本文在苏里格西区分别应用T₂-I和T₂-K_r转换模型求取含水饱和度和相对渗透率曲线,并进行产能预测,处理结果显示该方法具有很好的应用效果.     

Langzeitprognosen zum Sickerwasseraustrag von Schwermetallen aus Deponien von Müllverbrennungsschlacken

Long‐term Assessment for the Leachate Release of Heavy Metals from Municipal Solid Waste Incineration Bottom Ash Monofills Municipal solid waste incineration (MSWI) bottom ash was investigated by chemical, mineralogical, and microbiological methods as well as leaching‐ and laboratory lysimeter tests. Compared to geological material bottom ash shows a high content of soluble salts, organic carbon, and heavy metals. The heavy metals are mainly bound in alloys and glas. Addition of oxic and acetic solutions quickly oxigenize the metal‐phases and alloys. Only fixation in newly formed phases like carbonates or hydroxides prevents heavy metal release till pH 7 in case of pH‐reduce. In the long‐term the acid buffer is reduced by the environmental acid input in combination with the release of buffering phases (mostly calcite). Internal acid producing processes like decay of organic matter or oxidation of sulfides are not important for the pH‐decrease. Cu, Ni, and Zn are first released between pH 7 and 6 (mainly Zn) and a second time at pH values below 5 (mainly Cu). Pb is significantly released at pH values below 5, Cr only at pH < 4. Mainly metals, alloys, and the rims of glas are destroyed by leaching. Phases like metal hydroxides (mainly Fe‐phases) or amorphous, water bearing Fe‐Al‐Si‐oxides are finally formed. Long‐term leaching by acetic fluids increases the total availability of heavy metals (except Cr) with increasing time. Kinetic effects including changing of metal binding forms seem to be responsible for this development. Within deposit conditions of limited gas exchange (closed system) the pH of the carbonate buffering zone can drop below pH 7 in case of very strong acid input and quickly cause an enhanced metal release. But in reality such a strong acid input is not to be expected. Calcite will buffer between pH 8 and 7 for a long time. Depending on the environmental conditions (water balance, acidity of rain) and landfill design (compaction, permeability, cover, thickness) it can take hundreds till thousands of years until metal release will start. The long‐term metal release of matter with an acid buffer like carbonates can be approximately determined only by short‐term tests with powder (e.g. pH_static tests at pH 4).     

Cluster探测到磁尾等离子体注入的特征

利用Cluster卫星2001～2004年磁尾运行期间RAPID仪器的数据,确定了115例磁尾等离子体注入事件,借助时序叠加法统计研究磁尾等离子体注入现象的特征.注入事件主要分布于磁地方时夜晚20时至凌晨04时.与同步轨道区观测到的粒子注入事件类似,可以将磁尾粒子注入事件分成五类：（1）只有离子注入;（2）离子先于电子注入;（3）离子和电子同时注入;（4）电子先于离子注入;（5）只有电子注入.磁尾粒子注入时,质子（能量范围0～40 keV）的温度和数密度同时显著增加,沿地球径向的传播速度也明显增大.统计分析磁尾注入期间同时观测到的晨昏对流电场,发现电场可分为两类：（A）注入后电场突然增大,电场强度为正;（B）注入后电场突然增大,电场强度为负.利用磁层磁场（T89c）和电场（Volland-Stern）模型模拟粒子注入后赤道面的电漂移速度矢量,模拟结果与统计结果基本一致,表明晨昏对流电场引起的电漂移是驱动磁尾（-18R_EE）等离子体沿地球径向注入的机制之一.     

南海17940孔晚更新世末期以来菱形海线藻及其变种的古环境研究

通过对1994年南海17940孔硅藻数据进行分析,结果表明：该孔硅藻组合中菱形海线藻及其变种T. nitzschioides var. parva的百分含量比值具有一定的变化规律。通过比对南海17940孔已有温度记录（有孔虫G. rubberδ18O数据、FP-12E表层海水年平均温度）,进一步发现菱形海线藻变种（T. nitzschioides var. parva）与原种的比值所反应的温度变化与原有记录具有较好的一致性。其中,比值增加反映了古温度的升高;反之则说明气候变冷。因此,该比值可反映出自晚更新世末期以来该地区古温度的变化情况,是较好的古温度指示标志。     

Analysis of HST ultraviolet spectra for T Tauri stars: RU Lup

The ultraviolet spectra of the star RU Lup obtained with the Hubble Space Telescope are analyzed. Emission lines are identified. The presence of absorption components with a nearly zero residual intensity in the Mg II resonance doublet lines is indicative of mass outflow with a velocity V _∞?300 km s^?1. These lines also exhibit a broad (?1400 km s^?1 at the base) component originating in the star itself. The profiles of the (optically thin) Si II] and Si III]1892 Å lines for the first time unequivocally prove that these lines originate in an accretion shock wave rather than in the chromosphere, with the gas infall velocity being V ₀?400 km s^?1. The intensity ratio of the C IV 1550 Å and Si IV 1400 Å resonance doublet components was found to be close to unity, suggesting a high accreted-gas density, logN ₀>12.5. Molecular H₂ Lyman lines formed in the stellar wind were detected. The H I Lα luminosity of RU Lup was found from their intensities to exceed 10% of L _bol. Radiation pressure in the Lα line on atomic hydrogen may play a significant role in the initial acceleration of stellar-wind matter, but the effect of Lα emission on the dynamics of molecular gas is negligible.     

海上多波多分量地震技术新进展与发展方向

中国海洋石油领域开展了首次海上多波多分量地震试验。试验效果是不错的,主要表现在烃类检测和模糊区成像上。同时充分利用已有资料对方位各向异性进行了初步的研究和探讨。从纵横波剖面的对比和频谱分析结果看,浅层横波的纵向分辨率高于纵波,中深层二者差不多。我国在多波的基础性研究方面还很欠缺,在许多方面还有待加强。     

THREE-DIMENSIONAL DEFORMATION ALONG THE ALTYN TAGH FAULT ZONE AND UPLIFT OF THE ALTYN MOUNTAIN, NORTHERN TIBET

THREE-DIMENSIONAL DEFORMATION ALONG THE ALTYN TAGH FAULT ZONE AND UPLIFT OF THE ALTYN MOUNTAIN, NORTHERN TIBET     

Stability of LRS Bianchi type-I cosmological models in f(R,T)-gravity

This paper examines the stability of the transition from the early decelerating stage of the Universe to the recent accelerating stage for the perfect fluid cosmological locally rotationally symmetric(LRS) Bianchi-I model in f(R, T) theory. To determine the solution of field equations, the idea of a timevarying deceleration parameter(DP) which yields a scale factor, for which the Universe attains a phase transition scenario and is consistent with recent cosmological observations, is used. The time-dependent DP yields a scale factor a=exp■, where β and k are respectively arbitrary and integration constants. By using the recent cons_traints(H_0 _= 73.8, and q_0 =-0.54) from Type Ia Supernova(SN Ia) data in combination with Baryonic Acoustic Oscillations(BAO) and Cosmic Microwave Background(CMB) observations(Giostri et al.), we obtain the values of β = 0.0062 and k = 0.000016 for which we have derived a cosmological model from the early decelerated phase to the present accelerating phase. By applying_ other r_ecent constraints(H_0 = 73.8, q_0 =-0.73) from SNe Ia Union data(Cunha), we obtain the values of β = 0.0036 and k = 0.000084 for which we have derived a cosmological model in the accelerating phase only. We have compared both models with experimental data. The stability of the background solution has been examined also for the metric perturbations alongside the properties of future singularities in a Universe ruled by dark energy with phantom type fluid. We demonstrate the presence of a stable fixed point with a condition of state ω <-1 and numerically affirm this is really a late-time attractor in the ghost overwhelmed Universe. Some physical and geometric properties of the model are found and examined.