Physical Effects in the Atmosphere and Geospace due to Ground-Based Events as Exemplified by the Explosion in the City of Beirut on August 4, 2020. Theoretical Modeling Results

IF 0.5 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS Kinematics and Physics of Celestial Bodies Pub Date : 2021-07-02 DOI:10.3103/S0884591321030028
L. F. Chernogor
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引用次数: 1

Abstract

The study of direct and reverse, positive and negative interconnections among the subsystems in the Earth (internal spheres)–atmosphere–ionosphere–magnetosphere (EAIM) system is commonly based on high-power active experiments. One of the possible experiments is an impact of large chemical explosions in EAIM system. Examples include active experiments utilizing 5 kt TNT, 1.5 kt TNT, and 2 kt TNT yield explosions. A powerful chemical explosion has been shown earlier to affect all geospheres, viz., it generates seismic waves in the lithosphere, disturbances in the electric field, electromagnetic emissions, acoustic and atmospheric gravity waves (AGWs), traveling ionospheric disturbances, and MHD waves in the near-Earth plasma. The physical effects and ecological consequences of multiple chemical explosions and accompanying fires have also been studied earlier. The main conclusion that has been drawn in these studies is that a response to such an impact can appear in all EAIM system subsystems. This paper aims to describe the principle physical effects in the atmosphere and geospace accompanying the powerful explosion in the city of Beirut on August 4, 2020. A comprehensive analysis of the main physical processes accompanying the explosion has been performed to determine the following. The Beirut explosion yield is estimated to be approximately 1 kt TNT. More than 90% of the explosion energy was transformed into the energy of the shock, while the remaining caused damage leaving a crater roughly of 40 × 103 m3, and a 80 kt mass of the ground was ejected. The damage size and surface area have been estimated. The thermic was estimated to have ∼100 m horizontal size, ∼46 m/s speed of its ascending, and a 1.6 min time of the ascent up to the maximum altitude of approximately 4 km. At a distance of 250 km, near Cyprus, the intensity of sound was estimated to be no less than 76 dB. The shock wave traveling upwards caused significant disturbance in the atmosphere and geospace. The increase in the pressure caused by the wave is estimated to be dozens of percent in a 86–90 km altitude range. Shock wave dissipation in the 80–90 km altitude range could cause atmospheric heating by 10–20% and the generation of AGWs with δp ∼ 0.1 propagating to distances of thousands of kilometers from the epicenter. The secondary waves, on account of the dynamo effect, could generate periodic variations in the geomagnetic field with an amplitude of 0.1–0.3 nT.

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地面事件对大气和地球空间的物理影响——以2020年8月4日贝鲁特市爆炸为例理论建模结果
地球(内球)-大气-电离层-磁层(EAIM)系统中各子系统之间的正、逆、正、负相互关系的研究通常基于大功率有源实验。其中一个可能的实验是大型化学爆炸对EAIM系统的影响。例子包括利用5kt TNT、1.5 kt TNT和2kt TNT当量爆炸的活跃实验。一个强大的化学爆炸已经被证明影响所有的地球圈,即,它在岩石圈中产生地震波,在电场中产生扰动,电磁发射,声波和大气重力波(AGWs),电离层扰动和近地等离子体中的MHD波。多次化学爆炸和伴随火灾的物理效应和生态后果也在较早的时候进行了研究。这些研究得出的主要结论是,对这种影响的反应可能出现在所有EAIM系统子系统中。本文旨在描述2020年8月4日在贝鲁特市发生的强烈爆炸在大气和地球空间中的主要物理效应。对伴随爆炸的主要物理过程进行了综合分析,以确定以下情况。贝鲁特爆炸当量估计约为1吨TNT炸药。超过90%的爆炸能量转化为冲击波能量,而剩余的能量造成的破坏留下了一个大约40 × 103 m3的陨石坑,并喷出了80 kt质量的地面。已经估计了损坏的大小和表面积。据估计,热气流的水平大小为~ 100米,上升速度为~ 46米/秒,上升到最大高度约4公里的时间为1.6分钟。在塞浦路斯附近250公里处,声音强度估计不低于76分贝。向上传播的激波对大气和地球空间造成了明显的扰动。据估计,在海拔86-90公里的范围内,由波浪引起的压力增加将达到数十个百分点。在80-90 km高度范围内的激波耗散可以使大气升温10-20%,并产生δp ~ 0.1的AGWs,传播到距离震中数千公里的地方。由于发电机效应,次波可使地磁场产生0.1 ~ 0.3 nT的周期性变化。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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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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