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Assessment of Microbiologically Influenced Corrosion Potential in the International Space Station Internal Active Thermal Control System Heat Exchanger Materials: A 6-Month Study

机译:在国际空间站内部积极热控制系统热交换器材料中评估微生物学影响腐蚀潜力:6个月的研究

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The fluid in the Internal Active Thermal Control System (IATCS) of the International Space Station (ISS) is water based. The fluid in the ISS Laboratory Module and Node 1 initially contained a mix of water, phosphate (corrosion control), borate (pH buffer), and silver sulfate (Ag{sub}2SO{sub}4) (microbial control) at a pH of 9.5±0.5. Over time, the chemistry of the fluid changed. Fluid changes included a pH drop from 9.5 to 8.3 due to diffusion of carbon dioxide (CO{sub}2) through Teflon (DuPont) hoses, increases in dissolved nickel (Ni) levels, deposition of silver (Ag) to metal surfaces, and precipitation of the phosphate (PO{sub}4) as nickel phosphate (NiPO{sub}4). The drop in pH and unavailability of an antimicrobial has provided an environment conducive to microbial growth. Microbial levels in the fluid have increased from <10 colony-forming units (CFUs)/100 mL to 10{sup}6 CFUs/100 mL. The heat exchangers in the IATCS loops are considered the weakest point in the loop because of the material thickness (is approximately equal to 7 mil). It is made of a Ni-based braze filler/CRES 347. Results of a preliminary test performed at Hamilton Sundstrand indicated the possibility of pitting on this material at locations where Ag deposits were found. Later tests confirmed that corrosion of the heat exchanger material is a concern for this system. Accumulation of microorganisms on surfaces (biofilm) can also result in material degradation. This is known as microbiologically influenced corrosion (MIC). MIC can amplify the material damage caused by the exposure to the fluid. This paper will discuss the results of a 6-month test performed to characterize and quantify the damage from microbial accumulation on the surface of the ISS IATCS heat exchanger materials. The test was designed to quantify the damage to the materials under worst-case conditions with and without microorganisms present at pH 8.3 and 9.5.
机译:国际空间站(ISS)的内部有源热控制系统(IATCS)中的液体是水基。 ISS实验室模块和节点1中的流体最初含有水,磷酸盐(腐蚀控制),硼酸盐(pH缓冲液)和硫酸银(Ag {sub} 2SO} 4)(微生物对照)的混合物9.5±0.5。随着时间的推移,流体的化学改变。由于二氧化碳(Co {Sub} 2)扩散通过Teflon(DuPont)软管,溶解镍(Ni)水平的增加,将流体变化从9.5至8.3增加,溶解镍(Ni)水平增加,银(Ag)沉积到金属表面,磷酸盐(PO {Sub} 4)作为磷酸镍(NIPO {Sub} 4)沉淀。抗菌剂的pH和不可用的下降提供了一种有利于微生物生长的环境。流体中的微生物水平从<10个菌落 - 形成单位(CFU)/ 100ml至10 {sup} 6 cfus / 100ml增加。由于材料厚度(大约等于7密耳),IATCS环中的热交换器被认为是环路中的最弱点。它由基于Ni的钎焊填料/ CRES 347制成。在Hamilton Sundstrand中进行的初步试验结果表明在发现Ag沉积物的位置处的这种材料蚀的可能性。后来的试验证实,热交换器材料的腐蚀是该系统的关注。在表面上的微生物(生物膜)的积累也会导致物质降解。这被称为微生物学过腐蚀(MIC)。 MIC可以放大由暴露于流体引起的材料损伤。本文将讨论进行6个月试验的结果,以表征和量化在IS IATCS热交换器材料表面上的微生物积累损伤。该测试旨在在最坏情况下对材料的损坏量化,在pH 8.3和9.5的含有微生物,没有微生物。

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