Scale formation mechanisms of martensitic steels in high CO2/H2O-containing gases simulating oxyfuel environments
In oxyfuel power plants, metallic components will be exposed to service environments containing high amounts of CO 2 and water vapour. Therefore, the oxidation behaviour of a number of martensitic 9-12%Cr steels in a model gas mixture containing 70% CO 2 -30% H 2 O was studied in the temperature ran...
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Published in | Materials at high temperatures Vol. 26; no. 1; pp. 63 - 72 |
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Main Authors | , , , , , |
Format | Journal Article |
Language | English |
Published |
Leeds
Taylor & Francis
01.03.2009
Taylor & Francis Ltd |
Subjects | |
Online Access | Get full text |
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Summary: | In oxyfuel power plants, metallic components will be exposed to service environments containing high amounts of CO
2
and water vapour. Therefore, the oxidation behaviour of a number of martensitic 9-12%Cr steels in a model gas mixture containing 70% CO
2
-30% H
2
O was studied in the temperature range 550-700°C. The results were compared with the behaviour in air, Ar-CO
2
and Ar-H
2
O. It was found that in the CO
2
- and/or H
2
O-rich gases, the mentioned steels tended to form iron-rich oxide scales with significantly higher growth rates than the Cr-rich surface scales formed during air exposure. The iron-rich scales were formed as a result of a decreased flux of chromium in the bulk alloy toward the surface because of enhanced internal oxidation of chromium in the H
2
O-containing gases and carbide formation in the CO
2
-rich gases. Additionally, the presence of water vapour in the exposure atmosphere led to buckling of the outer haematite layer, apparently as a result of compressive oxide growth stresses. The Fe-base oxide scales formed in CO
2
(-H
2
O)-rich gases appeared to be permeable to CO
2
molecules resulting in substantial carburization of the steel. |
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Bibliography: | ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 23 ObjectType-Article-2 ObjectType-Feature-1 |
ISSN: | 0960-3409 1878-6413 |
DOI: | 10.3184/096034009X438185 |