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831.
武威市位于甘肃省中部,是一座典型的农业城市,分布有大量农业耕地。由于土壤疏松,地面容易受到降水和地下水的影响,易发生地面沉降地质灾害对居民的生产、生活造成不利影响。本文利用2017年2月至2022年12月的Sentinel-1A数据,通过PS-InSAR技术提取了武威市的地面沉降监测数据,包括视线向形变速率和累积形变量。对形变场的时空分布特征进行了详细分析,并引入Mogi模型反演地下深部变形范围。最后,结合研究区的降水数据和GRACE重力卫星获取到由陆地水负荷引起的地表形变数据,并对研究区的沉降成因进行了初步分析。结果表明,研究区存在两个主要沉降区,其中主沉降区A的最大累积沉降量达到-290.9 mm,视线向形变速率为-52.0 mm/a;主沉降区B的沉降量达到-178.1 mm,视线向形变速率为-43.8 mm/a。地表沉降呈现周期性变化,且向东南方向逐步扩展,与降水和地下水变化特征相似。通过Mogi模型反演,得出了主沉降区的地下影响范围(半径)和深度,其中主沉降区A为40.96 m和133.67 m,主沉降区B为38.60 m和140.78 m。按季节划分统计形变数据,结果表明,由于研究区所属干旱区,自然降水无法对地面沉降产生显著影响,而农耕时大量地下水的抽取才是导致区域地面沉降的主要原因。
相似文献832.
833.
Dev Niyogi Hsin-I Chang Fei Chen Lianhong Gu Anil Kumar Surabi Menon Roger A. Pielke Sr. 《Natural Hazards》2007,42(2):345-359
Aerosols can affect the cloud-radiation feedback and the precipitation over the Indian monsoon region. In this paper, we propose
that another pathway by which aerosols can modulate the multi-scale aspect of Indian monsoons is by altering the land–atmosphere
interactions. The nonlinear feedbacks due to aerosol/diffuse radiation on coupled interactions over the Indian monsoon region
are studied by: (1) reviewing recent field measurements and modeling studies, (2) analyzing the MODIS and AERONET aerosol
optical depth datasets, and (3) diagnosing the results from sensitivity experiments using a mesoscale modeling system. The
results of this study suggest that the large magnitude of aerosol loading and its impact on land–atmosphere interactions can
significantly influence the mesoscale monsoonal characteristics in the Indo-Ganges Basin. 相似文献
834.
In situ infiltration test using a reclaimed abandoned river bed: managed aquifer recharge in Shijiazhuang City,China 总被引:3,自引:1,他引:3
Managed aquifer recharge (MAR) is necessary for water resources management in arid and semiarid regions. Infiltration rate is often a decisive limiting factor in site selection for MAR. In order to avoid scale effects in the application of infiltration rate parameters, the largest in situ infiltration test in China was undertaken between August 19 and August 30, 2009 to measure the infiltration rate of the field selected for MAR in Shijiazhuang City, China. The in situ test lasted for 10 days, and about 1.82 × 107 m3 of water was introduced into the infiltration field. Groundwater level variations were monitored during the test. Monitoring showed that the infiltration rate of surface water was 1.5 m/day, which means that about 10–15 × 108 m3/a of water could be injected into the target aquifer. Also, groundwater level variations showed that the northern part of the infiltration field had a higher infiltration rate, as predicted, and the test result supplied a sound foundation for validation of the groundwater numerical simulation, which will be of benefit for future predictions of the response of the groundwater level to artificial recharge engineering. Finally, an artificial recharge plan was proposed based on the infiltration test results and the water source conditions, which would be useful for the development of MAR programs and management of local water resources. 相似文献
835.
含钒金红石可见光下催化降解亚甲基蓝实验研究 总被引:2,自引:0,他引:2
利用含有钒等杂质的金红石可部分吸收可见光的特性,以500 W卤素灯作为光源,实验研究了其对亚甲基蓝的可见光催化降解,结果表明,该金红石具有催化活性,7 h后亚甲基蓝可降解71 2%。经过加热、粉碎改性方法处理后的金红石光催化活性明显提高,加热1 100 ℃的金红石样品7 h后可使亚甲基蓝的降解率达到90 4%。增加光照强度、加入适当的H2O2 都可提高降解效果。实验为充分开发利用天然金红石提出了新的途径,为环境污染治理提出了新方法。 相似文献
836.
以1:5万地质填图和钻探验证为基础,经分析研究塔里木托云盆地的地层特征、聚煤期、古地理环境,从而建立起该区的沉积模式,总结出该盆地煤层发育于下侏罗统康苏组上段地层之中,含煤11层,煤层为不稳定发育,但分布具有一定的规律可寻,对进一步找煤具有一定的指导意义。 相似文献
837.
838.
839.
Multi-dimensional Seismic Response Analysis of Base-Isolated Frame Structure with 3D Isolator 总被引:1,自引:0,他引:1
XiongShishu HuangLiting ChenJinfeng SuJingsu 《中国地质大学学报(英文版)》2005,16(1):66-71,78
INTRODUCTIONAs a new and effective method for withstandingthe horizontal component of earthquake motion on abuilding structure, the base isolation technique hascome to the engineering application phase ( Hu,1988). However, for some important buildings andfoundation facilities in an earthquake region, it is im portant to consider the effects of 3D aseismatic analy sis, including the vertical component, due to themulti dimensional characteristics of earthquakes (Suand … 相似文献
840.
Shantanu Keshav Alexandre Corgne Michael Bizimis Yingwei Fei 《Geochimica et cosmochimica acta》2005,69(11):2829-2845
In this experimental study, we examine the mineral-melt partitioning of major and trace elements between clinopyroxene and CO2-rich kimberlitic melts at a pressure of 6 GPa and temperatures of 1410°C and 1430°C. The melts produced contain ∼ 28 wt% dissolved CO2, and are saturated with olivine and clinopyroxene. To assess the effects of temperature, crystal and melt compositions on trace element partitioning, experiments were performed in the model CaO-MgO-Al2O3-SiO2-CO2 system. Our results reveal that all the elements studied, except Al, Mg, Si, and Ga, are incompatible in clinopyroxene. Partition coefficients show a considerable range in magnitude, from ∼ 10−3 for DU and DBa to ∼ 2.5 for DSi. The two experimental runs show similar overall partitioning patterns with the D values being lower at 1430°C. Rare earth elements display a wide range of partition coefficients, DLa (0.012-0.026) being approximately one order of magnitude lower than DLu (0.18-0.23). Partition coefficients for the 2+ and 3+ cations entering the M2-site exhibit a near-parabolic dependence on radius of the incorporated cations as predicted from the lattice strain model. This underlines the contribution made by the crystal structure toward controlling the distribution of trace elements. Using data obtained in this study combined with that in the published literature, we also discuss the effects that other important parameters, namely, melt composition, pressure, and temperature, could have on partitioning.Our partition coefficients have been used to model the generation of the Group I (GI) kimberlites from South Africa. The numerical modeling shows that kimberlitic melts can be produced by ∼0.5% melting of a MORB-type depleted source that has been enriched by small-degree melts originating from a similar depleted source. This result suggests that the source of GI kimberlites may be located at the lithosphere-asthenosphere transition. Percolation of small degree melts from the asthenosphere would essentially create a metasomatic horizon near the bottom of the non-convecting sublithospheric mantle. Accumulation of such small degree melts together with the presence of volatiles and conductive heating would trigger melting of the ambient mantle and subsequently lead to eruption of kimberlitic melts. Additionally, our model shows that the GI source can be generated by metasomatism of a 2 Ga old MORB source ca. 1 Ga ago. Assuming that MORB-type mantle is the most depleted source of magmas on earth, then this is the oldest age at which the GI source could have existed. However, this age most likely reflects the average age of a series of metasomatic events than that of a single event. 相似文献