Effect of monoammonium phosphate particle size on flame propagation of aluminum dust cloud

2019 ◽  
Vol 60 ◽  
pp. 311-316 ◽  
Author(s):  
Haipeng Jiang ◽  
Mingshu Bi ◽  
Wei Gao

The mechanism and the rate of flame propagation through dust clouds of carbon, coal, aluminium and magnesium have been investigated. Any errors due to the upward buoyant motion of burnt gases and the downward settling velocity of dust particles were eliminated by conducting these experiments in a zero-gravity environment. A technique of flat-flame propagation was developed to measure the burning velocity accurately. The results show that the burning velocity is influenced by particle size, fuel transfer number, dust concentration, volatile matter (for coal), oxygen enrichment and heat loss by radiation from the burning fuel particles. A simple model to elucidate the structure and the mechanism of flame propagation is developed. Then expressions to predict the flame thickness and the burning velocity are derived. Attention is drawn to the similarity that exists between the mechanisms of flame propagation through dust clouds and through fuel mists. The importance of radiation heat loss is emphasized. It is shown that for a dust cloud of particle size 10 μ m of graphite or aluminium in oxygen, radiation loss from particles can reduce the burning velocity by as much as 40% or 25% respectively.


2013 ◽  
Vol 26 (4) ◽  
pp. 862-868 ◽  
Author(s):  
Mehdi Bidabadi ◽  
Saeedreza Zadsirjan ◽  
Seyed Alireza Mostafavi

2019 ◽  
Vol 101 ◽  
pp. 209-216 ◽  
Author(s):  
Lei Pang ◽  
Ran Ma ◽  
Shoutao Hu ◽  
Pengfei Lv ◽  
Kai Yang
Keyword(s):  

2020 ◽  
Vol 67 ◽  
pp. 104244
Author(s):  
Chen Yue ◽  
Wang Yujie ◽  
Wei Zhang ◽  
Beini Zhang ◽  
Ying Zhang ◽  
...  

2017 ◽  
Vol 317 ◽  
pp. 197-208 ◽  
Author(s):  
Xinyan Zhang ◽  
Jianliang Yu ◽  
Wei Gao ◽  
Dawei Zhang ◽  
Jinhua Sun ◽  
...  

Energies ◽  
2019 ◽  
Vol 12 (20) ◽  
pp. 3807 ◽  
Author(s):  
Junfeng Wang ◽  
Yansong Zhang ◽  
Huifeng Su ◽  
Jinshe Chen ◽  
Bo Liu ◽  
...  

Coal and oil shale are often mined and utilized together, and mixed dust is easily formed in these processes. In order to ensure safe production in these processes, the explosion characteristics of mixed dust were studied. Using a Godbert-Greenwold (G-G) Furnace experimental device, Hartmann tube experimental device, and 20 L explosion vessel, the oil shale and coal mixed dust ignition sensitivity experiment, flame propagation experiment, and explosion characteristics experiment were carried out. The minimum ignition temperature (MIT), minimum ignition energy (MIE), maximum explosion pressure (Pmax), maximum rate of pressure rise ((dp/dt)max), and explosibility index (KSt) parameters and the flame propagation behavior of the mixed dust were analyzed in detail. A scanning electron microscope (SEM) analysis of the coal and oil shale dust before and after the explosion was carried out to study the changes in the microscopic morphology of the dust particles. The results show that due to the oil shale having a high volatile content and low moisture content, in the mixture, the greater the percentage of oil shale, the more likely the dust cloud is to be ignited and the faster the explosion flame is propagated; the greater the percentage of oil shale, the greater the (dP/dt)max and KSt will be and, under a high dust concentration, a greater Pmax will be produced. During explosion, coal dust will experience particle pyrolysis and the gas phase combustion of the volatile matter, followed by solid phase combustion of coal char, whereas oil shale dust will only experience particle pyrolysis and the gas phase combustion of the volatile matter.


2016 ◽  
Author(s):  
Michèlle van der Does ◽  
Laura F. Korte ◽  
Chris I. Munday ◽  
Geert-Jan A. Brummer ◽  
Jan-Berend W. Stuut

Abstract. Mineral dust has a large impact on regional and global climate, depending on its particle size. Especially in the Atlantic Ocean downwind of the Sahara, the largest dust source on earth, the effects can be substantial but are poorly understood. This study focuses on seasonal and spatial variations in particle size of Saharan dust deposition across the Atlantic Ocean, using an array of submarine sediment traps moored along a transect at 12˚ N. We show that the particle size decreases downwind with increased distance from the Saharan source, due to higher gravitational settling velocities of coarse particles in the atmosphere. Modal grain sizes vary between 4 and 33 μm throughout the different seasons and at five locations along the transect. This is much coarser than previously suggested and incorporated into climate models. In addition, seasonal changes are prominent, with coarser dust in summer, and finer dust in winter and spring. Such seasonal changes are caused by transport at higher altitudes and at greater wind velocities during summer than in winter. Also the latitudinal migration of the dust cloud, associated with the Intertropical Convergence Zone, causes seasonal differences in deposition as the summer dust cloud is located more to the north, and more directly above the sampled transect. Furthermore, increased precipitation and more frequent dust storms in summer coincide with coarser dust deposition. Our findings contribute to understanding Saharan dust transport and deposition relevant for the interpretation of sedimentary records for climate reconstructions, as well as for global and regional models for improved prediction of future climate.


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