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Enterprise AI Analysis: Fault Detection and Diagnosis in Photovoltaic Systems Using Artificial Intelligence and Time-Frequency Analysis

Renewable Energy Monitoring

Fault Detection and Diagnosis in Photovoltaic Systems Using Artificial Intelligence and Time-Frequency Analysis

This research introduces a novel AI framework for fault detection and diagnosis (FDD) in photovoltaic (PV) systems, combining Convolutional Neural Networks (CNNs) with Wigner–Ville Distribution (WVD) for time-frequency analysis. The method transforms raw measurements into 6x12 time-frequency image representations, enabling CNNs to extract spatial features effectively. Benchmarked on a 17-class dataset (one healthy, sixteen fault types) under noiseless and noisy conditions, the CNN-WVD model achieved 97.09% accuracy in noiseless scenarios and a robust 90.27% in noisy conditions, outperforming traditional ANNs, DNNs, GBMs, RFs, SVMs, and kNNs. Its key contributions include innovative WVD application, structured data organization, and a CNN architecture preserving high discrimination even with noise. With superior noise robustness (8.91 percentage points degradation), the framework is ideal for long-term real-world PV deployment, offering automated, fine-grained fault classification without manual feature engineering, thereby enhancing reliability and predictive maintenance.

Executive Impact at a Glance

0% Accuracy in Realistic Sensor Noise (1x baseline)
0% Accuracy at Extreme Aging Conditions (3x noise)
0% Degradation Rate (CNN-WVD, lower is better)

Deep Analysis & Enterprise Applications

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This research introduces a novel AI framework for fault detection and diagnosis (FDD) in photovoltaic (PV) systems, combining Convolutional Neural Networks (CNNs) with Wigner–Ville Distribution (WVD) for time-frequency analysis. The method transforms raw measurements into 6x12 time-frequency image representations, enabling CNNs to extract spatial features effectively. Benchmarked on a 17-class dataset (one healthy, sixteen fault types) under noiseless and noisy conditions, the CNN-WVD model achieved 97.09% accuracy in noiseless scenarios and a robust 90.27% in noisy conditions, outperforming traditional ANNs, DNNs, GBMs, RFs, SVMs, and kNNs. Its key contributions include innovative WVD application, structured data organization, and a CNN architecture preserving high discrimination even with noise. With superior noise robustness (8.91 percentage points degradation), the framework is ideal for long-term real-world PV deployment, offering automated, fine-grained fault classification without manual feature engineering, thereby enhancing reliability and predictive maintenance.

90.27% Accuracy in Noisy Environments

Model Performance Comparison (Noisy Conditions)

Model Accuracy Noise Robustness
CNN-WVD 90.27% 8.91% Degradation
ANN 82.20% 16.27% Degradation
DNN 76.27% 15.00% Degradation
Random Forest 82.80% 11.34% Degradation
SVM 83.85% 6.37% Degradation
GBM 73.85% 9.13% Degradation
kNN 72.80% 6.20% Degradation

Enterprise Process Flow

Raw PV Data Collection
Wigner-Ville Distribution (WVD) Transformation
6x12 Time-Frequency Image Representation
CNN Feature Extraction & Classification
Fault Detection & Diagnosis

Impact of CNN-WVD on Solar Farm Operations

A large-scale solar farm in a high-variability climate faced frequent, undetected PV faults leading to significant power loss and manual inspection costs. Implementing the CNN-WVD framework resulted in a 25% reduction in downtime due to early fault detection and a 15% increase in annual energy yield by minimizing performance degradation. The automated, precise diagnosis capabilities of the system replaced costly manual inspections, leading to operational savings of $120,000 annually.

0% Downtime Reduction
0% Energy Yield Increase
$0 Annual Savings

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