Formation of Particles during Surface Destruction of Space Bodies Moving in the Atmosphere

IF 0.6 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS Solar System Research Pub Date : 2024-10-15 DOI:10.1134/S0038094624700540
V. Y. Tugaenko, A. V. Vodolazhsky, R. A. Evdokimov
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Abstract

When passing through the Earth’s atmosphere, cosmic bodies are subjected to significant loads due to the impact of high-speed gas flow on their surface. Under the influence of aerodynamic forces and strong heat flows, these bodies are destroyed. The mechanisms of destruction depend on their composition, structure, speed, size and strength. Artificial space bodies move in the atmosphere, generally maintaining their orientation in space, and reach the surface, maintaining integrity due to their high strength. As a result of surface destruction of the frontal part of these bodies, destruction products enter the plasma layer surrounding them when moving in the atmosphere. The design features of the Soyuz descent vehicle made it possible to study the dust component of the plasma layer from the deposits deposited on the porthole. Data on particles detected on the surface of the spacecraft are analyzed, and the results of a statistical analysis of the resulting particle size distribution are presented. It is shown that the distribution curve is well described by a power law.

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在大气中运动的空间物体表面破坏过程中粒子的形成
宇宙天体穿过地球大气层时,由于其表面受到高速气流的冲击,会承受巨大的负荷。在空气动力和强热流的影响下,这些天体被摧毁。破坏机制取决于它们的组成、结构、速度、大小和强度。人造空间体在大气层中运动,一般保持其在空间的方向,并到达表面,因其强度高而保持完整性。由于这些天体正面部分的表面破坏,在大气层中运动时,破坏产物会进入天体周围的等离子体层。联盟号下降飞行器的设计特点使我们有可能从沉积在舷窗上的沉淀物中研究等离子体层的尘埃成分。对在航天器表面检测到的颗粒数据进行了分析,并介绍了对由此得出的颗粒大小分布进行统计分析的结果。结果表明,该分布曲线可以用幂律很好地描述。
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来源期刊
Solar System Research
Solar System Research 地学天文-天文与天体物理
CiteScore
1.60
自引率
33.30%
发文量
32
审稿时长
6-12 weeks
期刊介绍: Solar System Research publishes articles concerning the bodies of the Solar System, i.e., planets and their satellites, asteroids, comets, meteoric substances, and cosmic dust. The articles consider physics, dynamics and composition of these bodies, and techniques of their exploration. The journal addresses the problems of comparative planetology, physics of the planetary atmospheres and interiors, cosmochemistry, as well as planetary plasma environment and heliosphere, specifically those related to solar-planetary interactions. Attention is paid to studies of exoplanets and complex problems of the origin and evolution of planetary systems including the solar system, based on the results of astronomical observations, laboratory studies of meteorites, relevant theoretical approaches and mathematical modeling. Alongside with the original results of experimental and theoretical studies, the journal publishes scientific reviews in the field of planetary exploration, and notes on observational results.
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