2022年1月15日汤加火山喷发造成的电子密度下降

IF 0.5 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS
L. F. Chernogor, Yu. B. Mylovanov
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引用次数: 0

摘要

爆发的汤加火山是其中一个独特的火山。其震级与喀拉喀托火山(1883年)、圣海伦火山(1980年)、埃尔Chichón火山(1982年)和皮纳图博火山(1991年)相同。汤加火山的独特之处在于,汤加火山喷发的产物达到了创纪录的50-58公里,而最强大的喀拉喀托火山喷发的高度只有40-55公里。汤加火山的热能估计为3.9 × 1018 J,火山爆发指数VEI约为5.8,火山震级M约为5.5,喷发强度i约为10.8。我们估计爆炸能量为16-18 Mt TNT。2022年1月15日观测到的电离层总电子含量(TEC)下降是汤加火山喷发引起的,证明电离层空穴主要参数的确定是亟待解决的问题。本研究旨在分析2022年1月15日汤加火山爆发所产生的电离层空洞的参数。利用著名的GPS技术,通过测量每个GPS卫星路径上两个频率的伪距离和积分相位数据,获得电离层TEC垂直柱的时间变化数据。空间天气条件有利于观测汤加火山爆发引起的电离层效应。作为参考日的1月13日和1月17日是受干扰最小的日期。主要结果如下:研究发现,参考日的TEC变化几乎是单调的。在火山喷发当天观测到TEC的非周期和准周期变化。非周期变化与TEC的减少有关。这种效应被称为电离层空洞。已经证明电离层空洞是由火山爆发造成的。随着火山与观测点距离的增加,孔洞的延迟时间增加,而TEC的绝对值和减少的相对值均减小。据估计,电离层空洞的水平尺寸不超过10 Mm,出现的时间延迟不超过122 min,扰动传播的垂直速度为36 ~ 72 m/s,水平速度为2.2 km/s。电离层空洞的寿命为120 ~ 200 min,电离层空洞的TEC随火山与观测点距离的增加而减少约2.5 ~ 10 TECU,相对减少幅度为- 17% ~ -34%。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Electron Density Reduction Caused by the Tonga Volcano Eruption on January 15, 2022

Electron Density Reduction Caused by the Tonga Volcano Eruption on January 15, 2022

The explosive Tonga volcano is among the unique ones. Its order of magnitude is the same as Krakatoa (1883), St. Helens (1980), El Chichón (1982), and Pinatubo (1991) volcanoes. The uniqueness of the Tonga volcano lies in the fact that the products of eruption of the Tonga volcano rose to a record height of 50–58 km, whereas the height of eruption of the most powerful Krakatoa volcano reached only 40–55 km. The Tonga volcano has estimates of 3.9 × 1018 J for thermal energy, approximately 5.8 for volcanic explosive index VEI, approximately 5.5 for volcano magnitude M, and approximately 10.8 for eruption intensity I. We have estimated the explosion energy to be 16–18 Mt TNT. The problems of proving that a decrease in the total electron content (TEC), which was observed on January 15, 2022, in the ionosphere, was caused by the Tonga volcano explosion, and determining the principal parameters of the ionospheric hole are very urgent problems. This study is aimed at analyzing the parameters of the ionospheric hole created by the Tonga volcano explosion on January 15, 2022. Well-known GPS technologies are used to obtain data on time variations of the ionospheric TEC in the vertical column by measuring the pseudo-range and the integrated phase data at two frequencies along the path to each GPS satellite. The space weather conditions were favorable for observing the ionospheric effects caused by the explosion of the Tonga volcano. The calendar dates of January 13 and 17, which are used as reference days, were the least disturbed ones. The main results are as follows. It was found that the TEC on the reference days varied almost monotonically. Aperiodic and quasi-periodic variations of TEC were observed on the day of volcano eruption. Aperiodic variations are associated with a decrease in the TEC. This effect is called the ionospheric hole. It has been proven that the ionospheric hole is caused by a volcanic explosion. The delay time of the hole increases with an increase in the distance between the volcano and the observation site, while both the absolute value of the TEC and the relative value of its decrease are reduced. According to estimates, the horizontal size of the ionospheric hole did not exceed 10 Mm, and the time delay of its appearance did not exceed 122 min. The vertical speed of disturbance propagation was 36–72 m/s, and the horizontal speed was 2.2 km/s. The lifetime of the ionospheric hole was 120–200 min. The TEC in the ionospheric hole was reduced by approximately 2.5–10 TECU, which is a function of the distance from the volcano to the observation site, and the relative decrease ranged from –17 to –34%.

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来源期刊
Kinematics and Physics of Celestial Bodies
Kinematics and Physics of Celestial Bodies ASTRONOMY & ASTROPHYSICS-
CiteScore
0.90
自引率
40.00%
发文量
24
审稿时长
>12 weeks
期刊介绍: Kinematics and Physics of Celestial Bodies is an international peer reviewed journal that publishes original regular and review papers on positional and theoretical astronomy, Earth’s rotation and geodynamics, dynamics and physics of bodies of the Solar System, solar physics, physics of stars and interstellar medium, structure and dynamics of the Galaxy, extragalactic astronomy, atmospheric optics and astronomical climate, instruments and devices, and mathematical processing of astronomical information. The journal welcomes manuscripts from all countries in the English or Russian language.
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