Microstructural features of dissimilar welds between 316LN austenitic stainless steel and alloy 800

Citation
M. Sireesha et al., Microstructural features of dissimilar welds between 316LN austenitic stainless steel and alloy 800, MAT SCI E A, 292(1), 2000, pp. 74-82
Citations number
27
Categorie Soggetti
Apllied Physucs/Condensed Matter/Materiales Science","Material Science & Engineering
Journal title
MATERIALS SCIENCE AND ENGINEERING A-STRUCTURAL MATERIALS PROPERTIES MICROSTRUCTURE AND PROCESSING
ISSN journal
09215093 → ACNP
Volume
292
Issue
1
Year of publication
2000
Pages
74 - 82
Database
ISI
SICI code
0921-5093(20001115)292:1<74:MFODWB>2.0.ZU;2-E
Abstract
For joining type 316LN austenitic stainless steel to modified 9Cr-1Mo steel for power plant application, a trimetallic configuration using an insert p iece (such as alloy 800) of intermediate thermal coefficient of expansion ( CTE) has been sometimes suggested for bridging the wide gap in CTE between the two steels. Two joints are thus involved and this paper is concerned wi th the weld between 316LN and alloy 800. These welds were produced using th ree types of filler materials: austenitic stainless steels corresponding to 316, 16Cr-8Ni-2Mo, and the nickel-base Inconel 182(1). The weld fusion zon es and the interfaces with the base materials were characterised in detail using light and transmission electron microscopy. The 316 and Inconel 182 w eld metals solidified dendritically, while the 16-8-2 (16%Cr-8%Ni-2%Mo) wel d metal showed a predominantly cellular substructure. The Inconel weld meta l contained a large number of inclusions when deposited from flux-coated el ectrodes, but was relatively inclusion-free under inert gas-shielded weldin g. Long-term elevated-temperature aging% of the weld metals resulted in emb rittling sigma phase precipitation in the austenitic stainless steel weld m etals, but the nickel-base welds showed no visible precipitation, demonstra ting their superior metallurgical stability for high-temperature service. ( C) 2000 Elsevier Science S.A. All rights reserved.