• Proceedings of the Korean Institute of Communication Sciences Conference
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• 2004.11a
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• pp.403-403
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• 2004

• The Bulletin of The Korean Astronomical Society
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• v.38 no.2
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• pp.32-32
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• 2013

The Korean VLBI Network (KVN) as a world-first multi-frequency VLBI system is operated at four bands of 22, 43, 86, and 129 GHz simultaneously. The performances of both single dish and VLBI network were already confirmed through single dish researches and VLBI evaluation test observations. The VLBI common use of the KVN at 22/43 GHz bands has been started from this autumn. The combined network of KVN and Japanese VERA (KaVA) will start the common use from the first half of next year. Here we present several observational results in the fields of star forming regions, late-type stars, and active galactic nuclei using the KVN and KaVA. The fringes of 44 GHz $CH_3OH$ (Class I) masers were detected from 26 sources for the first time using the KVN and imaging observations are under performing. Simultaneous observations of SiO and $H_2O$ masers toward about 1000 evolved stars showed the different maser properties between SiO and $H_2O$ masers according to the evolutionary stages of AGB and post-AGB stars. The catalog of correlated flux densities were established from a 43 GHz (Q-band) survey of 637 extragalactic sources. At 22 GHz (K-band), flux density measurement and fringe survey for new sources were performed toward a large number of sources. In addition, the large program of KVN and/or KaVA under planning is introduced.

• Proceedings of the KIEE Conference
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• 2008.04a
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• pp.193-194
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• 2008

This paper defines the electrical interfaces and limited items to integrate Ka-band communication payload on the satellite system, which includes the detailed interfaces such as bus voltage and data bus according to the related COMS requirements. And the BUS Electrical Interface Simulator introduces to use during the course of validating and accepting between the KA-Band payload and their EGSE. These interface design results are fully validated through the testing with the BEIS and is compliant with the satellite interface control interface requirements.

• Journal of IKEEE
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• v.17 no.2
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• pp.140-144
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• 2013

This paper presents the novel design of circular polarized Ka-band horn array antenna. The element antenna of the arrya is composed of two parts, microstrip patch and square horn, and the microstrip patch is fed by corner truncated microstrip patch for circular polarization. The patch antenna has the role of a feeder and polarizer of the horn, thus the whole size of the horn antennae can be considerably reduced. The $1{\times}8$ horn array was designed and fabricated by the spacing of $0.9{\lambda}_0$ among the element horn. The element horn has typical gain of 8dBi and axial-ratio bandwidth of 4.9% at 3dB, and the minimum gain and axial-ratio bandwithd of the array is 14dBi and 8.2%.

• Proceedings of the KIEE Conference
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• 2009.07a
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• pp.1013_1014
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• 2009

In this paper, the electrical interfaces used in between COMS satellite bus and Ka-band communication payload are analyzed to verify the robustness of data bus. The purpose of the serial data bus of satellite is to allow serial data transfer between one bus controller or source equipment to several user terminals or slave equipments. A serial data bus in COMS satellite is mainly used for Channel Amplifier and Digital Control Unit of Ka-band Payload.

• Proceedings of the Korean Institute of Communication Sciences Conference
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• 2004.07a
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• pp.465-465
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• 2004

• Proceedings of the Korean Institute of Information and Commucation Sciences Conference
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• 2012.05a
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• pp.74-76
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• 2012

In order to design Transceiver/Receiver antenna with high gain in Ka band, Fresnel zone plate lend(FZPL) antenna is considered and analyzed. Physical optics is applied to demonstrate the FZPL. The FZPL is configured to 11 elements diffraction zones and drived at 20GHz. As a result, calculated received gain using PO method is 33.01dB.

• Proceedings of the Korean Society of Broadcast Engineers Conference
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• 2009.11a
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• pp.101-104
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• 2009

이 연구는 Ka대역 위성 HDTV 방송 서비스를 제공하기 위해 강우강도에 따른 전송방안을 제안하였다. Ka대역은 Ku대역에 비하여 강우에 취약하기 때문에 이를 안정적으로 활용하기 위해서는 강우감쇠를 효과적으로 경감시키는 기술개발이 필수적이다. 유럽위성방송 표준인 DVB-S2에서는 강우감쇠에 대한 대처방안으로 채널상황에 따라 여러 변조방식과 채널 부호 율을 이용하는 적응형 변복조 방식을 지원하고 있으며, 이 논문에서는 DVB-S2기반의 전송방식과 Ka대역 중계기의 규격을 적용하여 강우강도에 따른 전송방안을 제안하였다. 이를 위하여 ITU-R P.618-9 강우감쇠 추정 모델과 기상청에서 측정한 1998년부터 2007년까지의 최근 10년간 국내 주요지역의 30분 누적강우량을 이용하여 지역별 강우 감쇠값을 도출하였고 강우강도와 시간 율 관계분석을 통하여 강우강도에 따른 강우감쇠 값을 획득하였다. 획득한 강우감쇠 값을 무궁화 위성 3호의 링크 설계에 적용하여 강우강도에 따른 적용 가능한 전송방안을 도출하였다. 이 연구를 바탕으로 강우의 지역적 편이가 높은 우리나라의 강우 특성을 유연하게 반영하여 각 지역에 맞는 적응적인 전송 방식을 고려할 수 있다.

• Proceedings of the Korean Society of Broadcast Engineers Conference
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• 2008.02a
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• pp.163-166
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• 2008

이 논문에서는 MPEG-4 SVC 신호를 DVB-S2 전송시스템에 적용하여 Ka대역 위성방송서비스를 제공하는 전송방안에 대한 연구를 하였다. SVC신호는 계층 수를 2개로 제한하였으며, 이러한 다계층 신호를 DVB-S2 전송시스템에 적용하기 위하여, 성상도상에서 각 계층의 신호를 동기적으로 합치는 Hierarchical 변조방식과 각 계층의 전송스트림을 RF 주파수 상에서 비동기적으로 합치는 방식인 Layered 변조방식을 사용하였다. 각 전송방안에서 변조방식과 채널 부호율을 결합 소스/채널 부호화 방안에 따라 변화시켜 최적의 전송기법을 도출하였다.

• The Journal of Korean Institute of Electromagnetic Engineering and Science
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• v.23 no.2
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• pp.262-265
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• 2012

In this paper, a Ka-band 8 W power amplifier module with WR-28 waveguide input and output ports is implemented and measured using four 2 W power amplifier modules and 4:1 waveguide power combiners with high isolation of 25 dB at 35 GHz. The 2 W power amplifier modules are fabricated using waveguide-to-microstrip transitions and show output power of 32.5~33.3 dBm and power gain of 26.9~28.7 dB at 35 GHz. Four 2 W power amplifier modules are combined through 4:1 waveguide power combiners with resistive septum and the combined power shows 39.0 dBm(8 W) under 6 V drain bias and 39.6 dBm(9.1 W) under 6.5 V drain bias at 35 GHz.