三峡大坝下游粗细颗粒泥沙输移规律及成因

以三峡下游河段为研究对象,利用1987-2014年原型观测数据,分析粗细颗粒在时间和空间的输移过程,并以水文站作为划分单元探讨其成因.三峡水库蓄水后坝下游d≤0.125 mm(细颗粒)各粒径组沙量沿程递增,并小于蓄水前均值;d0.125 mm(粗颗粒)沙量在宜昌—监利河段得到补给,其下游为淤积趋势,其中2003-2007年至监利站恢复程度最大.在成因上:(1)宜昌—沙市河段,河床粗化限制了粗细颗粒泥沙补给,其中细颗粒补给受制于总水量,粗颗粒受制于大流量持续天数和量值;(2)沙市—监利河段,粗细颗粒补给均受制于总水量;(3)监利—螺山河段,洞庭湖入汇对细颗粒补给起决定作用,河床补给量中洪水年大于中枯水年,粗颗粒为淤积趋势,且中洪水年淤积量小于中枯水年;(4)螺山—汉口河段,细颗粒增加受河床补给决定,2008-2014年补给强度弱于2003-2007年,2010年前后粗颗粒泥沙由淤转冲,与大流量持续天数和量值增加有关;(5)汉口—九江河段,细颗粒泥沙淤积,粗颗粒因河床冲刷得到补给,大水年补给量高于枯水;(6)九江—大通河段,鄱阳湖入汇和河床补给对细颗粒增加的贡献比例为1∶2.82,河床冲刷对粗颗粒泥沙起补给作用,受大流量持续天数和量值影响.     

三峡水库蓄水运用以来长江中下游沙量平衡分析

以三峡工程为核心的梯级水库群联合调度运用显著改变水沙条件,坝下游河段出现长时间、长距离的冲淤调整,长江中下游沙量平衡分析是合理评估水库群修建对河道影响的重要依据,是河湖管理与保护的关键支撑.本文基于长时间序列原型观测资料,采用沙量平衡法分析长江中下游不同时空尺度泥沙沿程恢复特征,对比断面地形法计算结果,结合河道空间区域性特征,从临底悬沙测验误差、断面代表性及断面间距、河道采砂等多角度深入揭示两种方法计算冲淤量产生差异的主要原因.结果表明:(1)2003-2018年宜昌至大通河段冲刷泥沙10.76亿t,其中粒径d<0.125 mm的泥沙冲刷量占比达90.9%.以螺山为界,宜昌至螺山段"粗细均冲",螺山至大通河段则"细冲粗淤";(2)宜昌至大通河段2003-2018年沙量平衡法与断面地形法计算冲淤量相对偏差为71%,从沿程差异分布来看,距离三峡大坝坝址较近的宜昌至沙市河段两方法计算绝对差值较小,而沙市至大通河段差值较大,占宜昌至大通全河段绝对偏差的近86%;(3)宜昌至沙市河段河道采砂量占实测河床冲刷量的比例约为20%,临底悬沙对输沙量的改正比例为13.2%~26.7%(平均约为20%),修正后,沙量平衡法、断面地形法计算结果吻合相对较好;沙市至大通河段泥沙测验、固定断面布设、河道采砂等是导致沙量平衡法与断面地形法出现差异的主要原因.     

三峡工程运用后长江中游河床调整沿程变化特点

三峡工程运行后,坝下游河道发生持续冲刷。本文研究了长江中游(955 km)不同河段沿程演变差异及其原因。总体而言,河床形态调整幅度自上而下减弱,这是因为在河床持续冲刷过程中,水流含沙量沿程恢复,故越往下游冲刷相对缓慢。平面形态方面,长江中游岸线崩退及洲滩变形的强度均呈沿程减弱趋势,且在荆江河段最为显著。断面形态方面,河床冲深幅度在宜枝下段>荆江河段>宜枝上段>城汉河段>汉湖河段。理论上距离三峡工程最近的河段冲刷应最为剧烈,但由于宜枝上段床沙粗化显著,限制了冲刷的进一步发展。过流能力方面,宜枝河段由于距洞庭湖较远,并未受到入汇顶托作用,故其平滩流量的调整基本由进口水沙条件控制,并随着河床冲深下切而增大;对于荆江、城汉和汉湖河段,河床冲刷虽显著,但支流或湖泊的入汇顶托对平滩流量产生的影响大于前者,故平滩流量总体随上下游水位差同步波动。     

金沙江下游梯级水库泥沙淤积和坝下河道冲刷规律

金沙江下游4个梯级水电站总装机容量相当于两座三峡水库,是“西电东送”中部地区的源头工程,工程效益发挥对经济社会发展意义重大。2012年以来,向家坝、溪洛渡、乌东德和白鹤滩电站等陆续蓄水运行,层层拦截金沙江的泥沙,2013—2020年向家坝出库年输沙量均值下降至152万t,减幅超过99%。大量泥沙淤积在梯级水库内,同时向家坝以下河道发生长距离冲刷。本文以自金沙江下游工程筹建以来的观测资料为基础,针对梯级水库的泥沙淤积和坝下游河道冲刷规律开展研究,结果表明:金沙江下游四个梯级电站自建成运行至2020年底,累计淤积泥沙约5.98亿m³,其中溪洛渡库区淤积量占比达92.5%,2013-2020年溪洛渡和向家坝水库排沙比分别为2.64%和22.2%,其水库泥沙主要淤积在常年回水区的干流河道内,以死库容内淤积为主,侵占有效库容的比例小于1.3%。金沙江下游库区干流河道的峡谷特征明显,淤积多表现为主河槽的平铺式淤高。溪洛渡和向家坝库区淤积的泥沙沿程分选特征明显,越靠近坝前,中数粒径减小、细颗粒泥沙沙量百分数增加,极细颗粒泥沙会在库区一定范围内大量沉积。向家坝下游河床普遍冲刷,但...     

三峡工程下游宜昌至沙市河段河床冲刷预测

在已建水库下游河床冲刷泥沙数学模型的基础上针对宜昌－沙市河段的河道特性，修改并建立了能够反映该河段水沙运动特性的一维水流泥沙数学模型，在此基础上，进行了三峡建库后，前２０年内宜昌－沙市河段的一维水沙运动及河床冲淤计算。     

三峡水库运用后荆江段非均匀悬沙恢复特性

三峡工程运用后,坝下游荆江段来沙量大幅度减小,处于严重的不平衡输沙状态,次饱和水流冲刷河床使悬沙量沿程恢复.基于实测水沙资料,分析了三峡工程运用后荆江段非均匀悬沙恢复特点.提出了恢复效率的概念用以表征悬移质沿程恢复的程度,并根据实测水沙资料计算了荆江段1994-2017年非均匀悬沙的恢复效率.结果表明：三峡工程运用前,荆江段各粒径组悬沙恢复效率绝对值均接近0,故该时期内各粒径组泥沙冲淤幅度不大;三峡工程运用后,各粒径组悬沙恢复效率绝对值均明显增大,且粗沙（d>0.125 mm）恢复效率绝对值远大于细沙（d<0.125 mm）,故粗沙恢复程度更高.这主要是由于荆江段床沙组成中粗沙部分含量大,而细沙含量小.最后建立了三峡水库蓄水后非均匀悬沙恢复效率与来水来沙条件（来沙系数）的关系,结果表明：各粒径组悬移质恢复效率均与来沙系数呈正相关关系,全沙、细沙和中沙的决定系数（R²）分别为0.89、0.67和0.69,相关性较高,故荆江段各粒径组悬移质泥沙恢复效率较大程度上受到来水来沙条件的影响.     

三峡工程运用后长江中下游河道冲刷特征及其影响

三峡及其上游干支流梯级水库建成运用后,大坝下游“清水下泄”引起了长江中下游河道发生长时间、长距离的冲刷。2001—2021年期间宜昌至长江口已累计冲刷了50.3亿m³,需厘清河道冲刷对河势、防洪、航运等方面产生影响。分析表明:三峡工程运用后,长江中下游河势总体稳定,弯道段出现切滩撇弯、汊道段出现塞支强干等现象;河道槽蓄量的持续增加,进一步增大了河道调蓄和行洪能力,但水流顶冲点的变化和近岸河床的冲刷下切,使得河道崩岸频发,并影响河势稳定和防洪安全;在河道冲刷、河势控制与航道工程综合作用下,长江中下游航道条件总体得到改善,但河道不均衡冲刷使得坝下游砂卵石河段出现“坡陡流急”,沙质河段出现洲滩散乱、航槽移位等现象,影响航道条件;同流量下枯水位呈下降态势,逢极枯年份影响长江中下游用水安全;江湖关系发生新变化,“三口”分流道由原淤积转为冲刷,两湖湖区水位不同程度的降低,枯水位出现时间有所提前,不利于湖区水资源和生态环境的安全与可持续发展;三峡工程实施枯水期补水调度和“压咸潮”调度以及长江口北支淤积减缓,对于遏制长江口咸潮入侵有利,入海泥沙显著减少引起长江口近岸河床冲刷,影响...     

三峡工程运行前后的长江中游河段冲淤变化(1975-2017年)

气候变化和流域人类活动等综合影响改变了河道演变的自然进程,尤其是流域大型水库的影响,深刻改变了下游的水沙通量与河道演变过程及趋势.以三峡工程为对象,研究坝下游水沙通量及河道演变过程对三峡工程运行的响应关系,可加深大型水利枢纽运行对下游河道演变影响的认识.本文以长江中游河段（宜昌-湖口河段）为研究对象,分析1975-2017年河道冲淤变化,结果表明：近40年来,长江中游河床已发生了累积性的冲刷,近坝段砂卵石河段冲刷强度先增强后减弱,沙质河段冲刷强度呈增强态势.三峡工程运行后不同河型演变特征归纳为：分汊河段江心洲以冲刷为主,上荆江河段内实施的航道整治工程稳定了江心洲形态,但面积受清水下泄的影响呈减小态势,枯水期主汊分流比呈减小态势,部分汊道发生了主支汊交替变化;下荆江及下游分汊河段江心洲面积虽然交替变化,整体上航道整治工程控制了江心洲规模;弯曲河段凸岸侧边滩以冲刷为主,急弯段的凹岸侧深槽淤积,微弯段凸岸边滩冲刷,对应的凹岸侧深槽相对稳定.     

长江中游沙质河段床沙级配调整过程计算

三峡工程运用后,长江中游荆江河段持续冲刷,床沙与推移质、悬移质泥沙不断交换,从而造成该河段床沙发生不同程度的调整,对长江中下游河床演变及非平衡输沙机理的研究具有重要影响.在新水沙条件下,总结分析了沙波运动特性及床沙交换方式,引入Markov三态转移概率及非均匀沙隐暴系数,得到基于状态转移概率的沙质河段床沙级配调整的计算模型.研究结果表明:(1)20092014年,沙市站年内床沙中值粒径有先增大后减小的趋势,而监利站年内床沙中值粒径则先减小后增大,且荆江河段年际床沙中值粒径总体呈上升趋势,粗化程度约为6.9%~9.3%;(2)20092014年,沙市站床沙组成中粒径d<0.062 mm的泥沙所占比重不变,0.062 mm≤d<0.25 mm的泥沙所占比重逐年减少(累计减少11.4%),d≥0.25 mm的泥沙所占比重逐年增加(累计增加11.4%),而监利站床沙组成均存在波动性变化;(3)荆江河段床沙转换为推移质的概率随着泥沙粒径的增大而增大,床沙转换为悬移质的概率随着泥沙粒径的增大而减小,而推移质和悬移质转换为床沙的概率均随着泥沙粒径的增大而增大,河床发生冲刷粗化时泥沙输移的主要形式为悬移质(概率为81%~87%),而淤积细化时床沙补给主要来源于推移质(概率为8%~12%).通过验证,本文概率模型的计算结果与实测资料符合较好,能够应用于长江中游沙质河段年际床沙粗化及年内床沙级配调整过程预报,为进一步开展三峡工程下游非均匀悬移质泥沙沿程恢复机理的研究提供理论基础.     

三峡工程运行后荆江河段分汇段航道水深资源及碍航驱动机制

系统解析长江中游河湖交汇区域航道水深资源的变化,可支撑“黄金航道”的可持续发展。本研究以洞庭湖-荆江交汇段为对象,研究洞庭湖分汇区域水沙条件、荆江河段滩槽演变与河湖交汇段航道水深资源的关系。研究表明:三峡工程运行以来,洞庭湖三口分流量和分沙量延续了三峡工程运行前的减少态势,伴随洞庭湖分流量减少,相对增加的长江干流径流量增强了河床冲刷强度,反馈使得洞庭湖三口分流量和分沙量均处于较低值;荆江河段河床冲刷给航道尺度提升奠定了有利基础,河湖分汇区域不满足4.5 m×200 m(水深×宽度)的长度为12.6 km,占荆江河段碍航总长度的68.35%。碍航驱动机制上:松滋口分流区段(枝城-昌门溪)的4.5 m水槽贯通但宽度不足200 m,汊道分流关系不稳定及洲滩萎缩制约航道条件稳定,枯水位下降及“坡陡流急”现象仍然严峻,不利于航道条件保障及船舶安全航行;太平口分流区段水位下降、洲滩萎缩、汊道交替发展使得枯水航路不稳定或水深不足4.5 m;藕池口分流区域的洲滩崩退、洲滩冲刷引起的向下游泥沙输移,碍航表现为航宽不足200 m或出现水深不足4.5 m的浅滩;洞庭湖入汇影响区段(熊家洲-城陵矶)受弯道冲淤...     

Contribution to the knowledge of the magmatic evolution by the study of the variation of the coefficient of viscosity

The determination of the coefficient of viscosity of eruptive products gives useful elements to the knowledge of possible variations of composition and physical conditions of the magmas.     

琼中地震台重力仪记录同震响应特征分析

2013年2月6-8日圣克鲁斯群岛发生6次强震,琼中地震台的重力仪记录都有同震响应出现。本文从重力仪记录的面波的延迟时间、最大变形幅度、同震持续时间3个方面研究了6次强震的同震响应特征。     

On the Mechanism of the Secular Tidal Acceleration of the Solid Inner Core and the Viscosity of the Liquid Core

As is known, the secular deceleration of the Earth's diurnal rotation is explained mainly by the tidal friction in the ocean. Below we consider this mechanism in some detail, taking into account also elastic deformations of the mantle under the action of ocean loading and the interaction between the tide-generating body, ocean tidal wave, liquid outer core, and solid inner core. It is shown that elastic displacements of the core-mantle boundary under the action of ocean loading are of about the same amplitude and phase as the elastic loading displacements of the Earth's outer surface. As a result, side by side with the mechanism of secular deceleration of diurnal rotation of the mantle, there are also (1) the opposite mechanism of secular acceleration of diurnal rotation of the outer liquid core and of the solid inner core and (2) the mechanism of excitation of differential rotation in the liquid core. Taking these effects into account, we compare theoretical and modern observed data on the eastward drift of the solid inner core. It is shown that the best agreement may be obtained if the turbulent viscosity of the liquid core is about 2 × 10 ³ Poise     

Evolution of the Source of the Active Region of the Sun

Geomagnetism and Aeronomy - The magnetic evolution of the active region of the Sun at the level of the photosphere has been studied. Magnetic synoptic maps of the 2007 Kitt Peak Observatory were...     

Comparison Between the Nutations of the Planet Mars and the Nutations of the Earth

The nutations of the planets Mars andEarth are investigated and compared. Alarge number of interior structureparameters are involved in the nutationcomputations. The comparison between the observations and the computationsprovides several constraints on these parmeters andtherefore allows a better understanding of the physics of the interior of theplanet. For the Earth, the high precision of the observations of the nutationshas led to a very good determination of interior properties of the planet. ForMars, observations of nutations are not yet available, and we review how theamplitude of the Martian nutations depends on the hypotheses consideredfor its interior. Although Mars is very similar to the Earth, its interior is not well known;for example, we don't knowif its core is liquid or solid. Only if the core is liquid,the Free Core Nutation (FCN) normal mode exists and can alter the nutationswhich are close to the resonance. From the observed geoids, it is known thatboth planets are not in hydrostatic equilibrium. The departure is larger forMars than for the Earth, and consequently, the implication of considering a convective mantle instead of a mantle in hydrostatic equilibrium described byClairaut's equation for the initial equilibrium state of the planet is largeron the Martian nutations than on the Earth nutations. The consequences of theuncertainty in the core dimensions are also examined and shown to be of a veryhigh influence for Mars if the core is liquid, due to the potential changes inthe FCN resonance. The influence of the presence of an inner core, which isknown to exist for the Earth, could be more important for Mars than for theEarth if the inner core is large. Due to the presence of Tharsis on Mars, thetriaxiality of this planet has, additionally, larger effects than on Earth.     

Pictorial Series of the Manifestations of the Dynamics of the Earth

Studia Geophysica et Geodaetica -     

动水压力对深水桥墩地震响应影响的研究综述

地震激励下处于深水中的桥墩和周围水体的相互作用将对桥梁结构的动力响应产生较大影响。首先对地震作用下水-桥墩的相互作用理论做了概括,给出了动水压力对桥墩的作用效应及各自的适用范围;对主要的三种考虑流固耦合效应的分析方法做了对比,探讨了地震作用下影响水-结构相互作用的主要因素,并对今后的研究提出了建议。     

Magnetic stratigraphy of the Ordovician in the lower reach of the Kotuy River: the age of the Bysy-Yuryakh stratum and the rate of geomagnetic reversals on the eve of the superchron

Until recently, the existing data prevented the geophysicists from accurately dating the Bysy-Yuryakh stratum, which outcrops in the middle reach of the Kotuy River, constraining the time of its formation to a wide interval from the end of the Late Cambrian to the beginning of the Silurian. The obtained paleomagnetic data unambiguously correlate the Bysy-Yuryakh stratum to the Nyaian regional stage and constrain its formation, at least a considerable part of it, by the Tremadocian. This result perfectly agrees with the data on the Bysy-Yuryakh conodonts studied in this work and yields a spectacular example of the successful application of paleomagnetic studies in solving important tasks of stratigraphy and, correspondingly, petroleum geology. Within the Bysy-Yuryakh stratum, we revealed a large normal-polarity interval corresponding to the long (>1 Ma) period when the geomagnetic reversals were absent. This result, in combination with the data for the Tremadocian and Middle–Upper Cambrian sequences of the other regions, indicates that (1) the rate of occurrence of the geomagnetic reversals on the eve of the Ordovician Moyero superchron of reversed polarity was at most one reversal per Ma; (2) the superchron does not switch on instantaneously but is preceded by a certain gradual change in the operation conditions of the dynamo mechanism which, inter alia, manifests itself by the reduction of the frequency of geomagnetic reversals with the approach of the superchron. This finding supports the views according to which a process preparing the establishment of the superchrons takes place at the core–mantle boundary.     

The effect of the pollution of the ground layer of the atmosphere on the albedo

Summary A simple model is proposed suitable for studying the effect of the ground layer of the atmosphere, polluted by aerosol, on the albedo. This model is founded on solving the equation of transfer of radiative energy. The numerical results are discussed, particular attention being paid to the analysis of errors due to neglecting the multiple reflection of solar radiation on the aerosol particles. A method which would also include the multiple reflection is proposed, and the conditions under which the presence of the aerosol is responsible for an increase or decrease of the solar radiation balance on the Earth's surface, are analysed.