• 한국항행학회논문지
• /
• 제27권3호
• /
• pp.281-286
• /
• 2023

본 논문은 고정위성업무(FSS; Fixed-Satellite Service) 및 방송위성업무(BSS; Broadcasting-Satellite Service)의 다운링크 대역을 통합하는 Ku 대역의 위성통신용 광대역 혼합 패치 배열 안테나의 설계에 관한 것으로써, 제안한 안테나는 FR4 기판 상에 사각 패치를 6 x 2 형태로 배열하여 구현되었다. FSS 다운링크 대역(10.7~10.95 GHz, 11.2~11.45 GHz) 및 BSS 다운링크 대역(11.7~12.5 GHz, 12.2~12.75 GHz, 11.7~12.2 GHz)을 모두 포함하는 광대역(10.7~12.75 GHz) 안테나를 설계하기 위해 11.5 GHz 및 12.5 GHz에서 동작하는 사각 패치를 각각 교대로 배열하였고 이를 통해 중심주파수의 30.8%에 해당하는 광대역을 확보하였다. 안테나의 성능을 확인하기 위해 제안한 안테나를 제작 및 측정하였고 모의시험 결과와 유사함을 확인하였으며 따라서 제안된 안테나는 FSS 및 BSS 다운링크를 위한 안테나로 적용이 가능하다.

• 천문학논총
• /
• 제18권1호
• /
• pp.97-110
• /
• 2003

WRC-03 was held between 9 June and 4 July 2003 in Geneva, Switzerland. Over 2,200 delegates from 138 ITU Member States attended the Conference. The delegates considered some 2,500 proposals, and over 900 numbered documents related to 50 agenda items. The final output of the Conference consists of 527 pages of new and revised text of the Radio Regulations. This paper provides some details about the outcome of the radio astronomy related issues at the WRC-03 Conference. It is divided into two part: a) Agenda item1.8.2 and b) Agenda item 1.32, related to radio astronomy. Relevant extracts from the Final Acts of WRC-03 are given in the Appendix. Agenda item 1.8.2 was one of the most controversial Agenda Items at WRC-03. Studies were carried out within ITU-R TG 1/7 for the last three years; the results of these studies are summarized in Recommendation ITU-R SM.1633. The Conference adopted a new footnote (5.347A), that calls for the application of Resolution 739 (WRC-03) in the 1452-1492 MHz, 1525-1559 MHz, 1613.8-1626.5 MHz, 2655-2670 MHz, 2670-2690 MHz and 21.4-22.0 GHz bands. Agenda item 1.32 is to consider technical and reglatory provisions concerning the band 37.5-43.5 GHz, in accordance with Resolutions 128 (Rev.WRC-2000) and 84 (WRC-2000). WRC-03 reviewed and adjusted the New footnotes 5.551H and 5.551I cover the protection of radio astronomy observations in the 42.5-43.5 GHz band from unwanted emissions by non-geostationary (5.551H) and geostationary (5.551I) FSS and BSS systems, respectively.