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Microstructure Analysis Of Directionally Solidified Aluminum Alloy Aboard The International Space Station

机译:国际空间站定向凝固铝合金的显微组织分析

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摘要

This thesis entails a detailed microstructure analysis of directionally solidified (DS) Al-7Si alloys processed in microgravity aboard the International Space Station and similar duplicate ground based experiments at Cleveland State University. In recent years, the European Space Agency (ESA) has conducted experiments on alloy solidification in microgravity. NASA and ESA have collaborated for three DS experiments with Al- 7 wt. % Si alloy, aboard the International Space Station (ISS) denoted as MICAST6, MICAST7 and MICAST12. The first two experiments were processed on the ISS in 2009 and 2010. MICAST12 was processed aboard the ISS in the spring of 2014; the resulting experimental results of MICAST12 are not discussed in this thesis. The primary goal of the thesis was to understand the effect of convection in primary dendrite arm spacings (PDAS) and radial macrosegregation within DS aluminum alloys. The MICAST experiments were processed with various solidification speeds and thermal gradients to produce alloy with differences in microstructure features. PDAS and radial macrosegregation were measured in the solidified ingot that developed during the transition from one solidification speed to another. To represent PDAS in DS alloy in the presence of no convection, the Hunt-Lu model was used to represent diffusion-controlled growth. By sectioning cross-sections throughout the entire length of solidified samples, PDAS was measured and calculated. The ground-based (1-g) experiments done at Cleveland State University CSU were also analyzed for comparison to the ISS experiments (0-g). During steady state in the microgravity environment, there was a reasonable agreement between the measured and calculated PDAS. In ground-based experiments, transverse sections exhibited obvious radial macrosegregation caused by thermosolutal convection resulting in a non-agreement with the Hunt- Lu model. Using a combination of image processing techniques and Electron Microprobe Analysis, the extent of radial macrosegregation was found to be a function of processing conditions and PDAS.
机译:本文需要对国际空间站微重力下定向凝固的(DS)Al-7Si合金进行详细的显微组织分析,并在克利夫兰州立大学进行类似的基于地面的重复实验。近年来,欧洲航天局(ESA)进行了微重力下合金凝固的实验。美国宇航局(NASA)和欧洲航天局(ESA)合作进行了3次Al-7重量比DS实验。在国际空间站(ISS)上以MICAST6,MICAST7和MICAST12表示的%Si合金。前两个实验分别在2009年和2010年在ISS上进行。MICAST12在2014年春季在ISS上进行了处理;本文不讨论MICAST12的实验结果。本文的主要目的是了解对流对DS铝合金内部主要枝晶臂间距(PDAS)和径向宏观偏析的影响。 MICAST实验采用各种凝固速度和热梯度进行处理,以生产出具有不同微观组织特征的合金。在从一种凝固速度向另一种凝固速度转变的过程中,在凝固的铸锭中测量了PDAS和径向宏观偏析。为了在不存在对流的情况下代表DS合金中的PDAS,使用Hunt-Lu模型来代表扩散控制的生长。通过在整个固化样品的整个长度上截取横截面,可以测量和计算PDAS。还分析了在克利夫兰州立大学CSU进行的地面(1-g)实验,以与ISS实验(0-g)进行比较。在微重力环境下的稳定状态下,实测和计算的PDAS之间存在合理的一致性。在基于地面的实验中,横截面表现出明显的径向宏观偏析,这是由热固对流引起的,导致与Hunt-Lu模型不一致。通过结合使用图像处理技术和电子微探针分析,发现径向宏观偏析的程度是处理条件和PDAS的函数。

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    Angart Samuel Gilbert;

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  • 年度 2015
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