河南省X.25分组交换网的建设

介绍了河南省气象台与地市局、国家基本站之间依托于邮电部门的Ｘ．２５分组交换网组建的全省Ｘ．２５分组交换网的设计思想和具体实现。     

Influence of pore size and geometry on peat unsaturated hydraulic conductivity computed from 3D computed tomography image analysis

In organic soils, hydraulic conductivity is related to the degree of decomposition and soil compression, which reduce the effective pore diameter and consequently restrict water flow. This study investigates how the size distribution and geometry of air‐filled pores control the unsaturated hydraulic conductivity of peat soils using high‐resolution (45 µm) three‐dimensional (3D) X‐ray computed tomography (CT) and digital image processing of four peat sub‐samples from varying depths under a constant soil water pressure head. Pore structure and configuration in peat were found to be irregular, with volume and cross‐sectional area showing fractal behaviour that suggests pores having smaller values of the fractal dimension in deeper, more decomposed peat, have higher tortuosity and lower connectivity, which influences hydraulic conductivity. The image analysis showed that the large reduction of unsaturated hydraulic conductivity with depth is essentially controlled by air‐filled pore hydraulic radius, tortuosity, air‐filled pore density and the fractal dimension due to degree of decomposition and compression of the organic matter. The comparisons between unsaturated hydraulic conductivity computed from the air‐filled pore size and geometric distribution showed satisfactory agreement with direct measurements using the permeameter method. This understanding is important in characterizing peat properties and its heterogeneity for monitoring the progress of complex flow processes at the field scale in peatlands. Copyright © 2010 John Wiley & Sons, Ltd.     

菱刈矿床矿脉群形成的构造环境

本文主要介绍菱刈矿床矿脉的赋存状态、裂隙体系分析、矿脉群赋存的构造环境。菱刈矿床属脉状浅成热液型金银矿床。矿床成因与裂隙系统的形成关系密切。矿脉群大致位于基底岩石(四万十层群)隆起的中央部位。     

Zircon geochronology constraints on the age and nature of ‘Precambrian metamorphic rocks’ in the Xing’an block of Northeast China

The Great Xing’an Range in Northeast China is located in the eastern part of the Central Asian Orogenic Belt. From north to south, the Great Xing’an Range is divided into the Erguna, Xing’an, and Songliao blocks. Previous U–Pb zircon geochronology results have revealed that some ‘Precambrian metamorphic rocks’ in the Xing’an block have Phanerozoic protolith ages, questioning whether Precambrian basement exists in the Xing’an block. We present laser ablation inductively coupled plasma mass spectrometry (LA–ICP–MS) U–Pb dating results for zircons from suspected Precambrian metamorphic rocks in the Xing’an block. Meta-rhyolites of the Xinkailing Group in Nenjiang yield magmatic ages of 355.8 Ma. Detrital zircons from phyllites of the Xinkailing Group in Duobaoshan yield populations of ca. 1505, ca. 810, and ca. 485 Ma, with the youngest peak constraining its depositional age to be <485 Ma. Zircons from amphibolitic gneisses of the Xinkailing Group in Nenjiang have magmatic ages of 308.6 Ma. Mylonitic granites of the Xinkailing Group in Nenjiang have zircon magmatic ages of 164 Ma. Detrital zircons from two-mica quartz schists of the Luomahu Group in the Galashan Forest yield ca. 2419, ca. 1789, ca. 801, ca. 536, ca. 480, and ca. 420 Ma, with the youngest peak indicating its depositional age as <420 Ma. Detrital zircons from mylonitized sericite–chlorite schist of the Ergunhe Formation in Taerqi yield populations of 982–948, ca. 519, and ca. 410 Ma, with the youngest peak demonstrating that its depositional age is <410 Ma. These zircon ages for a range of lithologies show that the Great Xing’an Range metamorphic rocks formed during the Phanerozoic (164–485 Ma) and that this crust is mostly Palaeozoic. Based on these results and published data, we conclude that there is no evidence of Precambrian metamorphic basement in the Xing’an block. In summary, the age data indicate that Precambrian metamorphic basement may not exist in the Xing’an region.     

哀牢山南段长安金矿地质特征及找矿方法研究

长安金矿位于哀牢山成矿带南段,是该成矿带上新近发现的又一大型金矿床。该区为哀牢山地体边缘地壳增生带,主要由深变质岩系组成,区内构造断裂发育,对岩浆活动和成矿作用有显著影响。本文总结了长安金矿的地质特征,并以该区的控矿断裂F6为主要研究目标,以地层岩性电性特征作为约束条件,分别展开了磁法、激电、瞬变电磁和大地电磁等综合物探手段的试验研究。研究结果表明,磁法对于该矿找矿效果不明显,瞬变电磁和大地电磁测深反演的电阻率低阻体,准确界定了控矿断裂F6的位置、倾向、断距以及深部延伸情况,通过激电异常可大致判断矿体的位置。所以在长安金矿区下一步的深部隐伏矿勘查中,结合瞬变电磁、激电、大地电磁等地球物理方法,辅以土壤化探异常进行约束,可以达到快速有效找矿之目的。     

基于Google Earth影像分析区域性大型“X”共轭节理系统对宏观岩溶作用的控制

从黔南、桂北的航天遥感图像上可以清楚地看出,地表的宏观岩溶地貌明显地受控于区域性大型“X”共轭节理系统,此类节理构成一幅巨型的渗滤网,成为大气降水下渗的主要通道,从而导致被其穿透的岩石遭受溶蚀,形成以线性岩溶谷地为主体的岩溶景观。即水平地层分布区,呈片状“X”形网络结构;直立地层分布区,呈羽状条带结构。水体下渗至潜水面后,将主要沿“X”节理走向向当地最低侵蚀基准面排泄,从而形成复杂的地下管道网络系统。首次利用网上Google Earth影像研究喀斯特环境,解决了只能依赖航片和卫星照片才能研究地球地貌的瓶颈,这对地貌研究和喀斯特石漠化的研究和治理提供了廉价便利的影像材料。     

土层地震反应中软弱夹层对加速度反应谱的影响

为了研究土层地震反应中软弱夹层对加速度反应谱的影响,本文构造了多种包含不同厚度、不同位置软夹层的土层结构,通过国内地震安评通用的ESE软件进行计算、分析。研究结果表明,软夹层的厚度、位置、输入地震动的幅值等对加速度反应谱均有不同程度的影响,上部含有软夹层的土层结构能造成反应谱出现双峰现象,引起加速度反应谱特征周期变大。本文研究结果对软土地区工程抗震设计有一定参考价值。     

CorelDRAW X5中基于VBA实现线渐变的技术研究

主要介绍在CorelDRAW X5中通过VBA的程序开发环境下实现线渐变的方法,通过开发出河流渐变工具,以单线河流渐变为例,解决了通过CorelDRAW X5进行地图制图过程中遇到的单线河流渐变的问题。     

The Flared Disc Project: RXTE and ASCA observations of X 1822−371

We present archival Rossi X-ray Timing Explorer ( RXTE ) and simultaneous Advanced Satellite for Cosmology and Astrophysics ( ASCA ) data of the eclipsing low mass X-ray binary (LMXB) X 1822−371. Our spectral analysis shows that a variety of simple models can fit the spectra relatively well. Of these models, we explore two in detail through phase-resolved fits. These two models represent the case of a very optically thick and a very optically thin corona. While systematic residuals remain at high energies, the overall spectral shape is well approximated. The same two basic models are fitted to the X-ray light curve, which shows sinusoidal modulations interpreted as absorption by an opaque disc rim of varying height. The geometry we infer from these fits is consistent with previous studies: the disc rim reaches out to the tidal truncation radius, while the radius of the corona (approximated as spherical) is very close to the circularization radius. Timing analysis of the RXTE data shows a time-lag from hard to soft consistent with the coronal size inferred from the fits. Neither the spectra nor the light curve fits allow us to rule out either model, leaving a key ingredient of the X 1822−371 puzzle unsolved. Furthermore, while previous studies were consistent with the central object being a 1.4 M_⊙ neutron star, which has been adopted as the best guess scenario for this system, our light curve fits show that a white dwarf or black hole primary can work just as well. Based on previously published estimates of the orbital evolution of X 1822−371, however, we suggest that this system contains either a neutron star or a low mass (≲2.5 M_⊙) black hole and is in a transitional state of duration shortward of 10⁷ yr.