• Proceedings of the Optical Society of Korea Conference
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• 2000.08a
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• pp.62-63
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• 2000

다양한 분야의 요구에 따라 반사율이 99.995% 이상인 고반사 저손실 반사경의 제작이 가능해 지면서 반사경의 산란, 투과, 흡수 및 손실 등을 측정하는 여러 측정 방법들도 더불어 연구되어 왔다. 적용 분야에 따라 사용될 반사경의 특성이 결정되는데 그 중 중력파 측정 장치$^{(1)}$ , 광자 감쇠 분광기$^{(2)}$ 등의 분야에서는 투과, 산란 및 흡수가 모두 작은 저손실 반사경을 요구한다. 한편 링 레이저 자이로스코프의 경우 반사경의 산란이 곧 lock-in을 결정하여 성능을 제한하는 중요한 변수가 된다. 따라서 이 응용의 경우 반사경의 산란을 정확히 측정하는 일은 중요하며 위치에 따른 산란분포 정보를 알면 링 레이저 자이로스코프의 성능 예측과 개선이 더욱 쉬워진다. 산란을 측정하는 직접적인 방법에는 ARS(angle resolved scattering)과 TIS(total integrated scattering)이 있는데, 본 연구에서는 TIS 측정 장비를 반사경의 위치에 따른 산란분포까지 측정할 수 있도록 mapping 기능을 첨가하고 이온빔 스퍼터링에 의해 제작된 저산란 반사경을 측정하기 위해 높은 분해능을 갖도록 구성하였다. 반사경의 응용분야의 필요에 의해 45$^{\circ}$ 산란을 측정하였다. (중략)

• Journal of the Korean earth science society
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• v.33 no.7
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• pp.608-617
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• 2012

The symbiotic nova Z Andromedae (And) was investigated, using the high dispersion spectra of spectral resolution, ${\Delta}{\lambda}{\sim}-0.1{\AA}$. The spectral observations were done with (1) the Hamilton Echelle Spectrograph (HES) and the high resolution spectra (exposures=1800s and 3600s) were obtained at Lick Observatory in 2001 August $30^{th}$ (phase ${\Phi}$=0.77), and 2002 August $12^{th}$ (phase ${\Phi}$=0.22), (2) with the Bohyunsan Echelle Spectrograph (BOES) at Bohyunsan Optical Astronomy Observatory and the high resolution spectra (exposure=1200s) were secured in 2009 October $21^{st}$ (phase ${\Phi}$=0.70). From both the HES and BOES spectral data in the $3600{\AA}-9500{\AA}$ wavelengths, we extracted the emission lines of HI, HeI, and HeII, which have been decomposed into double or triple Gaussian components for 3 consecutive phases. The emission zones responsible for these components appear to be closely related with the orbital motion of a white dwarf or a giant star. The presence of the Raman scattering $H{\alpha}$ broad wing feature and the kinematic characteristics of the line profile observed in each phase imply that the Z And emission lines are mostly from two Lagrangian points, $L_1$ and $L_2$, and the accretion disk around the white dwarf star. The Z And was most active in 2009 and 2001 during the outburst phase, while it remained quiescent in 2002 in spite of the complex line profiles.

• Journal of Nuclear Fuel Cycle and Waste Technology(JNFCWT)
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• v.12 no.2
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• pp.97-105
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• 2014

In the case of the direct measurement of $^{226}Ra$ using a HPGe gamma-ray spectrometer, the interference between gammarays with 186.21 keV of $^{226}Ra$ and 185.7 keV of $^{235}U$ should be corrected to calculate the net peak area in the energy spectrum. In general, it is very difficult to conduct peaks stripping with difference of about 0.5 keV, although a HPGe with the superior resolution is applied and the maximum channels is applied to the spectrometer. In this study, several interference correction techniques in the direct measurement were surveyed to evaluate the feasibility for the measurement of $^{226}Ra$ using the gamma-ray spectrometery. Applying the interference corrections to the analysis of raw materials and by-products, the method validation for the direct measurement of $^{226}Ra$ was conducted by evaluating the measurement uncertainty, linearity, and range. As a result, the optimum method of the interference correction was selected by comparing with the indirect measurement of which progenies of $^{226}Ra$, such as $^{214}Pb$ and $^{214}Bi$, were analyzed in the secular equilibrium state.

• Investigative Magnetic Resonance Imaging
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• v.6 no.1
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• pp.64-72
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• 2002

Purpose : To introduce and demonstrate the advantages of the new hybrid two-dimensional (2D) proton spectroscopic imaging (SI) over the single voxel spectroscopy (SVS) and conventional 2D SI in the clinical application of spectroscopy for pediatric cerebral disease. Materials and Methods : Eighty-one hybrid 2D proton spectroscopic imaging was performed in 79 children (36 normal infants and children, 10 with hypoxic-ischemic injury, 20 with toxic-metabolic encephalopathy, seven with brain tumor, three with meningoencephalitis, one with neurofibromatosis, one with Sturge-Weber syndrome and one with lissencephaly) ranging in age from the third day of life to 15 years. In adult volunteers (n=5), all three techniques including hybrid 2D proton SI, SVS using PRESS sequence, and conventional 2D proton SI were performed. Both hybrid 2D proton SI and SVS using PRESS sequence were performed in clinical cases (n=). All measurements were performed with a 1.5-T scanner using standard head quadrature coil. The 16$\times$16 phase encoding steps were set on variable field of view (FOV) depending on the size of the brain. The hybrid volume of interest inside FOV was set as $75{\times}75{\times}15{\;}\textrm{mm}^3$ or smaller to get rid of unwanted fat signal. Point-resolved spectroscopy (TR/TE=1,500 msec/135 or 270msec) was employed with standard chemical shift selective saturation (CHESSI pulses for water suppression. The acquisition time and spectral quality of hybrid 2D proton SI were compared with those of SVS and conventional 2D proton SI. Results : The hybrid 2D proton SI was successfully conducted upon all patients.

• Analytical Science and Technology
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• v.23 no.3
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• pp.225-232
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• 2010

In present study, a conventional sol-gel method was used to prepare Fe-ACF/$TiO_2$ composites, a kind of composite photocatalysts, whose capability was evaluated by degrading methylene blue (MB) solution. The particle size, surface structure, crystal phase and elemental identification of the composites prepared were characterized by BET, SEM, XRD and EDX, respectively. The spectra of MB concentration degraded under visible light were obtained by UV/Vis spectrophotometer. These obtained spectra demonstrated the photocaltalytic activity from removal concentrations of MB. It was considered that these photonic activities are induced by a strong synergetic reaction among ACF, $TiO_2$ and Fe in the composite photocatalysts under visible light.

• Korean Journal of Remote Sensing
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• v.13 no.1
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• pp.13-30
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• 1997

Recent improvements of satellite remote sensing sensors which are represented by hyperspectral imaging sensors and high spatial resolution sensors provide a large amount of data, typically several hundred megabytes per one scene. Moreover, increasing information exchange via internet and information super-highway requires the developments of more active service systems for processing and analysing of remote sensing data in order to provide value-added products. In this sense, an advanced satellite data processing system is being developed to achive high performance in computing speed and efficieney in processing a huge volume of data, and to make possible network computing and easy improving, upgrading and managing of systems. JAVA internet programming language provides several advantages for developing software such as object-oriented programming, multi-threading and robust memory managent. Using these features, a satellite data processing system named as GeoPixel has been developing using JAVA language. The GeoPixel adopted newly developed techniques including object-pipe connect method between each process and multi-threading structure. In other words, this system has characteristics such as independent operating platform and efficient data processing by handling a huge volume of remote sensing data with robustness. In the evaluation of data processing capability, the satisfactory results were shown in utilizing computer resources(CPU and Memory) and processing speeds.

• Korean Journal of Optics and Photonics
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• v.23 no.4
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• pp.167-171
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• 2012

This paper reports on the stray light analysis results of a compact imaging spectrometer (COMIS) for a microsatellite STSAT-3. COMIS images Earth's surface and atmosphere with ground sampling distances of 27 m at the 18~62 spectral bands (0.4 ~ 1.05 ${\mu}m$) for the nadir looking at an altitude of 700 km. COMIS has an imaging telescope and an imaging spectrometer box into which three electronics PCBs are embedded. The telescope images a $27m{\times}28km$ area of Earth surface onto a slit of dimensions $11.8{\mu}m{\times}12.1mm$. This corresponds to a ground sampling distance of 27 m and a swath width of 28 km for nadir looking posture at an altitude of 700 km. Then the optics relays and disperses the slit image onto the detector thereby producing a monochrome image of the entrance slit formed on each row of detector elements. The spectrum of each point in the row is imaged along a detector column. The optical mounts and housing structures are designed in order to prevent stray light from arriving onto the image and so deteriorating the signal to noise ratio (SNR). The stray light analysis, performed by a non-sequential ray tracing software (LightTools) with three dimensional housing and lens modeling, confirms that the ghost and stray light arriving at the detector plane has the relative intensity of ${\sim}10^{-5}$ and furthermore it locates outside the concerned image size i.e. the field of view of the optics.

• Applied Microscopy
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• v.26 no.2
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• pp.105-121
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• 1996

투과전자현미경을 이용한 최근의 재료 분석기술에 대해 일본 토호쿠대학의 ASMA (Atomic Scale Morphology Analysis) 연구실에서 얻은 실험결과를 중심으로 설명하였다. 현재 토호쿠대학에서 가동 중에 있는 가속전압 1250 kV의 초고압 투과전자현미경은 분해능이 약 0.1nm이며, 이 전자현미경으로부터 얻은 고분해능상은 대형컴퓨터를 이용한 시뮤레이션에 의해 해석 할 수 있음을 나타내었다. 또한, 이러한 뛰어난 고분해능 특성을 가진 초고압 투과전자현미경과 최근 재료 분야의 전자현미경 시료 제작기술의 하나로서 크게 주목받고 있는 초박절편법 (Ultramicrotomy)을 이용한 헤마타이트 미립자의 내부구조 해석 결과를 나타내었다. 새로운 전자현미경 분석기법을 위한 주변장비의 눈에 띄는 발달중의 하나로서 전자현미경상을 디지탈 형태로 기록하고, 이를 효과적인 화상처리 기법으로 해석할 수 있는 Imaging Plate (IP)를 주목할 수 있다. 본 논문에서는 IP의 응용 예로서 IP를 이용하여 기록한 고분해능 전자현미경상과 전자 회절패턴의 정량해석 결과에 대해 나타내었다. 에너지분산 X-선 검출기를 이용한 새로운 분석기법의 예로서 전자 채널링 효과를 이용한 ALCHEMI법을 Ni-Al-Mn계 화합물에 대한 실험결과와 함께 나타내었다. 또한, 전자에너지 손실 분광 분석법을 이용한 최근 분석 결과로서 여러 구리 화합물의 전자구조 차이에 따른 구리의 $L_{23}$ 가장자리 피이크 변화를 나타내었다. 새로운 전자현미경법인 에너지 필터를 사용하여 $Al_{0.5}In_{0.5}As$의 전자회절 패턴의 백그라운드를 제거한 결과를 에너지 필터를 사용하지 않은 $Al_{0.5}In_{0.5}As$의 전자회절 패턴과 비교하여 나타내었다.

• Bulletin of the Korean Space Science Society
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• 2006.10a
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• pp.177-180
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• 2006

We observed $2.1218{\mu}m$ $H_2$ 1-0 S(1) emission from H II region A, which is located just next to Sgr A East and one of the nearest star forming regions to the Gatactic center. Cooled Grating Spectrometer 4 (CGS4) at the 3.8 m United Kingdom Infrared Telescope (UKIRT) was used with aa echelle grating at a velocity resolution of ${\sim}$ 18km s^{-1}$ and an angular resolution of ${\sim}$ 2 arcsec. Comparing the distributions and kinematics of the observed $H_2$ emission with radio continuum and $NH_3$ emission, we find no evidence that this H II region is interacting with Sgr A East. This conclusion supports that the star formation in this region has not been stimulated by the blast wave of Sgr A East.

• Journal of the Korean Magnetics Society
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• v.16 no.1
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• pp.92-97
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• 2006

A study of the adsorption site of CO in the Ni(111)$(2\times2)$-O/CO coadsorbed phase over different sample preparation temperatures revealed that the atop site is favoured. The Ni-C spacing is given by $1.77\pm0.01\;{\AA}$. A study of the adsorption site of Co in the Ni(111)$(2\times2)$-O/CO coadsorbed phase over different sample preparation temperatures revealed that the atop site is favoured. The Ni-C spacing is given by $1.77\pm0.01\;{\AA}$. The data from the sample prepared at 265 K showed atop sites, which is well consistent with vibrational spectroscopy, whilst the data from the low temperature preparation appears the mixture of atop and hop $(35\%)$. The occupation of hop hollow sites is probably due to an incorrect pre-coverage of atomic oxygen (different from 0.25ml). Similar observation of site mixture also found in recent high resolution XPS measurements using C 1s and O 1s chemical shifts.