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Generative Spatio-temporal GraphNet for Transonic Wing Pressure Distribution Forecasting

Gabriele Immordino, Andrea Vaiuso, Andrea Da Ronch, Marcello Righi

TL;DR

This study presents a framework for predicting unsteady transonic wing pressure distributions, integrating an autoencoder architecture with graph convolutional networks and graph-based temporal layers to model time dependencies, ensuring efficient data representation while preserving essential features.

Abstract

This study presents a framework for predicting unsteady transonic wing pressure distributions, integrating an autoencoder architecture with graph convolutional networks and graph-based temporal layers to model time dependencies. The framework compresses high-dimensional pressure distribution data into a lower-dimensional latent space using an autoencoder, ensuring efficient data representation while preserving essential features. Within this latent space, graph-based temporal layers are employed to predict future wing pressures based on past data, effectively capturing temporal dependencies and improving predictive accuracy. This combined approach leverages the strengths of autoencoders for dimensionality reduction, graph convolutional networks for handling unstructured grid data, and temporal layers for modeling time-based sequences. The effectiveness of the proposed framework is validated through its application to the Benchmark Super Critical Wing test case, achieving accuracy comparable to computational fluid dynamics, while significantly reducing prediction time. This framework offers a scalable, computationally efficient solution for the aerodynamic analysis of unsteady phenomena.

Generative Spatio-temporal GraphNet for Transonic Wing Pressure Distribution Forecasting

TL;DR

This study presents a framework for predicting unsteady transonic wing pressure distributions, integrating an autoencoder architecture with graph convolutional networks and graph-based temporal layers to model time dependencies, ensuring efficient data representation while preserving essential features.

Abstract

This study presents a framework for predicting unsteady transonic wing pressure distributions, integrating an autoencoder architecture with graph convolutional networks and graph-based temporal layers to model time dependencies. The framework compresses high-dimensional pressure distribution data into a lower-dimensional latent space using an autoencoder, ensuring efficient data representation while preserving essential features. Within this latent space, graph-based temporal layers are employed to predict future wing pressures based on past data, effectively capturing temporal dependencies and improving predictive accuracy. This combined approach leverages the strengths of autoencoders for dimensionality reduction, graph convolutional networks for handling unstructured grid data, and temporal layers for modeling time-based sequences. The effectiveness of the proposed framework is validated through its application to the Benchmark Super Critical Wing test case, achieving accuracy comparable to computational fluid dynamics, while significantly reducing prediction time. This framework offers a scalable, computationally efficient solution for the aerodynamic analysis of unsteady phenomena.

Paper Structure

This paper contains 17 sections, 15 equations, 29 figures, 6 tables.

Figures (29)

  • Figure 1: Overview of the GST GraphNet architecture for predicting wing pressure distributions. Module A represents the autoregressive component, incorporating previously predicted $C_P$ values, while Module B processes spatial coordinates and motion data from previous timesteps.
  • Figure 2: Diagram of the pooling and unpooling modules used in the AE for dimensionality reduction and reconstruction.
  • Figure 3: Schematic of the pre-trained AE architecture for compressing and reconstructing the $C_P$ data within the GST GraphNet framework.
  • Figure 4: Impression of the BSCW CFD grid.
  • Figure 5: Training signal 1: DS with $\kappa_\theta = 0.114$, $a_\theta = 0.80$ [deg], $\kappa_\xi = 0.152$, and $a_\xi = -0.098$ [m].
  • ...and 24 more figures