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Relation between cooling rates and microstructures in gravity-die-cast AZ91D disks

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Abstract

In-die temperature measurements during the casting of 3.5- and 11.7-mm-thick disks in metal dies at 100 °C, 200 °C, and 400 °C enables calculation of the heat flux from the casting to the die as a function of the casting parameters. Using the flux so determined, the temperature field in the plates could be calculated in agreement with measured values. Increasing preheating temperatures reduced the heat flux, which extended the local solidification time and coarsened the structure. Directional solidification, from the wall of the die to the center of the disk, took place only when casting a thin disk in a die at 400 °C, because of the combination of low undercooling (which prevents homogeneous nucleation) and a sufficiently steep temperature gradient at the solidification front to ensure directional growth. A relatively long residence time at the high temperature, as occurs during casting in a die at 400 °C, leads to a more-uniform distribution of the Al, due to diffusion in the solid, and prevents the divorced eutectic, distinct from that obtained at slow solidification, of the AZ91D ingot.

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Avishei, A., Bamberger, M. Relation between cooling rates and microstructures in gravity-die-cast AZ91D disks. Metall Mater Trans B 30, 723–729 (1999). https://doi.org/10.1007/s11663-999-0034-5

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  • DOI: https://doi.org/10.1007/s11663-999-0034-5

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