| dc.creator | Stocker A.J., Siddle D.R., Warrington E.M., Mariotti G., Silvestri D., Zeqaj A., Tortora P., Argyriou A., De Vicente J., Abello R., Mercolino M. | en |
| dc.date.accessioned | 2023-01-31T10:04:02Z | |
| dc.date.available | 2023-01-31T10:04:02Z | |
| dc.date.issued | 2018 | |
| dc.identifier | 10.1029/2018RS006578 | |
| dc.identifier.issn | 00486604 | |
| dc.identifier.uri | http://hdl.handle.net/11615/79486 | |
| dc.description.abstract | Spacecraft communication systems operating at X band are strongly affected when the propagation path passes close to the Sun (which can be characterized by the Sun-Earth-Probe, SEP, angle). In this paper, a channel model that can generate a time series of signal amplitude and phase, and hence the signal in-phase and quadrature values, is presented. For X band, the channel model reproduces the observations well for SEP > 0.8°. While the model has not been experimentally validated at SEP angles below 0.8°, the behavior is consistent with measurements reported in the literature and is therefore likely to be suitable for use, with caution, in that region too. ©2018. American Geophysical Union. All Rights Reserved. | en |
| dc.language.iso | en | en |
| dc.source | Radio Science | en |
| dc.source.uri | https://www.scopus.com/inward/record.uri?eid=2-s2.0-85052953702&doi=10.1029%2f2018RS006578&partnerID=40&md5=a90291d1170e0220a38452defce61f38 | |
| dc.subject | Electrical engineering | en |
| dc.subject | Radio | en |
| dc.subject | Channel model | en |
| dc.subject | In-phase | en |
| dc.subject | Propagation paths | en |
| dc.subject | Radio channel modeling | 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 | Blackwell Publishing Ltd | en |
| dc.title | An X Band Radio Channel Model for Propagation Through the Solar Corona | en |
| dc.type | journalArticle | en |