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Material flammability in space exploration atmospheres.

机译:太空探索环境中的材料易燃性。

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In order to reduce the risk of decompression sickness associated with extravehicular activity, NASA is designing the next generation of exploration vehicles with a different cabin pressure and oxygen concentration than used previously. This work explores how the flammability of solid materials changes in this new environment. One method to evaluate material flammability is by its ease of ignition. To this end, piloted ignition delay tests were conducted in a small-scale wind tunnel subject to this new space exploration atmosphere (SEA -- 58.6 kPa and 32% oxygen) and compared to similar tests in standard atmospheric conditions. In these tests, polymethylmethacylate (PMMA) was exposed to a range of oxidizer flow velocities and externally applied heat fluxes. It was found that the ignition time was reduced by 27% in the intended space exploration atmosphere. It was also noted that the critical heat flux for ignition decreases in exploration atmospheres. These results show that materials are more susceptible to ignition than in current spacecraft atmospheres.;To further explore the effect of pressure and oxygen concentration, tests were performed for a wide range of pressures and oxygen concentrations. In all oxygen concentrations tested, the ignition delay time was seen to decrease with pressure, reach a minimum, and then increase with further reduction in pressure creating a classic u-shaped curve. No ignition was seen at sufficiently low pressures. The no ignition pressure depended on the oxygen concentration. Increasing the oxygen concentration uniformly decreases the ignition time; however, no significant differences were seen in oxygen concentrations above 24%. These results indicate there are several competing mechanisms controlling the ignition time. By reducing the pressure, the heat transfer coefficient and the mass flow rate of fuel to reach the lean flammability limit are reduced. Conversely, a reduction in pressure increases the gas-phase chemical induction time. The competition between these three mechanisms is responsible for the u-shaped dependence of ignition time on total pressure. In addition to gaining insight into the effect of pressure on piloted ignition, these results have practical applications including high altitude structures and airplane cabins.
机译:为了降低与舱外活动有关的减压病的风险,美国宇航局正在设计下一代探空车,其探空压力和氧气浓度与以前的使用不同。这项工作探索了在这种新环境中固体材料的可燃性如何变化。一种评估材料可燃性的方法是其易燃性。为此,在这种新的太空探索气氛(SEA-58.6 kPa和32%的氧气)下,在小型风洞中进行了引燃延迟试验,并将其与标准大气条件下的类似试验进行了比较。在这些测试中,聚甲基丙烯酸甲酯(PMMA)暴露于一定范围的氧化剂流速和外部施加的热通量下。发现在预期的太空探索气氛中点火时间减少了27%。还应注意的是,在探索气氛中,用于点火的临界热通量降低。这些结果表明,与当前的航天器大气相比,材料更容易着火。;为了进一步探讨压力和氧气浓度的影响,对各种压力和氧气浓度进行了测试。在所有测试的氧气浓度中,点火延迟时间随压力而减小,达到最小值,然后随压力进一步降低而增加,从而形成经典的U形曲线。在足够低的压力下没有发现点火。无点火压力取决于氧气浓度。增加氧气浓度可均匀减少点火时间;然而,氧浓度高于24%时,没有发现显着差异。这些结果表明有几种竞争机制控制着点火时间。通过降低压力,降低了达到稀薄燃烧极限的燃料的传热系数和质量流率。相反,降低压力会增加气相化学诱导时间。这三种机制之间的竞争是点火时间对总压力呈U形依赖性的原因。除了深入了解压力对引燃的影响外,这些结果还具有实际应用,包括高空结构和飞机机舱。

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