Propagation Effects of Temperature Variations of Moon Regolith

Gray, D., Kontis, K. and Le Kernec, J. (2022) Propagation Effects of Temperature Variations of Moon Regolith. In: IEICE Technical Committee on Antennas and Propagation (AP), Tochigi, Japan, 19 Aug 2024, pp. 29-34.

[img] Text
323348.pdf - Published Version

1MB

Abstract

The Moon’s surface temperature ranges from -193°C to 107°C over which the regolith relative permittivity changes from εr=1.4+j0.5 to εr=2.7. The effects of this variation on propagation at 2.5GHz between a pair of dipoles and a pair of patches over the Moon’s surface were modelled by empirical equation and full wave simulation. The peak and null positions for each antenna configuration did not change with temperature-dependent εr . The only appreciable effect was a small decrease in the peak amplitude caused by εr″.

Item Type:Conference Proceedings
Keywords:radio propagation, Moon regolith.
Status:Published
Refereed:Yes
Glasgow Author(s) Enlighten ID:Kontis, Professor Konstantinos and Gray, Dr Derek and Le Kernec, Dr Julien
Authors: Gray, D., Kontis, K., and Le Kernec, J.
College/School:College of Science and Engineering > School of Engineering
College of Science and Engineering > School of Engineering > Autonomous Systems and Connectivity
ISSN:2432-6380
Copyright Holders:Copyright © 2022 by IEICE
First Published:First published in IEICE Technical Report 122(153):29-34
Publisher Policy:Reproduced in accordance with the publisher copyright policy
Related URLs:

University Staff: Request a correction | Enlighten Editors: Update this record