Use of Engineering Methods in Assessment Ventilation of Protected Fire Escape Routes

2021 ◽  
Vol 109 ◽  
pp. 67-72
Author(s):  
Petra Okřinová ◽  
Ondřej Pilný

The design of protected fire escape routes is a process in which a number of technical aspects that are set by Czech technical standards must be considered. The assessment of protected fire escape route's ventilated premises is subject to strict values, which when designed, or when created additionally, often force us to resort to specific measures, like a forced ventilation, enlargement of openings, which leads to expensive construction. This paper focuses on the use of so-called engineering methods to solve this problem, specifically the computational fluid dynamics method, which finds application in the revalidation of otherwise unmet ventilation criteria.

2013 ◽  
Vol 662 ◽  
pp. 586-590
Author(s):  
Gang Lu ◽  
Qing Song Yan ◽  
Bai Ping Lu ◽  
Shuai Xu ◽  
Kang Li

Four types of Super Typhoon drip emitter with trapezoidal channel were selected out for the investigation of the flow field of the channel, and the CFD (Computational Fluid Dynamics) method was applied to simulate the micro-field inside the channel. The simulation results showed that the emitter discharge of different turbulent model is 4%-14% bigger than that of the experimental results, the average discharge deviation of κ-ω and RSM model is 5, 4.5 respectively, but the solving efficiency of the κ-ω model is obviously higher than that of the RSM model.


2021 ◽  
Vol 159 ◽  
pp. 106990
Author(s):  
Wanfu Zhang ◽  
Kexin Wu ◽  
Chengjing Gu ◽  
Haoyang Tian ◽  
Xiaobin Zhang ◽  
...  

2010 ◽  
Vol 439-440 ◽  
pp. 880-883
Author(s):  
Fu Zhao ◽  
Ping Wang ◽  
Yan Jue Gong ◽  
Yu De Liu ◽  
Hong Bin Xin

With the three-dimensional computational fluid dynamics method, the airflow effects over the huge telescope assemble is investigated in this article. The distributing of velocity field and natural convection are studied by modeling and simulating the turbulent airflow of the huge telescope. Numerical simulations show the best observation direction is the 90o angle between the main optics axis and the horizontal line in which the air velocity distribution is the least. And the air temperature distribution and uniformity around the telescope are also provided by simulation.


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