电磁卫星地面对比观测原型系统地电场观测资料特征分析          下载免费PDF全文

周卫东  牛延平  田野  苏小芸  陈丽君 《地震工程学报》2020,42(6):1517-1522

通过对电磁监测试验卫星地面对比观测原型系统中古丰、寺滩和坪城地电场观测数据特征研究，结果表明：（1）3个台站的地电场观测数据均具有较为明显的正常日变化形态；（2）在磁暴发生期间，地电场各测向均记录到了同步的地电暴变化，其最大变幅均明显高于正常日变；（3）寺滩地电场记录到临震前的数据异常现象，在时间和空间上都与地震事件吻合较好。  相似文献   

基于时相变化的晴空条件下Himawari-8 AHI火点检测     

鄢俊洁  瞿建华  冉茂农  张芳芳 《遥感学报》2020,24(5):571-577

Himawari-8静止气象卫星具有高空间分辨率、高观测频次和高时效特点,对于火点检测具有很强优势。对Himawari-8卫星的3.9μm和11.2μm两通道亮温进行了连续时相变化研究,得出两通道的亮温在时间上的变化差值稳定且规律明显。根据两通道的亮温时相特征,考虑白天可见光对3.9μm通道的影响,并结合火点产生时引起的亮温变化特征,提出了适用于晴空条件下改进的火点检测算法。在多处进行了此算法的实验,例如2018-11-27 T 16:40(UTC时)河北张家口市桥东区一化工厂附近发生的严重爆炸起火事件以及2019-02-28澳大利亚西南部发生的火灾事件,均快速有效的检测到了火点。实验表明,改进的火点检测算法能很好的进行火点检测,并能解决晨昏交界、冰雪下垫面、常规火源点、太阳耀光等火点检测的难题。  相似文献   

生物土壤结皮对风沙土和黄绵土膨胀特性的影响     

王国鹏  肖波  李胜龙  姚小萌  孙福海 《中国沙漠》2020,40(1):97-104

作为重要的土壤物理性质，膨胀性在影响土壤导水性、持水性、抗蚀性以及土壤结构的形成和发育等方面发挥着重要作用。为了探讨生物土壤结皮（BSCs）土壤的膨胀特性及其主要影响因素，针对黄土高原风沙土和黄绵土两种典型土壤，利用膨胀仪测定并比较了有、无藓结皮及其在不同因素（初始含水量、干湿循环、冻融循环、温度）下膨胀率的差异，分析了BSCs对土壤膨胀性的影响及其与环境因素和BSCs性质的关系。结果显示：风沙土上藓结皮的膨胀率为1.93%，较无结皮增加了8.65倍；而黄绵土上藓结皮的膨胀率为2.05%，与无结皮相比降低了76.68%。藓结皮的生物量和厚度与其膨胀率在风沙土上均呈线性正相关关系（P < 0.05），在黄绵土上分别呈二次函数（P=0.02）和线性正相关关系（P=0.02）。初始含水量同时影响了土壤最大膨胀率和稳定膨胀时间，影响程度风沙土远大于黄绵土（包括藓结皮和无结皮）；干湿循环次数对无结皮土壤膨胀率的影响程度大于藓结皮土壤，其中风沙土和黄绵土上无结皮的膨胀率分别是50.00%~620.00%和-2.28%~10.81%，而两种土壤上藓结皮的膨胀率分别是-5.70%~10.88%和-10.24%~-21.46%；冻融循环下4种土壤的膨胀率均有不同程度的降低，降幅为0~18.54%。黄绵土无结皮的膨胀率受温度影响程度较大，50℃下黄绵土无结皮的膨胀率分别是25℃和35℃下的1.17倍和1.21倍。BSCs显著地改变了风沙土和黄绵土表层的膨胀性，其影响的程度和方向取决于土壤类型。同时，BSCs的膨胀性受含水量、温度、干湿以及冻融循环等关键因素影响。  相似文献   

毛乌素沙地锦鸡儿（Caragana）根系微域细菌群落多样性特征     

周子渊  于明含  丁国栋  高广磊  何莹莹 《中国沙漠》2020,40(4):128-137

基于16S rRNA高通量基因测序技术，对毛乌素沙地小叶锦鸡儿（Caragana microphylla)、柠条锦鸡儿（Caragana korshinskii）根系微域（即根系、根际土、根区土、灌丛间空白土）间的细菌群落多样性和结构差异性进行表征。本研究对各根系微域间细菌群落的Alpha多样性指数进行了单因素方差分析以及基于OTU水平的PCA分析，探究其在根系微域间Alpha和Beta多样性的层级变化，证实了有关植物根系微域生态位分化的报道，并发现锦鸡儿属植物根系微域间细菌群落的多样性和结构组成随着4个微域类型由外及内呈现出显著的层级差异性（P<0.05）。通过对优势细菌群组的结构组成分析，发现锦鸡儿属植物对特定细菌群组具有显著的向根系内筛选富集的作用（P<0.05）。这种植物通过根系微域对特定细菌群组的逐级筛选富集作用，是导致锦鸡儿属植物灌丛下不同生态位间细菌群落结构和组成发生层级变异的主要原因。  相似文献   

Correspondence between the large volcanic eruptions and ENSO events over AD 1525–2000     

Fang  Xiuqi  Zheng  Xue  Zhang  Xing 《地理学报(英文版)》2020,30(1):103-118

ENSO is an interannual mode which may be affected by external forcing, such as volcanic eruptions. Based on the reconstructed volcanic eruptions chronology and ENSO sequences, both 195 large volcanic eruptions(VEI≥4) and 398 ENSO(El Ni?o and La Ni?a) events were extracted from 1525 to 2000. An analysis of the correspondence between the large volcanic eruptions and ENSO events was performed by matching the large volcanic eruptions with the types and magnitudes of ENSO events present in the 0–2 years after the eruptions. The results show the following:(1) The percentages of ENSO events within the 3 years after the large eruptions had increased to 68.3% from 31.7% compared with those with no-eruptions in the previous 0–2 years. In addition, the ratio of El Ni?o to La Ni?a events turned from 2:3 to 1:1, and more El Ni?o events occurred in the 0 year after eruptions in the low-latitudes of the Northern Hemisphere and in the tropics but more La Ni?a events occurred in the 0 year after in the high-latitudes of the Northern Hemisphere and the Southern Hemisphere.(2) After the eruptions, the weak(W) El Ni?o events had increased by 8 percentage points and the very strong(VS) El Ni?o events had decreased by 10 percentage points; conversely, there was a decrease by 15 percentage points of the weak La Ni?a events and an increase by 11.4 percentage points of the very strong La Ni?a events. Specifically, the percentages of strong La Ni?a events increased to a peak at 1(+1) year after the eruptions.(3) The percentage of eruptions followed by single-year ENSO was the greatest. The percentage of ENSO events that occurred in the consecutive 2 years following an eruption was approximately equal to the percentage of events that occurred consecutively 3 years following an eruption, and both sets of ENSO magnitudes showed a decreasing trend.  相似文献   

Simulations of the Impact of Lakes on Local and Regional Climate Over the Tibetan Plateau     

Lingjing Zhu  Xin Liu  Lei Tian  Qunhui Zhang 《大气与海洋》2018,56(4):230-239

ABSTRACT

Because of the high elevation and complex topography of the Tibetan Plateau (TP), the role of lakes in the climate system over the Tibetan Plateau is not well understood. For this study, we investigated the impact of lake processes on local and regional climate using the Weather Research and Forecasting (WRF) model, which includes a one-dimensional physically based lake model. The first simulation with the WRF model was performed for the TP over the 2000–2010 period, and the second was carried out during the same period but with the lakes filled with nearby land-use types. Results with the lake simulation show that the model captures the spatial and temporal patterns of annual mean precipitation and temperature well over the TP. Through comparison of the two simulations, we found that the TP lakes mainly cool the near-surface air, inducing a decreasing sensible heat flux for the entire year. Meanwhile, stronger evaporation produced by the lakes is found in the fall. During the summer, the cooling effect of the lakes decreases precipitation in the surrounding area and generates anomalous circulation patterns. In conclusion, the TP lakes cool the near-surface atmosphere most of the time, weaken the sensible heat flux, and strengthen the latent heat flux, resulting in changes in mesoscale precipitation and regional-scale circulation.  相似文献   

云南广南县老寨湾金矿地质特征及找矿标志     

高李阳  顾雄  吴小梅 《云南地质》2020,(1):71-75

广南县老寨湾金矿位于滇、黔、桂“金三角”重要成矿区带上,金矿体矿体呈似层状赋存于断层构造破碎带或层间构造破碎带中,构造控矿明显。矿体围岩均为下泥盆统坡松冲组第一段(D1ps1)硅化石英砂岩;矿床成因属中-低温热液叠加改造型金矿床,断层构造、硅化等矿化蚀变及地球化学异常是重要的找矿标志。  相似文献   

不同顶管组合方式的管幕冻结温度场模型试验   总被引：1，自引：1，他引：0  

段寅  荣传新  程桦  蔡海兵  解德柱  丁杨龙 《冰川冻土》2020,42(2):479-490

拱北隧道作为港珠澳大桥珠海连接线的关键性工程， 在国内外首次成功运用了管幕冻结技术。以此为背景， 为更加全面地掌握饱和软土地层中管幕冻结温度场的分布特点， 开展了不同顶管组合方式下的管幕冻结温度场模型试验研究。试验结果表明： 各测点温度曲线在积极冻结期前4 h急剧下降， 随后逐渐减缓， 降至砂土冰点后趋于平稳， 三种布管方式均满足冻结设计要求； 冻结管中低温盐水提供的冷量首先传递给顶管管壁， 再以“面”的形式均匀地传递给周围土体； 积极冻结21 h后， 采用四根空顶管组合的C区冻结壁竖向范围最大， 空管管壁正上方冻结壁平均厚度约为105 mm， 在满足管幕刚度设计要求的前提下， 可采此布管方式以达到快速形成冻结帷幕的目的。限位管开启后的4 h内， 实顶管中线垂直距离100 mm范围内测点温度曲线虽有明显回升但仍维持在冻土冰点以下， 超出此范围后温度变化影响逐渐减弱， 且顶管间冻结壁稳定存在， 表明限位管在满足管间有效封水的条件下， 能在一定范围内起到定向限制地层冻胀的作用。优化后的双圆形冻结管在满足冻结设计要求的同时， 更加便于安装且经济环保。  相似文献   

金伯利岩型金刚石矿床研究及其成矿模式探讨——以辽宁瓦房店地区金刚石原生矿矿床为例     

刘礼广  吴大天  韩双  万方来  林少全  杨献忠 《地质学报》2020,94(9):2650-2665

辽宁南部瓦房店金刚石矿是国内最大的金刚石矿产区，现已发现4处金刚石成矿带、120个岩体。其中金伯利岩岩管24个、岩脉89个、可疑岩体7个，累计提交1221万克拉储量，占全国金刚石储量52%。本文主要对该矿床的金刚石母岩—金伯利岩的岩石地球化学特征进行了全面系统分析，发现金伯利岩中MgO、NiO、Cr 2O 3的含量与TiO 2、Al 2O 3、Na 2O、K 2O、CaO、P 2O 5等偏碱性组分呈正相关关系；Ni、Cr、Co含量与金刚石含量呈正相关，而Ti、Zr、Ba元素含量与金刚石含量呈负相关。通过对瓦房店矿区金刚石中石榴石及单斜辉石包裹体、橄榄石- 石榴石矿物对、石榴石微量元素、尖晶石- 橄榄石等多种地质温、压计归纳得出金刚石矿的来源深度为150~210 km,压力5~7 GPa，温度1083~1261℃，在上述温、压条件下，结合岩浆化学组成，估算金伯利岩具有低氧逸度(fO 2=2. 913×1. 01325×10-6Pa)的特点。结合野外勘查工作，总结了该矿床的地质特征、控矿构造、矿体空间分布规律等要素，认为NEE向和NE向断裂控制着金伯利岩体的展布方向和矿体形态。脉状金伯利岩体一般呈NEE 70°~80°方向展布，严格受NEE至近EW向的密集节理或裂隙控制。提出了金刚石母岩—金伯利岩是由源于上地幔岩浆，在一定的封闭条件下，受构造与岩性双重控制，多期性的爆发与侵入交替作用所形成，并建立了具有较高氧逸度和较高密度的流变性软流圈，通过渗滤熔体浸蚀岩石圈形成金刚石的理想成因模式，希望为下一步找矿工作提供参考。  相似文献   

Northward cooling of the Kuncha nappe and downward heating of the Lesser Himalayan autochthon distributed to the south of Mt. Annapurna,western central Nepal     

Toru Nakajima  Harutaka Sakai  Hideki Iwano  Tohru Danhara  Takafumi Hirata 《Island Arc》2020,29(1)

We investigated the tectonothermal history of the Lesser Himalayan sediments (LHS), which are tectonically overlain by the Higher Himalayan Crystalline. Fission‐track dating and the track length measurement of detrital zircons obtained from the Kuncha nappe and the Lesser Himalayan autochthonous sediments in western central Nepal revealed northward cooling of the nappe and possible downward heating of the autochthon by the overlying hot nappe. Nine zircon fission‐track (ZFT) ages of the nappe showed northward‐younging linear distribution from 11.6 Ma in the front at Tamghas, 6 Ma in the central at Naudanda, and 1.6 Ma in the northernmost point at Tatopani. Thermochronological invert calculation of the ZFT length elucidated that the Kuncha nappe gradually cooled down (30 °C/Myr) at the front and rapidly cooled down (120 °C/Myr) at the root zone. In contrast, the ZFT age of the Chappani Formation, located just beneath the Kuncha nappe in the central part, demonstrated a totally reset age of 6.8 Ma, whereas the Virkot Formation, structurally far from the nappe, yielded a partially reset age of 457.3 Ma. This suggests that the LHS underwent downward heating, resulting in a thermal print on the upper part of the LHS; however, the thermal effect was not sufficient to anneal ZFT totally in the deeper part. Presently, the nappe cover is eroded and denuded from this area. Detrital zircons from the Chappani Formation in Tansen area to the south of the Bari Gad Fault did not show any evidence of annealing, suggesting that nappe never covered the LHS distributed to the south of the fault.  相似文献