z-logo
Premium
Metal dusting behaviour of several nickel‐ and cobalt‐base alloys in COH 2 H 2 O atmosphere
Author(s) -
Wu Q.,
Zhang J.,
Young D. J.
Publication year - 2011
Publication title -
materials and corrosion
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.487
H-Index - 55
eISSN - 1521-4176
pISSN - 0947-5117
DOI - 10.1002/maco.201005863
Subject(s) - cobalt , materials science , metallurgy , nickel , alloy , chromia , metal , spinel , base metal , coke , graphite , chromium , carbon fibers , composite number , composite material , welding
The metal dusting behaviour of total 11 nickel‐ and cobalt‐base alloys at 680 °C in a gas of 68%CO31%H 2 1%H 2 O ( a C  = 19.0, $p_{{\rm O}_{{\rm 2}} } $  = 5.4 × 10 −25  atm) was investigated. All samples were electropolished and reacted in a thermal cycling apparatus. On the basis of their reaction kinetics, these alloys can be classified into three groups: the first, with rapid carbon uptake and significant metal wastage, consists of alloys of relatively high iron content (AC 66, 800H and NS‐163); the second, with intermediate rates, consists of some Co‐base alloys (HAYNES 188, HAYNES 25 and ULTIMET) and the third, with very low reaction rates, consists of nickel‐base alloys with high chromium levels (601, HAYNES HR 160, 230, G‐35 and EN 105). An external chromia scale protected group 3 alloys from carburization and dusting. However, this protective scale was damaged and not rehealed for group 1 and group 2 alloys, allowing carbon attack. In all cases, coke deposited on the surface with two typical morphologies: filaments and graphite particle clusters. Subsurface spinel formation in high iron‐content alloys led to rapid dusting due to the significant volume expansion. Alloy carbon permeability was calculated from a simple law of mixtures, and shown to correlate reasonably well with initial dusting rate except for one cobalt‐base alloy in which iron spinel formation was significant.

This content is not available in your region!

Continue researching here.

Having issues? You can contact us here