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Characterization of as-welded microstructure of heat-affected zone in modified 9Cr-1Mo-V-Nb steel weldment

机译:改性9Cr-1Mo-V-Nb钢焊件热影响区的焊接组织特征

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Non-equilibrium microstructure of the heat-affected zone (HAZ) in the as-welded modified 9Cr-1Mo-V-Nb pipe steel (P91) weldment deposited by gas tungsten arc welding (GTAW) and flux core arc welding (FCAW) has been characterized by field-emission scanning electron microscope (FESEM) and electron backscatter diffraction (EBSD). The heterogeneous structures in the sub-layers of the as-welded HAZ are attributable to phase transformations caused by the welding thermal cycles and the local structure variations in the as-received base metal. Coarse-grained heat-affected zone (CGHAZ) has a prior austenite grain (PAG) size of 20 mu m. Fine uniformly-distributed precipitates and a higher fraction of MX carbonitrides are observed in the CGHAZ. Fine-grained heat-affected zone (FGHAZ) consists of the finest grains (1.22 mu m measured by EBSD, 5 mu m PAG size), coarse undissolved M23C6 carbides within the PAG boundaries and fine nucleated M23C6 particles within the martensite laths. Inter critical heat-affected zone (ICHAZ) consists of partially austenitized grains and over-tempered martensite laths. EBSD kernel average misorientation (KAM) map in the FGHAZ close to the ICHAZ illustrates the greatest local strain variations with a moderate normalized KAM value of 0.92 degrees. The majority (88.1%) of the matrix grains in the CGHAZ are classified as deformed grains by EBSD grain average misorientation (GAM) evaluation. The FGHAZ close to the ICHAZ has the most recrystallized grains with an area fraction of 14.4%. The highest density variation of precipitates within grains in the FGHAZ originates from the inhomogeneous chemistry in the base metal. (C) 2016 Published by Elsevier Inc.
机译:气态钨极电弧焊(GTAW)和药芯电弧焊(FCAW)沉积的改性9Cr-1Mo-V-Nb管材(P91)焊接后的热影响区(HAZ)的非平衡组织具有通过场发射扫描电子显微镜(FESEM)和电子背散射衍射(EBSD)对其进行了表征。焊接后的热影响区的子层中的异质结构归因于由焊接热循环和所接收的母材中的局部结构变化引起的相变。粗粒热影响区(CGHAZ)的先前奥氏体晶粒(PAG)尺寸为20微米。在CGHAZ中观察到细小均匀分布的沉淀物和较高比例的MX碳氮化物。细粒热影响区(FGHAZ)由最细的晶粒(通过EBSD测量为1.22微米,PAG尺寸为5微米),PAG边界内的粗大未溶M23C6碳化物和马氏体板条内的细核M23C6颗粒组成。临界热影响区(ICHAZ)由部分奥氏体晶粒和过度回火的马氏体板条组成。靠近ICHAZ的FGHAZ中的EBSD核平均取向错误(KAM)图显示了最大的局部应变变化,中度归一化KAM值为0.92度。通过EBSD晶粒平均取向错误(GAM)评估,CGHAZ中的大多数基体晶粒(88.1%)被分类为变形晶粒。靠近ICHAZ的FGHAZ重结晶晶粒最多,面积分数为14.4%。 FGHAZ中晶粒内沉淀物的最高密度变化源于贱金属中的不均匀化学。 (C)2016由Elsevier Inc.发布

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