• Proceedings of the Korean Vacuum Society Conference
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• 2011.08a
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• pp.149-149
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• 2011

아르곤 기체의 방사세기 또는 그 세기 비는 플라즈마 공정 진단에서 일반적으로 사용된다. 본 실험에서는 100 mTorr 압력 조건하의 유도결합 플라즈마(13.56 MHz)에서 E-H 모드 전이 영역, rf 바이어스(12.5 MHz) 전력 인가 및 N2 혼합 시 단순화한 충돌-방사 모델에 기초한 광방사 세기비 방법을 적용하여 플라즈마 변수를 진단하였다. 개발 프로그램 기반의 분광기를 사용하여 아르곤 기체의 특정 파장(750.4, 751.5 그리고 811.5 nm)들을 관측하였고, 동일한 조건하에서 정전 탐침법으을 이용하여 전자 에너지 분포함수의 변화도 측정 하였다. 맥스웰 전자 에너지 분포를 가정하는 일반적인 경우와 비교하여 볼 때 실제적인 전자 에너지 분포함수의 측정은 전자의 가열 메커니즘에 대한 상세한 정보를 제공함과 동시에 플라즈마 재흡수에 대한 보정을 가능하게 해준다. 광방사 세기비법에 의해 측정된 결과에 의하면, 750.4 nm/751.5 nm는 높은 에너지(>13.08 eV)의 전자들의 유효 전자온도에 대한 정보를 나타내는 반면 811.5 nm/750.4 nm는 아르곤 준안정 준위 밀도(1s5)에 대한 정보를 제공하게 된다. 수행된 실험 조건하에서, 측정된 준안정 준위 밀도는 E-H 모드 전이 영역에서 최대값을 나타내었고 바이어스 전압 및 N2 기체 혼합 비율이 증가함에 따라 감소하는 결과를 얻었다. 유효 전자온도의 경우 광방사 세기비법과 정전 탐침법 모두 같은 결과를 보여 주었는데, E-H 모드 전이 영역에서는 전자온도는 거의 일정하였고 바이어스 전압 및 N2 기체 혼합 비율이 증가함에 따라 전자온도는 증가하였다. 이러한 실험 결과는 방전 모드 전이, 바이어스 인가 그리고 혼합 기체 사용하는 공정 플라즈마를 이해하는데 있어 이들 변수의 진단이 중요한 요소임을 보여준다.

• Journal of the Korean Society for Aeronautical & Space Sciences
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• v.30 no.6
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• pp.124-129
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• 2002

KAISTAT-4 is the fourth experimental microsatellite of KITSAT series which has been developed by Satellite Technology Research Center of KAIST for the last two years. The launch of KAISTSAT-4 is scheduled in 2003. The primary experimental payloads consist of Far-ultraviolet Imaging Spectrograph and Space Physis Package. In a similar way to KITSAT series, the interior of KAISTSAT-4 comprises mainly a set of stacked aluminium-alloy module boxes, each being capable of acting as the primary load path in the mechanical structure. The KAISTSAT-4 qualification model is now designed, fabricated, integrated, and tested to verify if the electrical and mechanical components work and can withstand the launch environments. All the required structural tests have been performed to a sufficient degree to satisfy the intent of the test requirements. This paper presents the structural system and launch environmental test results of KAISTSAT-4 qualification model.

• Journal of the Korean Magnetics Society
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• v.15 no.2
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• pp.113-117
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• 2005

Multiferroic $HoMnO_3$ single crystal was prepared using 4-point focused floating zone furnace, and polycrystalline $HoMn_{1-x}\;^57Fe_xO_3$ (x=0.00, 0.01, 0.02, 0.05) powders have been prepared by solid state reaction. Their magnetic and crystallographic properties are studied using MPMS, PPMS, and $M\ddot{o}ssbauer$ spectroscopy. The crystal structure found to be a hexagonal and a magnetic easy-axis is (110) direction. As the external applied magnetic field increases, temperature of the dielectric constant anomaly is decreased. $HoMn_{0.95}\;^{57}Fe_{0.05}O_3$ shows huge quadrupole splitting value from the $M\ddot{o}ssbauer$ spectra.

• Journal of the Korean Magnetics Society
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• v.7 no.4
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• pp.196-204
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• 1997

In order to study the effect of substituted $Al^{3+}$ of goethite, which was collected from Shinpyeongli in Cheju Island, we used X-ray diffractometer and Mossbauer spectrometer. In X-ray diffraction analysis, the X-ray diffraction peaks of goethite are not detected due to the high substituted Al contents of goethite. Isomer shifts indicated that the valence of Fe ions is almost oxidized trivalent of high spin state. It is believed that the contents of substituted diamagnetic $Al^{3+}$ for $Fe^{3+}$ is about 15.5 mol%. It seems that Neel temperature and saturated magnetic hyperfine field of the clay goethite are about 250 K and 498 kOe, respectively. For the temperature lower than Neel temperature, quadrupole splittings of the clay goethite are greatly influenced by $Al^{3+}$ substitution. It is believed that the high decrease of Neel temperature and magnetic hyperfine field of the clay goethite results from the magnetic dilution produced by substituting the diamagnetic $Al^{3+}$/TEX> for $Fe^{3+}$.

• Journal of Korean Society for Geospatial Information Science
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• v.14 no.1 s.35
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• pp.13-19
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• 2006

When investigating the damage of a forest fire, quite a few are depending on the naked eye observation. However, if the damage spreads to another area, it is easy to use the satellite images because it is hard to reach all the damaged areas on foot. From this research, we did a statistical interpretation of after fire using satellite image data to classify the damage on first and second factor analysis. As a result, it was more easier to classify the river's plants and ridges between rice fields that were in the forest fire damage area in the second observation then the first observation. Also, we could classify the area by areas that were damaged more or less using the second factor analysis. To verify this, we used the forest fire images collected from the satellite images and the actual survey data collected from spectral radiometer to see if these two datawere correlated and as a result we found out that they were highly involved.

• Journal of the Korean Chemical Society
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• v.47 no.2
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• pp.109-114
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• 2003

The electronic absorption spectra of trans-$[CrX_2([15]aneN_4)]ClO_4\;([15]aneN_4$=1,4,8,12-tetraazacyclopentadecane; X=F, Cl) complexes have been interpreted using the ligand field theory. An AOMX program is used to optimize the differences between the calculated and the observed positions for the spin-allowed transition bands. The crystal field theory(CFT) parameter is directly related to the angular overlap model(AOM), normalized spherical harmonic hamiltonians(NSH), and semiempirical parameters. The various ligand field parameters are discussed in terms of their chemical significances. According to the ligand field analysis, we can confirm that the fluoride ligand is a very strong ${\sigma}-$ and ${\pi}-$donor while the chloride has weak ${\sigma}-$ and ${\pi}-$donor properties toward chromium(III) ion.

• 한국지구과학회:학술대회논문집
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• 2010.04a
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• pp.121-121
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• 2010

행성상 성운 NGC 7009와 NGC 7027의 모델을 연구하기 위해 1998년 8월 14일부터 16일 까지 3일간의 Keck I HIRES의 분광 관측 자료를 이용하였다. 사용한 파장 영역은 $3250{\AA}{\sim}8725{\AA}$이고, H I, He I, He II, C II, C III, N II, N III, [N II], [O I], [O II], [O III], [S II], [S III], [Cl III], [Cl IV], [Ar III], [Ne III] 등의 방출선을 얻었다. 본 연구에서는 이러한 방출선의 선윤곽(line profile)을 IRAF와 StarLink/Dipso를 이용해 분석하여 성분을 구하였는데 H I, He I, He II, [O III], [C III], [N II] 등 대부분은 2개로 분리되었고, [S II], [Ar III]의 경우에는 3개로 분리되었다. 후자의 경우 구각(shell)의 단순한 팽창뿐만 아니라 다른 제3의 방향으로 팽창하고 있는 성분이 존재함을 의미한다. 비교적 S/N가 양호한 선들의 FWHM(Full Width at Half Maximum)을 측정하여 팽창속도를 구한 후 이 선들이 생성에 기여한 지역의 온도 또는 이온화 에너지 (IP)에 대한 팽창속도의 변화를 조사하였다. 또한 두 행성상 성운의 물리적 특성과 화학 원소 함량을 결정하기위해 광이온 모델 Tlusty Code와 CLOUDY를 사용하여 NGC 7009의 선행연구 Hyung & Aller(1995), Kwitter & Henry(1998)와 비교하였고, NGC 7027은 Zhang & Liu(2005), Middlemass(1990)와 비교하였다. NGC 7009과 NGC 7027의 수소 밀도($N_H$)를 $8,000cm^{-3}$으로 가정했을 때, NGC 7009의 중심별의 온도는 77,000K이고, 구각(shell)의 크기는 0.031~0.044pc이며 장축에 대해서만 결과를 나타내었다. NGC 7027의 경우, 중심별의 온도는 180,000K이고, 구각(shell)의 크기는 0.015~0.02pc으로 판단된다.

• Aerospace Engineering and Technology
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• v.10 no.2
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• pp.29-36
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• 2011

The Science and Technology Satellite-3 (STSAT-3) is based on the KITSAT-1, 2, 3 and STSAT-1, 2 which were Korea micro-satellites for the mission of space and earth science. The objectives of the STSAT-3 are to support earth and space sciences in parallel with the demonstration of spacecraft technology. The STSAT-3 carries an infrared (IR) camera for space & earth observation and an imaging spectrometer for earth observation. The IR payload instrument of the STSAT-3, Multi-purpose Infrared Imaging System (MIRIS), will observe the Galactic plane and North/South Ecliptic poles to research the origin of universe. The secondary payload instrument, Compact Imaging Spectrometer (COMIS), images the Earth's surface. The data acquired from COMIS are expected to be used for various application fields such as monitoring of disaster management, water quality studies, and farmland assessment. In this paper we present the operations concept of STSAT-3 which will be launched into a sun-synchronous orbit at a nominal altitude of 600km in late 2012.

• Analytical Science and Technology
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• v.16 no.3
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• pp.226-231
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• 2003

We analyzed the concentrations of heavy metals associated airbone particles by using AAS made by both a domestic manufacturer and one of the foreign manufacturer. One model developed by a domestic manufacture showed excellent results in the selected wavelength with an excellent performance of a monochromator. It abandons a big drop except a fine drop to improve reproduction in atomizer, so that no remains should leave. Using the low pass filter we were able to reduce a noise of detection signal. The performance of our equipment was found to be highly compatible with that of a foreign company as we achieved the detection limit of about $0.015{\mu}g/L$ using a standard solution of Au. The PM samples had been collected from by main observation points in 7 areas of Seoul city from 2001 to the spring in 2002. with these PM sample we analyzed the concentrations of Pb, Cu, Mn, Cd, Ni, Fe, Cr, Co, Mg and Al.

• Journal of the Korean Vacuum Society
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• v.12 no.4
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• pp.275-280
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• 2003

Epitaxial Gd$_2O_3:Eu^{3+}$luminescent thin films have been grout on Si(III) substrates using ionized Cluster Beam Deposition (ICBD). After the film growing, they were implanted and post annealed to change the crystal structure. The initial growth stage was monitored by using in-situ Reflection High Energy Electron Diffraction (RHEED). The formed crystal structure was identified with X-ray diffraction (XRD) technique and Fourier transform infrared (FT-R) spectroscopy. The electronic states variations were investigated by Near Edge X-ray Absorption Fine Structure (NEXAFS). Photoluminescence (PL), Cathodoluminescence (CL). and Vacuum ultraviolet (VUV) spectrum were used for examining the optical properties. We report the optical property changes depending on crystal structure and the electronic states.