可靠性空间分析初探     

史文中  陈江平  詹庆明  舒红 《武汉大学学报(信息科学版)》2012,37(8):883-887,991

从工程和生命科学的可靠性概念出发,结合地理信息科学的自身特点,强调空间数据及分析的全过程质量和分析结果的决策可用性。首次给出了可靠性空间分析的概念,分析了可靠性空间分析的特点、面临的主要问题和研究方法,探讨了可靠性空间分析的主要理论、研究方向和应用领域,促进了空间分析从不确定性研究向可靠性空间分析方向的发展。  相似文献   

GPS对流层延迟模型的比较分析     

袁丰波  潘元进  何美琳  文鸿雁 《地理空间信息》2012,(2):119-121

基于GPS对流层模型,对几种模型进行实际应用的对比,通过GAMIT软件对CORS数据进行处理,分析得出了几种模型在GPS反演大气水汽含量应用中的精度。  相似文献   

地面几何标定的定向片自检校光束法区域网平差模型     

邹瑜  雷蓉  纪松  范大昭 《测绘工程》2012,21(5):8-12

针对航天线阵传感器,综合镜头光学畸变影响、像元尺寸与焦距的变化影响以及镜头的旋转作用,构建8标定参数的内方位自检校模型;利用定向片内插模型,描述影像的外方位元素变化;建立自检校光束法区域网平差模型,在对模型进行线性化的过程中,引入待标定的定向片外方位元素;利用SPOT5模拟数据对平差模型进行实验验证,结果表明,平差模型能够联合标定内方位自检校参数与外方位元素,标定结果准确。  相似文献   

The deep wind structure of the giant planets: Results from an anelastic general circulation model     

Yohai Kaspi  Glenn R. Flierl 《Icarus》2009,202(2):525-542

The giant gas planets have hot convective interiors, and therefore a common assumption is that these deep atmospheres are close to a barotropic state. Here we show using a new anelastic general circulation model that baroclinic vorticity contributions are not negligible, and drive the system away from an isentropic and therefore barotropic state. The motion is still aligned with the direction of the axis of rotation as in a barotropic rotating fluid, but the wind structure has a vertical shear with stronger winds in the atmosphere than in the interior. This shear is associated with baroclinic compressibility effects. Most previous convection models of giant planets have used the Boussinesq approximation, which assumes the density is constant in depth; however, Jupiter's actual density varies by four orders of magnitude through its deep molecular envelope. We therefore developed a new general circulation model (based on the MITgcm) that is anelastic and thereby incorporates this density variation. The model's geometry is a full 3D sphere down to a small inner core. It is nonhydrostatic, uses an equation of state suitable for hydrogen-helium mixtures (SCVH), and is driven by an internal heating profile. We demonstrate the effect of compressibility by comparing anelastic and Boussinesq cases. The simulations develop a mean state that is geostrophic and hydrostatic including the often neglected, but significant, vertical Coriolis contribution. This leads to modification of the standard thermal wind relation for a deep compressible atmosphere. The interior flow organizes in large cyclonically rotating columnar eddies parallel to the rotation axis, which drive upgradient angular momentum eddy fluxes, generating the observed equatorial superrotation. Heat fluxes align with the axis of rotation, and provide a mechanism for the transport of heat poleward, which can cause the observed flat meridional emission. We address the issue of over-forcing which is common in such convection models and analyze the dependence of our results on this; showing that the vertical wind structure is not very sensitive to the Rayleigh number. We also study the effect of rotation, showing how the transition from a rapidly to a slowly rotating system affects the dynamics.  相似文献   

Detection and temporal coherence of p‐modes below 1.4 mHz     

A. Eff‐Darwich  C. Rgulo  S.G. Korzennik  F. Prez Hernndez  T. Roca Corts 《Astronomische Nachrichten》2008,329(5):470-475

Data collected recently by the helioseismic experiments aboard the SOHO spacecraft have allowed the detection of low degree p‐modes with increasingly lower order n. In particular, the GOLF experiment is currently able to unambiguously identify low degree modes with frequencies as low as 1.3 mHz. The detection of p‐modes with very low frequency (i.e., low n), is difficult due to the low signal‐to‐noise ratio in this spectral region and its contamination by solar signals that are not of acoustic origin. To address this problem without using any theoretical a priory, we propose a methodology that relies only on the inversion of observed values to define a spectral window for the expected locations of these low frequency modes. The application of this method to 2920‐day‐long GOLF observations is presented and its results discussed. (© 2008 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

Modelling solar atmospheric gravity oscillation modes     

B. Pintr 《Astronomische Nachrichten》2008,329(5):503-507

Solar oscillations are investigated in a one‐dimensional hydrodynamic plane‐parallel model with an atmosphere. Besides the acoustic pressure (p) modes, the fundamental (f) and Lamb mode, another set of eigenmodes, a group of atmospheric gravity (g) modes, is found in the low‐frequency region of the spectrum. Their frequencies and spatial behaviour are studied. (© 2008 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

Antipodal effects of lunar basin-forming impacts: Initial 3D simulations and comparisons with observations     

Lon L. Hood  Natalia A. Artemieva 《Icarus》2008,193(2):485-502

3D simulations of basin-scale lunar impacts are carried out to investigate: (a) the origins of strong crustal magnetic fields and unusual terrain observed to occur in regions antipodal to young large basins; and (b) the origin of enhanced magnetic and geochemical anomalies along the northwest periphery of the South Pole-Aitken (SPA) basin. The simulations demonstrate that a basin-forming impact produces a massive, hot, partially ionized cloud of vapor and melt that expands thermally around the Moon, converging near the basin antipode approximately 1 h after the impact for typical impact parameters. In agreement with previous work, analytic calculations of the interaction of this vapor-melt cloud with an initial ambient magnetic field predict a substantial temporary increase in field intensity in the antipodal region. The time of maximum field amplification coincides with a period when impacting ejecta also converge near the antipode. The latter produce antipodal shock stresses within the range of 5-25 GPa where stable shock remanent magnetization (SRM) of lunar soils has been found experimentally to occur. Calculated antipodal ejecta thicknesses are only marginally sufficient to explain the amplitudes of observed magnetic anomalies if mean magnetization intensities are comparable to those produced experimentally. This suggests that pre-existing ejecta materials, which would also contain abundant metallic iron remanence carriers, may be important anomaly sources, a possibility that is consistent with enhanced magnetic anomalies observed peripheral to SPA. The latter anomalies may be produced by amplified secondary ejecta impact shock waves in the thick SPA ejecta mantle occurring near the antipodes of the Imbrium and Serenitatis impacts. Together with converging seismic compressional waves, these antipodal impact shocks may have produced especially deep fracture zones along the northwest edge of SPA near the Imbrium antipode, allowing the ascent of magma with enhanced KREEP concentrations.  相似文献   

基于区间非概率可靠性方法的岩溶区桩基下溶洞顶板稳定性评价     

秦溯  李云安  孙琳 《水文地质工程地质》2019,(5):81-88

岩溶区桩基下溶洞顶板稳定性影响因素取值的不确定性及其样本数量的有限性,给桩基下溶洞顶板稳定性的评价带来了一定困难。根据现有研究成果,建立桩基下溶洞顶板抗冲切、抗剪切和抗弯力学简化模型,并从理论上推导相应的稳定性验算公式。在此基础上,结合区间分析理论和结构非概率可靠性度量方法,提出了基于区间非概率可靠性方法的桩基下溶洞顶板稳定性评价方法。该方法采用MATLAB中的INTLAB工具箱进行区间运算,并运用截断法消除运算过程中的区间扩展现象,最后通过比较溶洞顶板体系的非概率可靠性指标η与1的大小来判断桩基下溶洞顶板稳定性。以丹霞高速互通中D匝道2#桩基下溶洞为例,计算出该桩基下溶洞顶板体系的非概率可靠性指标η=7.95,该值大于1说明该桩基下溶洞顶板处于稳定状态,且评价结果与工程实际相符,表明了该方法的合理性与可行性。分别以3种功能函数为单位,研究当区间变量的变异系数C不同时(C从0.01递增至0.1),对应非概率可靠性指标η的变化规律。研究表明,随各区间变量变异系数C的增大,相应非概率可靠性指标呈不同程度的降低,其中溶洞顶板厚度h的变异性对评价结果影响最大,其次为桩端阻力分担比T,桩顶反力F的影响相对最小。  相似文献   

基于可靠度理论的尾矿坝失稳概率及敏感性分析          下载免费PDF全文

李涛  刘国栋  王聪 《中国地质灾害与防治学报》2019,30(3):81-86

为了能够真实反映砭家沟尾矿库的稳定特性,运用Monte Carlo试验原理,考虑库区砂层的空间变异特性,利用Slope/W软件对尾矿库进行了概率分析与敏感性分析。分析表明,抽样方式的不同,使尾矿坝体失稳概率和可靠性指标发生了大幅波动,但是并没有使安全系数产生明显变化,也验证了仅将安全系数作为衡量尾矿坝体稳定性的唯一标准是不合适的;敏感性分析也表明了砂层主要参数对安全系数影响的敏感程度,同时也表明黏聚力是影响库区稳定的主要砂层因素。通过研究,为尾矿库今后的运行与管理提供了理论依据,具有一定的指导意义。  相似文献   

Reliability analysis of the induced damage for single-hole rock blasting     

Mahdi Shadab Far  Yuan Wang  Yousif A. H. Dallo 《Georisk: Assessment and Management of Risk for Engineered Systems and Geohazards》2019,13(1):82-98

Rock explosion has always been a complex problem because neither rock characteristics nor explosion waves could be accurately estimated. As such, this imposes a high uncertainty on deterministic methodologies available for damage prediction. In this paper, by defining two damage zones around the blast hole, including crushed and cracked zones, a first-order reliability analysis (FORM) was adopted to address this issue. For this purpose, FORM was used in a double-loop algorithm, where the inner loop was responsible for converging the FORM, and the outer loop was assigned to feed the inner loop with new cases. Using such nested-loop algorithm, the probability of exceedance was calculated for any desired damage zone radius. The maximum effect of the involved parameters on the failure probability induced around the blast hole was additionally studied using a parametric reliability analysis. The results showed that the radii for crushed and cracked zones are limited to 0.5 and 4.2?m, respectively, so that the probability of going beyond these limits is less than 1%. Moreover, the analyses of decoupled explosions showed that increasing the gap between the explosion charge and wall of the borehole could severely reduce the failure probability; however, the maximum effect of decoupling ratio occurs in the small range of radii between 0.3?mm and 2.35?m.  相似文献