估计由陀螺辐射引发的放电中尘埃云中碎石颗粒数量的方法

IF 1.1 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Astronomy Reports Pub Date : 2024-07-27 DOI:10.1134/S1063772924700379
A. S. Sokolov, T. E. Gayanova, A. K. Kozak, D. V. Malakhov, I. R. Nugaev, D. E. Kharlachev, V. D. Stepakhin
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引用次数: 0

摘要

摘要 文章提出了一种在模拟宇宙尘埃和月球尘埃与航天器表面相互作用的实验中估算粒子数量的新方法。实验的基础是,当模拟宇宙或月球尘埃的物质受到强大脉冲回旋加速器的辐射时,产生尘埃等离子体云。这种方法使用月球碎石模拟器进行了测试。使用 ImageJ 程序分析了微波放电产生的尘埃云中粒子的动态。
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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A Method for Estimating the Number of Regolith Particles in a Dust Cloud in a Discharge Initiated by Gyrotron Radiation

The article proposes a new method for estimating the number of particles in experiments on modeling the interaction of cosmic and lunar dust with the surface of spacecraft. The experiments are based on the creation of a dusty plasma cloud, when exposed to radiation from a powerful pulsed gyrotron on a substance simulating cosmic or lunar dust. This approach was tested using a lunar regolith simulator. The dynamics of particles in dust clouds obtained as a result of microwave discharge is analyzed using the ImageJ program.

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来源期刊
Astronomy Reports
Astronomy Reports 地学天文-天文与天体物理
CiteScore
1.40
自引率
20.00%
发文量
57
审稿时长
6-12 weeks
期刊介绍: Astronomy Reports is an international peer reviewed journal that publishes original papers on astronomical topics, including theoretical and observational astrophysics, physics of the Sun, planetary astrophysics, radio astronomy, stellar astronomy, celestial mechanics, and astronomy methods and instrumentation.
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