Three-Dimensional Reconstruction of Ionospheric Disturbances Using Tikhonov Regularization After 2022 Tonga Volcanic Eruption

IF 2.6 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS
Danial Abdollahi, M. Mahdi Alizadeh, Harald Schuh, Lung-Chih Tsai
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Abstract

Following significant natural hazards, traveling ionospheric disturbances (TIDs) are generated that affect the ionosphere. Understanding the three-dimensional structure of these TIDs is crucial for understanding their propagation mechanisms. Ionospheric tomography is a viable method to reconstruct these three-dimensional structures. In this study, Tikhonov regularization is used to solve the ill-posed problem of ionospheric tomography following the Tonga volcanic eruption. The New Zealand Global Navigation Satellite Systems network was used to detect TIDs to infer changes in electron density within the ionospheric layers. To validate the reconstructed results, the electron density changes obtained from the tomography were used to reconstruct the detrended slant total electron content (dSTEC) and compared with observed dSTEC values. In addition, electron density profiles from radio occultation data were used for further evaluation. The results showed that the root mean square error of the tomography results could reach 0.228 TEC unit in the dSTEC reconstruction. The most pronounced TIDs were observed at altitudes between 200 and 300 km in agreement with radio occultation observations. Estimation of the speed of atmospheric waves showed that the disturbances propagated through the troposphere at about 360 m/s and reached speeds of up to 609 m/s in the ionosphere. As altitude increases, wave speed also rises, this demonstrates the ionosphere's potential for early warning. The Tikhonov method offers significant advantages in TIDs tomography due to its non-iterative nature, enabling rapid and precise three-dimensional reconstruction. This enhances the understanding of TIDs, improving monitoring and analysis of such events.

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2022年汤加火山喷发后电离层扰动的吉洪诺夫正则化三维重建
在重大自然灾害之后,会产生影响电离层的行进电离层扰动(TIDs)。了解这些TIDs的三维结构对于了解它们的传播机制至关重要。电离层层析成像是重建这些三维结构的可行方法。本文采用吉洪诺夫正则化方法求解汤加火山喷发后电离层层析成像的不适定问题。新西兰全球导航卫星系统网络被用来探测tid,以推断电离层内电子密度的变化。为了验证重建结果,利用断层扫描获得的电子密度变化来重建去趋势倾斜总电子含量(dSTEC),并与观测到的dSTEC值进行比较。此外,利用射电掩星数据的电子密度分布图进行进一步评估。结果表明,在dSTEC重建中,断层扫描结果的均方根误差可达0.228 TEC单位。与射电掩星观测结果一致,在200至300公里之间的高度观测到最明显的tid。对大气波速度的估计表明,扰动以大约360米/秒的速度在对流层传播,并在电离层中达到609米/秒的速度。随着海拔高度的增加,波速也会上升,这表明电离层具有早期预警的潜力。Tikhonov方法由于其非迭代性质,在TIDs断层扫描中具有显著的优势,可以实现快速和精确的三维重建。这加强了对tid的理解,改进了对此类事件的监测和分析。
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来源期刊
Earth and Space Science
Earth and Space Science Earth and Planetary Sciences-General Earth and Planetary Sciences
CiteScore
5.50
自引率
3.20%
发文量
285
审稿时长
19 weeks
期刊介绍: Marking AGU’s second new open access journal in the last 12 months, Earth and Space Science is the only journal that reflects the expansive range of science represented by AGU’s 62,000 members, including all of the Earth, planetary, and space sciences, and related fields in environmental science, geoengineering, space engineering, and biogeochemistry.
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