Characterization of anodized aluminum alloy AL6061-T6 under simulated LEO plasma conditions

• Autorzy: Abdel-Aziz Yehia Ahmed , Abd El-Hameed Afaf M. , Abdelaziz Ahmed Magdy , Halawa Meirna G. , Tealib Shafeeq Kaheal

Identyfikatory

DOI

10.2478/arsa-2025-0004

• Języki publikacji: EN

Abstrakty

EN

The space plasma has relatively low energy but is dense in the low Earth orbit (LEO). In this study, we prepared various samples of anodic alloy surfaces with coating thicknesses of 20, 25, 35, and 45 μm to identify the most suitable characteristics for space applications. Ground-based tests were conducted at the Laboratory of Lean Satellite Enterprises and In-Orbit Experiments at the Kyushu Institute of Technology. A radio frequency (RF) plasma source was used to generate a simulated LEO plasma using argon gas in a vacuum chamber. The plasma properties were measured with a Langmuir probe under different test conditions. A negatively biased voltage of −450 V was applied to the samples to study charging/discharging phenomena. The samples were exposed to Ar-plasma for 1-2 h. The physical properties and structural morphology of various alloy samples were analyzed before and after exposure to plasma. This analysis involved ultraviolet (UV)/visible (Vis)/ NearInfrared (NIR) absorption spectra, Energy Dispersive X-ray (EDX) analysis, and surface roughness testing. The results showed that space plasma notably impacts the physical properties and morphology of the alloys. A coated thickness of around 25 μm is considered more suitable for spacecraft surface structures due to its improved optical stability and resistance to plasma degradation, as indicated by the experimental results.

Słowa kluczowe

EN

anodized aluminum alloy; simulated LEO plasma; RF plasma source; coating thickness; UV/Vis/NIR spectra; EDX analysis

• Wydawca: Centrum Badań Kosmicznych PAN ; De Gruyter
• Czasopismo: Artificial Satellites : Journal of Planetary Geodesy
• Rocznik: 2025
• Tom: Vol. 60, No. 2
• Strony: 70--90
• Opis fizyczny: Bibliogr. 42 poz., rys., tab.

Twórcy

autor

Abdel-Aziz Yehia Ahmed

• National Research Institute of Astronomy and Geophysics, 11421, Cairo, Egypt

autor

Abd El-Hameed Afaf M.

• National Research Institute of Astronomy and Geophysics, 11421, Cairo, Egypt

autor

Abdelaziz Ahmed Magdy

• National Research Institute of Astronomy and Geophysics, 11421, Cairo, Egypt

autor

Halawa Meirna G.

• National Research Institute of Astronomy and Geophysics, 11421, Cairo, Egypt

autor

Tealib Shafeeq Kaheal

• National Research Institute of Astronomy and Geophysics, 11421, Cairo, Egypt

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Uwagi

Opracowanie rekordu ze środków MNiSW, umowa nr POPUL/SP/0154/2024/02 w ramach programu "Społeczna odpowiedzialność nauki II" - moduł: Popularyzacja nauki (2025).