利用SEM照片获取土的孔隙结构参数

以土工实验和计算机图像处理技术为基础, 探讨利用SEM照片获取土的孔隙结构参数的方法, 并以重塑粘性土为例进行实证分析.为获取孔隙结构参数, 首先分3个步骤对土样的SEM照片进行图像处理: 即照片格式转换、颗粒边际线探测和颜色充填; 然后针对黑白二元图像测算孔隙结构参数.从设计制备的重塑粘性土的三轴试验样品中, 选择了12个不同水分状态和密度状态的样品, 经风干和烘干后, 进行SEM测试, 每个样品拍摄了3个尺度的SEM照片, 放大倍数依次为500倍、1000倍、2000倍.之后, 对所获得的SEM照片进行了图像处理分析, 计算了相应的平面孔隙比和平面孔隙率.数据分析表明: SEM照片测算的孔隙参数与通常三相图计算的孔隙参数有关联, 测算数据可以反映土的孔隙结构特征; 样品的不同脱水方式对SEM照片测算的孔隙参数有影响, 与三相图法计算数据相比, 风干土样测算的数据略有偏大, 烘干土样测算的数据偏小; 同一土样不同比例尺的SEM照片测算出的孔隙参数有所不同, 邻近三相图法计算结果上下波动; 利用SEM照片提取土的结构信息是可行的, 对SEM照片进行图像处理分析是获取土的孔隙结构参数的有效办法.      

Photoelectric photometry of comets in the system of standard IHW filters and the special case of comet P/Halley

Magnitudes of comets P/Giacobini-Zinner (1984e), P/Halley (1982i), P/Hartley-Good (1985 1), and Thiele (1985 m) in the bandpasses of the standard IHW comet filters are presented. For comet P/Halley production rates for CN, C₃, C₂, and solids were derived. For the gaseous components these show a strong dependence on heliocentric distance. The dependence is less steep for the solids which may be due to relatively pronounced backscattering properties in case of comet P/Halley. During one night (1985 Dec. 22/23) intensity profiles along three sections through the coma of comet P/Halley were measured. Compared with theoretical profiles they show a global anisotropy of the coma and possibly local structure.     

莺歌海盆地超压体系的成因及与油气的关系

莺歌海盆地独特的地质进程形成多套泥源层,泥源岩的压实与排液不均衡导致盆地内存在大规模的超压体系,大量的生烃及水热增压使盆地内超压进一步加剧。底辟作用将超压传递至浅层,使超压体系的分布在不同深度和不同构造带中的差异均较大。在中央底辟带,由于泥-流体底辟活动极强,突破的地层多,超压顶面埋深很浅;超压的释放不仅仅是孔隙流体的逸散,更重要的是烃源(主要是泥源层)所生成的油和气作为热流体的一部分,伴随热流体向上突破、运移到浅部分异、逸散和聚集形成气藏。     

Gas emission prediction and recovery in underground coal mines

Strata gas can be released and captured from non-active and active gas resources either from virgin or relaxed strata, both prior to and when mining activities take place. The high and irregular gas emissions associated with high production longwall mining have provided a need to optimise the methods used to predict these gas levels and the ventilation requirements for gas dilution. A forecast of gas emissions during development drivage and longwall mining indicated possible gas and ventilation problems requiring the introduction of various gas drainage techniques and in maintaining the necessary air quantities in ventilation systems to satisfy the statutory gas limitations for various coal production rates. Although there are sound principles used in world-recognised methods of gas emission prediction, a new approach developed from long-term practical experience in underground gassy coal mine practices and gas-rock mechanics studies appear most suitable for local conditions and mining systems in use. The Lunagas ‘Floorgas' and ‘Roofgas' geomechanical and gas emission models offer an effective solution to these problems. Both programs are the most advanced engineering, numerical tools available to calculate gas source contributions to total gassiness and improve the accuracy and quality of gas control, gas capture technologies and ventilation system design.     

川西坳陷中段新场地区天然气研究及气源对比

经过大量学者多年的研究总结,川西坳陷中段新场地区具备良好的生、储、盖等成藏组合。结合地质背景及碳同位素、轻烃的研究,认为新场地区天然气主要是Ⅲ型干酪根的煤型气,气藏主要分布在上三叠系的须二段和须四段,以及中侏罗系、上侏罗系地层中。     

Evidence for Chemical Heterogeneity in the Nucleus of C/1995 O1 (Hale–Bopp)

We present an analysis of OH, CN, and C₂ jets observed in thecoma of Comet Hale–Bopp on UT April 22, 23, and 25, 1997. Monte Carlomodels designed to simulate the gas jets were employed to analyze thenuclear active areas responsible for the observed coma gas jets. Ourresults indicate that four active areas are necessary to reproduce theCN and C₂ jets while five active areas are required to simulatethe OH jets. The additional OH active area must produce significantlevels of OH, but cannot emit measurable quantities of either carbonradical. This difference suggests that the nucleus of Comet Hale–Boppis chemically heterogeneous.     

Challenging a Paradigm: Do We Need Active and Inactive Areas to Account for Near-Nuclear Jet Activity?

We briefly describe an advanced 3D gas dynamical model developed for the simulation of theenvironment of active cometary nuclei. The model canhandle realistic nucleus shapes and alternative physical models for the gas and dust production mechanism.The inner gas coma structure is computed by solving self-consistently(a) near to the surface the Boltzman Equation(b) outside of it, Euler or Navier-Stokes equations.The dust distribution is computed from multifluid ``zero-temperature' Euler equations,extrapolated with the help of a Keplerian fountain model.The evolution of the coma during the nucleus orbital and spin motion,is computed as a succession of quasi-steady solutions. Earlier versions of the model using simple,``paedagogic' nuclei have demonstrated that the surface orographyand the surface inhomogeneity contribute similarly to structuring the near-nucleusgas and dust coma,casting a shadow on the automatic attribution of such structures to ``active areas'.The model was recently applied to comet P/Halley, for whichthe nucleus shape is available. In the companion paper of this volume,we show that most near-nucleus dust structuresobserved during the 1986 Halley flybys are reproduced, assuming that the nucleus is strictly homogeneous. Here, we investigate the effect of shape perturbations and homogeneityperturbations. We show that the near nucleus gas coma structure is robust vis-a-vissuch effects. In particular, a random distribution of active and inactive areaswould not affect considerably this structure, suggesting that such areas,even if present, could not be easily identified on images of the coma.     

A unified theory of the formation of galactic bars

We give arguments for a basically unified formation mechanism of slow (Lynden-Bell) and fast (common) galactic bars. This mechanism is based on an instability that is akin to the well-known instability of radial orbits and is produced by the mutual attraction and alignment of precessing stellar orbits (so far, only the formation of slow bars has been explained in this way). We present a general theory of the low-frequency modes in a disk that consists of orbits precessing at different angular velocities. The problem of determining these modes is reduced to integral equations of moderately complex structure. The characteristic pattern angular velocities Ω_p of the low-frequency modes are of the order of the mean orbital precession angular velocity \(\bar \Omega _{pr}\). Bar modes are also among the low-frequency modes; while \(\Omega _p \approx \bar \Omega _{pr}\) for slow bars, Ω_p for fast bars can appreciably exceed even the maximum orbital precession angular velocity in the disk Ω _pr ^max (however, it remains of the order of these precession angular velocities). The possibility of such an excess of Ω_p over Ω _pr ^max is associated with the effect of “repelling” orbits. The latter tend to move in a direction opposite to the direction in which they are pushed. We analyze the pattern of orbital precession in potentials typical of galactic disks. We note that the maximum radius of an “attracting” circular orbit r_c can serve as a reasonable estimate of the bar length l_b. Such an estimate is in good agreement with the available results of N-body simulations.     

H<Emphasis Type="Italic">α</Emphasis> survey of the local volume: Isolated southern galaxies

We present our Hα observations of 11 isolated southern galaxies: SDIG, PGC 51659, E 222-010, E 272-025, E 137-018, IC 4662, Sag DIG, IC 5052, IC 5152, UGCA 438, and E 149-003, with distances from 1 to 7 Mpc. We have determined the total Hα fluxes from these galaxies. The star formation rates in these galaxies range from 10^?1 (IC 4662) to 10^?4 M _⊙ yr^?1 (SDIG) and the gas depletion time at the observed star formation rates lies within the range from 1/6 to 24 Hubble times H ₀ ^?1 .     

“十三五”期间中国探矿权及地质勘查投资时空演变

基于详细的统计数据,从时间、空间、结构等多个纬度,对中国探矿权及地质勘查投资情况进行了时间序列、因素相关性等对比分析和综合研究,为政府管理部门制定政策和规划提供参考依据。通过研究,揭示了影响探矿权及地质勘查投资的主要因素、底层逻辑和发展规律,并认为受国内外宏观经济增速放缓、地缘政治等因素影响,特别是国内相关产业政策、生态和环境保护压力,“十三五”期间中国探矿权数、地质勘查投入和新发现矿产地持续大幅度减少。“十三五”期间,新立探矿权同比减少52.1%,注销探矿权数是“十二五”期间的3.7倍多。油气矿产的探矿权登记面积和地质勘查投资分别占全国的96%和77.6%;非油气矿产探矿权数占全国的90%以上,有近60%的非油气探矿权在西部地区;非油气地质勘查投资中,水工环及科技等投资额占居半壁江山。预计中国在能源矿产、战略性矿产等勘查领域将增加勘查投入,地质勘查投资将于2024年后逐渐走出低谷。