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Magnetic field coupling with lunar soil simulants
Wireless power transfer (WPT) using magnetically coupled resonators is being integrated into space vehicles destined for the lunar surface. The dusty soil on the Moon, called lunar regolith, is known to adhere to surfaces and is also known to contain iron, including iron oxides and metallic iron. Re...
Autores principales: | , , , |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
Nature Publishing Group UK
2023
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10272116/ https://www.ncbi.nlm.nih.gov/pubmed/37322259 http://dx.doi.org/10.1038/s41598-023-36527-0 |
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author | Garman, Shanti M. Roth, Melissa C. Roux, Vincent G. Smith, Joshua R. |
author_facet | Garman, Shanti M. Roth, Melissa C. Roux, Vincent G. Smith, Joshua R. |
author_sort | Garman, Shanti M. |
collection | PubMed |
description | Wireless power transfer (WPT) using magnetically coupled resonators is being integrated into space vehicles destined for the lunar surface. The dusty soil on the Moon, called lunar regolith, is known to adhere to surfaces and is also known to contain iron, including iron oxides and metallic iron. Regolith samples are limited, and lunar soil simulants are commonly used in space science research for efforts in surface vehicle navigation, in-situ resource utilization, and power infrastructure. However, most simulants contain no metallic iron, and research involving electromagnetic field interactions with regolith would benefit from incorporating metallic iron into test samples. This work presents experimental results from tests using WPT with magnetically coupled resonators in the presence of various standard lunar simulants, plus a new iron-enriched simulant and metallic iron powders. Results for power transfer efficiency, thermal response, and frequency response are presented and demonstrate that the presence of metallic iron and its particle size are critical factors affecting the coupling of the incident magnetic field with lunar simulants and iron powder samples. The importance of particle size-to-skin depth ratio is discussed. Attenuation constants for various iron powders are estimated from experimental data and compared to those of lunar regolith and simulants. |
format | Online Article Text |
id | pubmed-10272116 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2023 |
publisher | Nature Publishing Group UK |
record_format | MEDLINE/PubMed |
spelling | pubmed-102721162023-06-17 Magnetic field coupling with lunar soil simulants Garman, Shanti M. Roth, Melissa C. Roux, Vincent G. Smith, Joshua R. Sci Rep Article Wireless power transfer (WPT) using magnetically coupled resonators is being integrated into space vehicles destined for the lunar surface. The dusty soil on the Moon, called lunar regolith, is known to adhere to surfaces and is also known to contain iron, including iron oxides and metallic iron. Regolith samples are limited, and lunar soil simulants are commonly used in space science research for efforts in surface vehicle navigation, in-situ resource utilization, and power infrastructure. However, most simulants contain no metallic iron, and research involving electromagnetic field interactions with regolith would benefit from incorporating metallic iron into test samples. This work presents experimental results from tests using WPT with magnetically coupled resonators in the presence of various standard lunar simulants, plus a new iron-enriched simulant and metallic iron powders. Results for power transfer efficiency, thermal response, and frequency response are presented and demonstrate that the presence of metallic iron and its particle size are critical factors affecting the coupling of the incident magnetic field with lunar simulants and iron powder samples. The importance of particle size-to-skin depth ratio is discussed. Attenuation constants for various iron powders are estimated from experimental data and compared to those of lunar regolith and simulants. Nature Publishing Group UK 2023-06-15 /pmc/articles/PMC10272116/ /pubmed/37322259 http://dx.doi.org/10.1038/s41598-023-36527-0 Text en © The Author(s) 2023 https://creativecommons.org/licenses/by/4.0/Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article's Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article's Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/ (https://creativecommons.org/licenses/by/4.0/) . |
spellingShingle | Article Garman, Shanti M. Roth, Melissa C. Roux, Vincent G. Smith, Joshua R. Magnetic field coupling with lunar soil simulants |
title | Magnetic field coupling with lunar soil simulants |
title_full | Magnetic field coupling with lunar soil simulants |
title_fullStr | Magnetic field coupling with lunar soil simulants |
title_full_unstemmed | Magnetic field coupling with lunar soil simulants |
title_short | Magnetic field coupling with lunar soil simulants |
title_sort | magnetic field coupling with lunar soil simulants |
topic | Article |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10272116/ https://www.ncbi.nlm.nih.gov/pubmed/37322259 http://dx.doi.org/10.1038/s41598-023-36527-0 |
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