Extreme Learning Machines for Exoplanet Simulations: A Faster, Lightweight Alternative to Deep Learning
Tara P. A. Tahseen, Lu\'is F. Sim\~oes, Kai Hou Yip, Nikolaos Nikolaou, Jo\~ao M. Mendon\c{c}a, Ingo P. Waldmann

TL;DR
This paper demonstrates that Extreme Learning Machines (ELMs) can serve as fast, lightweight surrogates for complex physical models in astrophysics, outperforming traditional neural networks in training speed and efficiency.
Contribution
It introduces ELMs as an efficient alternative to deep learning for simulating astrophysical data, showing their effectiveness across different data structures and sizes.
Findings
ELMs achieve 100,000× faster training than BIRNN in sequential data.
An ensemble of ELMs matches CNN accuracy with 16.4× less training time in image data.
ELMs require significantly less data than traditional neural networks for comparable performance.
Abstract
Increasing resolution and coverage of astrophysical and climate data necessitates increasingly sophisticated models, often pushing the limits of computational feasibility. While emulation methods can reduce calculation costs, the neural architectures typically used--optimised via gradient descent--are themselves computationally expensive to train, particularly in terms of data generation requirements. This paper investigates the utility of the Extreme Learning Machine (ELM) as a lightweight, non-gradient-based machine learning algorithm for accelerating complex physical models. We evaluate ELM surrogate models in two test cases with different data structures: (i) sequentially-structured data, and (ii) image-structured data. For test case (i), where the number of samples >> the dimensionality of input data , ELMs achieve remarkable efficiency, offering a 100,000 faster…
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Taxonomy
TopicsIterative Learning Control Systems · Fault Detection and Control Systems · Advanced Data Processing Techniques
MethodsSPEED: Separable Pyramidal Pooling EncodEr-Decoder for Real-Time Monocular Depth Estimation on Low-Resource Settings
