| dc.creator | Stocker A.J., Siddle D.R., Warrington E.M., Mariotti G., Silvestri D., Zeqai A., Tortora P., Argyriou A., De Vicente J., Abello R., Mercolino M. | en |
| dc.date.accessioned | 2023-01-31T10:04:01Z | |
| dc.date.available | 2023-01-31T10:04:01Z | |
| dc.date.issued | 2017 | |
| dc.identifier.uri | http://hdl.handle.net/11615/79485 | |
| dc.description.abstract | Spacecraft communication systems operating at X-band are strongly affected when the propagation path passes close to the sun (characterised by the Sun-Earth-Probe, SEP, angle). In this paper, a channel model that can generate a time-series of signal amplitude and phase is presented. The channel model reproduces the observations well for SEP>2° and, with some caveats, works at smaller values of SEP. © 2017 Institution of Engineering and Technology. All rights reserved. | en |
| dc.language.iso | en | en |
| dc.source | IET Conference Publications | en |
| dc.source.uri | https://www.scopus.com/inward/record.uri?eid=2-s2.0-85047313321&partnerID=40&md5=21ad288059699f885bfbd1f9b910e28d | |
| dc.subject | Engineering | en |
| dc.subject | Channel model | en |
| dc.subject | Propagation paths | en |
| dc.subject | Radio channels | en |
| dc.subject | Signal amplitude | en |
| dc.subject | Solar corona | en |
| dc.subject | Sun earth probes | en |
| dc.subject | X bands | en |
| dc.subject | Solar radiation | en |
| dc.subject | Institution of Engineering and Technology | en |
| dc.title | A channel model for the propagation of X-band radio waves through the solar corona | en |
| dc.type | conferenceItem | en |
