生物刺激法对石油污染荒漠土的修复效应/[J]

利用生物法修复有机物污染土壤是一种低成本、无二次污染物产生的绿色修复方法,受到国内外学者的极大关注.目前,国内对石油污染土壤生物修复技术的研究工作集中于中东部地区,对干旱区石油污染土壤修复工作非常欠缺.本研究以干旱区石油污染荒漠土为研究对象,通过投加不同水平的营养元素,以刺激土壤微生物活性,探讨生物刺激法修复干旱区石油污染土壤的可行性及修复效果,为建立面向干旱区的石油污染土壤生物修复技术提供科学依据和技术支撑

原油对荒漠土微生物活性的影响[J]

石油进入土壤后改变了土壤质地,使原有土壤微生物群落、区系和土壤酶活性受到了不同程度的影响.目前,对干旱区原油污染和土壤微生物之间的关系,研究工作涉及较少.本文选取干旱胁迫环境中的荒漠土为研究对象,研究了原油对荒漠土中微生物活性的影响.研究结果对于评价干旱区石油污染对土壤生态环境的影响,揭示荒漠土土壤微生物对石油污染物的响应规律具有重要意义. 1 材料与方法 1.1 土样来源实验土样为荒漠土,采自新疆克拉玛依油田采气一厂.土壤基本理化性质为:pH值7.2,土壤有机质、总氮、总磷含量分别为0.7％、0.01％及0.02％.土壤机械组成为:粗砾(＞0.2 mm)、细沙(0.02-0.2 mm)、粉沙(0.002-0.02 mm)、黏粒(＜0.002 mm)含量分别为11％、54％、27％及8％

采气废水中有机物去除方法/Methods of organic contaminants removal in natural gas-produced wastewater[J]

新疆油田天然气开采过程中产生的大量高矿化度、高COD的含油废水,难以处理处置,严重影响了气田的正常生产活动,危害到气田周边土壤安全和荒漠植被的生存.为实现该类废水的达标排放,选取COD和总石油烃含量为考察指标,研究比较了紫外(UV)、臭氧(O3)及紫外臭氧联合处理(UV/O3)法对该类废水的处理效果,进一步考察了pH和O3发生量对UV/O3法处理效果的影响.研究结果表明,3种方法处理废水60 min后,废水COD由处理前的563 mg/L分别下降至处理后的479、334.9和314 mg/L,去除率分别达到14.9％、32.7％和44.2％;而总石油烃含量由处理前的3.86 mg/L分别降至处理后的3.05、1.26和0.20 mg/L,去除率分别达到21.2％、67.4％和94.8％;其中,UV/O3法处理90 min后废水COD降低至148 mg/L,达到《废水综合排放标准GB8978-1996》二级排放标准;pH为7,臭氧发生量为10 g/L时,UV/O3法可应用于采气废水的处理

Determination of the number of ψ(3686) events taken at BESIII

The number of ψ(3686) events collected by the BESIII detector during the 2021 run period is determined to be (2259.3±11.1)×106 by counting inclusive ψ(3686) hadronic events. The uncertainty is systematic and the statistical uncertainty is negligible. Meanwhile, the numbers of ψ(3686) events collected during the 2009 and 2012 run periods are updated to be (107.7±0.6)×106 and (345.4±2.6)×106, respectively. Both numbers are consistent with the previous measurements within one standard deviation. The total number of ψ(3686) events in the three data samples is (2712.4±14.3)×10^

Measurement of integrated luminosity of data collected at 3.773 GeV by BESIII from 2021 to 2024

We present a measurement of the integrated luminosity e+e- of collision data collected by the BESIII detector at the BEPCII collider at a center-of-mass energy of Ecm = 3.773 GeV. The integrated luminosities of the datasets taken from December 2021 to June 2022, from November 2022 to June 2023, and from October 2023 to February 2024 were determined to be 4.995±0.019 fb-1, 8.157±0.031 fb-1, and 4.191±0.016 fb-1, respectively, by analyzing large angle Bhabha scattering events. The uncertainties are dominated by systematic effects, and the statistical uncertainties are negligible. Our results provide essential input for future analyses and precision measurements