“大村庄制”合并村庄脆弱性评估——以宁夏永宁县试验区为个案     

刘学武  王旭东 《地域研究与开发》2022,41(1):151-155

宁夏永宁县试验区内各合并村庄受到外部扰动时会表现出一定程度的脆弱性,并通过敏感性与适应力状况表达出来。基于结构方程模型原理构建合并村庄测量模型、一阶脆弱性SEM,运算处理试验区内8个合并村庄1600份有效问卷的调查数据,优化出合并村庄脆弱性评估指标,估算评估指标权重;依据优化出的脆弱性评估指标及评估指标权重构建灰色定权聚类模型,从扰动、敏感性、适应力3个维度评估合并村庄的脆弱性。结果表明:试验区内合并村庄整体上扰动效果差、敏感性较强、适应力一般。脆弱性规律为扰动效果好则敏感性弱、适应力强、脆弱性程度低,扰动效果差则敏感性较强或强、适应力一般、脆弱性程度高或较高。  相似文献   

超燃冲压发动机凹腔内补氧的强化点火试验     

席文雄  王振国  李庆  刘卫东 《贵州气象》2013,(4):506-511

在超燃冲压发动机扩张型燃烧室中,对凹腔内局部补氧的点火强化方法进行了试验研究。采用高速摄影手段研究了不同的补氧方式对凹腔内火焰分布特征和燃烧强度的影响,并针对并联双凹腔燃烧室构型,研究了在单侧凹腔补氧条件下向异侧凹腔的火焰传播过程。试验结果表明,采用凹腔内补氧的方式能调节凹腔内的燃料浓度分布、改善凹腔内的燃烧过程,控制燃烧放热强度;稳态燃烧情况下,观察到凹腔驻留火焰的两种存在特征,分别表现为:由回流区热量反馈机制作用下的凹腔局部驻留火焰和燃烧室全局压力反馈影响下的凹腔剪切层火焰。只有在单侧凹腔燃烧建立了全局压力反馈的条件下才能实现凹腔火焰的异侧传播。   相似文献   

Runoff generative process and runoff yield from arid talus mantled slopes   总被引：3，自引：0，他引：3  

A. Yair  H. Lavee 《地球表面变化过程与地形》1976,1(3):235-247

Previous works dealing with the influence of a stone cover on runoff yield showed that runoff, attributed to the sealing effect of the topsoil by raindrops impact, was negatively related to the per cent of stone cover and stone size. These works were conducted on gentle slopes (3–11·5 degree) with a per cent of stone cover generally lower than 50 per cent, and composed of gravels. The present study deals with the runoff yield of steep talus slopes (26–36 degree) whose per cent of stone cover is very high (90–100 per cent), composed of cobbles and boulders. Three stimulated rainstorms were performed at various rainfall. intensities and durations on each one of six plots representative of the North eastern sector of Sinai. Although the contiguous stony cover prevented surface sealing by raindrops impact, runoff developed quite quickly on most slopes, and reached at peak discharge, after approximately ten minutes, up to 56 per cent of the rainfall. Differences between plots, in time lag, peak discharge and other hydrological variables, could be attributed mainly to the properties of the upper stony layer, with stone size as the most influential factor. Contrary to previous works, a positive relationship, was obtained between stone size to runoff yield. The result is explained by the process of water concentration. Each cobble and boulder behaves, on a smaller scale, like a bare rocky surface and yields per unit area water amounts beyond the infiltration rate of the limited uncovered areas. For a given stony cover the effect of water concentration is quicker with the big blocks than with gravels. A series of graphs trying to relate theoretically the relative importance of sealing and water concentration processes in runoff generation, at various conditions of stone cover and stone size, is proposed. The graphs enable to reconcile the results of the present study with those of previous works.  相似文献   

一种新的台风海面风场的拟合方法   总被引：6，自引：1，他引：6       下载免费PDF全文

盛立芳  吴增茂 《热带气象学报》1993,9(3):265-271

基于台风风场的经验风公式和修正的梯度风方程并考虑了台风气压场的非对称性,提出了一种新型的台风风场合成模式。经过对10多个不同类型热带气旋(台风)的检验,结果表明,新的模式可以模拟出各种强度及不同眼半径台风的海面风场,比以往常用模式能更真实地反映实际台风风场。  相似文献   

Pre-accretionary and parent body histories of a cometary aggregate particle     

Frans J.M. Rietmeijer 《Icarus》2011,211(2):948-959

Chondrite aggregate interplanetary dust particle IDP L2011K7, collected in the Earth’s lower stratosphere, is an agglomerate of diopside, Mg,Fe-olivine, rare Fe-sulfide and abundant amorphous Mg,Fe-silicates. The overwhelming majority of amorphous silicates have a serpentine-dehydroxylate [(Mg,Fe)₃Si₂O₇] composition; a few have a smectite-dehydroxylate [(Mg,Fe)₆Si₈O₂₂] composition. The cation ratios of the amorphous silicates are notably identical to those of serpentine and smectite phyllosilicates. This paper follows the chronological changes in the amorphous silicates that include (1) formation of nanometer scale crystalline silicates (Mg,Fe-olivine and pyroxene), (2) partial hydration and formation of antigorite-serpentine proto-phyllosilicates, (3) partial dehydration of these proto-phyllosilicates, and finally oxidation and Fe-oxide formation by flash heating during atmospheric entry. Environmental conditions capable of driving these changes in the diffuse interstellar medium or solar nebula, in a comet nucleus, or in circumsolar orbit as a cometary meteoroid were marginal at best. These changes could only proceed because of the unique amorphous silicate compositions. While this study cannot make a firm statement about an interstellar or solar nebula origin for its amorphous silicates that are irradiation-induced olivine, this study does find that amorphous silicates with serpentine and (rare) smectite compositions are an important fraction of the amorphous silicates in comets in addition to amorphous olivine and pyroxene. It is noted that an ice and water-free, millimeter-scale, structurally coherent crumb would be an ample ‘microenvironment’ to evolve micrometer-scale dust. After all IDP L2011K7 only measures 22 × 17 μm.  相似文献   

Retrieving optical depth from shadows in orbiter images of Mars     

N.M. Hoekzema  M. Garcia-Comas  O.J. Stenzel  H.U. Keller  W.A. Delamere 《Icarus》2011,214(2):447-461

The difference in brightness between shadowed and sunlit regions in space images of Mars is a measure of the optical depth of the atmosphere. The translation of this difference into optical depth is what we name the “shadow method”. Our analysis of two HRSC data-sets and a HiRISE data-set indicates that it is possible to estimate the optical depth with the shadow method. In colors between yellow and red the accuracy may be around ±15%, and in some cases ±8-10%. In other colors we found larger errors.We came to these results in two steps. First, we investigated in how far shadow method retrievals are proportional to the true optical depth. To this end we analyzed about 150 locations in Valles Marineris that were imaged by HRSC. Whereas the studied region spans about 8 km in altitude we were able to study the relation between altitude and shadow-method retrievals. Retrievals from five HRSC panchromatic (675 ± 90 nm) stereo images yielded scale-heights with an average of 12.2 ± 0.7 km, which is very close to the expected local pressure scale height. Many studies have shown that the scale-height of optical depth and pressure commonly are similar. This indicates that the shadow method retrievals are on average close to proportional to the optical depth, because otherwise these would probably not yield a correct scale-height. HRSC’s red image yielded very similar results, but the blue, green, and NIR images did not.Next, we compared optical depth measurements by the two MER rovers with shadow method retrievals from orbiter images of the rover exploration sites. Retrievals with the shadow method appear systematically smaller than the rover measurements; dividing the retrievals by a “correction factor” yields an estimate of the real optical depth. Retrievals from three HRSC panchromatic stereo images of a region near the Spirit rover yielded a correction factor of 0.63 ± 0.09 when the sunlit comparison regions were at varying and more or less arbitrary distances from the shadows and 0.71 ± 0.06 when these were close together. Twenty retrievals from a HiRISE red (650 ± 100 nm) image of the Opportunity exploration site similarly yielded 0.68 ± 0.09. The results from these two case studies suggest that the shadow method has an accuracy of about ±15% or around ±8-10% in the best cases.  相似文献   

Apollo video photogrammetry estimation of plume impingement effects   总被引：1，自引：0，他引：1  

Christopher Immer  Philip Metzger 《Icarus》2011,214(1):46-52

Future missions to the Moon may require numerous landings at the same site. Since the top few centimeters are loosely packed regolith, plume impingement from the Lander ejects the granular material at high velocities. Much work is needed to understand the physics of plume impingement during landing to protect hardware surrounding the landing sites. While mostly qualitative in nature, the Apollo Lunar Module landing videos can provide a wealth of quantitative information using modern photogrammetry techniques. The authors have used the digitized videos to quantify plume impingement effects of the landing exhaust on the lunar surface. The dust ejection angle from the plume is estimated at 1°-3°. The lofted particle density is estimated at 10⁸-10¹³ particles/m³. Additionally, evidence for ejection of large 10-15 cm sized objects and a dependence of ejection angle on thrust are presented. Further work is ongoing to continue quantitative analysis of the landing videos.  相似文献   

Mid-IR, Far-IR, Raman micro-spectroscopy, and FESEM-EDX study of IDP L2021C5: Clues to its origin     

R. Brunetto  J. Borg  F.J.M. Rietmeijer  C. Sandt  A. Rotundi  Z. Djouadi 《Icarus》2011,212(2):896-910

  相似文献   

Stretching lineation and transport direction in the Ibero-Armorican arc during the siluro-devonian collision     

Jean-Pierre Burg  Pascal Bale  Jean-Pierre Brun  Jacques Girardeau 《Geodinamica Acta》2013,26(1):71-87

Abstract

Large structures, lineations, foliations and sense of shear criteria are examined on the scale of the whole Ibero-Armorican Arc. Four sections (Galicia, Brittany-Vendée, Limousin and Eastern Massif Central) exemplify the major thrust sheets observed around the Arc. Stretching lineations are contemporaneous with the siluro-devonian metamorphism and are either transverse, oblique or parallel to the collision zone. A kinematic analysis shows that these lineations have resulted from a dominanüy transverse shear deformation which was followed by, or combined with, a longitudinal shear direction. On the scale of the entire Arc, this variation in the shear direction is interpreted as resulting from an early head on thrusting relative movement evolving to large scale movements parallel to the plate boundaries. Experiments with sand-silicone models support a model which generates the Arc by interaction between a transform sinistral direction, and a converning zone at a high angle to the transform direction.  相似文献   

沉积盆地热化学硫酸盐还原作用评述   总被引：29，自引：1，他引：28  

蔡春芳  李宏涛 《地球科学进展》2005,20(10):1100-1105

川东天然气藏H2S 气体泄露而导致重大伤亡事故后,热化学硫酸盐还原作用（TSR）成为了国内研究的热点。在油气储层条件下,尽管甲烷是最稳定的烃类,但TSR被诱发后,因为甲烷浓度远高于其它烃类,水溶甲烷能与硫酸根离子反应产生H2S 气体。同时,发现在参与TSR反应的有机质、起始温度、硫同位素分馏效应等方面,实验模拟结果均与地质实例观察结果有较大的差异,可能与TSR反应的催化剂等方面认识不足有关。并认为,TSR成因的H2S或元素硫可以在晚成岩期合并入有机质中,形成新的有机含硫化合物。但在自然界中,这类化合物很少被鉴别出来。  相似文献