• 천문학회보
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• 제43권1호
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• pp.63.4-64
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• 2018

High resolution spectroscopy of the yellow symbiotic star AG Draconis is performed with the Canada-France-Hawaii Telescope to analyse the line profiles of Raman scattered O VI broad emission features at $6825{\AA}$ and $7082{\AA}$ with a view to investigating the wind accretion process from the mass losing giant to the white dwarf. These two spectral features are formed through inelastic scattering of O $VI{\lambda}{\lambda}32$ and 1038 with atomic hydrogen. We find that these features exhibit double-component profiles with red parts stronger than blue ones with the velocity separation of ~ 60 km s-1 in the O VI velocity space. Monte Carlo simulations for O VI line radiative transfer are performed by assuming that the O VI emission region constitutes a part of the accretion flow around the white dwarf and that Raman O VI features are formed in the neutral part of the slow stellar wind from the giant companion. The overall Raman O VI profiles are reasonably fit with an azimuthally asymmetric accretion flow and the mass loss rate ~ 4 ${\times}$ 10^{-7} M_sun yr^{-1}. We also find that additional bipolar neutral regions moving away with a speed ~ 70 km s^{-1} in the directions perpendicular to the orbital plane provide considerably improved fit to the red wing parts of Raman features.

• 전력전자학회논문지
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• 제10권6호
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• pp.569-577
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• 2005

본 논문에서는 일반적으로 교류 전동기 구동을 위해 널리 사용되고 있는 6-switch IGBT module을 3상 SRM에 적용한 새로운 구동 방법을 제안한다 비대칭 브리지 컨버터의 경우 사용되는 소자수가 많고 복잡한 제어 및 구동회로를 요구하며 이로 인하여 전체적인 시스템 가격은 상승하게 된다. SRM구동을 위한 비대칭 브리지 컨버터의 구동 방법과 비교하여 본 논문에서 제안한 구동방법은 전체적인 시스템의 크기와 파격을 줄일 수 있다. 따라서 유도기, BLDC 모터, 그 외의 모터등과 비교할 수 있는 SRM 구동을 위한 새로운 토폴로지가 될 수 있다. 제안된 회로의 타당성을 검증하기 위해 비대칭 브리지 컨버터를 적응한 시스템과의 비교 실험을 진행하였다.

• Transactions on Electrical and Electronic Materials
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• 제18권4호
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• pp.229-236
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• 2017

This paper deals with the design and implementation of an efficient topology for cascaded multilevel inverters with reduced part counts. In the proposed design, a well-established basic unit is first developed. The series extension of this unit results in the formation of the proposed multilevel inverter. The proposed design minimizes the number of power electronic components including insulated-gate bipolar transistors and gate driver circuits, which in turn cuts down the size of the inverter assembly and reduces the operating power losses. An explicit control strategy with enhanced device efficiency is also acquired. Thus, the part count reductions enhance not only the economical merits but also the technical features of the entire system. In order to accomplish the desired operational aspects, three algorithms are considered to determine the magnitudes of the dc voltage sources effectively. The proposed topology is compared with the conventional cascaded H-bridge multilevel inverter topology, to reflect the merits of the presented structure. In continue, both the analytical and experimental results of a cascaded 31-level structure are analyzed. The obtained results are discussed in depth, and the exemplary performance of the proposed structure is corroborated.

• 천문학회보
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• 제44권1호
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• pp.67.2-67.2
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• 2019

We present the results of KVN and ALMA observations toward WX Psc (IRC+10011) which is a long-period variable OH/IR star. The SiO masers of v=1 and v=2, J=5-4, and the SiO thermal emission of v=0, J=5-4 were observed together with H2O v2=1 (232.6 GHz) and continuum emission at ALMA Band 6 in October 2017 (Cycle 5). This observation aims to investigate the physical association between the inner and outer parts of the circumstellar envelope (CSE) swept by the stellar winds, which is very crucial to understand the asymmetric outward motions developed during the evolutionary phases from the asymptotic giant branch (AGB) stars to the planetary nebulae (PNe). The strong SiO maser features and thermal emissions are detected together with the continuum emission in ALMA observation, which imply the elongated morphology of the CSE of WX Psc. While the spatial resolution of about 20 mas in ALMA observation cannot clearly resolve the detailed characteristics of the inner part of the CSE, the Korean VLBI Network (KVN) observations show the spatial distributions of the v=1 J=1-0, J=2-1, J=3-2 SiO masers emitted from the inner regions of CSE, which are the complementary to the ALMA results. Therefore, we expect these results reveal how the bipolar features of the 22 GHz H2O maser are connected to the innermost region of CSE through the dust condensation region, which is closely related to the enormous mass ejection of the evolved stars.

• 해양안보
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• 제1권1호
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• pp.93-117
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• 2020

2019년 5월과 6월, 호르무즈 해협에서 상선들의 연이은 피격으로 호르무즈 해협에서 해양안보의 불확실성은 증대되고 다수 국가들이 관심을 가지고 역내 안정을 도모하려 노력하고 있다. 한국도 청해부대 임무구역 확장이라는 독자적인 형태로 호르무즈 해협인근의 해양안보 안정화를 위해 노력 중이나, 호르무즈 해협의 주요 역내 행위자인 이란에 대한 세부적인 연구는 미진한 상황이며, 이란 또한 공식적으로 자국의 해양전략을 발표한 바가 없다. 따라서 본 연구는 현실주의적 시각, 특히 케네스 월츠로부터 시작된 방어적(구조적) 현실주의의 관점에서 아랍-페르시아의 양극체제로서의 중동의 정세를 분석하고, 아울러 이란의 독특한 이중화된 군 구조와 구분된 역할, 그리고 전력구성을 연구함으로서 이란의 국가전략과 해양전략을 도출하였다.

• 전력전자학회논문지
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• 제17권6호
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• pp.486-494
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• 2012

In this paper, we proposes the three-phase embedded Z-source inverter consisting of the three embedded Z-source converters and it's the output voltage control method. Each embedded Z-source converter can produce the bipolar output capacitor voltages according to duty ratio D such as single-phase PWM inverter. The output AC voltage of the proposed system is obtained as the difference in the output capacitor voltages of each converter, and the L-C output filter is not required. Because the output AC voltage can be stepped up and down, the boost DC converter in the conventional two-stage inverter is unnecessary. To confirm the validity of the proposed system, PSIM simulation and a DSP based experiment were performed under the condition of the input DC voltage 38V, load $100{\Omega}$, and switching frequency 30kHz. Each converter is connected by Y-connection for three-phase loads. In case that the output phase voltage is the same $38V_{peak}$ as the input DC voltage and is the 1.5 times($57V_{peak}$), the simulation and experimental results ; capacitor voltages, output phase voltages, output line voltages, inductor currents, and switch voltages were verified and discussed.

• 한국전자파학회논문지
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• 제18권2호
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• pp.177-182
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• 2007

본 논문은 InGaP/GaAs HBT 공정을 통해 제작한 적응성궤환 잡음제거시스템용 낮은 위상잡음을 갖는 LC 차동 전압제어 발진기를 제안합니다. 전압제어 발진기는 필터링 기술을 포함한 향상된 공진 탱크 구조를 갖습니다. 비대칭 인덕터 대칭 캐패시터 구조로 제안된 전압제어 발진기의 출력 가변 범위는 207 MHz입니다. 출력 전력은 balun과 케이블 손실을 포함하여 -6.68 dBm입니다. 10 kHz, 100 kHz, 1 MHz에서의 위상잡음은 각각 -102.02, -112.04 그리고 -130.4 dBc/Hz입니다. 이 전압제어 발진기는 총 $0.9{\times}0.9mm^2$ 면적 내에 집적화되었습니다.