• 한국환경과학회지
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• 제6권1호
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• pp.9-16
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• 1997

We investigated and analysed the actual conditions and characteristics of railroad noise levels for 17 sites in the vicinity of the Seoul-Pusan Line. The results i,we summarized as follows : 11 Railroad noise level ranged to 64 ~ 74 $L_{eq}$ dB(A) at day time and ranged to 60 ~ 72 $L_{eq}$ dB(A) at night time. 21 Increased night noise level depend on the increase of trains passing at night time. 31 The major factor of Increased noise level in the vicinity of stations are using loudspeakers and stream whistle on trains. 4) Decreased effect of noise according to distance is able to be described quantitatively using regression equations of multiplicative model. $L_{eq}$=$78.59^{X-0.056}$, n =25, r=-0.994, s.e. =1.007 $P_{av}$ = $105.68X^{-0.073}$, n =25, r =-0.997, s.e. = 1.007 Also increased and decreased effect of noise according to floor in apartment Is able to be described quantitatively using regression equations of multiplicative model. $L_{eq}$ = $64.238X^{0.0567}$, n = 39, r = 0.787, s.e. = 1.004 $P_{av}$ =79.963X0.0524, n =39, r =0.689, s.e. = 1.056 5) Average noise level in high floor is over 70 $L_{eq}$ dB(A) at day and night time. so more detailed soundproofing countermeasured in high floors apartment is required.

• 한국음향학회지
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• 제19권5호
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• pp.53-59
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• 2000

본 논문에서는 우리나라의 지형과 환경을 고려하여 전파환경을 분류하고, 1.95GHz에서 전파-전파특성을 연구하기 위해 PN 코드 상관 검파법을 이용한 다중지연파 측정 시스템을 구축하였다. 정확하고 기본적인 전파-전파 특성 측정을 위하여 우리나라의 특징적인 구조물인 시화공단을 선정하였다. 측정환경은 LOS와 N-LOS로 구분하여 전송거리에 따른 수신전력과 RMS 지연확산의 변화를 측정하였다. 측정결과 LOS의 수신전력은 -1.6dBm에서 -28.BdBm, RMS 지연확산은 0.023 ㎲∼0.22㎲이며 N-LOS의 수신전력은 -164Bm에서 -36.SdBm, RMS 지연확산은 0.068㎲∼0.37㎲가 측정되었다.

• 한국작물학회:학술대회논문집
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• 한국작물학회 1989년도 추계 학술대회지
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• pp.12-13
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• 1989

• 천문학회보
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• 제46권2호
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• pp.65.2-66
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• 2021

Observational studies of supernova (SN) feedback are limited. In our galaxy, most supernova remnants (SNRs) are located in the Galactic plane, so there is contamination from foreground/background sources. SNRs located in other galaxies are too far, so we cannot study them in detail. The Large Magellanic Cloud (LMC) is a unique place to study the SN feedback due to their proximity, which makes possible to study the structure of individual SNRs in some detail together with their environment. Recently, we carried out a systematic study of 13 LMC SNRs using [P II] (1.189 ㎛) and [Fe II] (1.257 ㎛) narrowband imaging with SIRIUS/IRSF, four SNRs (SN 1987A, N158A, N157B and N206), show [P II]/[Fe II] ratio much higher than the cosmic abundance. While the high ratio of SN 1987A could be due to enhanced abundance in SN ejecta, we do not have a clear explanation for the other cases. We investigate the [P II] knots found in SNRs N206, N157B and N158A, using optical spectra obtained last November with GMOS-S mounted on Gemini-South telescope. We detected several emission lines (e.g., H I, [O I], He I, [O III], [N II] and [S II]) that are present in all three SNRs, among other lines that are only found in some of them (e.g., [Ne III], [Fe III] and [Fe II]). Various line ratios are measured from the three SNRs, which indicate that the ratios of N157B tend to differ from those of other two SNRs. We will use the abundances of He and N (from the detection of [N II] and He I emission lines), together with velocity measurements to tell whether the origin of the [P II] knots are SN ejecta or CSM/ISM. For this purpose we have built a family of radiative shock with self-consistent pre-ionization using MAPPINGS 5.1.18, with shock velocities in the range of 100 to 475 km/s. We will compare the observed and modeled line fluxes for different depletion factors.

• 한국광학회지
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• 제7권3호
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• pp.227-231
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• 1996

2H-Pb $I_{2}$ 단결정의 반사스펙트럼을 10K에서 측정하였으며 기초흡수단 근처에서 n=1, 2, 3의 Wannier 엑시톤 계열과 $A_{EP}$ 선을 얻었다. $A_{EP}$ 선은 Nagamune 등의 보고와는 달리 라만스펙트럼의 2nd 포논에너지로부터 n=2 엑시톤과 2nd 포논의 결합상태로 생각된다. 또 2nd 포논은 이차 라만산란과정에서 LO 포논과 관련된 라만선으로 생각된다. Wannier 엑시톤 계열로부터 기상법으로 성장시킨 2H-Pb $I_{2}$ 단결정의 엑시톤 결합에너지와 반경은 각각 33meV와 14.angs.이었으며 n=1 엑시톤의 L-T 분리 에너지 값은 10K 에서 6.56meV로 동일 온도에서 측정된 발광스펙트럼에서도 같은 값으로 나타났다. 또 반사스펙트럼을 온도의 함수로 측정하였으며 그 결과 n=1 엑시톤의 반사선은 온도가 증가함에 따라 장파장 쪽으로 이동하였고 L-T 분리에너지가 증가하면서 엑시톤 반사선의 예리도도 감소함을 알 수 있었다.

• 대한기계학회:학술대회논문집
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• 대한기계학회 2001년도 춘계학술대회논문집E
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• pp.777-782
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• 2001

In this study, we used In-line orifice mixer for efficient chemicals mixing in water treatment. The method of using In-line orifice mixer has been already proved the improvement of water treatment efficiency. Numerical study was performed using FLUENT, a commercial code, to standard design and production of effective In-line orifice mixer. As variable for exactly standardizing, a proper ratio between an outer diameter of cone and a diameter of pipe, a distance between cone and orifice, a determination of orifice diameter for an optimal mixing, a distance between injection nozzle's position and cone, Numerical study has been performed for optimal standard and analyzed flow field on a basis of turbulent intensity in an orifice downstream.

• 한국자기학회지
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• 제14권1호
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• pp.52-57
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• 2004

본 연구에서는 ㎓ 대역의 박막 인덕터 특성을 수치해석 하였다. 인덕터의 기본 구조는 390$\mu\textrm{m}$${\times}$390$\mu\textrm{m}$, 5.5턴(turn), 선폭 10$\mu\textrm{m}$와 선간격 10$\mu\textrm{m}$의 사각 나선형이다. 주파수 특성은 10 ㎓까지 시뮬레이션 하였다. 기판은 Si, Sapphire, 유리와 GaAs를 모델로 하였고 도체는 Cu이다. 도체의 두께는 2$\mu\textrm{m}$로 고정하였다. 입력과 출력단자의 위치가 서로 반대가 되도록 하기 위하여 턴수는 n.5로 하였다. 기본 구조 인덕터는 초기 인덕턴스 13.0 nH,최대 인덕턴스 60.0 nH 그리고 공진주파수는 4.25 ㎓이었다. 기판의 유전상수가 증가하면 초기 인덕스는 거의 변화가 없으나 공진 주파수는 감소하였다. 인덕터의 턴수를 1.5에서 9.5로 변화시키면, 초기 인덕턴스는 2.9 nH며 16.9 nH로 포화되었으며 Q factor는 소폭 증가하였다. 인덕터의 선폭과 선간격을 증가시키면 초기와 최대 인덕턴스는 감소하였다. 공진 주파수는 증가하였으며, Q factor는 선폭과 선간격을 증가시키면 각각 증가와 감소를 나타내었다.

• 대한전기학회논문지:전기물성ㆍ응용부문C
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• 제53권10호
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• pp.495-499
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• 2004

Characteristics of ohmic Ni/Si/Ni contacts to n-type 4H-SiC are investigated systematically. The ohmic contacts were formed by annealing Ni/Si/Ni sputtered sequentially The annealings were performed at 950℃ using RTP in vacuum ambient and N₂ ambient, respectively. The specific contact resistivity(p/sub c/), sheet resistance(R/sub s/), contact resistance (R/sub c/) transfer length(L/sub T/) were calculated from resistance(R/sub T/) versus contact spacing(d) measurements obtained from TLM(transmission line method) structure. While the resulting measurement values of sample annealed at vacuum ambient were p/sub c/ = 3.8×10/sup -5/Ω㎠, R/sub c/ = 4.9 Ω and R/sub T/ = 9.8 Ω, those of sample annealed at N₂ ambient were p/sub c/ = 2.29×10/sup -4/Ω㎠, R/sub c/ = 12.9 Ω and R/sub T/ = 25.8 Ω. The physical properties of contacts were examined using XRD 3nd AES. The results showed that nickel silicide was formed on SiC and Ni was migrated into SiC. This result indicates that Ni/Si/Ni ohmic contact would be useful in high performance electronic devices.

• 천문학회지
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• 제43권3호
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• pp.65-74
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• 2010

We investigate ${\rho}$ Pup using the high resolution spectral observations taken from the VLT archive and observations at a 1.8m-Korean telescope with BOES spectrograph. The atmospheric parameters are determined using the iron-line abundance analysis. We derive an effective temperature value of $T_{eff}=6890{\pm}250K$, surface gravity of log g=$3.28{\pm}0.3$ dex, microturbulent velocity of ${\upsilon}_{micro}=4.1{\pm}0.4km\;s^{-1}$, and the iron abundance of log N=$7.82{\pm}0.15$. The projected rotational velocity of the star is close to ${\upsilon}$ sin i=3.5km $s^{-1}$. Asymmetric line profiles in the observed spectra and variation of this asymmetry with time show that both strong radial pulsation and weak non-radial pulsations are present in ${\rho}$ Pup.

• 전자공학회논문지D
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• 제34D권12호
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• pp.14-21
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• 1997

This study was conducte dto fabricate 2GHz circulator using Ca,Sn substituted UIG(yttrium iron garnet)ceramics. When the electric, magnetic and microwave properties were measured in Ca, Sn substituted YIG, the measured perimittivity and perfmeability in microwave frequencies were 16.25, 0.8964. For $Y_{2.4}$C $a_{0.3}$A $n_{0.3}$F $e_{3.5}$A $l_{1.5}$ $O_{12}$ garnet ceramics sintered at 1400.deg. C, the ferrimagnetic resonance line width (.DELTA.H) at 10GHz was 53 Oe and saturation magnetization was 375G. The strip-line circulator was simulated with 3-D FEM (finite element method) software and designed at the center frequency of 2GHz. The fabricated strip-line junction circulator using above YIG ceramics had insertion loss of 1.271dB, return loss of 23.843dB, isolation of 21.751dB at the center frequency 1.855GHz.z.z.z.z.z.z.