脉冲等离子法烟气脱硫的放大实验

锅炉烟气进行脉冲等离子法脱硫的扩大实验，得到与模拟烟气实验相近的结果。研究表明，脉冲等离子法对锅炉烟气中的ＳＯ２去除率可达９５％以上，烟气在反应器内的停留时间（ｔｓ）、脉冲电源的放电功率（Ｐ）和添加ＮＨ３等条件，对脱硫效率９η）有较大影响。ｔｓ、Ｐ越大、η越高。处理烟气量（Ｑ）、能耗（Ｐ）与η存在函数关系：η＝１１８．０（Ｐ／Ｑ）＾０．１１１１。烟气中加入适量ＮＨ３，对脱硫效率有显著提高，以ＮＨ３     

高强铝合金超塑挤压成形

主要介绍了工业牌号高强铝合金在供应态或经简单预处理后在通用油压机上超塑成形的实例,并分析探讨了非理想组织材料超塑成形中微观组织的变化。     

Purification and reclamation of wastewater by an integrated biological pond system

ＰｕｒｉｆｉｃａｔｉｏｎａｎｄｒｅｃｌａｍａｔｉｏｎｏｆｗａｓｔｅｗａｔｅｒｂｙａｎｉｎｔｅｇｒａｔｅｄｂｉｏｌｏｇｉｃａｌｐｏｎｄｓｙｓｔｅｍＷｕＺｈｅｎｂｉｎ；ＸｉａＹｉｃｈｅｎｇ；ＺｈａｎｇＹｏｎｇｙｕａｎ；ＤｅｎｇＪｉａｑｉ；ＣｈｅｎＸｉｔａ...     

The research of below-cloud scavengingof rainwater in Guilin City

Ｔｈｅｒｅｓｅａｒｃｈｏｆｂｅｌｏｗ－ｃｌｏｕｄｓｃａｖｅｎｇｉｎｇｏｆｒａｉｎｗａｔｅｒｉｎＧｕｉｌｉｎＣｉｔｙＢａｉＹｕｈｕａ；ＹａｏＲｏｎｇｋｕｉ；ＬｉＸｉｎ；ＴａｎｇＸｉａｏｙａｎ（ＴｈｅＤｅｐａｒｔｍｅｎｔｏｆＴｅｃｈｎｉｃａｌＰｈｙｓｉｅ...     

大气污染物排放系数及计算方法

在我国排放大气污染物许可证试点工作中,需要确定污染物排放量,以达到总量控制之目的,利用排放系数可以估算各污染源的排放置。本文介绍了有色冶炼,化工制酸排放SO_2,水泥生产中排放粉尘及钢铁工业排放烟尘的排放系数及计算方法。     

随机模拟在常州运河水质规划中的应用

以常州运河的水质规划为实例,讨论了确定性水质模型的随机模拟。讨论中引进了主观概率和客观概率的概念,用泰勒级数确定客观概率分布,用可能最大机率法估计主观概率分布,并给出了在实施不同规划方案时的水质概率曲线和水质达标的保证率。计算结果表明,使水质恶化的各种随机因素的作用不容忽视,各种水污染治理措施只能降低水质超标的风险水平。     

大气污染对儿童唾液溶菌酶含量的影响

本文分析了重庆市大气污染(SO_2、NO_x、TSP)的特征,报导重污染区儿童唾液溶菌酶含量明显低于相对污染区(P<0.00001),污染区儿童体内免疫功能下降;发现暴露于两种或两种以上因素(酸沉降物、被动吸烟、燃煤)时,对儿童唾液溶菌酶含量的影响远大于它们单一因素的作用(P<0.00001),经逐步回归分析,得Y=401.6869-68.1306X_5-42.3868X_1-20.8466X_4(r=0.7681,F值=185.08,P<0.00001);并针对重庆市大气污染的具体情况,提出一些有意义的建议措施。     

医用射线装置对环境辐射水平的影响

调查了上海市7家医院50余台x、γ射线装置,监测了工作环境和公众环境的辐射水平,并根据辐射防护规定进行评价。调查发现,由于少数设备老化,或防护门窗安装不当等,造成了环境剂量的增加。     

Atmospheric pollution in Beijing, China, as recorded in sediments of the Kunming Lake

The fluxes of heavy metals and magnetite, a fly-ash component, from coal burning, to sediments of the Kunming Lake in Beijing have increased measurably over the last fifty years. Ages were introduced to the sediment strata through Pb-210 geochronologies. Even with a doubling of coal usage by the year 2000, the anthropogenic metal fluxes will still be less than those recorded in metropolitan Tokyo and U.S. lakes.     

The nature of the redshift and directly observed quasar statistics

The nature of the cosmic redshift is one of the most fundamental questions in modern science. Hubble's discovery of the apparent Expansion of the Universe is derived from observations on a small number of galaxies at very low redshifts. Today, quasar redshifts have a range more than 1000 times greater than those in Hubble's sample, and represent more than 100 times as many objects. A recent comprehensive compilation of published measurements provides the basis for a study indicating that quasar observations are not in good agreement with the original predictions of the Expanding Universe theory, but are well fit by the predictions of an alternative theory having fewer adjustable parameters.