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Abdul Malik

Publications and source records attributed to Abdul Malik.

2 recordsLinked to original sources

Physics-Enhanced Deep Learning for Proactive Thermal Runaway Forecasting in Li-Ion Batteries

Accurate prediction of thermal runaway in lithium-ion batteries is essential for ensuring the safety, efficiency, and reliability of modern energy storage systems. Conventional data-driven approaches, such as Long Short-Term Memory (LSTM) networks, can capture complex temporal dependencies but often violate thermodynamic principles, resulting in physically inconsistent predictions. Conversely, physics-based thermal models provide interpretability but are computationally expensive and difficult to parameterize for real-time applications. To bridge this gap, this study proposes a Physics-Informed Long Short-Term Memory (PI-LSTM) framework that integrates governing heat transfer equations directly into the deep learning architecture through a physics-based regularization term in the loss function. The model leverages multi-feature input sequences, including state of charge, voltage, current, mechanical stress, and surface temperature, to forecast battery temperature evolution while enforcing thermal diffusion constraints. Extensive experiments conducted on thirteen lithium-ion battery datasets demonstrate that the proposed PI-LSTM achieves an 81.9% reduction in root mean square error (RMSE) and an 81.3% reduction in mean absolute error (MAE) compared to the standard LSTM baseline, while also outperforming CNN-LSTM and multilayer perceptron (MLP) models by wide margins. The inclusion of physical constraints enhances the model's generalization across diverse operating conditions and eliminates non-physical temperature oscillations. These results confirm that physics-informed deep learning offers a viable pathway toward interpretable, accurate, and real-time thermal management in next-generation battery systems.

cs.LG

A Statistical Analysis of Sunspot Active Longitudes

This research work is based on the study of the longitudinal distribution of the most active sunspot zones on the photosphere. Sunspot data has been analyzed for 12 solar cycles (cycles 12-23) separately for northern and southern hemisphere, and the entire solar sphere. The timelongitude diagrams and their corresponding histograms have been plotted to probe the formation, location, longitudinal spread, and lifetime of the most active sunspot longitudes. By the analysis and comparison of the time- longitude diagrams and histograms six active longitudes (>0, ~90, ~135, ~180, ~270 and <360 degrees) have been identified out of which three (~90, ~180 and ~270 degrees) are observed to be most frequent for the whole dataset analyzed. The comparison of the northern and southern hemisphere revealed that the hemispheres do not exhibit very similar kind of behavior. The lifetime and longitudinal spread of sunspot active longitudes is found to be 3-5 Carrington rotations and 20-30 degrees Carrington longitude respectively. This research work also includes the study of the movement of most active sunspot longitudes from higher to lower latitudes in northern hemispheres for six solar cycles (cycles 18-23). For this purpose the formation of sunspot active longitudes has been investigated in four latitudinal belts (40-30, 30-20, 20-10 and 10-0 degrees)). It is found that the sunspot active longitudes follow a certain longitudinal pattern during the evolution of the 11-year solar cycle. In the beginning of a solar cycle they seem to appear mostly around two longitudes ~0 degree and ~270 degrees in the latitudinal belt 40-30 degrees. As the solar cycle proceeds they tend to be stable around two longitudes ~90 degrees and ~270 degrees which are antipodal.

astro-ph.SR