Sediment deposition and overland flow hydraulics in simulated vegetative filter strips under varying vegetation covers

Vegetative filter strips (VFSs) can effectively trap sediment in overland flow, but little information is available on its performance in controlling high‐concentration sediment and the runoff hydraulics in VFS. Flume experiments were conducted to investigate the sediment deposition, hydraulics of overland flow and their relationships in simulating VFS under a great range of sediment concentrations with four levels of vegetation cover (bare slope and 4%, 11% and 17%) and two flow rates (15 and 30 L min^?1). Sediment concentrations varied from 30 to 400 kg m^?3 and slope gradient was 9°. Both the deposited sediment load and deposition efficiency in VFS increased as the vegetation cover increased. Sediment concentration had a positive effect on the deposited load but no effect on deposition efficiency. A lower flow rate corresponded to greater deposition efficiency but had little effect on deposited load. Flow velocities decreased as vegetation cover increased. Sediment concentration had a negative effect on the mean velocity but no effect on surface velocity. Hydraulic resistance increased as the vegetation cover and sediment concentration increased. Sediment deposition efficiency had a much more pronounced relationship with overland flow hydraulics compared with deposited load, especially with the mean flow velocity, and there was a power relationship between them. Flow regime also affected the sediment deposition efficiency, and the efficiency was much higher under subcritical than supercritical flow. The results will be useful for the design of VFS and the control of sediment flowing into rivers in areas with serious soil erosion. Copyright © 2015 John Wiley & Sons, Ltd.     

Shiyang River streamflow since AD 1765, reconstructed by tree rings,contains far‐reaching hydro‐climatic signals over and beyond the mid‐latitude Asian continent

In this study, the regional tree‐ring chronology of Picea crassifolia was used to estimate annual (September to August) streamflow of the Shiyang River for the period from AD 1765 to 2010. The linear regression model was stable and could explain 41.5% of the variance for the calibration period of 1955–2005. According to the streamflow reconstruction, dry periods with below average streamflow occurred in AD 1775–1804, 1814–1823, 1831–1856, 1862–1867, 1877–1885, 1905–1910, 1926–1932, 1948–1951, 1960–1963 and 1989–2002. Periods of relatively wet years are identified for AD 1765–1774, 1805–1813, 1824–1830, 1857–1861, 1868–1876, 1886–1904, 1911–1925, 1933–1947, 1952–1959, 1964–1988 and 2003–2010. Comparisons with the precipitation reconstructions from surrounding areas supplied a high degree of confidence in our reconstruction. Our reconstructed streamflow is significantly correlated with sea surface temperature in the eastern equatorial Pacific Ocean and the North Atlantic Ocean. The Multitaper spectral and correlation analyses also suggested that the reconstructed streamflow variation in the Shiyang River could be associated with large‐scale atmospheric‐oceanic variability, such as El Niño‐Southern Oscillation (ENSO). The linkages among the streamflow reconstruction, NAO and ENSO suggest the connection of regional streamflow variations to the Asian monsoon and westerlies circulations. Copyright © 2016 John Wiley & Sons, Ltd.     

京津渤地区的水资源及开发利用中的环境问題

作者初步估算了京津渤地区的水资源,全区水资源总量多年平均为129.67亿立方米,可供水资源为87.13亿立方米.进而讨论水资源开发利用中的几个环境问题:供需矛盾突出、旱涝频繁、地面沉降和水源污染.并就如何合理利用水资源和保护水资源问题提出了建议.     

The dynamo theory of plasma turbulence wave in rotating celestial bodies

The various modes of plasma turbulence waves (including MHD waves) are easily excited under cosmic circumstances. In this paper, if we consider that the celestial bodies rotate, there is a source term generated for the magnetic induced equation by the excited plasma turbulence waves. If we expand the turbulent field in the Fourier series and include rotation velocity, the dynamo equation for turbulent waves is obtained. We have also obtained the solutions of various wave forms corresponding to different rotation velocities and then we significantly discuss the magnetic fields in the Sun, planets, and other celestial bodies.     

Spatial distribution and luminosity function of OH/IR maser sources

In this paper, we study the galactic distribution and luminosity function of OH/IR maser sources. All the selected OH/IR sources have optical or infrared identification. Most of them are associated with late-type (>M5) Mira variables. Their derived density distribution shows a steep peak at a galactocentric distance of r₀-7.5 kpc and decreases rapidly at smaller and larger R₀. The FWHM of the distribution curve is 2.1 kpc. This is similar to the galactic distribution of Mira variables investigated by Glass et al.

We also derive the luminosity function of the identified OH/IR maser sources from their distances, their detection probabilities, and their corrected OH radio peak flux densities. The luminosity function ρ(L) varies as L_OH^−1.79. This is similar to that of unidentified maser sources. The range of luminosity of identified OH/IR sources is approximately from 0.16 Jy · kpc² to 1000 Jy · kpc². It is quite different from that of unidentified OH sources.

Finally, we discuss some differences and relations between identified and unidentified OH/IR maser sources.     

泌阳断陷东南缘深断裂特征及其与油藏分布关系研究

泌阳断陷断块圈闭、滚动背斜及其与砾岩体复合圈闭油藏的形成，与断陷东南缘由多条断层组成的具下道上正呈断阶状的深断裂带的演化有关。本文首先研究了泌阳断陷区域构造背景，对典型地震测线的原始采集资料进行了处理和解释。在此基础上，对断陷东南缘深断裂特征及其与油藏分布关系进行了研究。     

四川盆地油气地质研究

四川盆地是地台内通过深断裂活动而形成的构造—沉积盆地。这些深断裂卷入了上地幔或壳内低速层。深部构造作用控制盖层内的断褶构造发育。川东南高陡背斜带的形成和隐伏的深断裂活动有成因联系。海相致密的碳酸盐岩内气藏的形成和分布,主要受断褶构造发育程度及储层内后生孔洞缝发育程度的控制。低缓的及隐伏的构造圈闭以及后生孔洞缝系统是天然气聚集的场所。川东南及川西区已知的气藏基本上是分布这类的圈闭中。龙门山前隐伏的古逆冲断褶带伴生的构造及裂缝圈闭是重要的油气聚带。近年来的钻探证实了这一预测的正确性。     

SPOT地面场定标与星上定标结果的比较分析

本文研究是在遥感辐射定标场选择的基础。利用６Ｓ大气辐射传输模型进行ＳＰＯＴ遥感数据的定标和地物的光谱反射率反演,即在遥感器飞越辐射定标场上空,在定标场选择若干像元区,测量遥感器对应的各波段地物的光谱反射率和大气光谱参量,并利用大气辐射传输模型给出遥感器人瞳处各光谱带的辐射亮度,最后确定它与遥感器对应输出的数字量化的数量关系,求解定标系数。然后,对相应的研究训练区的遥感数据进行大气辐射校正,进而反演训练区内的地物光谱反射率。最后,通过将反演值与实地测量的地物光谱反射率进行对比分析,来估算定标不确定度,并比较说明两种不同方式定标差异及优势和限制。     

X-CT机空间分辨率测试规范的探讨

空间分辨率有四种测试方法：分辨成排圆孔模型测极限分辨率;分辨成排条形模型测极限分辨率;扫描针模计算ＭＴＦ曲线;扫描条形模型计算ＭＴＦ曲线。前二种方法直观、简单,但模体重、体积大,且测量结果有一定主观因素,这两种方法用于日常质量控制为宜。第三种方法能得到完整的ＭＴＦ曲线,但计算过程复杂,本文推荐使用最后一种方法,并简述其原理,认为该方法测量ＭＴＦ曲线简便易行。