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991.
992.
993.
994.
运用H、O同位素资料分析地下热水的补给来源——以鲁西北阳谷-齐河凸起为例 总被引:1,自引:0,他引:1
通过对阳谷-齐河凸起地下热水的化学成分、同位素及其地热地质条件的分析,对这一地区的地下热水的补给来源进行了研究。本区地下热水的δD为-65‰~-80.67‰,δ18O为-9.2‰~-10.2‰,均分布在全球雨水线的附近,说明该区地下热水主要为大气降水成因。济南北地热田地下热水的补给高程为256m,此范围大致相当于济南南部山区及其以南的泰山北麓;聊城东地热田地下热水的补给高程为411m,此范围大致相当于泰山山脉及其周边的中山区。聊城东地热田地下热水的2H过量参数d明显低于济南北地热田,说明聊城东地热田地下热水的补给区比后者更远。 相似文献
995.
借鉴油气藏数值模拟理论、技术和方法,对单一松软煤层的瓦斯抽采工艺进行了研究分析。根据单一松软煤层特点,提出了单一松软煤层的几何模型技术——单直径球型孔隙模型,在此基础上建立了煤层瓦斯抽采的地质和数理模型,并根据网格差分方法推导出数值解。以实际生产数据对新模型及其数值解进行验证,结果表明该模型可以用于指导单一松软煤层瓦斯抽采工艺的确定。 相似文献
996.
997.
Sarah E. Rothenberg Matthew E. Kirby Broxton W. Bird Margie B. DeRose Chu-Ching Lin Xinbin Feng Richard F. Ambrose Jennifer A. Jay 《Environmental Earth Sciences》2010,60(5):993-1005
In southern California, USA, wildfires may be an important source of mercury (Hg) to local watersheds. Hg levels and Hg accumulation
rates were investigated in dated sediment cores from two southern California lakes, Big Bear Lake and Crystal Lake, located
approximately 40-km apart. Between 1895 and 2006, fires were routinely minimized or suppressed around Big Bear Lake, while
fires regularly subsumed the forest surrounding Crystal Lake. Mean Hg concentrations and mean Hg accumulation rates were significantly
higher in Crystal Lake sediments compared to Big Bear Lake sediments (Hg levels: Crystal Lake 220 ± 93 ng g−1, Big Bear Lake 92 ± 26 ng g−1; Hg accumulation: Crystal Lake 790 ± 1,200 μg m−2 year−1, Big Bear 240 ± 54 μg m−2 year−1). In Crystal Lake, the ratio between post-1965 and pre-1865 Hg concentrations was 1.1, and several spikes in Hg levels occurred
between 1910 and 1985. Given the remote location of the lake, the proximity of fires, and the lack of point sources within
the region, these results suggested wildfires (rather than industrial sources) were a continuous source of Hg to Crystal Lake
over the last 150 years. 相似文献
998.
Adsorption of antimony(V) on kaolinite as a function of pH,ionic strength and humic acid 总被引:1,自引:0,他引:1
The present work investigated the adsorption and mobility (desorption) of Sb(V) on kaolinite using batch experiments. The
adsorption of Sb(V) on kaolinite was studied as a function of contact time, pH, ionic strength, humic acid (HA), initial Sb(V)
concentration and temperature. Kinetic studies suggest that the equilibrium is achieved within 24 h. The adsorption of Sb(V)
was strongly affected by changes in I at low ionic strength and unaffected at high ionic strength. The adsorption is weakly
dependent on the presence of humic acid, but is strongly dependent on pH. Within the range tested, the optimal pH for Sb(V)
adsorption is 3.6, and close to 75% removal can be achieved. Desorption is dependent on the original suspension pH. The addition
sequence of Sb(V)/HA do not influence the adsorption of Sb(V) on kaolinite. The adsorption data fit both the Freundlich and
Langmuir isotherm. The thermodynamic parameters (ΔH
0, ΔS
0 and ΔG
0) were calculated from the temperature dependence, and the results suggest the endothermic and spontaneous nature of the process. 相似文献
999.
1000.
Bidong Zhang Yangting Lin Jialong Hao Devin L. Schrader Meenakshi Wadhwa Randy L. Korotev William K. Hartmann Audrey Bouvier 《Meteoritics & planetary science》2023,58(10):1540-1551
About half of the lunar meteorites in our collections are feldspathic breccias. Acquiring geochronologic information from these breccias is challenging due to their low radioactive-element contents and their often polymict nature. We used high-spatial-resolution (5 μm) NanoSIMS (nanoscale secondary ion mass spectrometry) U-Pb dating technique to date micro-zircons in the lunar feldspathic meteorites Dhofar 1528 and Dhofar 1627. Three NanoSIMS dating spots of two zircon grains from Dhofar 1528 show a discordia with an upper intercept at 4354 ± 76 Ma and a lower intercept at 332 ± 1407 Ma (2σ, MSWD = 0.01, p = 0.91). Three spots of two zircon grains in Dhofar 1627 define a discordia with an upper intercept at 3948 ± 30 Ma and a lower intercept at 691 ± 831 Ma (2σ, MSWD = 0.40, p = 0.53). Both samples likely experienced shock metamorphism caused by impacts. Based on the clastic nature, lack of recrystallization and the consistent U-Pb and Pb-Pb dates of the zircons in Dhofar 1528, the U-Pb date of 4354 Ma is interpreted as the crystallization age of its Mg-suite igneous precursor. Some of the Dhofar 1627 zircons show poikilitic texture, a crystallization from the matrix impact melt, so the U-Pb date of 3948 Ma corresponds to an impact event, likely the Imbrium basin-forming event. These data are the first radiometric ages for these two meteorites and demonstrate that in situ (high spatial resolution) U-Pb dating has potential for extracting geochronological information about igneous activities and impact events from lunar feldspathic and polymict breccias. 相似文献