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dc.contributor.authorSauer, Michal
dc.contributor.authorFabík, Richard
dc.contributor.authorSchindler, Ivo
dc.contributor.authorKawulok, Petr
dc.contributor.authorOpěla, Petr
dc.contributor.authorKawulok, Rostislav
dc.contributor.authorVodárek, Vlastimil
dc.contributor.authorRusz, Stanislav
dc.date.accessioned2023-06-15T06:47:42Z
dc.date.available2023-06-15T06:47:42Z
dc.date.issued2023
dc.identifier.citationMaterials. 2023, vol. 16, issue 1, art. no. 288.cs
dc.identifier.issn1996-1944
dc.identifier.urihttp://hdl.handle.net/10084/149317
dc.description.abstractIt is not realistic to optimize the roll pass design of profile rolling mills, which typically roll hundreds of profiles, using physical modelling or operational rolling. The use of reliable models of microstructure evolution is preferable here. Based on the mathematical equations describing the microstructure evolution during hot rolling, a modified microstructure evolution model was presented that better accounts for the influence of strain-induced precipitation (SIP) on the kinetics of static recrystallization. The time required for half of the structure to soften, t(0.5), by static recrystallization was calculated separately for both situations in which strain-induced precipitation occurred or did not occur. On this basis, the resulting model was more sensitive to the description of grain coarsening in the high-rolling-temperature region, which is a consequence of the rapid progress of static recrystallization and the larger interpass times during rolling on cross-country and continuous mills. The modified model was verified using a plain strain compression test (PSCT) simulation of rolling a 100-mm-diameter round bar performed on the Hydrawedge II hot deformation simulator (HDS-20). Four variants of simulations were performed, differing in the rolling temperature in the last four passes. For comparison with the outputs of the modified model, an analysis of the austenite grain size after rolling was performed using optical metallography. For indirect comparison with the model outputs, the SIP initiation time was determined based on the NbX precipitate size distribution obtained by TEM. Using the PSCT and the outputs from the modified microstructure evolution model, it was found that during conventional rolling, strain-induced precipitation occurs after the last pass and thus does not affect the austenite grain size. By lowering the rolling temperature, it was possible to reduce the grain size by up to 56 mu m, while increasing the mean flow stress by a maximum of 74%. The resulting grain size for all four modes was consistent with the operating results.cs
dc.language.isoencs
dc.publisherMDPIcs
dc.relation.ispartofseriesMaterialscs
dc.relation.urihttps://doi.org/10.3390/ma16010288cs
dc.rights© 2022 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution.cs
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/cs
dc.subjectstatic recrystallizationcs
dc.subjectstrain-induced precipitationcs
dc.subjectmicrostructure evolutioncs
dc.subjectPSCTcs
dc.titleAnalysis of the microstructure development of Nb-microalloyed steel during rolling on a heavy-section millcs
dc.typearticlecs
dc.identifier.doi10.3390/ma16010288
dc.rights.accessopenAccesscs
dc.type.versionpublishedVersioncs
dc.type.statusPeer-reviewedcs
dc.description.sourceWeb of Sciencecs
dc.description.volume16cs
dc.description.issue1cs
dc.description.firstpageart. no. 288cs
dc.identifier.wos000910046300001


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© 2022 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution.
Except where otherwise noted, this item's license is described as © 2022 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution.