Speed and accuracy investigations of neural network algorithms for ionospheric modelling at an equatorial region

IF 1.8 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS Journal of Atmospheric and Solar-Terrestrial Physics Pub Date : 2024-10-05 DOI:10.1016/j.jastp.2024.106365
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Abstract

Neural networks are very efficient tools for modeling, including ionospheric modeling. The training algorithm is important for achieving the optimum performance of the trained network. This research is therefore meant to evaluate and compare the performances of ten neural network training algorithms based on their prediction accuracies, and the duration/times taken by each of the algorithms to establish the optimum result. The neural networks were trained using electron density measurements by Radio Occultation (RO) technique from the Constellation Observing System for Meteorology, Ionosphere, and Climate (COSMIC) satellites. Data for the period 2006 through 2021 was used. The networks were trained using about 2.9 million data points collected from the Kano region, Nigeria (5-degree rectangular region around geographic: 12.00° N, 8.59° E) after performing data quality control. The training algorithms considered in the work include: Bayesian Regularization (BR); Broyden-Fletcher-Goldfarb-Shanno Quasi-Newton (BFG); Conjugate Gradient with Powell/Beale (CGB); Fletcher-Reeves Conjugate Gradient (CGF); Gradient descent with momentum and adaptive learning rate (GDX); Levenberg Marquardt (LM); One Step Secant (OSS); Polak-Ribiére Conjugate Gradient (CGP); Resilient Backpropagation (RP); and Scaled Conjugate Gradient (SCG). The results showed that the BR and the LM algorithms gave the best performances in minimizing the errors of prediction (the mean RMSEs are respectively 112 and 114 ×103 electrons/cm3), but the RP algorithm, which came third in terms of accuracy, was significantly faster than both the LM and BR algorithms. The worst-performing algorithm in terms of accuracy was the GDX algorithm, although it was the fastest algorithm. The BFG algorithm was the worst-performing algorithm in terms of a combination of speed and accuracy. The developed neural network model was validated using ionosonde electron density measurements obtained from Ilorin, Nigeria (geographic: 8.5° N, 4.5° E; geomagnetic: 1.8° S). A comparison of the neural network, the NeQuick, and the IRI model predictions relative to the ionosonde measurements indicate that the neural network model was the best-performing model; the NN model predictions minimized the mean absolute errors (MAEs) in ∼44% of 399 ionosonde profiles investigated, the IRI model did so in ∼32%, and the NeQuick did so in ∼24%. The MAEs of the NeQuick however exhibited the best (least) variance. In overall, the NN model gave the least (best) mean of the MAEs (∼73 × 103 cm−3), compared to ∼82 × 103 cm−3 given by both the NeQuick and the IRI models, further supporting the idea that neural networks are excellent for present-day ionospheric modeling.
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用于赤道地区电离层建模的神经网络算法的速度和精度研究
神经网络是非常有效的建模工具,包括电离层建模。训练算法对于实现训练网络的最佳性能非常重要。因此,本研究旨在评估和比较十种神经网络训练算法的性能,依据是它们的预测精确度,以及每种算法建立最佳结果所需的时间。利用气象、电离层和气候星座观测系统(COSMIC)卫星通过无线电掩星技术测量的电子密度,对神经网络进行了训练。使用的是 2006 年至 2021 年的数据。在进行数据质量控制后,使用从尼日利亚卡诺地区(地理位置周围 5 度矩形区域:北纬 12.00°,东经 8.59°)收集的约 290 万个数据点对网络进行了训练。工作中考虑的训练算法包括贝叶斯正则化(BR);布洛伊登-弗莱彻-戈德法布-山诺准牛顿(BFG);鲍威尔/比尔共轭梯度(CGB);弗莱彻-里夫斯共轭梯度(CGF);具有动量和自适应学习率的梯度下降算法(GDX);Levenberg Marquardt 算法(LM);一步 Secant 算法(OSS);Polak-Ribiére 共轭梯度算法(CGP);弹性反向传播算法(RP);以及缩放共轭梯度算法(SCG)。结果表明,BR 算法和 LM 算法在最小化预测误差方面表现最佳(平均 RMSE 分别为 112 和 114 ×103 电子/立方厘米),但 RP 算法在准确度方面排名第三,速度明显快于 LM 算法和 BR 算法。精度表现最差的算法是 GDX 算法,尽管它是速度最快的算法。BFG 算法是速度和准确性综合表现最差的算法。利用从尼日利亚伊洛林(地理位置:北纬 8.5°,东经 4.5°;地磁:南纬 1.8°)获得的电离层探测仪电子密度测量数据对所开发的神经网络模型进行了验证。神经网络、NeQuick 和 IRI 模型预测结果与电离层探测仪测量结果的比较表明,神经网络模型是性能最好的模型;在所调查的 399 个电离层剖面中,神经网络模型预测结果有 44%的平均绝对误差(MAEs)最小,IRI 模型有 32%的平均绝对误差最小,NeQuick 有 24%的平均绝对误差最小。然而,NeQuick 的 MAEs 显示出最佳(最小)方差。总体而言,神经网络模型给出的平均最大误差最小(最佳)(∼73 × 103 cm-3),而 NeQuick 和 IRI 模型给出的平均最大误差都是∼82 × 103 cm-3,这进一步支持了神经网络是当今电离层建模的绝佳工具这一观点。
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来源期刊
Journal of Atmospheric and Solar-Terrestrial Physics
Journal of Atmospheric and Solar-Terrestrial Physics 地学-地球化学与地球物理
CiteScore
4.10
自引率
5.30%
发文量
95
审稿时长
6 months
期刊介绍: The Journal of Atmospheric and Solar-Terrestrial Physics (JASTP) is an international journal concerned with the inter-disciplinary science of the Earth''s atmospheric and space environment, especially the highly varied and highly variable physical phenomena that occur in this natural laboratory and the processes that couple them. The journal covers the physical processes operating in the troposphere, stratosphere, mesosphere, thermosphere, ionosphere, magnetosphere, the Sun, interplanetary medium, and heliosphere. Phenomena occurring in other "spheres", solar influences on climate, and supporting laboratory measurements are also considered. The journal deals especially with the coupling between the different regions. Solar flares, coronal mass ejections, and other energetic events on the Sun create interesting and important perturbations in the near-Earth space environment. The physics of such "space weather" is central to the Journal of Atmospheric and Solar-Terrestrial Physics and the journal welcomes papers that lead in the direction of a predictive understanding of the coupled system. Regarding the upper atmosphere, the subjects of aeronomy, geomagnetism and geoelectricity, auroral phenomena, radio wave propagation, and plasma instabilities, are examples within the broad field of solar-terrestrial physics which emphasise the energy exchange between the solar wind, the magnetospheric and ionospheric plasmas, and the neutral gas. In the lower atmosphere, topics covered range from mesoscale to global scale dynamics, to atmospheric electricity, lightning and its effects, and to anthropogenic changes.
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