Brightness,polarization and electron density of the solar corona of 1980 february 16

During the eclipse of 1980 February 16 we photographed the solar corona at an effective wavelength of 6300 å. Using a quadruple camera we also obtained the coronal pictures in polarized light for four Polaroid orientations. We have used these observations to derive the coronal brightness and polarization and from these the electron densities in the corona out to a distance of about 2.5 R⊙ from the centre of the disc. The coronal brightness matches well with that of the corona of 1958 October 12.     

Simulation of flow and solute coupled 2‐D problems with velocity‐dependent dispersion coefficient based on the network method

The governing equations of coupled density‐driven flow and solute transport problems in porous media, with velocity‐dependent dispersion coefficient, are strongly nonlinear and must be solved numerically. This contribution presents a network model, based on the network simulation method, capable of simulating the transient solution to this kind of problem efficiently and with a relatively low computational time. The mathematical model is formulated using the stream function and concentration variables. Simulation of the network model is carried out in the standard electric circuit simulation code, Pspice. The present model is first applied to simulate the original benchmark Henry problem, and the solution is compared with those obtained by other authors. A study of the grid size is also carried out. In addition, the modified version of Simpson and Clement of the Henry problem, as well as the groundwater flow in the closed desert basin of Pilot Valley, is studied using the proposed model. Copyright © 2011 John Wiley & Sons, Ltd.     

Drainage density on progressively tilted surfaces with different gradients,Wheeler Ridge,California

Wheeler Ridge in the Southern San Joaquin Valley, California, is an anticlinal fold which has been progressively uplifted during the last 250 ka. Drainage networks on the ridge become younger as the anticline's eastern tip is approached. Because of the fold's asymmetric shape, surfaces on opposite flanks of the ridge have similar ages but very different gradients. The ridge provides important insights into drainage development on progressively tilted surfaces, as existing studies are restricted to static topography. A surface gradient of between 4·8° and c.10° is needed to initiate channel networks. This gradient threshold is consistent with previous studies of the gradient and upslope area needed to incise a channel through overland flow. Comparison of coeval drainage networks on opposite flanks of the ridge allows the controversial relationship between drainage density and gradient to be investigated. A lower valley density is observed on the higher gradient flank of Wheeler Ridge. Field observations from the ridge indicate that this inverse relationship is associated with hillslope erosion by shallow mass-wasting, the rate of which increases rapidly as a threshold gradient is approached. Comparison of data from Wheeler Ridge with other field studies and numerical models, shows that the form of the relationship between gradient and drainage density is process-dependent. A positive correlation occurs when erosion is a result of overland flow, whilst a negative correlation occurs where erosion is dominated by shallow mass-wasting. Copyright © 1999 John Wiley & Sons, Ltd.     

Directed blasts and blast-generated pyroclastic density currents: a comparison of the Bezymianny 1956, Mount St Helens 1980, and Soufrière Hills,Montserrat 1997 eruptions and deposits

We compare eruptive dynamics, effects and deposits of the Bezymianny 1956 (BZ), Mount St Helens 1980 (MSH), and Soufrière Hills volcano, Montserrat 1997 (SHV) eruptions, the key events of which included powerful directed blasts. Each blast subsequently generated a high-energy stratified pyroclastic density current (PDC) with a high speed at onset. The blasts were triggered by rapid unloading of an extruding or intruding shallow magma body (lava dome and/or cryptodome) of andesitic or dacitic composition. The unloading was caused by sector failures of the volcanic edifices, with respective volumes for BZ, MSH, and SHV c. 0.5, 2.5, and 0.05 km³. The blasts devastated approximately elliptical areas, axial directions of which coincided with the directions of sector failures. We separate the transient directed blast phenomenon into three main parts, the burst phase, the collapse phase, and the PDC phase. In the burst phase the pressurized mixture is driven by initial kinetic energy and expands rapidly into the atmosphere, with much of the expansion having an initially lateral component. The erupted material fails to mix with sufficient air to form a buoyant column, but in the collapse phase, falls beyond the source as an inclined fountain, and thereafter generates a PDC moving parallel to the ground surface. It is possible for the burst phase to comprise an overpressured jet, which requires injection of momentum from an orifice; however some exploding sources may have different geometry and a jet is not necessarily formed. A major unresolved question is whether the preponderance of strong damage observed in the volcanic blasts should be attributed to shock waves within an overpressured jet, or alternatively to dynamic pressures and shocks within the energetic collapse and PDC phases. Internal shock structures related to unsteady flow and compressibility effects can occur in each phase. We withhold judgment about published shock models as a primary explanation for the damage sustained at MSH until modern 3D numerical modeling is accomplished, but argue that much of the damage observed in directed blasts can be reasonably interpreted to have been caused by high dynamic pressures and clast impact loading by an inclined collapsing fountain and stratified PDC. This view is reinforced by recent modeling cited for SHV. In distal and peripheral regions, solids concentration, maximum particle size, current speed, and dynamic pressure are diminished, resulting in lesser damage and enhanced influence by local topography on the PDC. Despite the different scales of the blasts (devastated areas were respectively 500, 600, and >10 km² for BZ, MSH, and SHV), and some complexity involving retrogressive slide blocks and clusters of explosions, their pyroclastic deposits demonstrate strong similarity. Juvenile material composes >50% of the deposits, implying for the blasts a dominantly magmatic mechanism although hydrothermal explosions also occurred. The character of the magma fragmented by explosions (highly viscous, phenocryst-rich, variable microlite content) determined the bimodal distributions of juvenile clast density and vesicularity. Thickness of the deposits fluctuates in proximal areas but in general decreases with distance from the crater, and laterally from the axial region. The proximal stratigraphy of the blast deposits comprises four layers named A, B, C, D from bottom to top. Layer A is represented by very poorly sorted debris with admixtures of vegetation and soil, with a strongly erosive ground contact; its appearance varies at different sites due to different ground conditions at the time of the blasts. The layer reflects intense turbulent boundary shear between the basal part of the energetic head of the PDC and the substrate. Layer B exhibits relatively well-sorted fines-depleted debris with some charred plant fragments; its deposition occurred by rapid suspension sedimentation in rapidly waning, high-concentration conditions. Layer C is mainly a poorly sorted massive layer enriched by fines with its uppermost part laminated, created by rapid sedimentation under moderate-concentration, weakly tractive conditions, with the uppermost laminated part reflecting a dilute depositional regime with grain-by-grain traction deposition. By analogy to laboratory experiments, mixing at the flow head of the PDC created a turbulent dilute wake above the body of a gravity current, with layer B deposited by the flow body and layer C by the wake. The uppermost layer D of fines and accretionary lapilli is an ash fallout deposit of the finest particles from the high-rising buoyant thermal plume derived from the sediment-depleted pyroclastic density current. The strong similarity among these eruptions and their deposits suggests that these cases represent similar source, transport and depositional phenomena.     

综合电法在新疆哈西金矿区寻找隐伏矿的应用

EH4电磁测深和高密度电法测量均为近年来发展起来的地球物理手段.EH4电磁测深是基于电磁原理的地球物理手段,探测深度大(可达1000m),可用于确定矿化系统深部的宏观构造格架和产状变化;高密度电法集电剖面和电测深于一体,对地质结构解析度高,且同时能够进行激发极化法测量,探明地下金属硫化物富集情况.这两种方法在新疆哈西金矿区综合运用,在寻找覆盖层下的隐伏矿方面取得了良好的效果.     

基于特征匹配的月球撞击坑自动提取研究

本文提出了一种基于特征匹配的撞击坑自动提取算法,该算法以单个撞击坑的5个典型影像特征为依据,用最大类间方差法将月面影像分割为暗区、亮区和背景3类;再使用区域生长将离散点聚合,通过特征匹配找出属于同一撞击坑的暗区与亮区,并利用八方向Sobel算子获取边缘控制点并拟合边缘。经过"嫦娥一号"和"嫦娥二号"部分遥感影像的验证,该算法对于纬度较高地区的月面影像提取效果较好,已成功应用到数字月球平台进行全月展示。     

Gaussian states in de Sitter spacetime and the evolution of semiclassical density perturbations.

The evolution of Gaussian quantum states in the de Sitter phase of the early universe is investigated. The potential is approximated by that of an inverted oscillator. We study the origin and magnitude of the density perturbations with special emphasis on the nature of the semiclassical limits     

利用卫星重力数据计算地球内部密度异常

地球外部重力场是由地球内部物质分布决定的。本文利用ＲＡＰＰ８１１８０阶卫星重力位系数根据异常源埋深与重力位系数阶数的关系和重力场分离方法计算了经度为９０°Ｅ的地球密度异常剖面，得到了地球内部不同深度的密度异常结果，并初步作了地球物理解释．计算结果得到的深度为６５ｋｍ处的低密度异常带与地球模型的ＬＩＤ层和Ｃ层较为接近。