Heat flow and crustal thermal structure in the Late Archaean Closepet Granite batholith,south India

The Late Archaean Closepet Granite batholith in south India is exposed at different crustal levels grading from greenschist facies in the north through amphibolite and granulite facies in the south along a ∼400 km long segment in the Dharwar craton. Two areas, Pavagada and Magadi, located in the Main Mass of the batholith, best represent the granitoid of the greenschist and amphibolite facies crustal levels respectively. Heat flow estimates of 38 mW m⁻² from Pavagada and 25 mW m⁻² from Magadi have been obtained through measurements in deep (430 and 445 m) and carefully sited boreholes. Measurements made in four boreholes of opportunity in Pavagada area yield a mean heat flow of 39 ± 4 (s.d.) mW m⁻², which is in good agreement with the estimate from deep borehole. The study, therefore, demonstrates a clear-cut heat flow variation concomitant with the crustal levels exposed in the two areas. The mean heat production estimates for the greenschist facies and amphibolite facies layers constituting the Main Mass of the batholith are 2.9 and 1.8 μW m⁻³, respectively. The enhanced heat flow in the Pavagada area is consistent with the occurrence of a radioelement-enriched 2-km-thick greenschist facies layer granitoid overlying the granitoid of the amphibolite facies layer which is twice as thick as represented in the Magadi area. The crustal heat production models indicate similar mantle heat flow estimates in the range 12–14 mW m⁻², consistent with the other parts of the greenstone-granite-gneiss terrain of the Dharwar craton.     

西藏天摩沟泥石流形成机制与成灾特征

西藏林芝市波密县天摩沟于2007年9月、2010年7月、2010年9月和2018年7月分别发生大型和巨型泥石流,4次泥石流活动均不同程度堵塞主河帕隆藏布,淤埋国道318或摧毁桥梁,堰塞湖淹没村道、溃决造成下游塌岸,给当地居民生命财产尤其是交通干道造成极大危害。文章针对以上4次泥石流活动,采用高分辨率遥感影像,对泥石流发生前的孕灾背景进行解译,同时结合无人机航空摄影和地面调查对天摩沟泥石流形成机制和成灾特征进行了对比分析,得到以下结论:(1)天摩沟内冰川发育,年际变化大,目前泥石流形成的主要方式为岩崩和堵溃,其中2018年和2007年为岩崩引发,2010年为堵溃引发,该沟同时具有冰川泥石流和降雨泥石流的特征。(2)经历了2007年和2010年3次大规模泥石流后,天摩沟内斜坡类物源储量增加了19.6%,绝大部分启动的冰碛物和崩滑物源都转化为泥石流沟道堆积物或冲出沟口。(3)天摩沟2018年泥石流容重为2.10g/cm^3,为黏性泥石流,流速快冲击力强,帕隆藏布河道受到挤压多次变道,历史上最大偏移距离为190m。(4)2018年7月11日泥石流成因为降雨条件下加剧冰川消融引发主沟沟源右侧岩崩,形成多阵次泥石流,主泥石流体积18×104m3,淤埋G318近220m。后续依然具有暴发大型泥石流的可能性,建议进行防治降低其危害程度。     

环抱式防波堤口门航道横流三维特性研究

环抱式防波堤口门易出现较大横流,且三维特性明显。针对连云港主港区深水航道,建立三维潮流数学模型,并用现场航槽实测资料进行验证,在此基础上计算分析了不同潮差条件下口门段进港航道横流的三维特性。研究结果表明:最大横流约出现在高潮位前1.5 h,自表层至底层相继出现,且表、底层出现时刻仅相差0.5 h;因航道边坡较小,最大横流时未见水流分离现象,航槽底部没有反向流;各层最大横流值均与涨潮潮差有关,且相关程度高;航道内最大横流垂向分布梯度随潮差增加略有增大。     

喀喇昆仑山西北部冰川运动速度地形控制特征

为了探讨地形和海拔对冰川季节和年平均运动速度的影响程度,利用2013-2018年GoLive数据与ASTER GDEM V2数据对喀喇昆仑山西北部3 389条冰川的地形（坡度、坡向、海拔）和冰川运动速度进行了综合分析。结果表明：冰川表面运动速度在物质平衡线处（3 970~4 770 m）达到最快,是冰川积极维持物质平衡的一种体现。坡度平缓地区在不同海拔下的冰川运动速度有明显的差别,但是不同坡度地区的冰川运动速度随海拔变化的趋势基本一致,均呈现先增大后减小。北坡冰川运动速度较平稳,南坡和西南坡的冰川运动速度（均为0.25 m·d^-1）最快并且变化幅度较大,最小值与最大值相差近4倍。冰川运动速度不是呈现单一的季节性变化,同时还会受到地形的控制。低海拔区域冰川运动速度在消融期（3-6月）较快,中海拔区域在消融前（11月至次年2月）较快。     

基于航空客流的中国城市层级结构分析

基于1995、2000和2003三个年份的航空客运统计数据,分析中国城际航空客流的结构,并以优势流(dominant flow)方法为主,辅以距离平方和聚类法,分析中国主要城市在国内客运航空网络中的层级及其变化。研究表明,通过航空客运方式产生的空间联系主要集中于东部地区,中部地区在航空网络的重要性方面落后于西部,北京、上海、广-深3个顶点组成全国航空网络的主干;从主导航空客流角度观察,自1995至2003年,一个高度集中的城市层级在3个全国性中心的控制下形成和发展,航空客运网络层级体系中的顶层结构业已清晰,而以下各层次的结构尚处于分化发展之中。     

Influences of coupled wind–water processes on suspended sediment grain size: an example from tributaries of the Yellow River / Influences de processus couplés éoliens-hydriques sur la granulométrie des matières en suspension: exemple d'affluents du Fleuve Jaune

Abstract

Some unique coupled wind–water erosion processes exist in the desert-loess transitional zone in the middle Yellow River basin. Based on data from 40 stations on 29 rivers, a study was made on the influence of such processes on suspended sediment grain-size characteristics of the tributaries of the Yellow River. Results show that the percentage of >0.05-mm grain size decreases with the increased annual mean precipitation, but increases with the increase in the annual mean number of sand-dust storm days. The percentage of <0.01-mm grain size increases with the increase in the annual mean precipitation, but decreases with the increase in the annual number of sand-dust storm days. Based on annual mean data from 40 stations, multiple regression equations were established between the percentages of >0.05-mm grain size (r _>0.05) and <0.01-mm grain size (r _<0.01), annual mean precipitation (P _m) and annual mean number of sand-dust storm days (D _ss). On this basis, the relative contributions of the variations in D _ss and P _m to the variation in r _>0.05 and r _<0.01 were estimated. The results indicate that the variation in sand-dust storm frequency exerts greater influences on the variation in grain-size characteristics of suspended load than does the variation in annual mean precipitation. With the increase in the coupled wind–water processes index, expressed by P _m/D _ss, the percentage of >0.05-mm grain size in suspended sediment decreases and the percentage of <0.01-mm grain size increases. With the variation in P _m/D _ss, different combinations of r _>0.05 with r _<0.01 appear, which have some influence on the formation of hyperconcentrated flows. There exist some optimal ratios of coarse to fine fractions in suspended sediment that make sediment concentrations of hyperconcentrated flows the highest. The optimal r _>0.05/r _<0.01 value is related to some range of the index P _m/D _ss. When the P _m/D _ss index falls in this range, the optimum combination of relative coarse with fine sediments in the suspended load appears, and thus results in the peak values of sediment concentration.     

变动流域滞时方程

流域滞时是流域汇流计算和预报中的一个重要因素。本文尝试将流域滞时表示成流域重心长度Lca(流域重心到流域出口断面的河道长度)与汇流速度v之比的函数,从而使流域滞时随汇流速度的不同而不同,而不再是一个常数。长度Lca反映了流域尺度和几何形态对滞时的影响,而汇流速度则反映流域动力条件对滞时的作用。5个小流域的实测资料检验表明结果较为满意。     

A Numerical Model for Natural Backfill of Pipeline Trenches Subjected to Unidirectional／Oscillatory Flows

A numerical model for the self-burial of a pipeline trench is developed. Morphological evolutions of a pipeline trench under steady-current or oscillatory-flow conditions are simulated with/without a pipeline inside the trench. The oscillatory flow in this study represents the action of waves. The two-dimensional Reynolds-averaged continuity and Navier-Stokes equations with the standard k-e turbulence closure, as well as the sediment transport equations, are solved with the finite difference method in a eurvilirrear coordinate system. Both bed and suspended loads of sediment transport are included in the morphological model. Because of the lack of experimental data on the backfilling of pipeline trenches, the numericalmodel is firstly verified against three closely-relevant experiments available in literature. A detailed measurement of the channel migration phenomenon under steady currents is employed for the assessment of the integral performance of themodel. The two experimental results from U-tube tests are used to validate the model‘s ability in predicting oscillatory flows. Different time-marching schemes are employed for the morphological computation under unidirectional and oscillatory conditions. It is found that vortex motions within the trench play an important role in the trench development.     

Physical sedimentology experiments with sulfuric acid solutions: Implications for Mars?

Physical sedimentology experiments have shown that sulfuric acid solutions may have formed some surface features seen on Mars. Recent data returned from Mars show the presence of jarosite, sulfate salts, hematite, phyllosilicates, and opaline silica, all of which precipitate from some terrestrial sulfuric acid solutions. There is a plethora of geochemical, mineralogical, and sedimentological data indicative of past sulfuric acid systems on Mars, but there has never been a comprehensive study published regarding sulfuric acid as a physical sedimentological agent. In the laboratory, we ran liquids of various compositions over sediments in order to test how these liquids entrain, transport, and deposit sediments. Pure water and concentrated sulfuric acid solutions produced the same general features, such as channels, gullies, and alluvial fans. However, sulfuric acid solutions yielded some distinct sedimentary features not produced by pure water runs. These features, narrow, deeply incised channels of consistent widths, rounded discrete fans, and air bubble “craters”, are similar to some Martian landscape features. These experimental results indicate that acid solutions should be considered a possible sedimentological agent on Mars.     

南海北部冬季和夏季逆风流机制初探Ⅱ.季风逆风流产生机制

分析讨论了季风风应力、大陆坡地形及底摩擦在产生季风逆风流的必要条件和间接逆风流诊断判据中的作用；应用季风逆风流必要条件和间接逆风流诊断判据，解释冬季风和夏季风逆风流是如何产生的。结果表明：季风风应力是产生季风逆风流的主导因素；冬季风风应力、大陆坡地形及底摩擦三者联合作用导致表层海水在大陆坡上产生辐合生成高水位带和高动力高度带，在大陆被北侧产生NE向的冬季逆风流，南侧产生SW向顺风流；夏季风风应力、大陆坡地形及底摩擦三者联合作用导致表层海水在大陆坡上产生辐散生成低水位带和低动力高度带，在大陆被北侧产生SW向的夏季逆风流，南侧产生NE向的顺风流；冬季风盛行期间，风致经巴士海峡流入南海的黑潮水，将加速冬季逆风流的形成，加大冬季逆风流的强度；夏季风盛行期间，风应力的作用使巴上海峡以东的黑潮水不能进入南海，即使别的原因令巴上海峡以东的黑潮水流入南海，但高温、高盐的黑潮水对夏季逆风流具有阻扼作用。