Magnetic field coupling with lunar soil simulants.


Journal

Scientific reports
ISSN: 2045-2322
Titre abrégé: Sci Rep
Pays: England
ID NLM: 101563288

Informations de publication

Date de publication:
15 Jun 2023
Historique:
received: 07 02 2023
accepted: 05 06 2023
medline: 16 6 2023
pubmed: 16 6 2023
entrez: 15 6 2023
Statut: epublish

Résumé

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.

Identifiants

pubmed: 37322259
doi: 10.1038/s41598-023-36527-0
pii: 10.1038/s41598-023-36527-0
pmc: PMC10272116
doi:

Substances chimiques

Soil 0
Powders 0
Iron E1UOL152H7

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Pagination

9713

Subventions

Organisme : National Aeronautics and Space Administration (NASA)
ID : 80LARC21CA001
Organisme : National Science Foundation (NSF)
ID : NNCI-2025489
Organisme : National Science Foundation (NSF)
ID : NNCI-1542101

Informations de copyright

© 2023. The Author(s).

Références

Science. 2007 Jul 6;317(5834):83-6
pubmed: 17556549
IEEE Trans Magn. 2010 Jul 1;46(7):2523-2558
pubmed: 20930943
Methods Mol Biol. 2017;1570:47-71
pubmed: 28238129
Sci Rep. 2018 Oct 9;8(1):15023
pubmed: 30301928

Auteurs

Shanti M Garman (SM)

Department of Electrical and Computer Engineering, University of Washington, Seattle, 98195, USA. shantig@uw.edu.

Melissa C Roth (MC)

Off Planet Research LLC, Everett, 98201, USA.

Vincent G Roux (VG)

Off Planet Research LLC, Everett, 98201, USA.

Joshua R Smith (JR)

Department of Electrical and Computer Engineering, University of Washington, Seattle, 98195, USA.
Allen School of Computer Science and Engineering, University of Washington, Seattle, 98195, USA.

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Classifications MeSH