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Microstructural Evolution in a 17-4 PH Stainless Steel after Aging at ...

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Fe & Cr / <strong>at</strong>. %<br />

(a)<br />

(b)<br />

Ni<br />

Si<br />

Cu<br />

Cr<br />

Cu<br />

100<br />

80<br />

60<br />

40<br />

20<br />

0<br />

30<br />

15<br />

0<br />

30<br />

15<br />

0<br />

70<br />

50<br />

30<br />

10<br />

0<br />

~30nm<br />

0 5 10 15 20 25<br />

Depth / ~nm<br />

~9nm<br />

Fig. 7 3DAP elemental mapp<strong>in</strong>g of the martensite phase aged <strong>at</strong><br />

580°C for 4 h. (a) The phase decomposition <strong>in</strong>to Cr enriched and<br />

depleted region occur <strong>in</strong> the martensite phase. (b) F<strong>in</strong>e spherical<br />

Cu rich precipit<strong>at</strong>e. (c) Concentr<strong>at</strong>ion depth profile obta<strong>in</strong>ed from<br />

the selected region near the Cu precipit<strong>at</strong>e.<br />

is a typical fe<strong>at</strong>ure of sp<strong>in</strong>odal decomposition. The periodicity<br />

of the fluctu<strong>at</strong>ion is on the order of 3 nm. The<br />

Cu mapp<strong>in</strong>g shows th<strong>at</strong> Cu-enriched particles approxim<strong>at</strong>ely<br />

8 nm <strong>in</strong> diameter are present. In direct contact<br />

with one of the Cu particle, a Ni and Si enriched particle<br />

is observed as <strong>in</strong>dic<strong>at</strong>ed by an arrow <strong>in</strong> Figure<br />

10(b). Such f<strong>in</strong>e particles are always observed <strong>in</strong> contact<br />

with Cu precipit<strong>at</strong>es, and they are believed to be<br />

the G-phase based on the TEM observ<strong>at</strong>ion shown <strong>in</strong><br />

Figure 8. Figure 10 (c) shows concentr<strong>at</strong>ion depth profiles<br />

across the Cu precipit<strong>at</strong>e and the G-phase <strong>in</strong>di-<br />

Fe<br />

Cr<br />

Published <strong>in</strong> Metall. M<strong>at</strong>er. Trans. A. Vol. 30A, pp. 345-353. 1999<br />

Fe &Cr / <strong>at</strong>.%<br />

(a)<br />

(b)<br />

110<br />

110<br />

(c) 011<br />

200<br />

(d)<br />

100nm<br />

Fig. 8 TEM (a) dark filed image, (b) [001], (c) [011] and (d) [111]<br />

SAD p<strong>at</strong>tern of the martensite phase aged 400°C for 5000 h. The<br />

dark field image was taken us<strong>in</strong>g the 1/2(011) reflection.<br />

Ni<br />

Si<br />

Mn<br />

Cu<br />

100<br />

80<br />

60<br />

40<br />

20<br />

0<br />

30<br />

15<br />

0<br />

30<br />

15<br />

0<br />

10<br />

0<br />

30<br />

15<br />

0<br />

0 500 1000 1500<br />

Number of Atoms / x50<br />

Fig. 9 1DAP concentr<strong>at</strong>ion depth profile of the martensite phase<br />

aged <strong>at</strong> 400°C for 5000 h. Ni, Si, and Mn appear to be partitioned<br />

<strong>in</strong>to the Cu precipit<strong>at</strong>e.<br />

110<br />

011

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