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581.
Analysis of ion concentration of samples taken sequentially during a storm event is important in order to reveal the relation between the atmospheric conditions and ion concentrations in each sub-event. This study presents the interrelationship among the chemical composition parameters and atmospheric variables for four storm events that were sampled in Istanbul during a) January 21-23, 2004 b) November 9-11, 2003 c) February 12-13, 2004 and d) October 27-28, 2003. These events lasted 53.3, 47.9, 27.5 and 13.2 h and the number of collected samples for each event was 22, 14, 7 and 4, in order. Generally values of pH and concentrations of ions in the first sub-events for all four cases were found higher than those of the other sub-event samples taken in sequence owing to the strong initial washout of the atmosphere by raindrops. Precipitation events a and c include rain and snow together where precipitation started as rain and continued as snow after 16th and 3rd sub-events. Higher concentration of ions in the snow in comparison with that of rain sub-events samples can be explained by more efficient below cloud scavenging of atmospheric constituents, especially aerosol particles, by snowflakes. In general, all of the ions sampled in the sub-events for four storms have variability similar to each other, with high correlation coefficient among themselves. Cl(-) and SO(4)(2-) were found to be the dominant ions in average overall sub-events. Calculated NSS concentration values of ions indicated that the main source of SO(4)(2-) was industrial and domestic emissions, most of the Ca(2+) and K(+) came from soil, nearly half of the Mg(2+) and all of the Cl(-) originated from sea. 相似文献
582.
在分析吸附机理研究方法的基础上,提出了一种判别吸附机理与模型的新方法.从影响吸附的诸因素入手,用灰色关联分析方法计算了不同颗粒粒径(26.9~38.9 μm)、SOC(8.85~17.15mg/g)和CEC(12.49~38.74 cmol/kg)的6种土壤吸附菲的反应中,SOC、CEC及颗粒粒径对吸附量的影响.结果表明,各影响因素的重要性顺序为:颗粒粒径>SOC>CEC;表面吸附理论是土壤吸附菲的主要吸附机理,分配理论次之.还讨论了描述此反应的吸附模型,认为多端元反应模型能较好地解释土壤吸附菲的反应.最后得到了一种判定土壤对有机污染物吸附机理与模型的数学方法,对机理研究有一定的指导意义. 相似文献
583.
A knowledge of the ignition properties of ammonia (NH)/hydrogen (H) mixtures is important because of their abundance in chemical engineering processes, and also because of their prospective role as fuels in future energy systems. In particular, the question arises if and how important characteristics like ignition limits and minimum ignition energies in NH/H mixtures are related to the physical conditions. To address this question, this work studies ignition process in ammonia/hydrogen mixtures by numerical simulations. These track the evolution of ammonia/hydrogen mixtures during and after the deposition of a certain ignition energy, using a detailed treatment of chemical reactions and molecular transport. Studies on the influence of different system parameters on the minimally required ignition energy are performed. These are the strain rate, hydrogen content, pressure and initial (pre-ignition) temperature. Significant findings include a quasi-linear correlation between the transition strain rate, defined as the strain rate below which no external energy is required to initiate successful ignition (auto-ignition) and a characteristic reaction rate, defined as the inverse of ignition delay time in homogeneous, quiescent mixtures. Also, the relative decay of minimum ignition energy with increasing hydrogen content is less pronounced for higher pressures. Analysis of the results supports a knowledge-based approach towards fail-proof ignition devices and reliable prevention of hazards. The simulations are used for assessing the ignitability of ammonia and its mixtures with hydrogen. 相似文献
584.