• 한국수소및신에너지학회논문집
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• 제17권1호
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• pp.75-81
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• 2006

Lean premixed combustion is a well known method for low $NO_x$ gas turbine combustor. But lean combustion is usually accompanied by flame instability. To overcome this problem, the hydrogen ($H_2$) was added to main fuel methane to increase flammable limit. In this paper, the effects of hydrogen addition on lean premixed combustion of methane ($CH_4$) were investigated numerically. Results showed that the extinction stretch rate increases and the extinction temperature constant with relatively small amount of $H_2$ addition. The flame temperature and NO emission increase with $H_2$ addition at the same stretch rate and equivalence ratio but it could increase the range of lean extinction and extinction equivalence ratio limit. Eventually, the $H_2$ addition case showed almost same or lower NO emission than no addictive $CH_4$ case in the extinction condition.

• Journal of the Optical Society of Korea
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• 제14권4호
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• pp.444-450
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• 2010

The traditional approach to inverting aerosol extinction makes use of the assumption of a constant LIDAR ratio in the entire Mie-LIDAR signal profile using the Fernald method. For the large uncertainty in the cloud optical depth caused by the assumed constant LIDAR ratio, an not negligible error of the retrieved aerosol extinction below the cloud will be caused in the backward integration of the Fernald method. A new algorithm to determine aerosol extinction below a cirrus cloud from Mie-LIDAR signals, based on a new cloud boundary detection method and a Mie-LIDAR signal modification method, combined with the backward integration of the Fernald method is developed. The result shows that the cloud boundary detection method is reliable, and the aerosol extinction below the cirrus cloud found by inverting from the modified signal is more efficacious than the one from the measured signal including the cloud-layer. The error due to modification is less than 10% taken in our present example.

• 한국항행학회논문지
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• 제11권4호
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• pp.437-446
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• 2007

$16{\times}40$ Gb/s WDM 전송 시스템에서 비트 에러율 (BER ; bit error rate)의 효과적 보상과 융통적 WDM 전송 시스템의 설계를 위한 광 위상 공액기 (OPC ; optical phase conjugator)의 최적 위치 값과 광섬유 구간의 최적 분산 계수 값들을 10 dB와 20 dB의 소광비(ER ; extinction ratio)에 따라 도출하였다. 모든 WDM 채널들의 BER의 효과적 보상을 위한 최적 파라미터 값들은 기존 연구들에서 살펴보았던 변조 파형 형식, 전송 채널수와 마찬가지로 신호의 소광비에 의존하는 것을 확인하였다. 그리고 최적 파라미터 값들을 이용한 융통적인 WDM 시스템 설계가 ER이 10 dB인 경우보다 ER이 20 dB인 경우가 더욱 유리한 것을 확인하였다.

• 한국항행학회논문지
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• 제28권1호
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• pp.123-128
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• 2024

전체 전송 거리의 중간에서 위상 공액파로 반전시키는 MSSI (mid-span spectral inversion)을 분산 제어 링크에 결합시키면 색 분산과 비선형 효과에 의한 파장 분할 다중 (WDM; wavelength division multiplexed) 신호의 왜곡 보상에 매우 효과적이다. 이러한 MSSI 결합 분산 제어 링크에서 분산 맵의 모양, 채널의 데이터율, 채널 파장과 파장 간격 등은 보상 정도에 영향을 미치고, 결과적으로 WDM 신호의 전송 거리와 용량을 결정하게 한다. 본 논문에서는 MSSI 결합 분산 제어 링크에서 WDM 신호를 구성하는 RZ (return-to-zero) 펄스의 소광비에 따른 보상 특성을 분석하였다. 시뮬레이션 결과 소광비가 커질수록 '1'과 '0' 신호의 전력 차이가 증가하여 수신 성능이 좋아지는 일반적인 광전송 시스템에서의 결과가 아닌 분산 맵의 형태와 분산 맵의 구체적 모양을 결정하는 광섬유 스팬 당 잉여 분산의 크기에 따라 최상의 보상을 얻을 수 있는 소광비가 결정되어야 한다는 것을 알 수 있었다.

• 천문학회지
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• 제39권3호
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• pp.73-80
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• 2006

We analyze the extinction law towards several B1V stars-members of our Galaxy, searching for possible discrepancies from the galactic average extinction curve. Our photometric data allow to build extinction curves in a very broad range: from extreme UV till infrared. Two-colour diagrams, based on the collected photometric data from the ANS UV satellite, published UBV measurements and on the infrared 2MASS data of the selected stars, are constructed. Slopes of the fitted straight lines are used to build the average extinction curve and to search for discrepant objects. The selected stars have also been observed spectroscopically from the Terskol and ESO Observatories; these spectra allow to check their Sp/L's. The spectra of only about 30% of the initially selected objects resemble closely that of HD144470, considered as the standard of B1 V type. Other spectra either show some emission features or belong clearly to another spectral types. They are not used to build the extinction curve. Two-colour diagrams, constructed for the selected B1 V stars, showing no emission stellar features, prove that the interstellar extinction law is homogeneous in the Galaxy. Both the shape of the curve and the total-to-selective extinction ratio do not differ from the galactic average and the canonical value(3.1) respectively. The circumstellar emissions usually cause some discrepancies from the average interstellar extinction law; the discrepancies observed in the extraterrestrial ultraviolet, usually follow some misclassifications.

• 대한기계학회논문집
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• 제19권8호
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• pp.1982-1988
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• 1995

Methane/Air premixed flames are studied numerically, using a detailed chemical model, to investigate the flame strech effects on the extinction in a counterflow. The finite difference method, time integration and modified Newton iteration are used, and adaptive grid technique and grid smoothing have been employed to adjust the grid system according to the spatial steepness of the solution profiles. Results show that the flame stretch, or the conventional nondimensionalized stretch having the tangential flow characteristics of the stretched flame alone cannot adequately describes the extinction phenomena. On the other hand, the local flame stretch having both the normal and tangential flow characteristics of the stretched flame can give a proper explanation to the extinction of the symmetric planar premixed flames stabilized in a counter flow. The extinction condition were found to be a constant local stretch regardless of the equivalence ratio.

• 한국전기전자재료학회:학술대회논문집
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• 한국전기전자재료학회 2002년도 춘계학술대회 논문집 디스플레이 광소자 분야
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• pp.97-100
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• 2002

We analyzed the excitation coefficients and the extinction ratio as a function of waveguide width, center to center distance, and angle of input waveguide for a directional coupler. The variation of thc difference between excitation coefficients is similar to that of the extinction ratio. Also, the smaller the difference between those is, the better the extinction ratio is. This concept will have application to devices using optical coupling.

• Journal of the Optical Society of Korea
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• 제15권3호
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• pp.209-215
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• 2011

A new iterative algorithm is developed to estimate LIDAR ratio for a thin cirrus cloud over an aerosol layer. First, the thin cirrus cloud is screened out and replaced by a modeled LIDAR signal and the extinction coefficients of the aerosol layer are derived using the Fernald backward method. These aerosol coefficients are referred as the "actual values". Second, the original LIDAR signal which includes the thin cirrus cloud is also inverted by the Fernald backward method down to the aerosol layer but using different LIDAR ratio for the thin cirrus cloud. Depending on the different assumptions about the LIDAR ratio of the thin cirrus cloud, different sets of aerosol extinction can be derived. The "actual values" which are found in the first step can be used to constrain this iterative progress and the correct LIDAR ratio of the thin cirrus cloud can be found. The detailed description of this method and retrieval examples are given in the paper. The cases compared with other methods are presented and the statistical result is also shown and agrees well with other studies.

• 천문학회보
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• 제46권2호
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• pp.66.1-66.1
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• 2021

Extinction curves observed toward individual Active Galactic Nuclei (AGN) usually show a steep rise toward Far-Ultraviolet (FUV) wavelengths and can be described by the Small Magellanic Cloud (SMC)-like dust model. This feature suggests the dominance of small dust grains of size a < 0.1 ㎛ in the local environment of AGN, but the origin of such small grains is unclear. In this paper, we aim to explain this observed feature by applying the RAdiative Torque Disruption (RATD) to model the extinction of AGN radiation from FUV to Mid-Infrared (MIR) wavelengths. We find that in the intense radiation field of AGN, large composite grains of size a > 0.1 ㎛ are significantly disrupted to smaller sizes by RATD up to dRATD > 100 pc in the polar direction and dRATD ~ 10 pc in the torus region. Consequently, optical-MIR extinction decreases, whereas FUV-near-Ultraviolet extinction increases, producing a steep far-UV rise extinction curve. The resulting total-to selective visual extinction ratio thus significantly drops to RV < 3.1 with decreasing distances to AGN center due to the enhancement of small grains. The dependence of RV with the efficiency of RATD will help us to study the dust properties in the AGN environment via photometric observations. In addition, we suggest that the combination of the strength between RATD and other dust destruction mechanisms that are responsible for destroying very small grains of a <0.05 ㎛ is the key for explaining the dichotomy observed "SMC" and "gray" extinction curve toward many AGN.

• 대한전자공학회논문지SD
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• 제39권5호
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• pp.31-40
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• 2002

스위칭 동작 유도 영역, 소멸비 조절 영역과 소멸비 향상 영역으로 구성된 수직 방향성 결합기 스위치를 제안하였다. 스위칭 동작 유도 영역에서는 코어 한 개의 굴절율 값을 변화시키어 크로스 상태 (cross state)와 바 상태 (bar state)의 스위칭 동작을 유도하였으며, 소멸비 향상 영역에서의 코어 굴절율의 비대칭을 조절하여 소자의 끝단에서 30㏈ 이상의 소멸비를 가지는 크로스 상태와 바 상태를 얻을 수 있었다. 두 코어의 굴절율 값이 같은 대칭형 결합기의 소멸비 조절 영역를 진행하면서 스위칭 동작 유도 영역의 끝단에서 다른 크로스 상태와 바 상태의 소멸비는 소멸비 조절 영역의 끝단에서 같은 값이되어 소멸비 향상 영역에서 최대 소멸비를 가지기 위한 코어 굴절율의 비대칭 값과 소멸비 향상 영역의 길이가 같게된다. 또한 여러 코어 굴절율 값과 안쪽 클래딩의 두께에 따른 크로스 상태와 바 상태의 소멸비 계산 결과의 분석을 통하여 30 ㏈ 이상의 높은 소멸비를 보이며 큰 제작 공차를 얻기 위한 비대칭 수직 방향성 결합 스위치의 설계 지침을 제시하였다.