Thresholds for post-wildfire debris flows: Insights from the Pinal Fire,Arizona, USA     

Carissa A. Raymond  Luke A. McGuire  Ann M. Youberg  Dennis M. Staley  Jason W. Kean 《地球表面变化过程与地形》2020,45(6):1349-1360

Wildfire significantly alters the hydrologic properties of a burned area, leading to increases in overland flow, erosion, and the potential for runoff-generated debris flows. The initiation of debris flows in recently burned areas is well characterized by rainfall intensity-duration (ID) thresholds. However, there is currently a paucity of data quantifying the rainfall intensities required to trigger post-wildfire debris flows, which limits our understanding of how and why rainfall ID thresholds vary in different climatic and geologic settings. In this study, we monitored debris-flow activity following the Pinal Fire in central Arizona, which differs from both a climatic and hydrogeomorphic perspective from other regions in the western United States where ID thresholds for post-wildfire debris flows are well established, namely the Transverse Ranges of southern California. Since the peak rainfall intensity within a rainstorm may exceed the rainfall intensity required to trigger a debris flow, the development of robust rainfall ID thresholds requires knowledge of the timing of debris flows within rainstorms. Existing post-wildfire debris-flow studies in Arizona only constrain the peak rainfall intensity within debris-flow-producing storms, which may far exceed the intensity that actually triggered the observed debris flow. In this study, we used pressure transducers within five burned drainage basins to constrain the timing of debris flows within rainstorms. Rainfall ID thresholds derived here from triggering rainfall intensities are, on average, 22 mm h⁻¹ lower than ID thresholds derived under the assumption that the triggering intensity is equal to the maximum rainfall intensity recorded during a rainstorm. We then use a hydrologic model to demonstrate that the magnitude of the 15-min rainfall ID threshold at the Pinal Fire site is associated with the rainfall intensity required to exceed a recently proposed dimensionless discharge threshold for debris-flow initiation. Model results further suggest that previously observed differences in regional ID thresholds between Arizona and the San Gabriel Mountains of southern California may be attributed, in large part, to differences in the hydraulic properties of burned soils. © 2019 John Wiley & Sons, Ltd.  相似文献   

顾及基准站坐标动态特性与稳定性的区域框架构建     

蒋光伟  王斌  王延伟  李康  孙洋洋 《地球物理学进展》2020,(1):8-15

基准站受构造运动与非线性因素的影响,如何构建高精度、现势性强的精细区域框架是位置服务与形变分析的的关键.笔者提出顾及基准站坐标动态特性与稳定性的区域框架构建方法.以我国西部与东部某城市的多年连续运行基准站数据为例进行试算比对,试验结果表明:该方法是可行的,较好地顾及了基准站的坐标特性与非线性影响,考虑了基准站的垂直运动规律,可构建高精度的区域基准,可发现区域基准的微动态变化.  相似文献   

黄海透光层悬浮半导体矿物组成及其促进微生物胞外电子传递过程初探     

刘佳  孙元  任桂平  鲁安怀  李艳  丁竑瑞 《岩石矿物学杂志》2020,39(1):96-104

在地球上最为活跃的海洋透光层体系中,矿物-微生物交互作用的形式十分丰富。系统采集了黄海近海透光层水体样品,测试分析发现其中分布大量悬浮半导体矿物及微生物群落。通过电感耦合等离子质谱仪(ICP-MS)、环境扫描电子显微镜(ESEM)及配有的EDX能谱仪,从宏观到微区对悬浮颗粒矿物的化学元素组成进行了测试分析,发现其主要矿物组成元素为Si、O、Na、K、Ca、Al等,且含有较高含量的Mn、Fe、Ti等金属元素;通过X射线衍射光谱(XRD)、拉曼光谱(Raman)测试从整体到局部分析悬浮颗粒矿物的物相组成,发现其主要组成矿物为石英、钠长石、方解石、云母和绿泥石等,还有锐钛矿、金红石、板钛矿、针铁矿等铁、钛金属氧化物半导体矿物。通过16S rRNA高通量测序分析海水中主要微生物群落为Proteobacteria、Actinobacteria、Bacteroidetes、Planctomycetes、Woeseia、Fluviicola等,并通过构建双室反应体系对海水微生物与悬浮矿物间氧化还原作用及胞外电子传递过程进行了表征,结果显示增加海水悬浮矿物作为电子受体后,体系开路电压由330. 80 mV提升至426. 59 mV,提升比率达130%,最大输出功率由8. 376 9 mW/m^2提升至12. 096 8 mW/m^2,为原体系的1. 44倍。实验研究表明,海水透光层悬浮矿物能有效参与并促进微生物胞外电子传递过程,为后续深入研究基于电子能量传递利用的半导体矿物-微生物协同作用以及元素循环调控机制奠定初步基础。  相似文献   

辽宁省数字化形变观测自然干扰分析     

姚菲菲  宫长盛  梁永信 《地震地磁观测与研究》2020,41(4):148-156

对数字形变观测过程中辽宁丹东地震台、营口地震台、抚顺地震台、朝阳地震台DSQ水管仪、SS-Y伸缩仪存在的自然干扰现象进行研究，对其机理和数据形态作了对比分析，为快速、准确地判别自然干扰提供了科学依据。  相似文献   

多元素衬值累加地球化学方法在找矿中的应用——以青海省夏日哈-什多龙远景区为例     

赵志飞 《地质与勘探》2020,56(2):328-336

青海省夏日哈-什多龙成矿远景区位于青藏高原东昆仑东段,西起都兰县夏日哈镇,东至兴海县什多龙一带,跨祁漫塔格北坡-夏日哈岩浆弧和北昆仑岩浆弧,是青海省重要的成矿区。为了在该区寻找新的成矿有利地段,本文在对该区区域地质背景、矿产特征及区内典型矿床地质特征系统研究的基础上,利用多元素衬值累加地球化学找矿方法,在区域上优选出一批找矿靶区。多元素衬值累加地球化学找矿方法首先收集远景区1∶5万水系沉积物测量成果,经过数据处理,绘制远景区衬值累计地球化学图,进而建立典型矿床找矿模式,最终通过对比分析,选出新的找矿靶区。对圈定的找矿靶区进行野外踏勘检查,均发现不同程度的矿化线索,为今后在该区进一步找矿起到了很好的指导作用。通过本次工作,发现了该方法在靶区圈定方面的优势:(1)可快速圈定异常,提高工作效率;(2)编制的地球化学图浓集中心更显著;(3)圈定的找矿靶区找矿成果显著,尤其针对陆相火山岩型多金属矿、斑岩型铜钼矿、矽卡岩型多金属矿找矿成果突出;(4)能直观反映背景变化趋势,有助于评价异常。  相似文献   

贵州苗匡热矿水地热区水化学特征及热储条件分析     

杨晓飞 《地质与勘探》2020,56(1):94-101

贵州苗匡热矿水地热区大地构造位于江南复合造山黔南坳陷铜仁复式褶皱变形带,区域构造为红石古断裂带与苗匡断裂交汇锐角区,区内出露的地层有前南华系板溪群、南华系、震旦系、寒武系;热矿水水化学类型为HCO_3-Na型,含高氟、锶、锂、偏硅酸;弱碱性水;呈带状中低温热储;区域大地热流供给热量;地下热矿水补给为构造破碎带深远程补给;区域性红石活动断裂带具有导热导水储水性,热矿水被温差、压力差等驱动循环运移至断裂破碎带富集,苗匡次级断裂带在该热储起到连通传导作用;热矿水井口温度45℃,出水量560 m~3/d。研究结果可对该区热矿水勘查开发及利用提供参考和借鉴。  相似文献   

Kainsaz(CO3)陨石中两个富Al球粒的氧同位素组成特征与形成演化     

戴德求  包海梅  刘爽  尹锋 《岩石学报》2020,36(6):1850-1856

富Al球粒是原始球粒陨石中一种矿物岩石学特征介于富钙铝包体(CAIs)和镁铁质硅酸盐球粒之间的特殊集合体,所以常常认为富Al球粒在认识CAIs和镁铁质硅酸盐球粒形成演化过程中的相互联系具有特殊意义。然而,对富Al球粒的初始物质组成以及形成演化过程一直存在较多争议,而氧同位素组成研究能够对球粒演化和早期星云环境等提供重要的信息。在本文中我们报导了来自Kainsaz(1937年降落于俄罗斯,CO3型)碳质球粒陨石中的2个富Al球粒(编号K1-CH1和K2-CH2)的矿物岩石学和氧同位素组成特征。K1-CH1的矿物组成主要为橄榄石、低钙辉石和富钙长石,K2-CH2为橄榄石和富钙长石。2个球粒中的矿物均具有贫~(16)O同位素组成特征。K1-CH1中矿物的△~(17)O组成基本上位于2个区间:-11.1‰～-8.7‰和-3.9‰～0.4‰;而K2-CH2的△~(17)O介于-6.6‰～-0.6‰之间,且具有从中部至边部升高的趋势。矿物岩石学和氧同位素特征表明,这2个富Al球粒的初始物质组成为富CAIs和镁铁质硅酸盐。在球粒熔融结晶过程中,与贫~(16)O同位素组成(△~(17)O:-8.7‰～-7.8‰)的星云发生了氧同位素交换。球粒形成后,发生迁移进入陨石母体,在相对更贫~(16)O同位素组成(△~(17)O:-0.6‰～0.4‰)的母体中(流体参与)发生变质作用,并再次发生了氧同位素交换。  相似文献   

Evaluating new fault-controlled hydrothermal dolomitization models: Insights from the Cambrian Dolomite,Western Canadian Sedimentary Basin     

Ardiansyah Koeshidayatullah  Hilary Corlett  Jack Stacey  Peter K. Swart  Adrian Boyce  Hamish Robertson  Fiona Whitaker  Cathy Hollis 《Sedimentology》2020,67(6):2945-2973

Fault-controlled hydrothermal dolomitization in tectonically complex basins can occur at any depth and from different fluid compositions, including ‘deep-seated’, ‘crustal’ or ‘basinal’ brines. Nevertheless, many studies have failed to identify the actual source of these fluids, resulting in a gap in our knowledge on the likely source of magnesium of hydrothermal dolomitization. With development of new concepts in hydrothermal dolomitization, the study aims in particular to test the hypothesis that dolomitizing fluids were sourced from either seawater, ultramafic carbonation or a mixture between the two by utilizing the Cambrian Mount Whyte Formation as an example. Here, the large-scale dolostone bodies are fabric-destructive with a range of crystal fabrics, including euhedral replacement (RD1) and anhedral replacement (RD2). Since dolomite is cross-cut by low amplitude stylolites, dolomitization is interpreted to have occurred shortly after deposition, at a very shallow depth (<1 km). At this time, there would have been sufficient porosity in the mudstones for extensive dolomitization to occur, and the necessary high heat flows and faulting associated with Cambrian rifting to transfer hot brines into the near surface. While the δ¹⁸O_water and ⁸⁷Sr/⁸⁶Sr ratios values of RD1 are comparable with Cambrian seawater, RD2 shows higher values in both parameters. Therefore, although aspects of the fluid geochemistry are consistent with dolomitization from seawater, very high fluid temperature and salinity could be suggestive of mixing with another, hydrothermal fluid. The very hot temperature, positive Eu anomaly, enriched metal concentrations, and cogenetic relation with quartz could indicate that hot brines were at least partially sourced from ultramafic rocks, potentially as a result of interaction between the underlying Proterozoic serpentinites and CO₂-rich fluids. This study highlights that large-scale hydrothermal dolostone bodies can form at shallow burial depths via mixing during fluid pulses, providing a potential explanation for the mass balance problem often associated with their genesis.  相似文献   

中国东部层积云发展过程中云微物理特征的演变   总被引：1，自引：0，他引：1       下载免费PDF全文

李思聪  李昀英  孙国荣  宋文婷 《地球物理学报》2019,62(12):4513-4526

基于2007—2010年的CloudSat卫星观测数据,以云层液态水路径为指标将层积云的发展过程划分为五个阶段,对比研究了中国东部降水与非降水层积云发展过程中云微物理特征和云微物理机制的演变,并分析了其海陆差异.研究表明:非降水层积云中,云滴增长主要通过凝结过程完成,但云滴的凝结增长有限,难以形成降水,在非降水层积云发展的旺盛阶段,云层中上部云滴发生较弱的碰并过程.降水层积云中云滴碰并增长活跃,当云层液态水路径小于500 g·m~(-2)时,云滴在从云顶下落至云底的过程中持续碰并,并在云底附近出现云水向雨水的转化;当降水层积云液态水路径超过500 g·m~(-2)时,云滴碰并增长主要发生在云层上部,在云层中部,云液态水含量、液态粒子数浓度和液态粒子有效半径达到最大,云水向雨水的转化最为活跃.层积云微物理特征的海陆差异主要是由海陆上空气溶胶浓度和云中上升气流强度不同导致的.在非降水层积云中下部,陆地丰富的气溶胶为云滴凝结增长提供了充足的云凝结核,因而云微物理量的量值在陆地上空更大,而在云层中上部,云滴凝结增长达到极限,海洋充足的水汽输送使云微物理量的量值在海洋上空更大.当降水层积云液态水路径大于500 g·m~(-2)时,陆地层积云中更强的上升气流使大量云滴在云层中上部累积滞留,云滴碰并增长活跃,云层中上部云微物理量的量值在陆地上空更大.  相似文献   

甘肃北山老金厂金矿床载金矿物特征、原位硫同位素组成及其对成矿的指示意义     

黄式庭  于晓飞  吕志成  刘家军  李永胜  杜泽忠  吕鑫  孙海瑞  杜轶伦 《吉林大学学报(地球科学版)》2020,50(5):1387-1403

老金厂金矿床是北山成矿南带最具代表性的中低温岩浆热液型金矿床之一，其规模为中型。依据脉体穿插、矿物共生组合和矿石结构构造等特征，将矿床矿化作用过程划分为石英-黄铁矿阶段（Ⅰ）、石英-含砷黄铁矿-毒砂阶段（Ⅱ）、石英-黄铁矿-多金属硫化物阶段（Ⅲ）和石英-方解石阶段（Ⅳ）。利用电子探针研究了不同成矿阶段载金矿物的元素组成及其分布规律。Ⅰ阶段：黄铁矿以粗粒自形立方体为主，粒度为0.50~1.50 mm，贫As、Au；毒砂含量极少，呈细粒他形。Ⅱ阶段：含砷黄铁矿周围常有大量毒砂产出，含砷黄铁矿多为立方体、五角十二面体，粒度为0.30~1.00 mm，富As、Au；该阶段矿化最为强烈，毒砂主要形成于此时期，多呈棱柱状、柱状、放射状集合体，显示富S亏As特征。Ⅲ阶段：多以黄铁矿-黄铜矿-闪锌矿共生组合脉的形式产出，黄铁矿多呈长条状，以富S、Cu、Zn、Au和贫Fe、As为特征。Ⅳ阶段：矿化作用极弱，毒砂、黄铁矿含量极少，为细粒他形。原位硫同位素组成显示：Ⅰ阶段黄铁矿δ³⁴S_V-CDT值为-3.8‰~-2.9‰，均值为-3.3‰；Ⅱ阶段黄铁矿和毒砂δ³⁴S_V-CDT值为-4.7‰~2.6‰，均值为-3.3‰；Ⅲ阶段黄铁矿和闪锌矿δ³⁴S_V-CDT值主要分布于-1.9‰~1.0‰之间，均值为0.1‰。此3个阶段硫同位素组成反映了成矿期硫主要来源于幔源岩浆，混入了部分地层硫。综合前人研究成果，认为成矿早期至晚期，成矿流体总体上由富S贫As向富As贫S演化。Ⅰ阶段体系处于中性稳定的环境，硫源充足；Ⅱ阶段为贫S富As的高氧逸度环境，由于大气降水对地层的淋滤渗透，混入富As流体，Au可能与As结合形成Au-As络合物，在成矿有利部位富集沉淀；Ⅲ阶段成矿元素种类丰富，体系为富S贫As的弱还原环境，Au很可能与HS^-、S^-形成络合物进入黄铁矿晶格。  相似文献