The Physics-Informed Neural Network Gravity Model: Generation III
This work solves reliability problems in gravity field modeling for scientific applications, representing an incremental improvement over previous PINN-based methods.
The paper tackles failure modes in machine learning gravity models by introducing PINN-GM-III, which addresses issues like feature divergence and extrapolation error, and demonstrates its robustness through six evaluation metrics and improved modeling accuracy on a heterogeneous density asteroid compared to other models.
Scientific machine learning and the advent of the Physics-Informed Neural Network (PINN) have shown high potential in their ability to solve complex differential equations. One example is the use of PINNs to solve the gravity field modeling problem -- learning convenient representations of the gravitational potential from position and acceleration data. These PINN gravity models, or PINN-GMs, have demonstrated advantages in model compactness, robustness to noise, and sample efficiency when compared to popular alternatives; however, further investigation has revealed various failure modes for these and other machine learning gravity models which this manuscript aims to address. Specifically, this paper introduces the third generation Physics-Informed Neural Network Gravity Model (PINN-GM-III) which includes design changes that solve the problems of feature divergence, bias towards low-altitude samples, numerical instability, and extrapolation error. Six evaluation metrics are proposed to expose these past pitfalls and illustrate the PINN-GM-III's robustness to them. This study concludes by evaluating the PINN-GM-III modeling accuracy on a heterogeneous density asteroid, and comparing its performance to other analytic and machine learning gravity models.