Please use this identifier to cite or link to this item: http://hdl.handle.net/10397/108056
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Title: Flame spread over polyethylene film : effects of gravity and fuel inclination
Authors: Zhu, F
Huang, X 
Wang, S
Issue Date: Jun-2022
Source: Microgravity science and technology, June 2022, v. 34, no. 3, 26
Abstract: The flammable thermoplastics are widely used in our daily life and manned space travels in microgravity, posing a potential fire risk. This work studies the flame spread along with the thin polyethylene (PE) film (15–100 µm) in the microgravity drop tower and normal gravity. Microgravity flame spread faster than vertically downward flame spread in normal gravity due to the weak buoyancy flow and greater flame preheating length. For the ultra-thin film, the influence of melting on the opposed flame spread is negligible. The upward flame spread rate reaches a maximum constant (45 ± 10 mm/s for 20 μm film) when the inclination angle is larger than 30°, due to the dripping removal of molten fuel. The upward flame spread rate changes under the competition between the enhanced flame heating by buoyancy and the dripping removal of the molten fuel. The vertically upward spreading flame cannot be maintained due to the dripping removal of the molten fuel, and a critical extinction condition was determined and analyzed. This work provides valuable data on flame dynamics in plastic films and can help develop more sophisticated material flammability tests for fire safety in space travel.
Keywords: Extinction
Flame spread
Inclination angle
Microgravity combustion
PE
Publisher: Springer Dordrecht
Journal: Microgravity science and technology 
ISSN: 0938-0108
EISSN: 1875-0494
DOI: 10.1007/s12217-022-09945-4
Rights: © The Author(s), under exclusive licence to Springer Nature B.V. 2022
This version of the article has been accepted for publication, after peer review (when applicable) and is subject to Springer Nature’s AM terms of use (https://www.springernature.com/gp/open-research/policies/accepted-manuscript-terms), but is not the Version of Record and does not reflect post-acceptance improvements, or any corrections. The Version of Record is available online at: http://dx.doi.org/10.1007/s12217-022-09945-4.
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