Experimental study on the influence of vegetation on the slope flow concentration time     

Peng  Qinge  Liu  Xingnian  Huang  Er  Yang  Kejun 《Natural Hazards》2019,98(2):751-763

Due to the steep slope of mountainous watersheds and large changes in vegetation coverage degree, flood response processes after rainstorms are complicated. The flow concentration time of the slope is a key parameter for the simulation of flood processes. The most widely used flow concentration time formula currently in the distributed hydrological model is T?=?L^0.6n^0.6i^?0.4S^?0.3, which is derived from the kinematic wave theory (Melesse and Graham in J Am Water Resour As 40(4):863–879, 2004; Lee in Hydrol Sci 53(2):323–337, 2008). The flow confluence time T is characterized by the constant exponent of the slope length L, roughness n, effective rainfall intensity i and slope S, and the influence of vegetation on the flow concentration time is implied by the roughness. In this study, a series of heavy rainfall slope surface confluence tests under different slopes and vegetation coverage were carried out, a vegetation coverage factor, C, which was introduced, a statistical analysis method was used, and the vegetation coverage index was fitted. The results showed that the types of vegetation have a certain influence on the flow concentration time of slope, and the flow confluence time under turf vegetation was larger than the flow confluence time under shrubs vegetation; especially in the slope of the larger slope, the relative impact is more significant; at the same time, the influence of vegetation coverage on the flow concentration time of slope was more significant; no matter the condition of turf or shrub, the slope confluence time increased obviously with the increase in vegetation coverage. The index of vegetation coverage factor C varied with the slope and rain intensity. In general, the index of vegetation coverage factor C increased with the decrease in slope and decreased with the increase in rain intensity. In regard to the turf vegetation coverage index, when the slope is 45° and 30°, the decreasing trend of the vegetation coverage index a₀ is obvious with increasing rainfall intensity. When the slope is 15°, the vegetation coverage index a₀ also decreases with increasing rainfall intensity. When the slope is 5°, the vegetation coverage index a₀ basically has no change. In regard to the shrubs vegetation coverage index, when the slope is 45° and 30°, the decreasing trend of the vegetation coverage index a₀ is obvious with increasing rainfall intensity. When the slope is 15°, the vegetation coverage index a₀ also decreases with increasing rainfall intensity. When the slope is 5°, the vegetation coverage index a₀ basically has no change.

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Assessment of excavatability,abrasivity and slope stability in a sandstone quarry in Istanbul,Turkey     

Selman Er  Murat Yilmaz  Altay Ertin  Atiye Tugrul  Nuray Tokgöz 《Journal of the Geological Society of India》2017,89(5):581-588

The Cebeci region is characterized by outcrops of Carboniferous sandstone, including diabase dykes. This region is very important area for aggregate production in Istanbul, Turkey. The aim of this study is to determine the engineering geological properties of sandstones to assess the excavatability, abrasivity and stability of cut slopes in a quarry site. Firstly, the sandstone samples were used to determine their petrographical and mineralogical characteristics. Then, physico-mechanical tests were performed on these samples. In order to determine rock mass properties, scan-line surveys were performed, and the major orientations of discontinuities were analyzed through the stereographic projection technique. Kinematical analyses were also made to determine the potential failures at the quarry site. According to the results obtained, excavatability is changed from easy ripping to hard ripping on sandstones; the carbonated sandstone is less abrasive than other sandstones. Based on the field studies and stability analyses of the cut slopes, optimum slope geometry and necessary support measures, such as wire mesh and rock fall barriers, are suggested.  相似文献   

Identifying sediment sources from the inter-gully area and gully area in a small watershed in the Loess Hilly Region of China     

Mian Li  Er Yang  Ping Li  Zhenzhou Shen  Hongzhe Bao  Yongxin Ni 《Environmental Earth Sciences》2017,76(22):776

Understanding the sediment source is very significant for erosion control in small watersheds. On the Loess Plateau of China, over 110 thousands of check dams were constructed in the past 60 years, which played an important role in controlling soil loss and also kept much information of erosion and sediment yield in the past. The objective of this investigation is to identify the sediment source by the ¹³⁷Cs tracing method in a small watershed in the Loess Hilly Region of China. Fifty-five sampling sites were selected from the watershed (44 from the inter-gully area, 7 from the gully sides and 4 from the reference sites), and a total of 114 soil samples were collected from three sediment profile cores at the Sidizui watershed check dam constructed in 1959. Based on the erosion rate from the inter-gully area by the ¹³⁷Cs models, and the total erosion amount deposited in the check dam since 1963, the relative contributions of sediment from the inter-gully area and gully area were estimated during 1963–2013. By comparing the difference of ¹³⁷Cs activities of surface soils from the check dam (deposited in the 2011–2013 flood events), the inter-gully and gully areas, the relative contributions of sediment derived from the two source areas to the flood sediment during recent years (2011–2013) were estimated by a simple mixing model. Results showed that the erosion rate from the inter-gully area was about 3054 t/km² a during 1963–2013, and the relative contributions of sediment from the inter-gully area and gully area were estimated to be 27 and 73%, respectively. The sediment from the inter-gully area was about 20% of the total sediment yield amount to the 2011–2013 floods, and from the gully area it was about 80%. The relative contribution of sediment from the inter-gully or gully area was not a fixed value in the watershed. Both of the inter-gully erosion and gully erosion should be simultaneously controlled, and more erosion control measures on the gully area should be taken in the subsequent watershed management in order to reduce the erosion amount in this region.  相似文献   

Analysis of runoff in ungauged mountain watersheds in Sichuan, China using kinematic-wave-based GIUH model     

Shuyou Cao  Kwan Tun Lee  Juiyi Ho  Xingnian Liu  Er Huang  Kejun Yang 《山地科学学报》2010,7(2):157-166

Floods are one of the most common natural hazards occurring all around the world. However, the knowledge of the origins of a food and its possible magnitude in a given region remains unclear yet. This lack of understanding is particularly acute in mountainous regions with large degrees in Sichuan Province, China, where runoff is seldom measured. The nature of streamflow in a region is related to the time and spatial distribution of rainfall quantity and watershed geomorphology. The geomorphologic characteristics are the channel network and surrounding landscape which transform the rainfall input into an output hydrograph at the outlet of the watershed. With the given geomorphologic properties of the watershed, theoretically the hydrological response function can be determined hydraulically without using any recorded data of past rainfall or runoff events. In this study, a kinematic-wave-based geomorphologic instantaneous unit hydrograph (KW-GIUH) model was adopted and verified to estimate runoff in ungauged areas. Two mountain watersheds, the Yingjing River watershed and Tianquan River watershed in Sichuan were selected as study sites. The geomorphologic factors of the two watersheds were obtained by using a digital elevation model (DEM) based on the topographic database obtained from the Shuttle Radar Topography Mission of US’s NASA. The tests of the model on the two watersheds were performed both at gauged and ungauged sites. Comparison between the simulated and observed hydrographs for a number of rainstorms at the gauged sites indicated the potential of the KW-GIUH model as a useful tool for runoff analysis in these regions. Moreover, to simulate possible concentrated rainstorms that could result in serious flooding in these areas, synthetic rainfall hyetographs were adopted as input to the KW-GIUH model to obtain the flow hydrographs at two ungauged sites for different return period conditions. Hydroeconomic analysis can be performed in the future to select the optimum design return period for determining the flood control work.  相似文献   

春季生殖真鲷仔、稚、幼鱼的摄食与生长   总被引：7，自引：0，他引：7  

张雅芝  陈而兴 《海洋科学》1998,22(3):57-62

１９９６年５￣６月份在本院海水育苗试验场对人工培养的春季生殖真鲷仔、稚、幼鱼的摄食和生长特性进行分析,旨在为该种群早期发育阶段的生物学积累资料,并为开展大批量苗种生产提供依据。结果表明,在水温在２３℃时,仔鱼约经５５￣６０ｈ左右开口摄食,开口饵料为小型臂尾轮虫。以后随着鱼体的生长（〉１０ｍｍ）,摄食桡足类的比例迅速增加。对２８５尾仔、稚、幼鱼观察,在实验条件下,其摄食率达１００％。摄食量约占体重的  相似文献   

Rossby波和热带对流活动对2010年6月梅雨发生前后我国东部两次强降水过程的影响          下载免费PDF全文

李慧  陆尔  翟盘茂  李肇新  陈阳  甘如玉 《大气科学学报》2019,42(6):824-834

基于574台站的逐日降水资料及NCEP/NCAR逐日再分析资料,在比较2010年梅雨期前后(6月7—11日和18—22日)我国东部两次强降水过程的大尺度环流型差异的基础上,从Rossby波活动通量及热带对流活动探讨了这两次强降水过程的异同。结果表明,相同之处在于:两次强降水过程期间中高纬度地区都存在Rossby波向下游传播,中纬度地区呈现双阻型式,低纬度地区西太平洋副热带高压(以下简称西太副高)强度偏强、西伸脊点位置偏西。不同之处在于:1)第一次降水过程中Rossby波的波源位于北欧地区附近,贝加尔湖地区为低槽,使得冷空气南下到36°N左右;同时孟加拉湾活跃的对流系统使西太副高加强西伸到95°E左右,冷暖空气交汇,导致强降水发生;2)第二次降水过程中Rossby波的波源位于北欧地区和中西伯利亚地区附近,东亚地区的低槽较第一次过程明显加深,有利于冷空气到达长江中下游地区(30°N左右),西太平洋暖池地区活跃的对流系统使得西太副高加强西伸到90°E左右,冷暖空气在长江中下游及其以南地区交汇,导致强降水发生。  相似文献   

On-line Tools for Solar Data Compiled at the Debrecen Observatory and Their Extensions with the Greenwich Sunspot Data     

T. Baranyi  L. Győri  A. Ludmány 《Solar physics》2016,291(9-10):3081-3102

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Gamma rays from colliding winds of massive stars     

Anita Reimer  Olaf Reimer  Martin Pohl 《Astrophysics and Space Science》2007,309(1-4):351-357

Colliding winds of massive binaries have long been considered as potential sites of non-thermal high-energy photon production. This is motivated by the detection of non-thermal spectra in the radio band, as well as by correlation studies of yet unidentified EGRET γ-ray sources with source populations appearing in star formation regions. This work re-considers the basic radiative processes and its properties that lead to high energy photon production in long-period massive star systems. We show that Klein–Nishina effects as well as the anisotropic nature of the inverse Compton scattering, the dominating leptonic emission process, likely yield spectral and variability signatures in the γ-ray domain at or above the sensitivity of current or upcoming gamma ray instruments like GLAST-LAT. In addition to all relevant radiative losses, we include propagation (such as convection in the stellar wind) as well as photon absorption effects, which a priori can not be neglected. The calculations are applied to WR 140 and WR 147, and predictions for their detectability in the γ-ray regime are provided. Physically similar specimen of their kind like WR 146, WR 137, WR 138, WR 112 and WR 125 may be regarded as candidate sources at GeV energies for near-future γ-ray experiments. Finally, we discuss several aspects relevant for eventually identifying this source class as a γ-ray emitting population. Thereby we utilize our findings on the expected radiative behavior of typical colliding wind binaries in the γ-ray regime as well as its expected spatial distribution on the γ-ray sky.  相似文献   

Diagnostics of solar ions: Ne VI,Mg VI,Si VIII and Mg VIII observed by SERTS     

B. N. Dwivedi  Anita Mohan 《Solar physics》1995,156(1):81-94

Diagnostics of solar ions Nevi, Mgvi, Siviii, and Mgviii in an active region observed by SERTS have been presented. Density, temperature, and electron pressure in the emitting source have been derived from theoretical line-ratio curves and its EUV spectrum obtained by SERTS. The variation of neon-to-magnesium and silicon-to-magnesium abundances has been discussed in the interpretation of the active region spectrum obtained by SERTS.  相似文献   

Visible and near-infrared spectrophotometry of the Deep Impact ejecta of Comet 9P/Tempel 1     

Klaus W. Hodapp  Greg Aldering  Anita L. Cochran  Emmanuel Pécontal  Nathalie Blanc  David K. Lynch  S. Mazuk  Richard C. Puetter 《Icarus》2007,187(1):185-198

We have obtained optical spectrophotometry of the evolution of Comet 9P/Tempel 1 after the impact of the Deep Impact probe, using the Supernova Integral Field Spectrograph (SNIFS) at the UH 2.2-m telescope, as well as simultaneous optical and infrared spectra using the Lick Visible-to-Near-Infrared Imaging Spectrograph (VNIRIS). The spatial distribution and temporal evolution of the “violet band” CN (0-0) emission and of the 630 nm [OI] emission was studied. We found that CN emission centered on the nucleus increased in the 2 h after impact, but that this CN emission was delayed compared to the light curve of dust-scattered sunlight. The CN emission also expanded faster than the cloud of scattering dust. The emission of [OI] at 630 nm rose similarly to the scattered light, but then remained nearly constant for several hours after impact. On the day following the impact, both CN and [OI] emission concentrated on the comet nucleus had returned nearly to pre-impact levels. We have also searched for differences in the scattering properties of the dust ejected by the impact compared to the dust released under normal conditions. Compared to the pre-impact state of the comet, we find evidence that the color of the comet was slightly bluer during the post-impact rise in brightness. Long after the impact, in the following nights, the comet colors returned to their pre-impact values. This can be explained by postulating a change to a smaller particle size distribution in the ejecta cloud, in agreement with the findings from mid-infrared observations, or by postulating a large fraction of clean ice particles, or by a combination of these two.  相似文献