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
V. Y. Tugaenko, A. V. Vodolazhsky, R. A. Evdokimov
{"title":"Formation of Particles during Surface Destruction of Space Bodies Moving in the Atmosphere","authors":"V. Y. Tugaenko,&nbsp;A. V. Vodolazhsky,&nbsp;R. A. Evdokimov","doi":"10.1134/S0038094624700540","DOIUrl":null,"url":null,"abstract":"<p>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.</p>","PeriodicalId":778,"journal":{"name":"Solar System Research","volume":"58 6","pages":"709 - 714"},"PeriodicalIF":0.6000,"publicationDate":"2024-10-15","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Solar System Research","FirstCategoryId":"101","ListUrlMain":"https://link.springer.com/article/10.1134/S0038094624700540","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q4","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0

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.

Abstract Image

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。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
求助全文
约1分钟内获得全文 求助全文
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.
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
联系我们:info@booksci.cn Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。 Copyright © 2023 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术官方微信