共查询到20条相似文献,搜索用时 62 毫秒
1.
城市住宅电气设计中应注意的几个问题 总被引:3,自引:0,他引:3
在目前住宅电气应用的基础上,对影响住宅电气设计的因素,如负荷计算、供电系统、配电系统、弱电设计、插座布置等进行分析,从住宅电气设计角度提出提高住宅电气设计安全性和可靠性的技术措施。 相似文献
2.
3.
在目前住宅电气应用的基础上,对影响住宅电气设计的因素,如负荷计算、供电系统、配电系统、弱电设计、插座布置等进行分析,从住宅电气设计角度提出提高住宅电气设计安全性和可靠性的技术措施. 相似文献
4.
5.
6.
论文通过对重庆市现有住宅建筑的调查,对重庆市的住宅建筑节能状况和人们对住宅节能改造的看法和认可程度进行实地调研,得出需要改造的重庆市典型住宅的模型.为今后提供可实际操作的节能技术做基础资料,并为相关部门制定政策提供参考依据,为重庆市节能改造工作的进行提供建议和意见. 相似文献
7.
介绍目前多层及小高层钢结构住宅采用的几种典型的结构体系,总结各结构体系的受力特点及应用;通过对不同结构体系的分析比较,初步认为钢框架—支撑体系和钢框架—钢板剪力墙体系更适合8度抗震设防区Ⅲ类场地的多层及小高层钢结构住宅。 相似文献
8.
从新疆地区的住宅阳台近十多年的设计和使用状况分析,根据有关空间设计的原理,提出阳台设计和改造的思路。 相似文献
9.
《北华航天工业学院学报》2015,(5):23-24
本文采用市场分析、市场调查、市民问卷调查等形式,以武汉市地铁2号线为例,分析城市轨道交通对沿线居民住宅房地产价格的增值效应。通过分析发现:轨道交通沿线房地产价格的影响存在着一定的规律,通过对这一规律的深入研究,得出每靠近武汉地铁2号线100m将会产生24.1元/m2的增值的结论。 相似文献
10.
从新疆地区的住宅阳台近十多年的设计和使用状况分析,根据有关空间设计的原理,提出阳台设计和改造的思路. 相似文献
11.
12.
本文针对近期石油涨价以及全社会都在提倡节约的大气候,从现有能源的利用和新能源的开发两大方面谈能源合理利用与人类住区的可持续发展过程中应注意的问题,并提出相应的看法和建议。 相似文献
13.
为了给载人航天器乘员营造一个良好的生活工作环境,需要将众多空气环境参数控制在指标范围内。文章结合载人航天器专业知识,基于Modelica统一建模语言建立了一种载人航天器环热控系统仿真分析模型;利用该模型仿真分析了温湿度控制风机取不同转速时,载人航天器空气环境参数随乘员代谢水平的变化趋势。结果表明:在其他参数不变的情况下,温湿度控制风机转速越大,空气温度越低,相对湿度越高;乘员代谢水平变化对空气环境参数有显著影响,通过调节系统运行参数可将各空气参数有效控制在指标范围内。舱体温度与氧分压、二氧化碳分压、舱体相对湿度有密切关系且相互影响,不可单独分析。 相似文献
14.
Interactions of a cavity flameholder with an upstream injected jet in a Ma 2.52 supersonic flow are investigated numerically. A hybrid RANS/LES (Reynolds-Averaged Navier–Stokes/Large Eddy Simulation) method acting as wall-modeled LES is adopted, for which the recycling/rescaling method is introduced to treat the unsteady turbulent inflow. Patterns of the fluid entrainment into the cavity and escape from the cavity are identified using a scalar-tracing method. It is found that the jet–cavity interactions remarkably enhanced the mass exchange between the fluids in and out of the cavity, resulting in reduced residence time of the cavity fluids. Increasing the distance between the fuel injection and the cavity leading edge tends to attenuate the jet–cavity interactions, leading to weaker mass exchange. Raising the injection pressure appears to enhance the jet–cavity interactions, resulting in a shorter residence time of the cavity fluids. Moreover, the mass decay processes for the fuel and air within the cavity are basically the same while the entrainment processes for the fuel and air into the cavity seem quite different. 相似文献
15.
16.
17.
18.
19.
Sequin AM 《Acta Astronautica》2005,56(9-12):980-995
The human fascination with exploring and inhabiting the space that lies beyond Earth's atmosphere continues to grow. Nevertheless, 40 years of experience to date have clearly established that humans in outer space routinely suffer significant psychological impairment arising from their stressful extraterrestrial living conditions. This paper explores those extraterrestrial conditions through the interactions between the extraordinarily harsh environment of outer space, the sensations that humans encounter in space, and the qualities of a habitat that physically interposes itself between the two. The objective of this paper is to develop a habitat that expresses the extraterrestrial condition while supporting the mental health of its inhabitants, so as to augment the success of prolonged extraterrestrial residence and interplanetary travel. 相似文献
20.
A Kereszturi 《Astrobiology》2012,12(6):586-600
The astrobiological significance of certain environment types on Mars strongly depends on the temperature, duration, and chemistry of liquid water that was present there in the past. Recent works have focused on the identification of signs of ancient water on Mars, as it is more difficult to estimate the above-mentioned parameters. In this paper, two important factors are reviewed, the duration and the volume of water at different environment types on past and present Mars. Using currently available information, we can only roughly estimate these values, but as environment types show characteristic differences in this respect, it is worth comparing them and the result may have importance for research in astrobiology. Impact-induced and geothermal hydrothermal systems, lakes, and valley networks were in existence on Mars over the course of from 10(2) to 10(6) years, although they would have experienced substantially different temperature regimes. Ancient oceans, as well as water in outflow channels and gullies, and at the microscopic scale as interfacial water layers, would have had inherently different times of duration and overall volume: oceans may have endured from 10(4) to 10(6) years, while interfacial water would have had the smallest volume and residence time of liquid phase on Mars. Martian wet environments with longer residence times of liquid water are believed to have existed for that amount of time necessary for life to develop on Earth between the Late Heavy Bombardment and the age of the earliest fossil record. The results of this review show the necessity for more detailed analysis of conditions within geothermal heat-induced systems to reconstruct the conditions during weathering and mineral alteration, as well as to search for signs of reoccurring wet periods in ancient crater lakes. 相似文献