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首页> 外文期刊>Metallurgical and Materials Transactions, E. Materials for Energy Systems >Calorimetric Investigation of Thermal Stability of 304H Cu (Fe-17.7Cr-9.3Ni-2.95Cu-0.91 Mn-0.58Nb-0.24Si-0.1C-0.12N-Wt Pct) Austenitic Stainless Steel
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Calorimetric Investigation of Thermal Stability of 304H Cu (Fe-17.7Cr-9.3Ni-2.95Cu-0.91 Mn-0.58Nb-0.24Si-0.1C-0.12N-Wt Pct) Austenitic Stainless Steel

机译:304H Cu(Fe-17.7Cr-9.3Ni-2.95Cu-0.91 Mn-0.58Nb-0.24Si-0.1C-0.12N-Wt Pct)奥氏体不锈钢的热稳定性的量热研究

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摘要

The sequence of phase instabilities that take place in a Fe-17.7Cr-9.3Ni-0.58Nb-2.95Cu-0.12N (wt pct) austenitic stainless steel (304H Cu grade) as a function of temperature has been investigated using dynamic calorimetry. The results obtained from this investigation are supplemented by Thermo calc-based equilibrium and Scheil-Gulliver nonequilibrium solidification simulation. The following phase transformation sequence is found upon slow cooling from liquid: L→L + γ→ L + γ + MX →γ + MX + δ→γ+ MX + M_(23)C_6 → γ + MX + M_(23)C_6 + Cu. Under slow cooling, the solidification follows austenite + ferrite (AF) mode, which is in accordance with Thermocalc prediction and Scheil-Gulliver simulation. However, higher cooling rates result in skeletal δ-ferrite formation, due to increased segregation tendency of Nb and Cr to segregate to interdendritic liquid. The solidification mode is found to depend on combined Nb + Cu content. Experimental estimates of enthalpy change associated with melting and secondary phase precipitation are also obtained. In addition a semi-quantitative study on the dissolution kinetics of M_(23)C_6 type carbides has also been investigated. The standard solution treatment at 1413 K (1140 °C) is found to be adequate to dissolve both Cu and M_(23)C_6 into γ-austenite; but the complete dissolution of MX type carbonitrides occurs near the melting region.
机译:已经使用动态量热法研究了Fe-17.7Cr-9.3Ni-0.58Nb-2.95Cu-0.12N(wt pct)奥氏体不锈钢(304H Cu级)中相变的顺序随温度的变化。从这项研究中获得的结果得到了基于Thermo calc的平衡和Scheil-Gulliver非平衡凝固模拟的补充。从液体缓慢冷却后,发现以下相变顺序:L→L +γ→L +γ+ MX→γ+ MX +δ→γ+ MX + M_(23)C_6→γ+ MX + M_(23)C_6 +铜在缓慢冷却下,固化遵循奥氏体+铁素体(AF)模式,这与Thermocalc预测和Scheil-Gulliver模拟一致。但是,由于Nb和Cr偏析到枝晶间液体的趋势增加,因此较高的冷却速率会导致形成δ铁素体。发现凝固模式取决于结合的Nb + Cu含量。还获得了与熔融和第二相沉淀相关的焓变的实验估计。此外,还对M_(23)C_6型碳化物的溶解动力学进行了半定量研究。发现在1413 K(1140°C)下进行标准固溶处理足以将Cu和M_(23)C_6溶解到γ奥氏体中。但是MX型碳氮化物的完全溶解发生在熔化区附近。

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