首页> 外文会议>International astronautical congress >THE INFLUENCE OF BUOYANCY ON EQUIAXED GRAIN NUCLEATION AND GROWTH CHARACTERISTICS AS OBSERVED VIA IN SITU X-RADIOGRAPHY OF AL-CU ALLOYS
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THE INFLUENCE OF BUOYANCY ON EQUIAXED GRAIN NUCLEATION AND GROWTH CHARACTERISTICS AS OBSERVED VIA IN SITU X-RADIOGRAPHY OF AL-CU ALLOYS

机译:浮力对Al-Cu合金原位X射线照相法观察到的均匀晶粒成核和生长特性的影响

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Laboratory-based near-isothermal solidification experiments were performed on a number of Al-Cu alloys utilising in situ real-time X-radiography. These experiments were carried out in preparation for an upcoming sub-orbital microgravity solidification experiment on board the European Space Agency Sounding Rocket, MASER 13, with a view to quantifying the buoyancy effects on solidification dynamics within the sample cell. A number of thin (200 urn) Al-Cu samples, of varying copper concentrations and Al-5Ti-lB (wt%) grain refiner addition levels, were solidified near-isothermally at constant cooling rates in the range 0.025 to 0.5 K/s, thereby promoting equiaxed solidification within the X-ray field-of-view (FOV). To control the effect of gravity-induced equiaxed grain buoyancy, the X-ray FOV was oriented both perpendicular and parallel to the gravity vector, with the latter case exhibiting solidification dynamics similar to those observed under normal casting conditions. In the former case, however, with gravity acting along the thin dimension of the sample, macro-scale equiaxed grain buoyancy was largely eliminated from the FOV, providing solidification conditions similar to those observed under microgravity conditions. It was observed that, using a combination of low cooling rates and inoculant addition levels, equiaxed grain buoyancy caused a significant reduction in the final grain size due to early grain coherency resulting in a cessation of primary growth. Higher inoculant addition levels caused an increase in the grain density, resulting in a lower sensitivity to cooling rate, along with a morphological change from dendritic to cellular-equiaxed.
机译:利用原位实时X射线照相技术对许多Al-Cu合金进行了基于实验室的近等温凝固实验。进行这些实验是为了在欧洲航天局探测火箭MASER 13上为即将进行的亚轨道微重力凝固实验做准备,以量化浮力对样品池内凝固动力学的影响。在0.025至0.5 K / s的恒定冷却速率下,将近乎等温地固化了许多不同铜浓度和Al-5Ti-1B(wt%)晶粒细化剂添加量的薄(200 urn)Al-Cu样品,从而促进X射线视场(FOV)内的等轴凝固。为了控制重力引起的等轴晶粒浮力的影响,X射线视场的方向垂直于重力矢量,也平行于重力矢量,后一种情况下的凝固动力学类似于在常规铸造条件下观察到的凝固动力学。但是,在前一种情况下,由于重力沿样品的薄尺寸作用,因此从FOV中大大消除了宏观等轴晶浮力,从而提供了与在微重力条件下观察到的凝固条件相似的凝固条件。观察到,结合使用低冷却速率和孕育剂添加量,由于早期晶粒的连贯性,等轴晶粒的浮力导致最终晶粒度显着减小,从而导致初级生长的停止。较高的孕育剂添加量会导致晶粒密度增加,从而导致对冷却速率的敏感性降低,以及从树突状到细胞平衡的形态变化。

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