• 한국통신학회논문지
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• 제12권1호
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• pp.36-49
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• 1987

하이브리드 모드 마이크로 스트립 線路에서 周波數의 函數인 實效誘電率 및 實效幅에 따른 正規化 位相速度와 特性 임피던스의 分散特性을 計算하기 爲한 Planar Waveguide 모델이 提示되었으며. Eeff(f)와 Weff(f)는 周波數에 따른 實驗關係式과 CAD를 目的으로 設定된 計算式을 利用하여 Planar Waveguide모델 計算에 適用하였고, 多樣한 比誘電率과 스트립 幅/基板 두께(W/h)는 $0.5$\leq$W/h\leq2.5의$ 比를 使用하여, 그 結果를 稱的値, Spectral domain 解析 및 實驗關係 結果 等과 比較하였다. 컴퓨터 시뮬레이션 結果, Planar Waveguide 모델을 利用할 境遇가 이미 發表된 바 있는 다른 方法보다 周波數가 增加함에 따라 周波數 別 正規化 位相速度는 1/ 의 값에 가장 接近하였고 特性 임피던스는 더욱 增加하였다. 또한, CAD를 目的으로 設定된 Eeff(f)를 本 提案 모델이 適用한 境遇가 實驗關係式을 利用한 境遇보다 더 좋은 結果를 얻을 수 있었다.

• 천문학논총
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• 제32권1호
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• pp.77-81
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• 2017

A wide spectral coverage from near-infrared (NIR) to far-infrared (FIR) of AKARI both for imaging and spectroscopy enables us to efficiently study the emission from gas and dust in the interstellar medium (ISM). In particular, the Infrared Camera (IRC) onboard AKARI offers a unique opportunity to carry out sensitive spectroscopy in the NIR ($2-5{\mu}m$) for the first time from a spaceborn telescope. This spectral range contains a number of important dust bands and gas lines, such as the aromatic and aliphatic emission bands at 3.3 and $3.4-3.5{\mu}m$, $H_2O$ and $CO_2$ ices at 3.0 and $4.3{\mu}m$, CO, $H_2$, and H I gas emission lines. In this paper we concentrate on the aromatic and aliphatic emission and ice absorption features. The balance between dust supply and destruction suggests significant dust processing taking place as well as dust formation in the ISM. Detailed analysis of the aromatic and aliphatic bands of AKARI observations for a number of H ii regions and H ii region-like objects suggests processing of carbonaceous dust in the ISM. The ice formation process can also be studied with IRC NIR spectroscopy efficiently. In this review, dust processing in the ISM divulged by recent analysis of AKARI data is discussed.

• 천문학회보
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• 제36권2호
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• pp.115.1-115.1
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• 2011

We analyzed the line profiles of the planetary nebula (PN) NGC 7009 secured with the Keck I HIES and BOES's spectral data. The 5 positions were taken over the nebular image, 4 points on the bright rim plus 1 point at the central position. The covered spectral wavelength range was $3250{\AA}-8725{\AA}$ in these observations. We decomposed the lines of HI, HeI, HeII, CII, NIII, [ClIII], [NII], [OII], [OIII], [SII], [SIII], [ClIII], and [ArIII] using the IRAF and StarLink/Dipso. After correcting the Earth's movement and the PN's radial velocities, -48.6 & -48.9 km/s, respectively, for the Keck & BOES, we produced the line profiles in a velocity scale. The zero velocity at each line profile clearly indicates which part of the components is approaching or receding, giving a general information of the kinematical structure. Almost all of the low-to-medium excitation lines, such as [NII], [SII], [O III], and [ArIII], secured at the central position and four positions along the major & minor axes, showed 3 components, double peak + a wide wing component, suggesting the fast outflow structures are present. The overall geometry is a prolate shell which also has a fainter outer shell in the halo zone, but there appears to be some peculiar sub-structures inside the main shell. The high excitation He I, HeII, NIII lines which might be formed close to the inner boundary of the shell show unusual features, completely different from the other lines. The HeII and these high excitation lines may be indicative of a relative recent fast outflow from the central star and the permitted lines such as NIII might be affected by the innermost structure. We discuss a possible presence of a jet-like fast outflow structure in an out-flow axis different from the main axis of the spheroid shell.

• Earthquakes and Structures
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• 제8권6호
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• pp.1363-1386
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• 2015

The October 23 2011 Van Earthquake is studied from an earthquake engineering point of view. Strong ground motion processing was performed to investigate features of the earthquake source, forward directivity effects during the rupture process as well as local site effects. Strong motion characteristics were investigated in terms of peak ground motion and spectral acceleration values. Directiviy effects were discussed in detail via elastic response spectra and wide band spectograms to see the high frequency energy distributions. Source parameters and slip distribution results of the earthquake which had been proposed by different researchers were summarized. Influence of the source parameters on structural response were shown by comparing elastic response spectra of Muradiye synthetic records which were performed by broadband strong motion simulations of the earthquake. It has been emphasized that characteristics of the earthquake rupture dynamics and their effects on structural design might be investigated from a multidisciplinary point of view. Seismotectonic calculations (e.g., slip pattern, rupture velocity) may be extended relating different engineering parameters (e.g., interstorey drifts, spectral accelerations) across different disciplines while using code based seismic design approaches. Current state of the art building codes still far from fully reflecting earthquake source related parameters into design rules. Some of those deficiencies and recent efforts to overcome these problems were also mentioned. Next generation ground motion prediction equations (GMPEs) may be incorporated with certain site categories for site effects. Likewise in the 2011 Van Earthquake, Reverse/Oblique earthquakes indicate that GMPEs need to be feasible to a wider range of magnitudes and distances in engineering practice. Due to the reverse faulting with large slip and dip angles, vertical displacements along with directivity and fault normal effects might significantly affect the engineering structures. Main reason of excessive damage in the town of Erciş can be attributed to these factors. Such effects should be considered in advance through the establishment of vertical design spectra and effects might be incorporated in the available GMPEs.

• Journal of Biosystems Engineering
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• 제41권4호
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• pp.396-407
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• 2016

Background: Although hyperspectral imaging was originally introduced for military, remote sensing, and astrophysics applications, the use of analytical hyperspectral imaging techniques has been expanded to include monitoring of agricultural crops and commodities due to the broad range and highly specific and sensitive spectral information that can be acquired. Combining hyperspectral imaging with remote sensing expands the range of targets that can be analyzed. Results: Hyperspectral imaging technology can rapidly provide data suitable for monitoring a wide range of plant conditions such as plant stress, nitrogen status, infections, maturity index, and weed discrimination very rapidly, and its use in remote sensing allows for fast spatial coverage. Conclusions: This paper reviews current research on and potential applications of hyperspectral imaging and remote sensing for outdoor field monitoring of agricultural crops. The instrumentation and the fundamental concepts and approaches of hyperspectral imaging and remote sensing for agriculture are presented, along with more recent developments in agricultural monitoring applications. Also discussed are the challenges and limitations of outdoor applications of hyperspectral imaging technology such as illumination conditions and variations due to leaf and plant orientation.

• 한국초지조사료학회지
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• 제26권1호
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• pp.53-62
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• 2006

본 연구는 시료 및 스펙트럼의 전처리 방법이 근적외선 분광법을 이용한 옥수수 사일리지의 화학적 조성분의 예측능력에 미치는 영향을 평가하기 위해 수행되었다. 시료의 전처리 방법은 건조하여 분쇄하는 방법(Oven Dried Grinding), 액화 질소처리 후 분쇄하는 방법(Liquid Nitrogen Grinding) 그리고 생사일리지(Intact Fresh)처리로 하였으며 4개의 스펙트럼의 수처리(1,4,4, 2,6,4, 2,10,5) 방법을 이용하여 다변량회귀분석법인 변형부분최소자승회귀법(MPLS)을 통해 검량식을 작성하였다. 시료의 전처리 방법에 의해서 유도된 검량식의 예측 능력은 섬유소 성분(NDF, ADF)과 일반 조성분(CP, Ash) 모두에서 Oven dried grinding (ODG) > Liquid nitrogen grinding (LNG)>Intact fresh (IF) 처리 순으로 우수하였다. 또한 스펙트럼의 수처리 방법에 의한 결과는 시료의 전처리 방법에 따라 그 예측 능력이 다르게 나타났다. 옥수수 사일리지의 섬유소 함량을 예측하기 위한 최적의 시료 전처리 및 스펙트럼 수처리 방법은 NDF는 ODG 처리에 2,10,5 수처리 방법 $(R^2=0.86)$, ADF는 ODG 처리에 2,10,5 수처리 방법 $(R^2v=0.93)$이 가장 우수한 전처리 방법으로 나타났다. 조단백질 함량과 조회분 함량을 측정하기 위한 최적의 시료 전처리 및 스펙트럼 수처리 방법은 조단백질은 ODG 처리에 1,4,4 수처리 방법$(R^2v,=0.91)$, 조회분은 ODG 처리에 2,10,5 수처리 방법$(R^2v=0.89)$이 가장 우수한 전처리 방법으로 판단된다. 이상의 연구 결과를 종합해보면 근적외선 분광법을 이용한 사일리지의 화학적 조성분 함량 측정은 적은 오차 범위 내에서 신속하고 정확한 분석법이 될 수 있음을 확인 할 수 있었다. 비록 원물 생시료(IF)에 대한 직접적인 측정은 다소 예측 정확성이 떨어지지만 현장 적용성과 편리성을 높이기 위해서는 생시료의 측정시 오차를 줄일 수 있는 스펙트럼의 수처리 방법이나 산란보정 방법과 같은 데이터 처리기법에 대한 더 많은 연구가 앞으로 진행되어야 한다고 생각되어진다.

• 한국지진공학회:학술대회논문집
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• 한국지진공학회 2000년도 춘계 학술발표회 논문집 Proceedings of EESK Conference-Spring
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• pp.44-48
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• 2000

Several parameters to represent the characteristics of the observed at the domestic networks from several earthquakes occurred in the Korean Peninsula. Parameters to fit most the multiple Fourier amplitude spectra of the observed accelerations are estimated. This study adopts the stochastic ground motion model referred to the BLWN mode in which the energy is distributed randomly over the duration of the source and which has proven to be very effective in modeling a wide range of ground motion observations. The stochastic ground motion model employed here uses an omega-squared ({{{{ omega ^2 }}) Brune source model with a single corner frequency and a constant stress drop,. The {{{{ omega ^2 }} source model has become a seismological standard because of its simplicity an ability to predict spectral amplitudes and shapes over an extremely broad ranges of magnitudes distances and from the inversion show very unstable based on the fact of high values of mean/median. These results may imply that more observed data and more precise site classification including accurate preparation analysis of data such as more accurate scaling from counts to kine are needed for more stable are effective inversion of Fourier amplitude spectrum of the observed ground motions.

• Journal of the Optical Society of Korea
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• 제17권2호
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• pp.142-147
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• 2013

In order to deduce the difficulty of fixing the Ritchey-Chretien (R-C) dual reflective optical system and enhance the stability of the secondary mirror, a compact integral structure is presented here composed of two transmitting and two reflective aspheric surfaces. The four surfaces were manufactured from a single germanium lens and integrated together. The two reflective surfaces formed by coating the inner reflecting films were assembled in one lens. It makes the installation of the two mirrors easier and the structure of the secondary mirror more stable. A design of mid-wave infrared (MWIR) compact imaging system is presented with a spectral range chosen as $3.7-4.8{\mu}m$. The effective focal length is f=90 mm. The field of view (FOV) for the lens is $4.88^{\circ}$. It has good imaging capability with Modulation Transfer Function (MTF) of all field of view more than 0.55 close to the diffraction limitation. Outdoor experiments were carried out and it is shown that the integral catadioptric optical system performs well on imaging.

• 대기
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• 제23권1호
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• pp.39-45
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• 2013

A parameterization for the scattering of longwave radiation by ice clouds has been developed based on spectral scattering property calculations with shapes and sizes of ice crystals. For this parameterization, the size distribution data by Fu (1996) and by Michell and Arnott (1994) are used. The shapes of ice crystal considered in this study are plate, solid column, hollow column, bullet-rosette, droxtal, aggregate, and spheroid. The properties of longwave scattering by ice crystals are presented as a function of the extinction coefficient, single-scattering albedo, and asymmetry factor. The heating rate and flux by the radiative parameterization model are calculated for wide range of ice crystal sizes, shapes, and optical thickness. The results are compared with the calculated results using a six-stream discrete ordinate scattering algorithm and Chou's method. The new method (with various habits and size distributions) provides a good simulation of the scattering properties and cooling rate in optically thin clouds (optical thickness < 5). Depending on the inclusion of scattering by ice clouds, the errors in the calculation of the cooling rates are significantly different.

• 한국진공학회지
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• 제15권5호
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• pp.435-450
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• 2006

자유전자레이저는 고에너지 전자빔의 운동에너지를 빛 에너지로 바꾸는 장치로서, 다른 어떤 종류의 광원으로도 제공할 수 없는 넓은 범위의 파장가변성과 우수한 분광특성을 갖고 있어, 기초연구에서부터 산업응용에 이르기까지 다양하게 활용될 수 있을 것으로 기대된다. 이 논문에서는 자유전자레이저의 원리와 특성, 요소기술을 소개하고, 최근 주목받고 있는 테라헤르츠파 자유전자레이저와 에너지 회수형 고출력 자유전자레이저에 대하여 자세하게 소개하였다.