An X Band Radio Channel Model for Propagation Through the Solar Corona-Reference-Cited by-同舟云学术

An X Band Radio Channel Model for Propagation Through the Solar Corona

Published:2018-09 Issue:9 Volume:53 Page:1014-1022
ISSN:0048-6604
Container-title:Radio Science
language:en
Short-container-title:Radio Sci.

Author:

Stocker A. J.¹^ORCID,Siddle D. R.¹^ORCID,Warrington E. M.¹^ORCID,Mariotti G.²³^ORCID,Silvestri D.²⁴,Zeqaj A.²,Tortora P.²^ORCID,Argyriou A.⁵,De Vicente J.⁶,Abello R.⁶,Mercolino M.⁶

Affiliation:

1. Department of Engineering; University of Leicester; Leicester UK

2. Department of Industrial Engineering; University of Bologna; Forli Italy

3. Now at SITAEL S.p.A.; Mola Italy

4. Now at Unisorting S.r.l.; Bertinoro Italy

5. Department of Electrical and Computer Engineering; University of Thessaly; Volos Greece

6. ESA; Darmstadt Germany

Funder

European Space Agency

General Study Programme (GSP) of the European Space Agency

Publisher

American Geophysical Union (AGU)

Subject

Electrical and Electronic Engineering,General Earth and Planetary Sciences,Condensed Matter Physics

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1029/2018RS006578/fullpdf

Reference10 articles.

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2. Lanucara , M. 2013 Spacelink impairments by solar effects

3. Performance study of a deep space communications system with low-density parity-check coding under solar scintillation;Li;International Journal of Communications,2012

4. Solar-induced fluctuations on spacecraft signal amplitude observed during solar superior conjunctions of the Cassini spacecraft;Morabito;Radio Science,2007

5. The Cassini 2000 solar conjunction;Morabito;IEEE Transactions on Antennas and Propagation,2003

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