Exploring the stemflow dynamics and driving factors at both inter- and intra-event scales in a typical subtropical deciduous forest     

Haixia Zhang  Congsheng Fu  Aimin Liao  Can Zhang  Jiufu Liu  Niu Wang  Bin He 《水文研究》2021,35(3):e14091

Numerous efforts have been made to understand stemflow dynamics under different types of vegetation at the inter-event scale, but few studies have explored the stemflow characteristics and corresponding influencing factors at the intra-event scale. An in-depth investigation of the inter- and intra-event dynamics of stemflow is important for understanding the ecohydrological processes in forest ecosystems. In this study, stemflow volume (F_V), stemflow funnelling ratio (F_R), and stemflow ratio (F_%) from Quercus acutissima and Broussonetia papyrifera trees were measured at both inter- and intra-event scales in a subtropical deciduous forest, and the driving factors, including tree species and meteorological factors were further explored. Specifically, the F_V, F_R and F_% of Q. acutissima (52.3 L, 47.2, 9.6%) were lower than those of B. papyrifera (85.1 L, 91.2, 12.4%). The effect of tree species on F_V and F_% was more obvious under low intensity rainfall types. At the inter-event scale, F_V had a strong positive linear correlation with rainfall amount (G_P) and event duration (D_E) for both tree species, whereas F_R and F_% had a positive logarithmic correlation with G_P and D_E only under high-intensity, short-duration rainfall type. F_R and F_% were mainly affected by wind speed and the maximum 30-min rainfall intensity under low-intensity, long-duration rainfall type. At the intra-event scale, for both tree species, the mean lag time between the start of rainfall and stemflow was the shortest under high-intensity, short-duration rainfall type, while the mean duration and amount of stemflow after rain cessation were the greatest under high-amount, long-duration rainfall type. The relationship between stemflow intensity and rainfall intensity at the 5-min interval scale also depended greatly on rainfall type. These findings can help clarify stemflow dynamics and driving factors at both inter- and intra-event scales, and also provide abundant data and parameters for ecohydrological simulations in subtropical forests.  相似文献   

Near-surface soil stabilization by enzyme-induced carbonate precipitation for fugitive dust suppression     

Song  Jun Young  Sim  Youngjong  Jang  Jaewon  Hong  Won-Taek  Yun  Tae Sup 《Acta Geotechnica》2020,15(7):1967-1980

Acta Geotechnica - To resolve the environmental and sustainability issues from fugitive dust emission and conventional mitigation methods, multiple experiments were conducted to evaluate the...  相似文献   

赣南狮吼山硫铁多金属矿区花岗岩地球化学、年代学特征及其成因     

贺根文  路思明  彭琳琳  于长琦  李伟  刘翠辉 《吉林大学学报(地球科学版)》2020,50(5):1491-1504

狮吼山矿区是江西省内规模最大的矽卡岩型硫铁多金属矿床，伴生W、Cu、Au多种成矿元素，成矿作用与矿区出露的茶山迳复式花岗岩体有关。岩体主要包括茶山迳似斑状黑云母二长花岗岩和莲湖细粒二长花岗岩两期，为研究成矿岩体的侵位时代、岩石成因及与成矿的关系，本次工作进行了U-Pb锆石定年、岩相学和岩石地球化学等测试分析。结果表明：岩体具有高硅、高钾、富铝的特征，属高钾钙碱性系列花岗岩；轻重稀土元素分馏明显，均为右倾型，弱Eu负异常，以富集Cs、Rb、Th、U、Pb，亏损Ba、Nb、Sr、和Ti等元素为主要特征，属于低Ba-Sr壳源花岗岩类；锆石具较好晶形，具典型岩浆锆石特征，利用LA-ICP-MS进行U-Pb测年，获得谐和年龄为（162.4±0.6）Ma（MSWD=1.8），加权平均年龄为（162.4±1.4）Ma（MSWD=1.4），谐和年龄与加权平均年龄在误差范围内高度一致，表明茶山迳复式岩体侵位于燕山早期中侏罗世；综合考虑岩体矿物组合、主微量元素及高分异特征，认为其成因分类应属于S型花岗岩；对比中国花岗岩成矿元素平均含量，茶山迳两期花岗岩均具有较高的W、Mo、Bi、Pb等成矿元素含量，可同时为成矿作用提供热源、流体及物质。  相似文献   

基于三维生态足迹的可持续发展实证研究——以重庆市为例     

张晓雨  周宝同  明弘 《中国岩溶》2020,39(5):705-713

文章借鉴Niccolucci的三维生态足迹模型，通过计算“国家公顷”，更新均衡因子和产量因子，添加污染物账户，改进传统生态足迹模型，并利用改进模型分析重庆市2008-2017年生态足迹的历时性。在此基础上，构建可持续发展能力综合指数，以研究重庆市可持续发展能力的动态变化。结果表明:（1）存流量指数除2008年、2012年、2013年及2014年之外，其他年份均小于1，说明重庆市存量资本的消耗有所下降；（2）生态资源利用效率指数整体呈逐年降低状态，重庆市资源利用效率逐年提高；（3）生态多样性指数整体呈阶梯式上升，重庆市生态系统的稳定性增强；（4）可持续发展能力综合指数总体上升了13.85%，重庆市可持续发展能力总体增强；（5）生态压力指数介于1.51～2.00之间，生态环境尚处在很不安全状态，存量资本依然在被占用，重庆市尚处于非可持续发展状态，且2017年可持续发展能力综合指数出现小幅度下跌，故应牢固树立绿色发展理念，及时采取措施警惕其继续下滑。   相似文献   

历史遗址类旅游地的生命周期研究——以美国14家历史遗址公园为例     

杨小露  张红  张春晖 《地理科学进展》2019,38(6):918-929

实证研究中旅游地生命周期理论的运用潜力备受质疑。论文选取美国14家国家历史遗址公园为例,采用旅游研究中较少使用的四参数Logistic模型结合一次函数、二次函数、三次函数、高斯多峰分析法拟合旅游地的生命周期。研究发现：四参数Logistic模型结合一次函数、二次函数、三次函数能较好地拟合旅游地的生命周期;利用四参数Logistic曲线的上弯点、拐点、下弯点能定量的划分出旅游地的起步探索、发展、巩固、停滞阶段,一次函数、二次函数、三次函数能拟合旅游地的衰退或复兴阶段,这回答了学者们对生命周期阶段难以定量划分的质疑。根据旅游地停滞期之后的发展趋势还能归纳出该类旅游地的生命周期类型;高斯多峰分析法将旅游地的生命周期拟合成一个个波动的高斯峰,更大程度上保留了旅游地演进的波动特征;将高斯多峰分析法与四参数Logistic模型结合起来,不仅能定量划分旅游地的生命周期阶段,还能准确地描述在生命周期阶段内的波动情况,甚至分析各生命周期阶段对整个生命周期的影响和作用。  相似文献   

基于空间插值的浙江省城市流时空演变特征研究          下载免费PDF全文

魏国恩  贺清云  朱翔  欧阳晓 《干旱区地理》2019,42(1):215--222

为了探寻发达省份内城市间相互作用的时空特征，该文以浙江省为样本单元，选取2005、2010年和2015年3个时间截面，采用反距离权重法和空间插值手段，从城市流强度视角展开了实证分析。结果表明：（1） 城市间的联系在不断加强，期间城市流强度值随时间的推移而整体得到提升，空间上由初始的“中心点”通过发展扩散向“中心域”转变，中心城市的辐射带动作用开始发挥成效。（2）结构上呈现出相对稳定的北高南低的分布格局，以杭州市为龙头，宁波为副核心，温州、绍兴、舟山为重要节点的多中心城市网络结构雏形初步形成。（3） 城市流强度的空间分异特征分析明显，但分异程度有了些许的改善，侧面说明空间上由初始的“中心点”通过发展扩散向“中心域”转变的基本观点。最后就浙江省如何加强省内城市间“流”的规模性、区域协调性和可持续性展开了讨论。  相似文献   

东海盆地西湖凹陷天台区始新世平湖组风暴岩的发现及其地质意义     

何玉平 《吉林大学学报(地球科学版)》2020,50(2):500-508

风暴岩对于古地理和古环境具有良好的指相意义。东海盆地西湖凹陷天台区始新世平湖组发育典型的风暴岩。通过详细的岩心观察，发育的风暴沉积标志主要有冲刷-充填构造、风暴撕扯构造和丘状-洼状交错层理构造等。根据风暴岩垂向上的组合特征及沉积构造差异，识别出了近源和远源两种风暴沉积类型，分别指示了不同的沉积背景：近源风暴岩表现为不完整的风暴岩垂向沉积序列，呈风暴砾屑层段（A）+泥岩段（E）叠加，为潮坪潮下带沉积；远源风暴岩具完整和不完整的风暴岩垂向沉积序列，以粒序段（B）+平行层理段（C）+丘状（洼状）层理段（D）叠加为特征，属浅海陆棚沉积。风暴层序自下而上沉积环境为浅海陆棚→潮坪，风暴岩的分布差异表明形成环境向上变浅的沉积特征。该发现为本区古环境的演变提供了重要依据。  相似文献   

宁德市东部海域浮游动物群落及其与水环境因子的关系   总被引：1，自引：0，他引：1       下载免费PDF全文

程宏  徐炳旭  刘溢馨  马祖友  石志洲 《海洋开发与管理》2019,36(8):18-23

浮游动物在海洋生态系统中发挥重要作用,也是海洋食物链的主要环节。为科学保护和评价海洋生态环境和渔业资源,文章基于2016年春、秋季宁德市东部海域的相关调查结果,采用多样性指数、丰富度指数、均匀度指数和优势度指数以及去趋势对应分析法和冗余分析法,分析浮游动物群落及其与温度、pH值、溶解氧、无机氮、无机磷和化学需氧量6个水环境因子的关系。研究结果表明:春、秋季调查共鉴定浮游动物12类67种,季节和站位差异不大,均以水母类、桡足类和浮游幼虫为主;共出现优势种18种,春、秋季分别以桡足类和水母类为主,相同优势种仅有2种;3种指数分布无明显季节差异,但秋季指数总体较高;春、秋季浮游动物种类分别与各水环境因子呈正相关或负相关关系,其中温度是影响浮游动物种类的最主要水环境因子。  相似文献   

The galaxy luminosity function in the LAMOST Complete Spectroscopic Survey of Pointing Area at the Southern Galactic Cap     

Pin-Song Zhao  Hong Wu  Cong Kevin Xu  Ming Yang  Fan Yang  Yi-Nan Zhu  Man I Lam  Jun-Jie Jin  Hai-Long Yuan  Hao-Tong Zhang  Shi-Yin Shen  Jian-Rong Shi  A-Li Luo  Xue-Bing Wu  Yong-Heng Zhao  Yi-Peng Jing 《天文和天体物理学研究(英文版)》2019,(8)

We present optical luminosity functions(LFs) of galaxies in the~(0.1) g,~(0.1) r,~(0.1) i bands, calculated using data in~40 deg~2 sky area of the LAMOST Complete Spectroscopic Survey of Pointing Area(LaCoSSPAr) in the Southern Galactic Cap. Redshifts for galaxies brighter than r = 18.1 were obtained mainly with LAMOST. In each band, LFs derived using both parametric and non-parametric maximum likelihood methods agree well with each other. In the0.1 r band, our fitting parameters of the Schechter function are φ_*=(1.65 ± 0.36) × 10~(-2) h~3 Mpc~(-3), M_*=-20.69 ± 0.06 mag and α =-1.12 ± 0.08,which agree with previous studies. Separate LFs are also derived for emission line galaxies and absorption line galaxies. The LFs of absorption line galaxies show a dip at~(0.1) r ~18.5 and can be fitted well by a double-Gaussian function, suggesting a bimodality in passive galaxies.  相似文献   

New photometric investigation of the low-mass-ratio contact binary star V1853 Orionis     

Jia-Jia He  Sheng-Bang Qian  Boonrucksar Soonthornthum  Amornrat Aungwerojwit  Niang-Ping Liu  Thawicharat Sarotsakulchai 《天文和天体物理学研究(英文版)》2019,(4)

Four-color charge-coupled device(CCD) light curves in the B, V, Rc and I c bands of the totaleclipsing binary system V1853 Orionis(V1853 Ori) are presented. By comparing our light curves with those published by previous investigators, it is determined that the O'Connell effect on the light curves has disappeared. By analyzing those multi-color light curves with the Wilson-Devinney code(W-D code),it is discovered that V1853 Ori is an A-type intermediate-contact binary with a degree of contact factor of f = 33.3%(3.7%) and a mass ratio of q = 0.1896(0.0013). Combining our 10 newly determined times of light minima together with others published in the literature, the period changes of the system are investigated. We found that the general trend of the observed minus calculated(O-C) curve shows a downward parabolic variation that corresponds to a long-term decrease in the orbital period with a rate of d P/dt =-1.96(0.46)×10~(-7) d yr~(-1). The long-term period decrease could be explained by mass transfer from the more-massive component to the less-massive one. By combining our photometric solutions with data from Gaia DR_2, absolute parameters were derived as M_1 = 1.20 M⊙, M_2 = 0.23 M⊙, R_1 = 1.36 R⊙and R_2 = 0.66 R⊙. The long-term period decrease and intermediate-contact configuration suggest that V1853 Ori will evolve into a high fill-out overcontact binary.  相似文献