Response of soil aggregate disintegration to the different content of organic carbon and its fractions during splash erosion     

Hairu Li  Gang Liu  Ju Gu  Hong Chen  Hongqiang Shi  Mohamed A. M. Abd Elbasit  Feinan Hu 《水文研究》2021,35(2):e14060

Aggregate disintegration is a critical process in soil splash erosion. However, the effect of soil organic carbon (SOC) and its fractions on soil aggregates disintegration is still not clear. In this study, five soils with similar clay contents and different contents of SOC have been used. The effects of slaking and mechanical striking on splash erosion were distinguished by using deionized water and 95% ethanol as raindrops. The simulated rainfall experiments were carried out in four heights (0.5, 1.0, 1.5 and 2.0 m). The result indicated that the soil aggregate stability increased with the increases of SOC and light fraction organic carbon (LFOC). The relative slaking and the mechanical striking index increased with the decreases of SOC and LFOC. The reduction of macroaggregates in eroded soil gradually decreased with the increase of SOC and LFOC, especially in alcohol test. The amount of macroaggregates (>0.25 mm) in deionized water tests were significantly less than that in alcohol tests under the same rainfall heights. The contribution of slaking to splash erosion increased with the decrease of heavy fractions organic carbon. The contribution of mechanical striking was dominant when the rainfall kinetic energy increased to a range of threshold between 9 J m⁻² mm⁻¹ and 12 m⁻² mm⁻¹. This study could provide the scientific basis for deeply understanding the mechanism of soil aggregates disintegration and splash erosion.  相似文献   

From soil aggregates to riverine flocs: a laboratory experiment assessing the respective effects of soil type and flow shear stress on particles characteristics          下载免费PDF全文

T. Grangeon  I. G. Droppo  C. Legout  M. Esteves 《水文研究》2014,28(13):4141-4155

Particles eroded from hillslopes and exported to rivers are recognized to be composite particles of high internal complexity. Their architecture and composition are known to influence their transport behaviour within the water column relative to discrete particles. To‐date, hillslope erosion studies consider aggregates to be stable once they are detached from the soil matrix. However, lowland rivers and estuaries studies often suggest that particle structure and dynamics are controlled by flocculation within the water column. In order to improve the understanding of particle dynamics along the continuum from hillslopes to the lowland river environment, soil particle behaviour was tested under controlled laboratory conditions. Seven flume erosion and deposition experiments, designed to simulate a natural erosive event, and five shear cell experiments were performed using three contrasting materials: two of them were poorly developed and as such can not be considered as soils, whilst the third one was a calcareous brown soil. These experiments revealed that soil aggregates were prone to disaggregation within the water column and that flocculation may affect their size distribution during transport. Large differences in effective particle size were found between soil types during the rising limb of the bed shear stress sequence. Indeed, at the maximum applied bed shear stress, the aggregated particles median diameter was found to be three times larger for the well‐developed soil than for the two others. Differences were smaller in the falling limb, suggesting that soil aggregates underwent structural changes. However, characterization of particles strength parameters showed that these changes did not fully turn soil aggregates into flocs, but rather into hybrid soil aggregate–floc particles. Copyright © 2013 John Wiley & Sons, Ltd.  相似文献   

带竖向构造钢筋再生混凝土砖结构振动台试验研究     

曹万林  周中一  董宏英  张勇波 《地震工程与工程振动》2012,32(4):111-117

提出了带竖向构造钢筋再生混凝土砖砌体结构,进行了2个两层再生混凝土砖砌体房屋结构1/2缩尺模型的模拟地震振动台试验研究,2个结构模型的墙体厚度均为120 mm,一层设有门洞和窗洞,二层设有窗洞。2个模型中,1个为带竖向构造钢筋再生混凝土砖砌体房屋,1个为普通无竖向构造钢筋再生混凝土砖砌体房屋。试验中输入El Centro地震动,测试分析了台面加速度反应、一层和二层顶板加速度反应、结构层间位移反应以及各阶段结构损伤与破坏特征等。研究表明:带竖向构造钢筋再生混凝土砖砌体房屋比普通再生混凝土砖砌体房屋的破坏程度轻,墙体裂缝位置相对错动小,抗震性能显著提高;带竖向构造钢筋再生混凝土砖砌体房屋可用于地震区村镇建筑。  相似文献   

Mud dispersal across a Cretaceous prodelta: Storm‐generated,wave‐enhanced sediment gravity flows inferred from mudstone microtexture and microfacies     

A. Guy Plint 《Sedimentology》2014,61(3):609-647

Determining sediment transport direction in ancient mudrocks is difficult. In order to determine both process and direction of mud transport, a portion of a well‐mapped Cretaceous delta system was studied. Oriented samples from outcrop represent prodelta environments from ca 10 to 120 km offshore. Oriented thin sections of mudstone, cut in three planes, allowed bed microstructure and palaeoflow directions to be determined. Clay mineral platelets are packaged in equant, face‐face aggregates 2 to 5 μm in diameter that have a random orientation; these aggregates may have formed through flocculation in fluid mud. Cohesive mud was eroded by storms to make intraclastic aggregates 5 to 20 μm in diameter. Mudstone beds are millimetre‐scale, and four microfacies are recognized: Well‐sorted siltstone forms millimetre‐scale combined‐flow ripples overlying scoured surfaces; deposition was from turbulent combined flow. Silt‐streaked claystone comprises parallel, sub‐millimetre laminae of siliceous silt and clay aggregates sorted by shear in the boundary layer beneath a wave‐supported gravity flow of fluid mud. Silty claystone comprises fine siliceous silt grains floating in a matrix of clay and was deposited by vertical settling as fluid mud gelled under minimal current shear. Homogeneous clay‐rich mudstone has little silt and may represent late‐stage settling of fluid mud, or settling from wave‐dissipated fluid mud. It is difficult or impossible to correlate millimetre‐scale beds between thin sections from the same sample, spaced only ca 20 mm apart, due to lateral facies change and localized scour and fill. Combined‐flow ripples in siltstone show strong preferred migration directly down the regional prodelta slope, estimated at ca 1 : 1000. Ripple migration was effected by drag exerted by an overlying layer of downslope‐flowing, wave‐supported fluid mud. In the upper part of the studied section, centimetre‐scale interbeds of very fine to fine‐grained sandstone show wave ripple crests trending shore normal, whereas combined‐flow ripples migrated obliquely alongshore and offshore. Storm winds blowing from the north‐east drove shore‐oblique geostrophic sand transport whereas simultaneously, wave‐supported flows of fluid mud travelled downslope under the influence of gravity. Effective wave base for sand, estimated at ca 40 m, intersected the prodelta surface ca 80 km offshore whereas wave base for mud was at ca 70 m and lay ca 120 km offshore. Small‐scale bioturbation of mud beds co‐occurs with interbedded sandstone but stratigraphically lower, sand‐free mudstone has few or no signs of benthic fauna. It is likely that a combination of soupground substrate, frequent storm emplacement of fluid mud, low nutrient availability and possibly reduced bottom‐water oxygen content collectively inhibited benthic fauna in the distal prodelta.  相似文献   

岩溶石漠化山地不同退耕模式土壤抗蚀性及其与结构体分形关系研究   总被引：6，自引：3，他引：3  

胡宁  傅瓦利  马志敏  甄晓君  袁红 《中国岩溶》2008,27(2):115-121

通过对岩溶石漠化山地中小尺度范围内的现有三种主要退耕模式及对照地土壤抗蚀性主成分分析及与各级结构体分形维数关系研究,结果表明：（1）研究区退耕地在3～6年内土壤抗蚀性均发生了比较明显的变化,但都介于传统耕地与马尾松次生灌丛之间,其中以具有复式结构的退耕樟树＋草被退耕模式的抗蚀效果较理想;（2）与传统旱耕地不同,各退耕模式土壤抗蚀性均是A层土壤强于B层土壤,表明退耕有利于A层土壤抗蚀性迅速提高,尤其是草本＋乔灌模式对A层土壤抗蚀性的提高更为显著;（3）〉O．25mm水稳性团聚体含量及破坏率、水稳性指数、有机质含量为评价土壤抗蚀性的最佳四指标;（4）微团聚体、风干团聚体分形维数表征土壤抗蚀性有一定的局限性,而机械组成、水稳定性团聚体分维数与抗蚀性综合分值相关性较高,尤其是水稳性团聚体分形维数可较好地反映出土壤的抗蚀特性。  相似文献   

基于灰色模糊聚类分析的吉林省黑土结构综合评价   总被引：1，自引：0，他引：1  

秦焱  王清  陈慧娥  范建华 《吉林大学学报(地球科学版)》2008,38(5)

通过对黑土结构指标的定量研究,确定颗粒组成、团聚性和孔隙性3个方面的9个结构指标,建立结构综合评价体系,并采用灰色模糊聚类分析法对黑土的结构进行综合评价,确定吉林黑土的结构质量及肥力状况。结果表明,肥力中-低等样品数量占总量的53%,吉林黑土总体肥力状况不容乐观。以灰色模糊聚类分析法评价土壤结构不需要建立评价的分级标准,可以根据评价对象的实际情况进行最优聚类分析,采用结构性指标对黑土肥力和退化进行评价是可行的。  相似文献   

Electric Discharges in the Protoplanetary Nebula as a Source of Impulse Magnetic Fields to Promote Dust Aggregation     

Túnyi  I.  Guba  P.  Roth  L. E.  Timko  M. 《Earth, Moon, and Planets》2003,93(1):65-74

Lightning discharge generated in the protoplanetary nebula is viewed as a temporally isolated surge in the flow of electrically charged particles, similar to that of terrestrial lightning. If the current is intense enough, a powerful circular impulse magnetic field is generated around the instantaneous virtual electric conductor. Such magnetic field is capable of magnetizing dust grains containing ferromagnetic components present in its vicinity to their saturation levels. As a result, dust grains attract one another, forming the aggregates. This magnetically driven attraction suggests an important process possibly operational at an early stage of the planetary accretion. Based on both a classical model for electric conductor, and the theory of Lienard–Wiechert electromagnetic potentials, our calculations show that the magnetic impulse due to a discharge channel of a few cm in diameter transferring a charge of about 10⁴ electrons reaches as high as 10 T. At these magnetic fields, the ferromagnetic dust grains, and possibly the already-formed larger aggregates as well, are easily magnetized to the saturation levels, producing compact clusters exhibiting permanent magnetic moments.  相似文献   

粗粒料强度和变形的大型三轴试验研究   总被引：14，自引：5，他引：14  

秦红玉  刘汉龙  高玉峰  戴鹏飞 《岩土力学》2004,25(10):1575-1580

通过大型三轴试验，对高低围压下粗粒料的应力应变特性、抗剪强度、内摩擦角和颗粒破碎特性进行了对比分析，并探讨了不同泥岩含量对堆石坝料强度的影响。结果表明：中高围压下粗粒料表现出应变硬化特性和剪缩，强度包线和不同围压下的最大主应力比与剪胀率的关系近似为线性，而低围压下主要表现为应变软化和剪胀，抗剪强度包线等表现为非线性。随着围压的增加，主应力比降低、颗粒破碎率增大、内摩擦角减小。泥岩含量的增加使颗粒表面的摩擦阻力与粒间的咬合力减弱，导致抗剪强度降低。  相似文献   

Amoeboid olivine aggregates and related objects in carbonaceous chondrites: records of nebular and asteroid processes     

Alexander N. Krot  Michail I. Petaev  Shoichi Itoh  Timothy J. Fagan  Hisayoshi Yurimoto  Michael K. Weisberg  Matsumi Komatsu  Klaus Keil 《Chemie der Erde / Geochemistry》2004,64(3):185-239

Amoeboid olivine aggregates (AOAs) are the most common type of refractory inclusions in CM, CR, CH, CV, CO, and ungrouped carbonaceous chondrites Acfer 094 and Adelaide; only one AOA was found in the CB_b chondrite Hammadah al Hamra 237 and none were observed in the CB_a chondrites Bencubbin, Gujba, and Weatherford. In primitive (unaltered and unmetamorphosed) carbonaceous chondrites, AOAs consist of forsterite (Fa_<2), Fe, Ni-metal (5-12 wt% Ni), and Ca, Al-rich inclusions (CAIs) composed of Al-diopside, spinel, anorthite, and very rare melilite. Melilite is typically replaced by a fine-grained mixture of spinel, Al-diopside, and ±anorthite; spinel is replaced by anorthite. About 10% of AOAs contain low-Ca pyroxene replacing forsterite. Forsterite and spinel are always ¹⁶O-rich (δ^17,18O∼−40‰ to −50‰), whereas melilite, anorthite, and diopside could be either similarly ¹⁶O-rich or ¹⁶O-depleted to varying degrees; the latter is common in AOAs from altered and metamorphosed carbonaceous chondrites such as some CVs and COs. Low-Ca pyroxene is either ¹⁶O-rich (δ^17,18O∼−40‰) or ¹⁶O-poor (δ^17,18O∼0‰). Most AOAs in CV chondrites have unfractionated (∼2-10×CI) rare-earth element patterns. AOAs have similar textures, mineralogy and oxygen isotopic compositions to those of forsterite-rich accretionary rims surrounding different types of CAIs (compact and fluffy Type A, Type B, and fine-grained, spinel-rich) in CV and CR chondrites. AOAs in primitive carbonaceous chondrites show no evidence for alteration and thermal metamorphism. Secondary minerals in AOAs from CR, CM, and CO, and CV chondrites are similar to those in chondrules, CAIs, and matrices of their host meteorites and include phyllosilicates, magnetite, carbonates, nepheline, sodalite, grossular, wollastonite, hedenbergite, andradite, and ferrous olivine.Our observations and a thermodynamic analysis suggest that AOAs and forsterite-rich accretionary rims formed in ¹⁶O-rich gaseous reservoirs, probably in the CAI-forming region(s), as aggregates of solar nebular condensates originally composed of forsterite, Fe, Ni-metal, and CAIs. Some of the CAIs were melted prior to aggregation into AOAs and experienced formation of Wark-Lovering rims. Before and possibly after the aggregation, melilite and spinel in CAIs reacted with SiO and Mg of the solar nebula gas enriched in ¹⁶O to form Al-diopside and anorthite. Forsterite in some AOAs reacted with ¹⁶O-enriched SiO gas to form low-Ca pyroxene. Some other AOAs were either reheated in ¹⁶O-poor gaseous reservoirs or coated by ¹⁶O-depleted pyroxene-rich dust and melted to varying degrees, possibly during chondrule formation. The most extensively melted AOAs experienced oxygen isotope exchange with ¹⁶O-poor nebular gas and may have been transformed into magnesian (Type I) chondrules. Secondary mineralization and at least some of the oxygen isotope exchange in AOAs from altered and metamorphosed chondrites must have resulted from alteration in the presence of aqueous solutions after aggregation and lithification of the chondrite parent asteroids.  相似文献   

不同栽杉代数土壤抗蚀性的变化   总被引：7，自引：2，他引：5  

杨玉盛  陈光水  彭加才  邱仁辉 《山地学报》1999,17(2):163-167

采用标准地定位研究方法对杂木林及１代,２代,３代和４代杉木人工林土壤颗粒,土壤团聚体组成进行比较分析,结果表明：杂木要受人为干扰少,土壤颗粒及土壤团聚体组成较好,抗蚀性最好;但１代,２代,３代和４代分别是在杂木林及前１代林的采伐迹地上经再度干扰建立起来的,土壤结构破坏率加大,土壤团聚体稳定性减小,因而随着杉木林取代杂木林及杉木连栽代数增加,土壤抗蚀性减弱。  相似文献