汶川地震断裂带科学钻探项目WFSD-4孔强缩径地层钻进工艺研究

介绍了汶川地震断裂带科学钻探项目WFSD-4孔强缩径地层钻进的技术问题。在分析地层缩径机理和影响因素的基础上,提出了强缩径地层的钻进工艺措施。措施在WFSD-4孔中实施取得了显著的效果。     

雅鲁藏布江深厚砂砾卵石覆盖层钻探工艺

为了开展雅鲁藏布江流域综合规划及其水资源开发利用与保护专题研究工作,在雅鲁藏布江干流里龙坝址和本宗坝址共布置了4个200~300 m深的钻孔。主要通过在西藏高寒地区4个深厚覆盖层钻孔的成功实施经验,对西藏高寒地区深厚覆盖层勘探成孔工艺与技术进行研究探讨。     

深孔及松软地层大口径绳索取心钻具的研究与应用

为解决深孔大口径及松软地层取心难的问题,推进取心钻探技术的发展,研发了一套大口径绳索取心钻具。着重介绍了大口径绳索取心钻具的结构特点、技术参数、技术创新及使用效果。应用结果表明,该大口径绳索取心钻具结构合理、各机构动作可靠、岩心采取率高,能够满足深孔及松软地层的取心要求。     

GYD-20型全液压动力头工程钻机的研制

针对传统工程钻机生产制造周期长、自动化程度低、劳动强度大、施工效率低等弊端,研制了GYD-20型全液压动力头工程钻机。介绍了该钻机的结构特点及其应用于大口径基础桩孔、煤矿通风孔钻进的情况和效果。     

矿山井下罗盘仪测量数据处理程序设计

在金属矿山井下测量生产实践中,经常会遇到罗盘仪测量计算数据处理问题。由于其计算公式较为复杂,计算量大,手工计算不仅烦琐,而且常常出错。因此,本设计针对以上问题应用Visual Basic6.0编程语言,建立相应的数学模型,编写矿山井下测量数据处理程序。程序采用多重窗体界面,界面清晰、易懂。程序对输入数据进行自动化处理,输出数据格式符合常用测绘软件(南方CASS)数据格式要求,能减轻金属矿山地采测量工作者内业处理数据负担,提高工作效率,具有一定的广泛性、实用性。     

Towards a new standard model for black hole accretion

We briefly review recent developments in black hole accretion disk theory, emphasizing the vital role played by magnetohydrodynamic (MHD) stresses in transporting angular momentum. The apparent universality of accretion-related outflow phenomena is a strong indicator that large-scale MHD torques facilitate vertical transport of angular momentum. This leads to an enhanced overall rate of angular momentum transport and allows accretion of matter to proceed at an interesting rate. Furthermore, we argue that when vertical transport is important, the radial structure of the accretion disk is modified at small radii and this affects the disk emission spectrum. We present a simple model demonstrating how energetic, magnetically-driven outflows modify the emergent disk emission spectrum with respect to that predicted by standard accretion disk theory. A comparison of the predicted spectra against observations of quasar spectral energy distributions suggests that mass accretion rates inferred using the standard disk model may be severely underestimated.     

Model dependence of transonic properties of accretion flows around black holes

We analytically study how the behaviour of accretion flows changes when the flow model is varied. We study the transonic properties of the conical flow, a flow of constant height and a flow in vertical equilibrium, and show that all these models are basically identical, provided that the polytropic constant is suitably changed from one model to another. We show that this behaviour is extendible even when standing shocks are produced in the flow. The parameter space where shocks are produced remains roughly identical in all these models when the same transformation among the polytropic indices is used. We present applications of these findings.     

Studies of accretion flows around rotating black holes – II. Standing shocks in the pseudo-Kerr geometry

Standing, propagating or oscillating shock waves are common in accretion and winds around compact objects. We study the topology of all possible solutions using the pseudo-Kerr geometry. We present the parameter space spanned by the specific energy and angular momentum and compare it with that obtained from the full general relativity to show that the potential can work satisfactorily in fluid dynamics also, provided the polytropic index is suitably modified. We then divide the parameter space depending on the nature of the solution topology. We specifically study the nature of the standing Rankine–Hugoniot shocks. We also show that as the Kerr parameter is increased, the shock location generally moves closer to the black hole. In future, these solutions can be used as guidelines to test numerical simulations around compact objects.     

On the Geometry of Broad-Line Regions in BL Lac Objects

The geometry of broad-line regions (BLRs) in active galactic nuclei (AGNs) is still controversial. We use a sample of BL Lac objects, of which the black hole masses Mbh are estimated from their host galaxy absolute magnitude at R-band, MR, by using the empirical relation between MR and black hole mass Mbh. The sizes of the broad-line regions for Mgn are derived from the widths of Mgn lines and the black hole masses. Compared with the empirical relation between BLR size RBLR and MgII line luminosity LMgII, it is found the BLR sizes in the BL Lac objects derived in this paper are 2-3 orders of magnitude higher. If the BLR geometry of these sources is disklike, then the viewing angle between the axis and the line of sight is in the range of ~ 2°-15°, which is consistent with the unification scheme.