The direct observation of surface martensite formation upon cooling to temperatures close to ambient in a heat treated AISI 301 stainless steel

Conference of the South African Advanced Materials Initiative 2018

Mukarati, T.W.^1 ; Mostert, R.J.^1 ; Siyasiya, C.W.^1

University of Pretoria, Private bag X20, Hatfield

0028, South Africa^1

关键词: Austenitic grain size;    Direct observations;    Electron back scatter diffraction;    Glow-discharge optical emission spectroscopy;    Interstitial elements;    Martensite Formation;    Martensite start temperature;    Surface concentration;   

Others  :  https://iopscience.iop.org/article/10.1088/1757-899X/430/1/012042/pdf
DOI  :  10.1088/1757-899X/430/1/012042

来源: IOP

【 摘 要 】

Martensitic transformation, either athermal or strain-induced, in metastable AISI 301 austenitic steel is of high technical interest as this facilitates manipulation of mechanical properties. This work is part of a project aimed at identifying the influence of variables that determine the athermal α′-martensitic transformation in this steel in order to ensure consistent martensite formation and optimized mechanical properties. The influences of initial austenitic grain size and surface concentrations of interstitial elements (C, N) on martensite start temperature were investigated. The surface concentrations of both carbon and nitrogen were decreased through decarburisation and the formation of martensite upon cooling from ambient temperatures was directly observed using a cryogenic Scanning Electron Microscope (cryo-SEM). It was found that martensite formed on the heat-treated surfaces at much higher temperatures than that expected for AISI 301 steel. The observations were confirmed using electron backscatter diffraction (EBSD). Other analytical techniques including glow-discharge optical emission spectroscopy (GDOES), and Neutron Diffraction were carried out to explain the observations.