• 한국소음진동공학회:학술대회논문집
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• 한국소음진동공학회 2014년도 추계학술대회 논문집
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• pp.20-22
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• 2014

선박, 해양플랜트에 적용되는 PAGA System 는 선내 모든 선원 및 승객에 대하여 정보전달 기능뿐 아니라 위급 상황 발생시 신속한 상황 전달 및 대피를 위한 안전상의 이유로서 매우 중요시 되고 있다. PAGA 의 핵심이 되는 Audio Coverage 의 경우, 초기 설계단계에서 해석을 통해 스피커 배치가 이루어지는데, 본 논문에서는 이러한 PAGA Audio Coverage 관련 요구조건과 합리적인 적용방안, 해석 및 평가 방안에 대하여 사례를 통해 소개하고자 한다.

• Journal of Advanced Marine Engineering and Technology
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• 제40권7호
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• pp.613-621
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• 2016

본 논문에서는 현장 및 원격지에서 해양플랜트 및 선박의 내부 IP기반 네트워크 장비의 운용, 설정과 원격지 통제 지원을 위하여 네트워크 장비, CCTV, PAGA, IP-PBX, Legacy를 연동하고 원격지에서 장비의 상태, 작업 상황, 알림 등의 모니터링과 제어가 가능한 네트워크 장비 통합 관리 시스템의 운영 프로그램을 구현하였다. 개발된 운용 프로그램을 위성지구국과 운항중 선박에 적용하여 선육간 통신 구간에서의 데이터 유실 및 송수신 지연에 대한 성능을 시험한 결과 FBB, MVSAT 환경에서 네트워크 장비, PAGA, IP-PBX, Legacy의 실시간 모니터링 및 제어와 CCTV의 제어 기능이 정상적으로 동작함을 확인하였다. 단 데이터량이 비교적 큰 CCTV 영상 수신과 음성 데이터의 송수신은 다소 지연되어 데이터의 실시간 송수신을 위한 데이터 압축 및 변환 기술 개발이 필요함을 확인하였다.

• Journal of Advanced Marine Engineering and Technology
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• 제39권8호
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• pp.863-869
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• 2015

This study analyzed the offshore plant industry and related regulations such as ISO, IEC, and Norsok Standards to develop an integrated network management system (INMS) capable of both on-site and remote management and configuration of IP-based network equipment in offshore plants. The INMS was designed based on actual specifications and POS plans, and a plan of management was verified through an offshore plant engineering company. Various modules such as PAGA interface modules, CCTV, IP-PBX, and HF-radio communication modules were developed for system implementation. Protocol and data design and screen design were followed by framework development and introduction of the automatic satellite communication function.

• 천문학회보
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• 제44권2호
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• pp.51.3-51.3
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• 2019

Its ability to measure the polarization of light at four frequencies makes the KVN a "plasma physics observatory" that can probe the internal physics (e.g., magnetic fields, outflow geometries) of AGN radio jets and cores. We initiated a Key Science Program, the Plasma-physics of Active Galactic Nuclei (PAGaN) project, dedicated to polarimetric monitoring of 14 radio-bright AGN. We have been able to measure the Faraday rotation measure of the cores of our targets as function of frequency; the observed scaling relation is in good agreement with conically expanding outflows to first order. We are further probing a polarized hotspot in the jet of 3C84 and possible systematic differences in the Faraday rotation in BL Lacertae objects and flat spectrum radio quasars.

• 천문학회지
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• 제48권5호
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• pp.299-311
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• 2015

We report first results from KVN and VERA Array (KaVA) VLBI observations obtained in the frame of our Plasma-physics of Active Galactic Nuclei (PAGaN) project. We observed eight selected AGN at 22 and 43 GHz in single polarization (LCP) between March 2014 and April 2015. Each source was observed for 6 to 8 hours per observing run to maximize the uv coverage. We obtained a total of 15 deep high-resolution images permitting the identification of individual circular Gaussian jet components and three spectral index maps of BL Lac, 3C 111 and 3C 345 from simultaneous dual-frequency observations. The spectral index maps show trends in agreement with general expectations – flat core and steep jets – while the actual value of the spectral index for jets shows indications for a dependence on AGN type. We analyzed the kinematics of jet components of BL Lac and 3C 111, detecting superluminal proper motions with maximum apparent speeds of about 5c. This constrains the lower limits of the intrinsic component velocities to ~ 0.98c and the upper limits of the angle between jet and line of sight to ~20°. In agreement with global jet expansion, jet components show systematically larger diameters d at larger core distances r, following the global relation d ≈ 0.2r, albeit within substantial scatter.

• 천문학회지
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• 제48권5호
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• pp.285-298
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• 2015

Active Galactic Nuclei (AGN) with bright radio jets offer the opportunity to study the structure of and physical conditions in relativistic outflows. For such studies, multi-frequency polarimetric very long baseline interferometric (VLBI) observations are important as they directly probe particle densities, magnetic field geometries, and several other parameters. We present results from first-epoch data obtained by the Korean VLBI Network (KVN) within the frame of the Plasma Physics of Active Galactic Nuclei (PAGaN) project. We observed seven radio-bright nearby AGN at frequencies of 22, 43, 86, and 129 GHz in dual polarization mode. Our observations constrain apparent brightness temperatures of jet components and radio cores in our sample to > 10^8.01 K and > 10^9.86 K, respectively. Degrees of linear polarization m_L are relatively low overall: less than 10%. This indicates suppression of polarization by strong turbulence in the jets. We found an exceptionally high degree of polarization in a jet component of BL Lac at 43 GHz, with m_L ~ 40%. Assuming a transverse shock front propagating downstream along the jet, the shock front being almost parallel to the line of sight can explain the high degree of polarization.