2022年1月15日汤加火山爆发引起的近区域电离层扰动

Q4 Physics and Astronomy
L. Chernogor, Yu. Mylovanov
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To detect ionospheric disturbances generated by the volcanic eruption, temporal variations of the total electron content (TEC) in a vertical column in the ionosphere were analyzed. The total error of the TEC estimation did not exceed 0.1 TECU. Results. The quantitative characteristics of ionospheric disturbances caused by the explosive eruption of the Tonga volcano have been obtained. It was proved that the appearance of the ionospheric \"hole\" was caused directly by the volcanic explosion. With dis- tance away from the volcano, the TEC deficit in absolute values decreased from ~10 to ~2.5 TECU. As that was happening, the time taken to form the ionospheric \"hole\" increased from ~20 to ~100 min. Three groups of disturbances were observed. One group picks out disturbances having an N-shaped profile and caused by a blast wave with a speed exceeding ~1 000 m/s. 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引用次数: 0

摘要

主题和目的。汤加火山的热能达到3.9。1018 J,其功率为9.1。1013 W。冲击波的能量和威力接近(6.7…7.5)。1013j和1011w。2022年1月15日汤加火山爆发引起的电离层效应受到了应有的关注。结果表明,电离层扰动在全球范围内传播,近区扰动最大。本文的目的是描述由汤加火山爆发开始并发生在电离层附近的非周期和准周期扰动。方法和方法论。为了探测火山喷发引起的电离层扰动,分析了电离层垂直柱中总电子含量(TEC)的时间变化。TEC估计的总误差不超过0.1 TECU。结果。得到了汤加火山爆发引起的电离层扰动的定量特征。证明了电离层“洞”的出现是由火山爆发直接引起的。随着离火山距离的增加,TEC损失绝对值从~10 TECU减少到~2.5 TECU。当这种情况发生时,形成电离层“洞”所需的时间从~20分钟增加到~100分钟。一组选择具有n形轮廓的扰动,并且由速度超过~ 1000m /s的冲击波引起。另一类包括传播速度在~340…620m /s,这是电离层高度大气重力波的特征。最后一组以扰动传播速度在~110 ~ 320 m/s范围内指定。这种扰动可以由海啸、兰姆波和大气重力波产生。扰动周期在~ 5 ~ 20min之间,扰动幅度在0.5 ~ 1.0 TECU之间。结论。已经证明,近区的非周期和准周期电离层扰动是由汤加火山爆发直接引起的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
NEAR-ZONE IONOSPHERIC DISTURBANCES CAUSED BY EXPLOSIVE ERUPTION OF TONGA VOLCANO ON 15 JANUARY 2022
Subject and Purpose. The thermal energy of the Tonga volcano reached 3.9 . 1018 J, its power amounted to 9.1 . 1013 W. The energy and power of the blast waves approached (6.7...7.5) . 1013 J and 1011 W, respectively. Ionospheric effects caused by the explosive eruption of the Tonga volcano on January 15, 2022 have received due attention. It was established that the ionospheric disturbances spread over global distances, with the greatest disturbances occurring in the near zone. The aim of the present paper is to describe aperiodic and quasi-periodic disturbances started by the Tonga volcano explosion and occurring in the near ionospheric zone. Methods and Methodology. To detect ionospheric disturbances generated by the volcanic eruption, temporal variations of the total electron content (TEC) in a vertical column in the ionosphere were analyzed. The total error of the TEC estimation did not exceed 0.1 TECU. Results. The quantitative characteristics of ionospheric disturbances caused by the explosive eruption of the Tonga volcano have been obtained. It was proved that the appearance of the ionospheric "hole" was caused directly by the volcanic explosion. With dis- tance away from the volcano, the TEC deficit in absolute values decreased from ~10 to ~2.5 TECU. As that was happening, the time taken to form the ionospheric "hole" increased from ~20 to ~100 min. Three groups of disturbances were observed. One group picks out disturbances having an N-shaped profile and caused by a blast wave with a speed exceeding ~1 000 m/s. Another group includes disturbances with a propagation speed within ~340...620 m/s, which is characteristic of atmospheric gravity waves at ionospheric heights. The last group is specified by the disturbance propagation speed within ~110 to 320 m/s. The disturbances of the kind can be generated by tsunamis, Lamb waves and atmospheric gravity waves. The wave disturbance periods varied within ~ 5 to 20 min, the disturbance amplitudes were within 0.5...1.0 TECU. Conclusions. It has been proven that aperiodic and quasi-periodic ionospheric disturbances in the near zone were caused directly by the explosion of the Tonga volcano.
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来源期刊
Radio Physics and Radio Astronomy
Radio Physics and Radio Astronomy Physics and Astronomy-Physics and Astronomy (miscellaneous)
CiteScore
0.60
自引率
0.00%
发文量
18
审稿时长
8 weeks
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