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http://dx.doi.org/10.5140/JASS.2008.25.1.043

RF ENVIRONMENT TEST ON A PROPOSED SITE FOR THE SENSOR STATION OF THE NEXT GENERATION SATELLITE NAVIGATION SYSTEM, GALILEO: I. THE RESULT OF THE TEST ON THE VICINITY OF KVN TAMLA SITE IN THE YEAR OF 2006 BY KASI  

Jo, Jung-Hyun (Space Geodesy Division, Korea Astronomy & Space Science Institute(KASI))
Je, Do-Hyeung (Radio Astronomy Division, Korea Astronomy & Space Science Institute(KASI))
Cho, Sung-Ki (Space Geodesy Division, Korea Astronomy & Space Science Institute(KASI))
Choi, Byung-Kyu (Space Geodesy Division, Korea Astronomy & Space Science Institute(KASI))
Baek, Jeong-Ho (Space Geodesy Division, Korea Astronomy & Space Science Institute(KASI))
Lee, Dae-Kyu (Space Geodesy Division, Korea Astronomy & Space Science Institute(KASI))
Chung, Hyun-Soo (Radio Astronomy Division, Korea Astronomy & Space Science Institute(KASI))
Lim, Hvung-Chul (Space Geodesy Division, Korea Astronomy & Space Science Institute(KASI))
Cho, Jung-Ho (Space Geodesy Division, Korea Astronomy & Space Science Institute(KASI))
Lee, Woo-Kyoung (Space Geodesy Division, Korea Astronomy & Space Science Institute(KASI))
Jung, Sung-Wook (Space Geodesy Division, Korea Astronomy & Space Science Institute(KASI))
Park, Jong-Uk (Space Geodesy Division, Korea Astronomy & Space Science Institute(KASI))
Choe, Nam-Mi (Policy Development Team, Korea Aerospace Research Institute(KARI))
Publication Information
Journal of Astronomy and Space Sciences / v.25, no.1, 2008 , pp. 43-52 More about this Journal
Abstract
As the next generation of global satellite navigation system, the Galileo project is about to witness an initial orbit validation stage as the successful test of navigation message transmission from Giove-A in 2007. The Space Geodesy division ana the Radio Astronomy division of the Korea Astronomy & Space Science Institute had collaborated on the field survey for the Galileo Sensor Station (GSS) RF environment of the proposed site near Jeju Tamla University from August 3rd to August 5th, 2006. The power spectrums were measured in full-band $(800{\sim}2000MHz)$ and in-band (E5, E6 and L1 band) in frequency domain for 24 hours respectively. Finally, we performed a time domain analysis to characterize strong in-band interference source based on the result of the previous step.
Keywords
Galileo satellite navigation system; Galileo sensor station; RF environment; RFI;
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  • Reference
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