基辅流星体造成的物理影响:2

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

摘要

对 2023 年 4 月 19 日基辅流星体的通过和爆炸在所有地球圈引起的热、湍流和等离子体过程进行了全面的建模研究。对基辅流星体通过时的热力学和等离子体效应以及湍流效应进行了估算。结果表明,天体通过时形成了气体-尘埃羽流。流星体的受热痕迹冷却了几秒钟。考虑了垂直方向上羽流运动的简化一维模型。对羽流的加速度和速度进行了估算。结果表明,羽流的初始加速度最初达到 117 m/s2 的最大值,并持续了 ~1 毫秒。其速度从 0 m/s 增加到 ~1 m/s,然后逐渐减小到 0 m/s。在此速度下,烟羽上升的高度几乎没有增加。热气中含有的爆炸产物、微尘和气溶胶进一步参与了以下三个过程:缓慢沉降到地球表面、与环境空气发生湍流混合,以及被全球主要风向吹散。事实证明,湍流在径迹中的作用非常明显,而磁湍流的作用则不明显。我们估算了尾迹中等离子体的下列基本参数:单位长度和单位体积电子密度的高度依赖性、它们的弛豫时间、粒子碰撞频率、等离子体比电导率和电子温度弛豫时间。研究表明,在初始时刻,迹线中的线性电子密度和体积电子密度分别约等于 1017-1023 m-3 和 1017-1022 m-3,等离子体比电导率约等于 103 欧姆-1 m-1。尘埃等离子体成分的作用微不足道。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Physical Effects from the Kyiv Meteoroid: 2

Comprehensive modeling studies of the thermal, turbulent, and plasma processes induced in all geospheres by the passage and explosion of the Kyiv meteoroid on April 19, 2023, were performed. Thermodynamic and plasma effects, as well as the effects and turbulence, accompanying the passage of the Kyiv meteoroid were estimated. It has been shown that the passage of the celestial body led to the formation of a gas-dust plume. The heated trail of the meteoroid cooled for several seconds. A simplified one-dimensional model of plume motion in the vertical direction is considered. The acceleration and speed of the plume are estimated. It has been shown that the initial acceleration of the plume initially reached a maximum value of 117 m/s2 and lasted ~1 ms. Its speed increased from 0 to ~1 m/s, then gradually decreased to 0 m/s. At this speed, the height of the plume’s ascent hardly increased. The products of the explosion contained in the thermal, specks of dust and aerosols, further took part in the following three processes: a slow precipitation to the surface of the Earth, turbulent mixing with the ambient air, and transport by the predominant winds around the globe. The effect of turbulence in the trail has been shown to be well-pronounced, while the effect of magnetic turbulence has been shown to be absent. The following basic parameters of the plasma in the trail have been estimated: the height dependences of the electron densities per unit length and per unit volume, their relaxation times, the particle collision frequencies, the plasma specific conductivities, and the electron temperature relaxation time. At the initial moment, the linear and volume electron densities in the trail have been shown to be equal to approximately 1017–1023 and 1017–1022 m–3, respectively, and the plasma specific conductivity to be equal to ~103 Ohm–1 m–1. The role of the dusty plasma component was insignificant.

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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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