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Ka 대역을 공유하는 정지궤도 위성망과 지상망간 주파수 간섭 평가 연구
오대섭(Dae-Sub Oh),김수영(Sooyoung Kim),안도섭(Do-Seob Ahn) 한국통신학회 2008 韓國通信學會論文誌 Vol.33 No.3A
오늘날의 다양한 무선 시스템을 통한 서비스의 공존은 간섭 문제를 야기시킬 수 있으며, 제한된 주파수 대역을 효율적으로 활용하기 위해서는 보다 정확하고 효과적인 주파수 공유 기술에 대한 연구가 필수적이라고 할 수 있다. 특히 위성시스템이 가지는 광역성으로 인하여 지상시스템과의 주파수 공유는 필수적이다. Ka 대역 주파수를 사용하는 위성 시스템은 지향성 안테나를 사용하게 되므로 위성의 방위각을 고려한 주파수 공유 결과에 대한 분석은 주파수 효율성을 높이는데 매우 큰 역할을 할 수 있다. 본 논문에서는 위성망과 지상망과의 간섭을 안테나의 방위각을 고려하여 분석한 결과를 제시하고, 주파수 공유 시 요구되는 망간 최소 이격 거리를 분석한 결과를 제시함으로써 분석 결과가 실제 시스템 설계 및 구현에 활용될 수 있도록 하고 있다. Co-existence of various wireless systems may cause frequency interference problem. For this reason, frequency sharing studies play a very important role in order to use limited spectrum resources efficiently. Especially, because a satellite system covers a global area in nature, the frequency sharing between the satellite system and terrestrial systems is essential. For satellite systems using Ka bands, we can increase spectrum efficiency by considering off-axis angles of earth station antenna. In this paper, we demonstrate the analysis result of separation distance between the satellite earth station and a terrestrial repeater, and the presented results can be used to design and implement Ka band wireless systems.
정현수,노덕규,제도흥,박종민,김효령,안도섭,오대섭,Chung, Hyun-Soo,Je, Do-Heung,Park, Jong-Min,Kim, Hyo-Ryoung,Ahn, Do-Seob,Oh, Dae-Sub 한국천문학회 2003 天文學論叢 Vol.18 No.1
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.
감혜미(Hyemi Gam),오대섭(Dae-Sub Oh),안도섭(Do-Seob Ahn) 한국전자파학회 2009 한국전자파학회논문지 Vol.20 No.12
본 논문에서는 저궤도 위성망(LEO satellite network)과 FS 시스템(Fixed Service system)이 동일한 하향 링크 주파수를 사용하는 통신 환경에서 두 시스템이 간섭 영향 없이 운용될 수 있는 방안을 연구하였다. 저궤도 위성망에 의한 FS 시스템으로의 간섭 시나리오의 경우 동시에 운용되는 저궤도 위성 빔의 수에 따라 FS 시스템의 영역을 정의하여 각 영역에서의 간섭 영향을 분석하였다. 또한 FS 시스템에 의한 지구국으로의 간섭 시나리오에서는 지구국의 보호 영역을 정의하여 보호 영역의 반경에 따른 간섭 영향을 분석하였다. 분석한 결과는 두 시스템이 간섭 영향 없이 운용될 수 있는 공유 조건으로 FS 시스템의 설계 단계에 활용될 수 있다. This paper addresses the analysis of the interference produced between the LEO(Low Earth Orbit) satellite constellation and FS(Fixed Service) system operating in the same frequency and area. At first, we calculates the interference of FS system from the LEO satellite constellation depending on the number of LEO satellite antenna beams. Simulation results show that the amount of interference that was calculated from each region. This result can be used to define the carrier level for protecting FS system from total interference by LEO satellite constellation. In the second scenario, we calculates the interference of LEO satellite system earth station by the FS link depending on radius of protection area. The presented results can be used to design FS systems minimizing interference to earth station.
정현수,노덕규,제도흥,김효령,박종민,안도섭,오대섭,CHUNG HYUNSOO,ROH CUK-GYOO,JE DO-HEUNG,KIM HYO-RYOUNG,PARK JONG-MIN,AHN DO-SEOB,OH DAE-SUB 한국천문학회 2004 天文學論叢 Vol.19 No.1
In the past, radio astronomers have sought isolation from man-made signals by placing their telescopes in remote locations. These measures may no longer safeguard scientific observations, since NGSO satellite systems, particularly low-Earth orbit (LEO) systems, are usually designed to provide global or wide regional coverage. Further, radio astronomers have historically made their observations in the frequency bands allocated for their use by the member countries of the International Telecommunication Union (ITU). The science of radio astronomy could be adversely impacted by the deployment of large constellations of new non-geostationary orbiting (NGSO) satellites for telecommunications, navigation and Earth observation, and the proliferation of new, high-power broadcasting and telecommunication satellites in geostationary (GSO) orbits. Radio telescopes are extremely sensitive, and, in certain situations, signals from satellites can overwhelm the signals from astronomical sources. This paper describes the problem in detail and identifies ways to mitigate it without adversely affecting the continued vigorous growth of commercial space-based telecommunications.