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Potential Perturbation of the Ionosphere by Megaconstellations and Corresponding Artificial Re-entry Plasma Dust

2023/12/06 by S. Solter-Hunt, Solter-Hunt, S. · 13 voices
Engineering · Physics and Astronomy · #Astro and Planetary Science #Ionosphere and magnetosphere dynamics #Space Satellite Systems and Control #astro-ph.EP #astro-ph.SR #physics.ao-ph #physics.space-ph

paper · pdf · doi:10.48550/arxiv.2312.09329

openalex publication_date 2023/12/06 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

500,000 to 1 million satellites are expected in the next decades, primarily to build internet constellations called megaconstellations. These megaconstellations are disposable and will constantly re-enter and be replaced, hence creating a layer of conductive particulate. Here it will be shown that the mass of the conductive particles left behind from worldwide distribution of re-entry satellites is already billions of times greater than the mass of the Van Allen Belts. From a preliminary analysis, the Debye length in spaceflight regions is significantly higher than non-spaceflight regions according to CCMC ionosphere data. As the megaconstellations grow, the Debye length of the satellite particulate may exceed that of the cislunar environment and create a conductive layer around the earth worldwide. Thus, satellite reentries may create a global band of plasma dust with a charge higher than the rest of the magnetosphere. Therefore, perturbation of the magnetosphere from conductive satellites and their plasma dust layer should be expected and should be a field of intensive research. Human activity is not only impacting the atmosphere, it is clearly impacting the ionosphere.

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