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   

马尔科夫链分析在东海陆架盆地花港组沉积微相分析中的应用     

胡求红  张昌民  侯国伟  朱锐  陈哲 《地质与资源》2020,29(1):7-20

通过对东海陆架盆地某凹陷取心井岩心仔细观察和描述，采用双属性划分标准，在研究区花港组岩心中识别出了28种岩石相类型.其中砾岩相5种，砂岩相15种，细粒岩相8种.针对22口取心井岩心详细划分沉积微相和岩石相，共取得2227个岩石相数据.针对研究区发育的湖泊、三角洲、河流3种沉积体系，运用马尔科夫链分析不同沉积微相类型中岩石相沉积序列模式，建立了不同沉积微相类型可能的岩石相组合规律及岩石相定量组合概率，为后期研究相同或相似类型的沉积相提供地质知识库，并为沉积相的识别提供定量的基础.  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   

Mantle transition zone structure beneath the Central Asian Orogenic Belt     

Jing HE  Qingju WU 《中国科学:地球科学(英文版)》2020,63(4):548-560

Over the past decades, there have been hot debates in the geodynamic community regarding to the deep evolution mechanisms of Cenozoic volcanism in the Central Asian Orogenic Belt(CAOB). Of all the constraints available, high resolution structure of upper mantle discontinuities, especially the discontinuities at depths of 410 km(D410) and 660 km(D660), is of the most important, which may provide reliable clues on the magma channel as well as its evolution. In this work, we adopt the common conversion point stacking technique with teleseismic radial P-wave receiver functions to examine the D410 and D660 discontinuities. The primary results exhibit that the major characteristics of the mantle transition zone(MTZ) obtained by different velocity models are largely consistent. Obviously elevated D410 and slightly depressed D660 are observed beneath the Hannuoba Volcano, suggesting possible delamination of the local lithosphere deposited at the D410. This process may induce upwelling of the asthenospheric materials filling the space left by the delaminated lithosphere, and subsequently trigger volcanic eruptions. Strong depressions are observed at both D410 and D660 depths beneath west of the Dariganga Volcano, and the depression of D660 is more pronounced. It leads to the apparently thickened MTZ, indicating the presence of cold material at the D660. This cold material is speculated as a stagnant slab from the subducted Pacific Plate or the remains of a detached island arc system from the collision and formation of the CAOB. Slightly thinner MTZ is found beneath the Hentey Mountains and the Middle Gobi Volcano. Apparently, this thinner MTZ is not significant enough to support the existence of high thermal anomalies,which may rule out the possibility of large-scale hot material upwelling from either the local MTZ or even the lower mantle.  相似文献   

2018年斐济M_W8.2深震:高频辐射过程和发生原因          下载免费PDF全文

张喆  许力生  杜海林 《地球物理学报》2019,62(11):4279-4289

2018年8月19日，在斐济东部海域563 km深处发生了一次M_W8.2地震.我们首先挑选位于美国阿拉斯加地区的131个宽频带台站构成台阵，选用垂直分量0.5~2 Hz的高频信号，利用广义台阵反投影技术对这次地震的破裂过程进行了成像，然后基于破裂速度对地震的辐射效率进行了估计.结果表明，这次地震总体上呈单侧破裂，破裂方位在3.0°左右，破裂总长度约51 km，持续时间22 s，平均破裂速度为2.5 km·s^-1.但能量释放有2次高峰，形成两次子事件.第一次为前10 s，峰值在7 s左右，破裂速度为2.9 km·s^-1，辐射效率为45%.第二次为10~22 s，峰值在15 s左右，破裂速度为1.6 km·s^-1，辐射效率为26%.结合震源位置、震源机制、破裂速度以及辐射效率，我们认为这次地震是由于俯冲板块前缘受到下部地幔物质上浮阻力引起的剪切失稳所致，起初板块内部的脆性破裂表现突出，致使辐射效率较高，后来震源处高温高压下的熔融耗散特征逐渐凸现，致使辐射效率下降.  相似文献   

四川地区震后应急会商资料快速产出系统的设计与实现     

祁玉萍  汪小厉  林圣杰  肖本夫  何畅  廖晓峰 《震灾防御技术》2020,15(1):176-183

地震预报意见以大量资料为基础，依靠专家经验和多学科知识并通过会商讨论形成。显著地震发生后，快速、准确、有效地研判震情可为后期应急指挥和地震现场工作奠定基础。本文以Datist软件为平台，基于四川及邻区的基础资料，设计研发符合四川震情的震后会商资料快速产出系统，当四川及邻区发生中强地震时，通过该系统可在收到地震短信5分钟内以请求触发的方式快速产出应急会商资料，并以微信、PowerPoint和Word的形式将基础资料发送给分析预报人员，为后期趋势分析奠定基础。  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   

城镇增长下的收缩：以武汉为例     

高喆  尹宁玮  童馨仪  李东欣  顾江 《热带地理》2019,39(1):29-36

首先从人口、经济、用地3个维度综合考察武汉市增长与收缩的全貌，并采用县区及街道2个尺度的数据定量描述了武汉市增长与收缩的特征与空间格局，发现武汉市下辖青山区、硚口区、汉阳区和蔡甸区存在局部较严重的收缩现象，空间上形成集聚，形态上呈“穿孔式”。进一步以青山区为案例，着重从资本视角探讨发生局部收缩的内在机制，发现其存在老龄化、少子化趋势，但局部收缩的主因是资本从产业部门的“逃逸”。  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   

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