砂岩单轴压缩试验P波速度层析成像及声发射特性研究     

张光  吴顺川  张诗淮  郭沛 《岩土力学》2023,(2):483-496

深部矿井开采极易诱发矿柱型岩爆,矿柱型岩爆严重威胁着矿山的安全高效开采,为探究矿柱型岩爆破坏机制和前兆信息,选用自贡红砂岩进行单轴压缩试验,并采用主动超声和被动声发射对破裂过程进行监测,联合主动超声与被动声发射监测数据对波速进行层析成像反演,分析试样破裂过程中波速演化规律。研究结果表明：砂岩试样在加载过程中速度模型呈现高度非均质性,在加载过程中会出现低速区,且声发射事件集中出现在低速区内部;P波速度离散度可反映全局波速变化特征,在峰值附近变化剧烈,随荷载增加P波速度离散度持续增大;声发射事件在峰前、峰后定位结果相差较大,峰前阶段声发射事件随机分布,峰后阶段声发射事件定位结果集中。此外,研究发现选用均质速度模型进行声发射事件定位会增大定位误差,试样最终失稳前b值的降低表明试样大尺度裂纹活动加剧,导致岩石非均质性增大,也间接证明了采用非均质速度模型进行声发射震源定位的必要性。该研究结果可用于现场矿柱稳定性监测,定期反演获得矿柱波速变化为矿柱型岩爆提供先兆预警信息。  相似文献   

青藏高原南部及邻区深部碳释放规模与成因     

赵文斌  郭正府  李菊景  马琳  刘嘉麒 《岩石学报》2022,38(5):1541-1556

不同构造背景下的深部碳释放通量与机制研究对于深刻理解长时间尺度的气候变化具有重要意义,以往的相关研究多集中在洋中脊、大洋俯冲带和大陆裂谷等地质单元,缺少对大陆碰撞带深部碳释放规模与机理的关注,从而制约了对大陆碰撞带深部碳循环过程及其气候环境效应的进一步认识。青藏高原起源于印度和欧亚大陆的碰撞,是研究大陆碰撞带深部碳循环的理想地区。为此,在近年来青藏高原温室气体释放野外观测与研究的基础上,本文估算了高原南部及邻区火山-地热区的CO₂释放规模并探讨了其释放模式。气体He-C同位素地球化学与温泉水热活动特征等显示,青藏高原南部及邻区的深部碳释放主要受深部岩浆房、断裂和浅部水热系统等因素的控制。依据深部流体源区和上升运移控制因素的差异,可以将青藏高原南部及邻区的深部碳释放划分为三大类：(1)以壳内水热系统脱碳为主的藏南地区;(2)深大断裂控制的以水热系统脱碳为主的川西地区;(3)深部岩浆房和浅部水热系统共同控制的滇西南地区。青藏高原南部土壤微渗漏CO₂释放通量介于18.7～52.3Mt/yr之间,温泉溶解无机碳释放通量约为0.13Mt/yr;高原邻区...  相似文献   

冻融温变速率对岩石受载特性的影响规律     

刘成禹  郑道哲  张向向  陈成海  曹洋兵 《岩土力学》2022,43(8):2071-2082

以贺兰山岩画、云冈石窟等中常见的硅质胶结砂岩为研究对象,对不同温变速率冻融后岩样进行称重、超声波测试和单轴压缩试验,探究了冻融后岩石物理力学性质随冻融温变速率的变化规律;根据冻融后岩石受载过程中的声发射和微震特征,揭示了温变速率对冻融后岩石内部不同尺度裂纹扩展的影响规律及其内在机制。研究表明：（1）随着温变速率增加,岩样冻融后的微裂纹增多,颗粒间联结强度减弱,峰值强度、弹性模量降低,破坏应变及损伤参量D_e、D_v增大;（2）冻融岩石受载过程中,微裂纹具有“初始压密―扩展孕育―急速扩展”的演化特征,宏观裂纹演化过程可分为“匀速扩展－急速扩展”两个阶段,其中宏观裂纹的急速扩展阶段还呈现出“孕育－扩展－再孕育－再扩展”的波浪式发展特点;温变速率越大,冻融后岩石受载过程中的微裂纹、宏观裂纹扩展越快,且更易于进入急速扩展阶段;当温变速率增大到一定数值后,微裂纹、宏观裂纹从加载开始即以较高速率扩展,直至岩样破坏;（3）微裂纹孕育阶段和加载全过程的声发射振铃相对增长速率,以及宏观裂纹匀速扩展阶段的相对时长、微震振铃相对增长速率均与损伤参量D_e、D_v具有较好的拟合关系,能够反映冻融循环对岩石的初始损伤作用;（4）冻胀力随温变速率增加而增大,导致不同温变速率冻融后岩样的初始损伤不同,这是引起冻融后岩石受载过程中裂纹扩展、声震特性出现显著差异的内在原因。  相似文献   

赣南北部黄陂河流域离子型稀土矿地区水质与健康风险评价   总被引：1，自引：0，他引：1  

刘斯文  黄园英  赵文博  魏吉鑫  徐春丽  马嘉宝  刘久臣  黄采文 《岩矿测试》2022,(3):488-498

水质安全和健康是保障中国赣南老区乡村振兴发展的重要因素。赣南离子型稀土矿长期开发利用,导致浸矿剂和矿体中重金属元素等危害人体健康的物质进入水循环系统,给周边乡村饮用水卫生安全带来了潜在风险。目前,针对当地复垦后稀土矿及周边地区水质和健康风险缺乏系统调查评价,本文以《生活饮用水卫生标准》(GB 5749—2006)为评价依据,选择赣南北部黄陂河流域典型离子型稀土矿及周边的水体开展调查研究,采用电感耦合等离子体发射光谱/质谱等技术测定锰、镉等元素含量,采用水质指数(WQI)、危害商(HQ)、致癌风险(CR)评价了锰和铅等9种指标及其健康风险。结果表明：地表水中的异常指标有氨氮(平均值750μg/L)、锰(平均值207μg/L),地下水中的异常指标有氨氮(平均值4533μg/L)、锰(平均值4009μg/L);世界卫生组织(WHO)公布的Ⅰ类致癌物砷在地表水及地下水均未见异常。WQI显示研究区内85.7%的地表水适宜饮用。地表水及地下水中氨氮的HQ平均值<1,对人类健康没有不良影响;地下水中锰的HQ平均值>1,可能会对人类健康产生不良影响。地表水及地下水中致癌元素砷的CR值分布区...  相似文献   

四川昭觉县中部乡镇表层土壤硒地球化学特征     

赵辰  孙彬彬  贺灵  吴超  成晓梦  曾道明  刘冬 《岩矿测试》2022,(3):412-426

硒元素是人体必需的微量元素之一,食用富硒农产品是人体获取和补充硒元素的主要途径,调查区域硒地球化学特征是有效地利用富硒土地资源以及开发富硒农副产品的重要依据。本文选择四川省昭觉县域内较为重要的农耕乡镇采集表层土壤样品,采用原子荧光光谱法、X射线荧光光谱法、电感耦合等离子体质谱/发射光谱法等方法测定1328件土壤、19件玉米及20件土豆中硒等地球化学指标含量,利用相关分析与统计学等方法,结合距离加权反比插值法,探讨研究区硒含量、分布和影响因素等地球化学特征,评价土壤与作物的富硒情况及安全性。结果表明：(1)研究区表层土壤硒含量范围为0.04～1.50mg/kg,平均值为0.33mg/kg,划定富硒土壤面积为7.23km~2,占全区土壤面积的30.31%,玄武岩发育的土壤硒含量最高,平均值为0.4mg/kg,表明区内地质背景与土壤硒含量密切相关,区内富硒土壤主要受含玄武岩夹苦橄岩、凝灰质砂泥岩的峨眉山玄武岩组地层控制;(2)不同的用地类型和土壤类型对硒元素的富集能力不同,人为农业活动导致土壤对硒的吸附能力下降,黄棕壤土层中黏粒或铁氧化物等易与硒结合富集;酸性土壤中硒含量与pH值成反比;土壤...  相似文献   

煤柱-顶板系统协同作用的脆性失稳与非线性演化机制   总被引：12，自引：2，他引：10  

秦四清  王思敬 《工程地质学报》2005,13(4):437-446

把坚硬顶板视为弹性梁,把煤柱视为应变软化介质并采用W e ibu ll分布描述它的损伤本构模型,本文对坚硬顶板和煤柱组成的力学系统,用突变理论方法研究了它的演化失稳过程。通过对建立的尖点突变模型的分析发现,系统失稳主要取决于系统的刚度比k与材料的均匀性或脆性指标m值,并给出了失稳的充要条件力学判据和失稳突跳量的表达式。考虑煤柱介质的粘性或蠕变性,建立了系统演化的非线性动力学模型物理预报模型,并给出了根据顶板沉降观测数据反演非线性动力学模型的方法和稳定性判别准则。对木城涧矿根据观测序列进行了动力学模型的反演分析,一个重要发现是:D值在临近失稳时陡增出现峰值而后急剧下降。根据材料损伤与声发射累计计数的对应关系,建立了系统演化过程中声发射率的动力学模型,并进行了声发射模拟分析和分维分析,发现m值与系统的演化路径对系统演化的声发射活动规律及分维特征有重要影响,单纯根据声发射监测和降维现象预报冲击地压是不可靠的。  相似文献   

Morphologies of AGN host galaxies using HST/ACS in the CDFS-GOODS field     

Priya Hasan 《Astrophysics and Space Science》2007,312(1-2):63-77

Using HST/ACS images in four bands F435W, F606W, F775W and F850LP, we identify optical counterparts to the X-ray sources in the Chandra Deep Field South in the GOODS South field. A detailed study has been made of these sources to study their morphological types. We use methods like decomposition of galaxy luminosity profiles, color maps and visual inspection of 192 galaxies which are identified as possible optical counterparts of Chandra X-ray sources in the CDFS-GOODS field. We find that most moderate luminosity AGN hosts are bulge dominated in the redshift range (z≈0.4–1.3), but not merging/interacting galaxies. This implies probable fueling of the moderate luminosity AGN by mechanisms other than those merger driven.  相似文献   

Assessing uncertainties in dust emission in the Aral Sea region caused by meteorological fields predicted with a mesoscale model     

Kremena Darmenova  Irina N. Sokolik   《Global and Planetary Change》2007,56(3-4):297

This study investigates how the choice of the planetary boundary layer (PBL) parameterization and dust emission scheme affects the prediction of dust entrainment simulated with a regional mesoscale model. For this analysis we consider a representative dust episode which occurred on April 2001 in the Aral Sea region. The meteorological fields were simulated using the PSU/NCAR MM5 modeling system considering two different boundary layer parameterizations. In each case, emitted dust fluxes were computed off-line by incorporating MM5 meteorological fields into the dust module DuMo. Several dust emission schemes with a prescribed erodible fraction and fixed threshold wind speed were the subject of our analysis. Implications to assessment of the anthropogenic fraction of dust emitted in the Aral region were investigated by conducting the full, half, and no lake modeling experiments.Our results show that the discrepancies in dust fluxes between the two different PBLs are much higher compared to the discrepancy associated with the use of considered dust production schemes. Furthermore, the choice of the PBL affects the timing and duration of a modeled dust event. We demonstrate that different combinations of the PBL parameterization and wind- or friction velocity-driven dust emission schemes can result in up to about a 50% difference in predicted dust mass caused by the Aral Sea desiccation. We found that the drying-up of the Aral cannot only affect the dust emission by expanding the source area, but also by affecting atmospheric characteristics, especially winds. These competitive factors add further complexity to quantification of the anthropogenic dust fraction in the region.  相似文献   

Glacier inventory of the Gran Campo Nevado Ice Cap in the Southern Andes and glacier changes observed during recent decades   总被引：2，自引：2，他引：0  

Christoph Schneider  Michael Schnirch  Csar Acua  Gino Casassa  Rolf Kilian 《Global and Planetary Change》2007,59(1-4):87

The Gran Campo Nevado (GCN) forms an isolated ice cap on the Península Muñoz Gamero (PMG) located 200 km to the south of the Southern Patagonia Icefield (SPI). We present a glacier inventory of the GCN made up by 27 drainage basins (in total 199.5 km²) and other small cirque and valley glaciers of the southern part of PMG (in total 53 km²). The glacier inventory is based on a digital elevation model (DEM) and ortho-photos. Contour lines from maps, relief information derived from Landsat TM satellite imagery from 1986 and 2002 and stereoscopic data from aerial photos were combined in a knowledge-based scheme to obtain a DEM of the area. A digital ortho-photo map based on aerial photos from 1998 and several ortho-photos based on aerial photos from 1942 and 1984 could be produced from the initial DEM. A geographical information system (GIS) served to outline the extent of the present glaciation. All major glaciers of the GCN show a significant glacier retreat during the last 60 yr. Some of the outlet glaciers lost more than 20% of their total area during this period. Overall glacier retreat amounts to 2.8% of glacier length per decade and the glacier area loss is 2.4% per decade in the period from 1942 to 2002. We hypothesise that GCN glaciers may have reacted faster and more synchronously with the observed warming trend during recent decades when compared with the SPI.  相似文献   

Evidence of the Link between Broad Emission Line Regions and Accretion Disks in Active Galactic Nuclei     

Yun Xu    Xin-Wu Cao Shanghai Astronomical Observatory  Chinese Academy of Sciences  Shanghai  Graduate School of Chinese Academy of Sciences  Beijing 《中国天文和天体物理学报》2007,7(1):63-70

1 INTRODUCTION Most bright active galactic nuclei (AGNs) exhibit broad emission lines, with full width at half maximum (FWHM ≥ 103 km s?1) (Peterson et al. 1999). Some type 1 AGNs could have very broad emission lines (FWHM≥ 20 000 km s?1). Type 2 AGNs s…  相似文献