Abstract
This paper considers the problem of the dynamic modelling of macro slip in spherical roller bearings. By revisiting the fundamental physics which drive these systems, potential issues in existing models have been identified. Furthermore, in pure rolling conditions it was found that governing differential equations become “stiff”, requiring the use of implicit methods of time integration. The problem of individual roller macro slip in a wind turbine main bearing is then investigated using a simplified representation of system dynamics. Model results indicate clear links between slip/friction and the operational strategy of the wind turbine, as well as significantly higher frictional effects in the downwind main bearing row. Due to modelling simplifications, these results should not yet be considered conclusive, with further work required.
Zusammenfassung
Dieser Beitrag befasst sich mit dem Problem der Dynamischen Modellierung des Makroschlupfs in Pendelrollenlagern. Durch eine Überprüfung der grundlegenden physikalischen Zusammenhänge, die diese Systeme antreiben, wurden potenzielle Probleme in bestehenden Modellen identifiziert. Darüber hinaus wurde festgestellt, dass die maßgeblichen Differentialgleichungen unter reinen Rollbedingungen „steif“ werden, was den Einsatz impliziter Methoden der Zeitintegration erfordert. Das Problem des Makroschlupfes einzelner Rollen in einem Hauptlager einer Windturbine wird dann anhand einer vereinfachten Darstellung der Systemdynamik untersucht. Die Modellergebnisse zeigen klare Zusammenhänge zwischen Schlupf/Reibung und der Betriebsstrategie der Windkraftanlage sowie deutlich höhere Reibungseffekte in der windabgewandten Hauptlagerreihe. Aufgrund von Vereinfachungen der Modellierung sollten diese Ergebnisse noch nicht als abschließend betrachtet werden; weitere Arbeiten sind erforderlich.
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Notes
More specifically, \(\mathbf{L}_{\text{CoM}}\) is the angular momentum (relative to \(\mathcal{O})\) of a point mass with mass equal to that of the rigid body, and with position and velocity equal to the body centre-of-mass at each point in time.
An example of such an orbit being that of our tidally-locked moon.
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Acknowledgements
The authors would like to thank to Dr Tim Rogers (University of Sheffield) for helpful discussions which greatly supported this research. This work forms part of project AMBERS (Advancing Main-BEaRing Science for wind and tidal turbines). Elisha de Mello’s PhD project is funded by the Powertrain Research Hub, co-funded by the Offshore Renewable Energy Catapult. Edward Hart is funded by a Brunel Fellowship from the Royal Commission for the Exhibition of 1851. This work was authored in part by the National Renewable Energy Laboratory, operated by Alliance for Sustainable Energy, LLC, for the U.S. Department of Energy (DOE) under Contract No. DE-AC36-08GO28308. Funding provided by the U.S. Department of Energy Office of Energy Efficiency and Renewable Energy Wind Energy Technologies Office. The views expressed in the article do not necessarily represent the views of the DOE or the U.S. Government. The U.S. Government retains and the publisher, by accepting the article for publication, acknowledges that the U.S. Government retains a nonexclusive, paid-up, irrevocable, worldwide license to publish or reproduce the published form of this work, or allow others to do so, for U.S. Government purposes.
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Appendix
Appendix
1.1 Stiff differential equation example
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de Mello, E., Hart, E., Guo, Y. et al. Dynamic modelling of slip in a wind turbine spherical roller main bearing. Forsch Ingenieurwes 87, 297–307 (2023). https://doi.org/10.1007/s10010-023-00652-z
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DOI: https://doi.org/10.1007/s10010-023-00652-z