Key research themes
1. How can advanced signal processing and domain transformation techniques improve gearbox fault diagnosis under non-stationary and noisy operating conditions?
This theme investigates the application and enhancement of signal processing methods to effectively detect gearbox faults given the challenges of non-stationary vibration signals, fluctuating load and speed conditions, and high noise levels commonly experienced in operational gearboxes. These methods aim to achieve early and reliable fault detection by transforming the measurement domain (time, angular, frequency), enhancing fault signature extraction, and mitigating noise interference without relying on intrusive measurements or additional hardware like tachometers.
2. What role do machine learning and feature extraction methods play in automating and improving accuracy in gearbox fault classification?
This research area centers on leveraging machine learning algorithms combined with optimized feature extraction techniques to develop automated, accurate, and generalized gearbox fault diagnosis systems. Key focuses include coping with variations in gearbox constructions, signal non-stationarity, and load conditions using data-driven approaches that do not rely heavily on prior knowledge or models. The use of adaptive filters, neural networks, support vector machines, and optimized entropy measures are explored to extract discriminative features and classify multiple fault types effectively.
3. How do unique mechanical structures and operating environments of planetary gearboxes influence the development of specialized fault diagnosis methods and parameters?
Given the distinct kinematic behavior, multi-mesh load sharing, and complex transmission paths in planetary gearboxes, conventional diagnostic methods for fixed-axis gearboxes may be suboptimal. This research area explores dynamic modeling, simulation, and specialized signal processing techniques tailored to planetary gearboxes to extract meaningful fault signatures. Additionally, it involves proposing new diagnostic parameters that account for unique sideband structures and transmission complexities, enhancing sensitivity to planet gear faults and other damage types within the planetary gear train.