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991.
崔娟  王浩  刘杰  王越  卢立栋  陈洁 《中国沙漠》2021,41(2):59-66
基于2013-2018年榆林市沙尘天气和环境空气质量逐日数据,定量分析了沙尘天气对榆林市空气质量指数(AQI)、可吸入颗粒物(PM10)和细颗粒物(PM2.5)的绝对贡献和相对贡献率.结果表明:沙尘天气对榆林市AQI的贡献率为0.7%-11.1%(平均值±标准差6.4%±3.8%);对PM10的绝对贡献为 1.0-13...  相似文献   
992.
The strong increase in the flux of relativistic electrons during the recovery phase of magnetic storms and during other active periods is investigated with the help of Hamiltonian formalism and simulations of test electrons which interact with whistler waves. The intensity of the whistler waves is enhanced significantly due to injection of 10–100 keV electrons during the substorm. Electrons which drift in the gradient and curvature of the magnetic field generate the rising tones of VLF whistler chorus. The seed population of relativistic electrons which bounce along the inhomogeneous magnetic field, interacts resonantly with the whistler waves. Whistler wave propagating obliquely to the magnetic field can interact with energetic electrons through Landau, cyclotron, and higher harmonic resonant interactions when the Doppler-shifted wave frequency equals any (positive or negative) integer multiple of the local relativistic gyrofrequency. Because the gyroradius of a relativistic electron may be the order of or greater than the perpendicular wavelength, numerous cyclotron, harmonics can contribute to the resonant interaction which breaks down the adiabatic invariant. A similar process diffuses the pitch angle leading to electron precipitation. The irreversible changes in the adiabatic invariant depend on the relative phase between the wave and the electron, and successive resonant interactions result in electrons undergoing a random walk in energy and pitch angle. This resonant process may contribute to the 10–100 fold increase of the relativistic electron flux in the outer radiation belt, and constitute an interesting relation between substorm-generated waves and enhancements in fluxes of relativistic electrons during geomagnetic storms and other active periods.  相似文献   
993.
WATERQUALITYSIMULATIONOFHEAVYMETALTRANSPORTATIONINTHEYELLOWRIVERSHENXianchen1,FENGHuihua2,WANGFengrong3andLIULinhua4ABSTRACTA...  相似文献   
994.
During June and July 2003 the Sources and Origins of Atmospheric Cloud Droplets experiment (SOACED) was carried out on a mountain-top site in central Sweden. The main objective of the experiment was to characterise the microphysical and chemical properties of cloud droplet residuals and interstitial aerosol particles in continental clouds and to understand the processes controlling cloud properties at this location.Interstitial and residual aerosol size distributions, cloud liquid water content and species- and size-resolved aerosol mass concentrations are the main variables employed to address questions pertaining to the cloud droplet number concentration and scavenging efficiency during a stratocumulus cloud event observed on July 28, 2003. In this cloud event, about 56% of the aerosol mass was associated with organic species, whilst SO4 accounted for 23% and NH4 for 14%. NO3 and Cl made up about 7% of the total mass.The partitioning of the aerosol particles between cloud droplets and interstitial air has been studied in terms of their microphysical properties. The scavenging efficiency, defined as the fraction of particles activated into cloud elements compared to the total amount of particles, was investigated as a function of size. The scavenging efficiency curves displayed different shapes during the cloud event, from an S-shaped curve, with low scavenging efficiency in the Aitken mode and larger scavenging efficiency in the accumulation mode, to more unusual shapes where Aitken-mode particles were either solely activated or activated in addition to accumulation-mode particles.This study suggests that alterations of the aerosol chemical composition occurred during the measurement period, changing the hygroscopic nature of the CCN and decreasing their activation diameter. It is also hypothesized that entrainment of drier air aloft may have introduced inhomogeneities in the supersaturation field and modified the S-shaped scavenging curves.  相似文献   
995.
Numerical simulation of flows in shallow reservoirs has to be checked for its consistency in predicting real flow conditions and sedimentation patterns. Typical flow patterns may exhibit flow separation at the inlet, accompanied by several recirculation and stagnation areas all over the reservoir surface. The aim of the present research project is to study the influence of the geometry of a reservoir on sediment transport and deposition numerically and experimentally, focusing on a prototype reservoir depth between 5 and 15 m as well as suspended sediment transport.
A series of numerical simulations is presented and compared with scaled laboratory experiments, with the objective of testing the sensitivity to different flow and sediment parameters and different turbulence closure schemes. Different scenarios are analyzed and a detailed comparison of preliminary laboratory tests and some selected simulations are presented.
The laboratory experiments show that suspended sediment transport and deposition are determined by the initial flow pattern and by the upstream and downstream boundary conditions. In the experiments, deposition in the rectangular basin systematically developed along the left bank, although inflow and outflow were positioned symmetrically along the centre of the basin. Three major horizontal eddies developed influencing the sediment deposition pattern. Although asymmetric flow patterns are privileged, a symmetric pattern can appear from time to time. This particular behaviour could also be reproduced by a two-dimensional depth-averaged flow and sediment transport model (CCHE2D). The paper presents numerical simulations using different turbulence closure schemes (k-ε and eddy viscosity models). In spite of the symmetric setup, these generally produced an asymmetric flow pattern that can easily switch sides depending on the assumptions made for the initial and boundary conditions. When using the laboratory experiment as a reference, the most reliable numerical results have been obtai  相似文献   
996.
月球、小行星等无大气行星体具有独特的反射光谱太空风化改造特征,其成因主要被归结于纳米级—亚微米级不透明颗粒等太空风化特征产物.本研究结合Apollo 返回月壤样品、普通球粒和碳质球粒陨石样品的模拟实验结果,综合分析了太空风化特征产物的来源和成因,并讨论了其可能的光谱效应.研究结果表明,np-Fe0 (纳米级单质金属铁)...  相似文献   
997.
Laboratory experiments were conducted at two institutes to reveal the relationship between acoustic backscatter strength and suspended sediment concentration (SSC). In total, three acoustic Doppler velocimeters (ADVs) with different frequencies (5, 10 and 16 MHz) were tested. Two different commercial clays and one natural sediment from Clay Bank site in the York River were checked for acoustic responses. The SSCs of selected sediments were artificially changed between a selected low and a high value in tap or de-ion water. Each ADV showed quite different backscatter responses depending on the sediment type and SSC. Not all devices had a good linear relationship between backscatter strength and SSC. Within a limited range of SSC, however, the backscatter strength can be well correlated with the SSC. Compared with optical backscattering sensor (OBS), the fluctuation of ADV backscatter signals was too noisy to be directly converted to the instantaneous changes of SSC due to high amplification ratio and small sampling volume. For the more accurate signal conversion for finding the fluctuation of SSC, the ensemble average should be applied to increase the signal-to-noise ratio. There are unexpected responses for the averaged backscatter wave strength: (1) high signals from small particles but low signals from large particles; and (2) two linear segments in calibration slope. These phenomena would be most likely caused by the different gain setting built in ADVs. The different acoustic responses to flocculation might also contribute somewhat if flocs are tightly packed. This study suggests that an ADV could be a useful instrument to estimate suspended cohesive sediment concentration and its fluctuation if the above concerns are clarified.  相似文献   
998.
利用"9210"系统下发的FY-2C图像资料数字化信息,依据高云、中云、低云在可见光波段和红外波段具有不同的光谱特性,结合水汽通道和红外通道对密蔽云系的辐射特性,分析了2008年华南低温雨雪冰冻期间红外、水汽、可见光3个通道云系的辐射特征,发现了有利于识别水云、冰云和冰水混合云的方法。同时指出,对于密蔽云系,当水汽亮温值大于0℃而红外亮温值小于0℃时,云顶粒子的热力学相态为过冷却液态水的可能性大于冰晶结构的可能性。根据上述辐射特性分析制定了云类的识别方法。实例分析结果表明这种方法能较好地分离出易产生冻雨的云体中缺少成冰核的过冷却液态水云。  相似文献   
999.
成都市大气可吸入颗粒物来源解析研究   总被引:7,自引:2,他引:7  
通过对成都市能源结构及产业布局的分析,对可吸入颗粒物来源进行了定性识别和分类,确定了对可吸入颗粒物可能产生贡献的源类的化学成分谱,用化学质量平衡受体模型(CMB)对成都市可吸入颗粒物的来源进行定量解析,确定了成都市PM10的主要来源。  相似文献   
1000.
借助稀释通道采样系统,采集了5种民用煤(3种块煤、1种蜂窝煤和1种煤球)燃烧排放的PM2.5和单颗粒样品.利用ICP-MS分析了PM2.5中16种金属元素(Mg、Al和K 3种轻金属;V、Cr、Mn、Fe、Co、Ni、Cu、As、Rb、Sr、Cd、Ba和Bi共13种重金属)的含量,并运用TEM和SEM-EDX研究了燃煤...  相似文献   
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