Laboratory Simulations of Plasma Generated Around the Atmospheric Reentry Spacecraft

In this paper, plasma will be generated in a laboratory as a simulation of what happens to spacecraft when they enter the atmosphere of Earth. Parameters of plasma generation were determined in terms of pressures of 0.1, 0.2, 0.3, 0.4, and 0.5 mbar and generation energy 200 W. The parameters of the generated plasma were calculated using the optical emission spectroscopy two intensity ratio method, and the electron temperature, electron density, Debye length, and plasma frequency were calculated. Compare the results with the actual results, electron temperatures were 2.26–1.71 eV and plasma frequency 8.09 x1011-6.7x1011 at 0.1-0.5 mbar pressure.

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Publication Details

Journal
Iraqi Journal of Science
Published
2024-11-15
DOI
https://doi.org/10.24996/ijs.2024.65.10(si).3
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
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article

Laboratory Simulations of Plasma Generated Around the Atmospheric Reentry Spacecraft

Waleed Ibrahim Yaseen, Nabaa Ahmed Abdulmuttaleb
Iraqi Journal of Science
Ionosphere and magnetosphere dynamics
article

Laboratory Simulations of Plasma Generated Around the Atmospheric Reentry Spacecraft

Waleed Ibrahim Yaseen, Nabaa Ahmed Abdulmuttaleb
article en

Abstract

In this paper, plasma will be generated in a laboratory as a simulation of what happens to spacecraft when they enter the atmosphere of Earth. Parameters of plasma generation were determined in terms of pressures of 0.1, 0.2, 0.3, 0.4, and 0.5 mbar and generation energy 200 W. The parameters of the generated plasma were calculated using the optical emission spectroscopy two intensity ratio method, and the electron temperature, electron density, Debye length, and plasma frequency were calculated. Compare the results with the actual results, electron temperatures were 2.26–1.71 eV and plasma frequency 8.09 x1011-6.7x1011 at 0.1-0.5 mbar pressure.

Iraqi Journal of Science
University of Baghdad (IQ)
Affordable and clean energy
Openalex Percentile: Top 85%
Ionosphere and magnetosphere dynamics
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