Optimizing a deep learning framework for accurate detection of the Earth's ionospheric plasma structures from all-sky airglow images

被引:2
|
作者
Chakrabarti, Satarupa [1 ]
Patgiri, Dipjyoti [1 ]
Rathi, Rahul [1 ]
Dixit, Gaurav [2 ,3 ,5 ]
Krishna, M. V. Sunil [1 ,4 ]
Sarkhel, Sumanta [1 ,4 ,6 ]
机构
[1] Indian Inst Technol Roorkee, Dept Phys, Roorkee 247667, Uttarakhand, India
[2] Indian Inst Technol Roorkee, Dept Management Studies, Roorkee 247667, Uttarakhand, India
[3] Indian Inst Technol Roorkee, Mehta Family Sch Data Sci & Artificial Intelligenc, Roorkee 247667, Uttarakhand, India
[4] Indian Inst Technol Roorkee, Ctr Space Sci & Technol, Roorkee 247667, Uttarakhand, India
[5] Indian Inst Technol Roorkee, Dept Management Studies, Roorkee, Uttarakhand, India
[6] Indian Inst Technol Roorkee, Dept Phys, Roorkee, Uttarakhand, India
关键词
All-sky Airglow Images; Ionospheric Plasma Structures; Deep Learning; Convolutional Neural Network; Cost-effective Models; Bootstrap-; ping; ATMOSPHERIC GRAVITY-WAVES; IMAGING OBSERVATIONS; ATOMIC OXYGEN; SPREAD-F; DISTURBANCES; NIGHTGLOW; EMISSIONS; NETWORK; BANDS;
D O I
10.1016/j.asr.2024.03.014
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
The ionosphere, part of the Earth's atmosphere, where different plasma irregularities/structures are generated through various electrodynamical processes. Airglow imaging is one of the tools to observe various morphological features of these irregularities. We aim to help all -sky airglow imaging -based ionospheric research by proposing novel deep learning at the edge framework for the detection of different types of mid -latitude ionospheric plasma structures (medium scale traveling ionospheric disturbances with single and multiple bands, and plasma bubbles). The primary challenge was to find an optimal deep neural network by considering the trade-off between accuracy and inference time. In order to address this, a novel hyperparameter optimization technique has been used that integrates the approaches of random and grid search mechanisms as a compact function. The random function generates the subspace for hyperparameters to check the convergence of the model while the grid search creates possible combinations to tune these hyperparameters. Our novel optimization method for deep learning inference at the edge led us to a low-cost, high -accuracy convolutional neural network (CNN) model, which outperformed the complex state-of-the-art deep learning models such as Inception -v3, DenseNet169, VGG16, and VGG19. For airglow image -based plasma structure detection, the proposed model recorded an accuracy of 99.9% with an inference time of 5.8 s. This was an improvement of about 4% in accuracy while 85% reduction in inference time over the best -performing baseline. There was about 93% reduction in the number of model parameters with respect to the best -performing baseline. Uncertainty quantification has also been performed in the present work through bootstrapping to validate the robustness of the proposed model. The findings of our study show the promise of deep learning at the edge for all -sky airglow imaging systems by demonstrating an alternate low-cost, high -accuracy deep neural network. (c) 2024 COSPAR. Published by Elsevier B.V. All rights reserved.
引用
收藏
页码:5990 / 6005
页数:16
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