Advanced austenitic stainless steels, such as Super 304H, have been used in reheater and
superheater tubes in supercritical and ultra-supercritical power plants for many years now. It is
important to characterise the microstructure of ex-service reheater and superheater tubes as this
will help to understand long-term microstructural evolution and degradation of the material which
can impact the performance and lifetime of the components that are in service. In this research, the
microstructure of an ex-service Super 304H reheater tube that has been in service for 99,000 hours
at an approximate metal temperature of 873K (600°C), has been characterised. The characterisation
techniques used were electron microscopy based and include imaging and chemical analysis
techniques. Seven phases were observed as a result of the characterisation work. The phases
observed were, MX carbo-nitrides rich in niobium, copper rich particles, M23C6, sigma, Z phase, a
cored phase and a BCC phase.
Funding
The authors would like to acknowledge the Engineering and Physical Research Council (EPSRC)
and the Centre for Carbon Capture and Storage and Cleaner Fossil Energy (EP/L016362/1) for their
support on this project.
History
School
Aeronautical, Automotive, Chemical and Materials Engineering
Department
Materials
Published in
Joint EPRI-123HiMAT International Conference on Advances in High Temperature Materials
Citation
PULSFORD, C. ... et al., 2019. Characterisation of the microstructural evolution of aged super 304H (UNS30432) advanced austenitic stainless steel. Presented at the Joint EPRI-123HiMAT International Conference on Advances in High Temperature Materials, Nagasaki, Japan, 21-25th October.
This work is made available according to the conditions of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0) licence. Full details of this licence are available at: https://creativecommons.org/licenses/by-nc-nd/4.0/