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211.
科学评估工业水资源效率并识别其影响因素是缓解水资源供需矛盾的重要前提。基于非期望产出的超效率EBM(Epsilon-based measure)模型测度了沿黄九省2010—2019年的工业水资源效率,然后构建Tobit模型分析其全局影响因素,在此基础上选取显著性影响因素纳入时空地理加权回归模型,探究各影响因素的时空异质性。结果表明:沿黄九省工业水资源效率均值为0.77,未达到有效水平,但呈现出波动上升态势。各省份之间效率差异明显,山东最高(1.064),宁夏最低(0.424)。在影响因素的宏观层面,技术水平和工业化程度对工业水资源效率攀升有正向促进作用;水资源禀赋、社会发展水平、工业用水强度和政府规制程度皆存在抑制效应,但显著程度不同,且高显著性影响因素的效应具有不同的时间演化趋势;在微观层面,各省份工业水资源效率的主导影响因素及其效应存在空间差异。 相似文献
212.
云南弥渡县云景预查区位于巍山县扎村金矿东缘,属于西南三江成矿省昌都-普洱成矿带。本文结合前人地质资料以及野外地物化遥等多元勘查手段,对该预查区多元地学信息进行分析和集成。研究发现,该区成矿作用与区内浅层侵入岩关系密切,接触交代成矿作用明显,矿化受南北向构造控制,构造交汇部位矿化集中发育。斑岩体构成了区内主要的磁性源,含矿石英砂岩体具有接触过渡带高阻、高极化率的特征,中深部找矿潜力巨大;地球化学异常特征表现为热液叠加改造型金矿的元素组合特征,亲铜元素相对富集,成矿阶段呈多期次性,金成矿贯穿早期高温热液成矿阶段。通过多元地学信息集成提出了适合本区的热液叠加改造型金矿找矿模型。 相似文献
213.
鄂尔多斯盆地马六段在盆地大部分地区被剥蚀,仅在盆地周缘地区分布,因此,有关该盆地马六段白云岩成因研究较少。本文通过对马六段白云岩岩石学特征、阴极发光特征、微量元素特征以及碳氧同位素地球化学特征进行分析,对鄂尔多斯盆地南部马六段白云岩特征及形成机制进行了研究。研究结果表明,盆地南部马六段白云岩主要由细—中晶白云岩组成,白云石具"雾心亮边"结构,阴极发光呈暗红色光。微量元素总体上具有较低的Fe、Mn值,平均值分别为447×10~(-6)和62×10~(-6),较高的K、Na值,平均值分别为517×10-6和252×10~(-6),以及中等含量的Sr元素值,平均值为155×10~(-6)。δ~(13)C值平均为-0.617‰,δ~(18)O值平均为-7.6‰,以上特征均反映出海源流体特征。白云石的"雾心"和"亮边"结构中微量元素含量相差不大,认为是在相同成岩环境的不同成岩阶段形成,其中"雾心"形成于浅埋藏环境的渗透回流白云石化作用,而"亮边"是在深埋藏环境下对早期白云石的调整和加强。 相似文献
214.
根据索道所处的极易遭受雷击的独特环境、信息系统的电子器件对雷电干扰极其敏感以及索道接地效果恶劣且泄放电流不畅的实际情况,引进现行其他行业成熟防雷技术原则,提出定量计算方法进行索道防雷分类。如果能够利用监测的雷暴日数Td、结合实际环境特征分段选取合适的校正系数k,计算索道年预计雷击次数N值会更趋向真实可靠。 相似文献
215.
根据长江路三期软土路基的工程地质条件及道路工程的施工特征,分析与探讨了适用于道路工程中深层搅拌桩质量的检测方法和桩身质量的综合评价方法,通过对此道路工程中深层搅拌桩质量的检测,总结出了适合道路工程的,轻便触探结合钻探取心的,快捷、方便、可靠、经济合理的较为理想的检测方法。 相似文献
216.
分析泰安基准地震台YRY-4型钻孔应变仪仪器受不同位置抽水的影响,就地下岩石含水变化所产生的地形变干扰,简要分析地下水与地下岩石间的相互作用。这对地震前兆的研究有重要实用意义。 相似文献
217.
Examining the Relationship Between Spatial Configurations of Urban Impervious Surfaces and Land Surface Temperature 总被引:1,自引:0,他引:1
The urban heat island(UHI) effect has significant effects on the quality of life and public health. Numerous studies have addressed the relationship between UHI and the increase in urban impervious surface area(ISA), but few of them have considered the impact of the spatial configuration of ISA on UHI. Land surface temperature(LST) may be affected not only by urban land cover, but also by neighboring land cover. The aim of this research was to investigate the effects of the abundance and spatial association of ISAs on LST. Taking Harbin City, China as an example, the impact of ISA spatial association on LST measurements was examined. The abundance of ISAs and the LST measurements were derived from Landsat Thematic Mapper(TM) imagery of 2000 and 2010, and the spatial association patterns of ISAs were calculated using the local Moran’s I index. The impacts of ISA abundance and spatial association on LST were examined using correlation analysis. The results suggested that LST has significant positive associations with both ISA abundance and the Moran’s I index of ISAs, indicating that both the abundance and spatial clustering of ISAs contribute to elevated values of LST. It was also found that LST is positively associated with clustering of high-ISA-percentage areas(i.e.,>50%) and negatively associated with clustering of low-ISA-percentage areas(i.e.,<25%). The results suggest that, in addition to the abundance of ISAs,their spatial association has a significant effect on UHIs. 相似文献
218.
219.
Shen Wang Wei-Wei Zhu Di Li Zhi-Chen Pan Pei Wang James M.Cordes Shami Chatterjee Ju-Mei Yao Lei Qian You-Ling Yue Lei Zhang Ru-Shuang Zhao Shuang-Qiang Wang Jia-Rui Niu Mao Yuan Chen-Chen Miao Xiao-Yao Xie Zhi-Jie Liu Xu-Hong Yu Shan-Ping You Ling-Qi Meng FAST Collaboration 《天文和天体物理学研究(英文版)》2021,(10):97-107
We present Arecibo 327 MHz confirmation and follow-up studies of seven new pulsars discovered by the Five-hundred-meter Aperture Spherical radio Telescope (FAST).These pulsars are discovered in a pilot program of the Commensal Radio Astronomy FAST Survey (CRAFTS) with the ultra-widebandwidth commissioning receiver.Five of them are normal pulsars and two are extreme nulling slow pulsars.PSR J2111+2132’s dispersion measure (DM:78.5 pc cm~(-3)) is above the upper limits of the two Galactic free electron density models,NE2001 and YMW16,and PSR J2057+2133’s position is out of the Scutum-Crux Arm,making them uniquely useful for improving the Galactic free electron density model in their directions.We present a detailed single pulse analysis for the slow nulling pulsars.We show evidence that PSR J2323+1214’s main pulse component follows a non-Poisson distribution and marginal evidence for a sub-pulse-drift or recurrent period of 32.3±0.4 rotations from PSR J0539+0013.We discuss the implication of our finding to the pulsar radiation mechanism. 相似文献
220.
Early Paleozoic subduction of the Paleo-Asian Ocean: Geochronological and geochemical evidence from the Dashizhai basalts,Inner Mongolia 总被引:10,自引:0,他引:10
Zircon U-Pb results of basalt from the Dashizhai Town in Inner Mongolia, NE China, shows that the basaltic lava was erupted
at 439±3 Ma, much older than the “Permian basalts” as previously thought. These rocks show arc-type trace element patterns
(i.e., Nb-Ta depletion and light REE and large ion lithophile element enrichment) and unradiogenic Sr and highly radiogenic
Nd and Hf isotope compositions. They can be subdivided into two petrogenetic groups: Group 1 basalts have relatively high
TiO2, MgO and compatible elements and low Sr and Th, characterized by mid-oceanic ridge basalt (MORB)-type Sr-Nd-Hf isotope compositions
(87Sr/86Sr(i)=0.7028−0.7032, εNd(t)=+9.8−+11.2, εHf(t)=+16.1−+18.4). Group 2 has lower TiO2, MgO and compatible elements and higher Sr and Th, and relatively evolved Sr-Nd-Hf isotope compositions (87Sr/86Sr(i)=0.7037−0.7038, εNd(t)=+5.7−+7.3, εHf(t)=+12.6−+13.0). Both groups were interpreted as melts derived from a metasomatized mantle wedge formed during the subduction
of Paleo-Asian Ocean. The mantle source for Group 1 was probably a highly isotopically depleted oceanic mantle modified by
predominant slab fluids; whereas subducted sediments had an important contribution to the melting source for Group 2. The
petrogenesis of the Dashizhai basalts provides clear evidence for early Paleozoic subduction of the Paleo-Asian Ocean, and
the highly radiogenic Nd and Hf compositions in these rocks suggest that these lavas and their possible intrusive counterparts
were one of the important components for Phanerozoic crustal growth. Our and previous studies on the “Dashizhai Formation”
volcanic rocks yield an unrealistic eruption range of 440-270 Ma for different rock types, we thus advise to disassemble the
previously defined “Dashizhai Formation” into multiple lithologic units and to reinterpret the spatial and temporal distributions
of different volcano-sedimentary associations.
Supported by National Basic Research Program of China (Grant No. 2006CB403504) 相似文献