aiqbench analysis
This research introduces STO-PNP-CSI, a method that combines stochastic optimization with a Swin-Conv-UNet denoiser to accelerate electromagnetic inversion while maintaining reconstruction accuracy under noise. By solving for only one contrast source vector per iteration and leveraging deep learning priors, the scheme significantly reduces computational costs compared to standard approaches. This advancement is relevant to AI/quantum readers as it demonstrates how machine learning regularization can stabilize ill-posed inverse problems in computational physics.
A Contrast-Source Inversion Scheme Based on Stochastic Optimization and Plug-and-Play Regularization
arXiv:2610.05130v1 Announce Type: cross Abstract: An electromagnetic inversion scheme that integrates stochastic optimization (STO) and plug-and-play (PNP) regularization into contrast-source inversion (CSI), termed STO-PNP-CSI, is developed. Standard CSI solves for the contrast source vector of every transmitter at each iteration, which is expensive in a multi-transmitter configuration. STO instead solves for only one randomly selected contrast source vector per iteration, which reduces the per-iteration cost and can help the inversion escape poor local minima and saddle points. The resulting loss of information, however, increases the ill-posedness of the inversion. To counter this, the Swin-Conv-UNet (SCUNet) denoiser is plugged into the CSI scheme as an implicit regularizer, supplying a learned prior that is stronger than conventional hand-crafted ones and stabilizes the reconstruction. The proposed STO-PNP-CSI is applied to both synthetic and experimental data. The results show that it yields accurate reconstructions at substantially lower computational cost than CSI, including under strong nonlinearity and measurement noise.
Abstract:An electromagnetic inversion scheme that integrates stochastic optimization (STO) and plug-and-play (PNP) regularization into contrast-source inversion (CSI), termed STO-PNP-CSI, is developed. Standard CSI solves for the contrast source vector of every transmitter at each iteration, which is expensive in a multi-transmitter configuration. STO instead solves for only one randomly selected contrast source vector per iteration, which reduces the per-iteration cost and can help the inversion escape poor local minima and saddle points. The resulting loss of information, however, increases the ill-posedness of the inversion. To counter this, the Swin-Conv-UNet (SCUNet) denoiser is plugged into the CSI scheme as an implicit regularizer, supplying a learned prior that is stronger than conventional hand-crafted ones and stabilizes the reconstruction. The proposed STO-PNP-CSI is applied to both synthetic and experimental data. The results show that it yields accurate reconstructions at substantially lower computational cost than CSI, including under strong nonlinearity and measurement noise.
Computational Physics (physics.comp-ph); Information Theory (cs.IT); Machine Learning (cs.LG)
arXiv:2610.05130 [physics.comp-ph]
(or arXiv:2610.05130v1 [physics.comp-ph] for this version)
https://doi.org/10.48550/arXiv.2610.05130 Focus to learn more arXiv-issued DOI via DataCite (pending registration)
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