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Microstructural Evolution and Age Hardening in Aluminium Alloys ...

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<strong>Microstructural</strong> <strong>Evolution</strong> <strong>in</strong> <strong>Age</strong>d Al <strong>Alloys</strong> 107(100} Sn // {111} <strong>and</strong> [010 Sn // 112 [45].[Mixed notation <strong>in</strong>dices are used to representplanes (hkl} <strong>and</strong> directions [uvw oftetragonal structures.] Figure 5 shows themicrostructure after 1 h at 190C, where it isseen that precipitates were often foundassociated with these particles, suggest<strong>in</strong>gthat they had provided sites at which heterogeneousnucleation of could occur. TheSn particles appeared to be <strong>in</strong>coherent withthe Al matrix, because they were visibleonly through diffraction <strong>and</strong> structure factorcontrast, <strong>and</strong> no stra<strong>in</strong> was observedunder two-beam conditions. The Sn particlesare <strong>in</strong> contact with the narrow, noncoherentplanes of . Further 1DAP analysesrevealed that Sn was not segregated to the/matrix <strong>in</strong>terfaces either across the coherentbroad face of the plate or across therim or edge. These results support the proposalby Kanno et al. [41–43] that Sn (Cd orIn) facilitates precipitation of at elevatedtemperatures by provid<strong>in</strong>g heterogeneousnucleation sites. The rapid cluster<strong>in</strong>g <strong>and</strong>precipitation of Sn <strong>in</strong> this alloy has been expla<strong>in</strong>ed<strong>in</strong> terms of evidence for a preferredSn–vacancy <strong>in</strong>teractions dur<strong>in</strong>g, or immediatelyfollow<strong>in</strong>g, quench<strong>in</strong>g, <strong>and</strong> the factthat the diffusion rate of Sn <strong>in</strong> Al may exceedthat of Cu by at least two orders ofmagnitude [45].Figure 6(a) shows an FIM micrograph ofa general high-angle gra<strong>in</strong> boundary <strong>in</strong> theAl–1.7Cu–0.01Sn alloy follow<strong>in</strong>g ag<strong>in</strong>g 3m<strong>in</strong> at 200C. Figure 6(b) shows an <strong>in</strong>tegratedconcentration–depth profile acrossthe gra<strong>in</strong> boundary. The <strong>in</strong>tragranular concentrationof Cu determ<strong>in</strong>ed from this datais significantly larger than the equilibriumsolid solubility (0.1 at. %), <strong>and</strong> this is consistentwith the observation that is <strong>in</strong> theearly stages of precipitation. However, aCu–solute-depleted region is evident <strong>in</strong> theregion of the gra<strong>in</strong> boundary, <strong>and</strong> there isno evidence of Sn segregation <strong>in</strong> theboundary. The solute depleted region wasestimated to be 10nm thick. Narrow precipitatefree zones (PFZ) approximately0.1m either side of the boundaries, to-FIG. 4. (a) Field ion micrograph (He) from the Al–1.7Cu–0.01Sn alloy aged at 190C, 3 m<strong>in</strong>. The 1DAP results<strong>in</strong> (b) <strong>in</strong>dicate that the brightly imag<strong>in</strong>g regionsare Cu-rich nuclei, heterogeneously nucleated on Snparticles. After R<strong>in</strong>ger et al. [45].FIG. 5. Transmission electron micrograph of the Al–1.7Cu–0.01Sn alloy follow<strong>in</strong>g ag<strong>in</strong>g for 1 h at 190C. Af<strong>in</strong>e <strong>and</strong> uniform dispersion of precipitates is seen,which are nucleated on spherical Sn particles (arrowed).After R<strong>in</strong>ger et al. [45].

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