• 천문학회지
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• 제29권spc1호
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• pp.123-124
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• 1996

Snapshots of eight SA and standard fields from low to high galactic latitudes were made using the KPNO 0.9m 2K $\times$ 2K CCD with a limiting magnitude from 19 to 22.5. The purpose of this study is to determine the vertical distribution of stars with respect to Galactic latitude and z-distance in comparison with the model simulation between intermediate population to the 'thick disk' component of scale height of a few kpc. Comparison of the preliminary results between observed and model simulation for 3 of the S fields shows good agreement both in V-mag and B- V color distributions. A bimodal distribution in B- V at high galactic latitude seems to be represented by a halo and 'thick disk' dwarf in the blue and by a normal disk dwarf population in the red.

• 천문학회보
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• 제43권1호
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• pp.36.2-36.2
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• 2018

Radiative transfer models were developed to understand the optical polarizations in edge-on galaxies, which are observed to occur even outside the geometrically thin dust disk, with a scale height of ~0.2 kpc. In order to reproduce the vertically extended polarization structure, we find it is essential to include a geometrically thick dust layer in the radiative transfer model, in addition to the commonly-known thin dust layer. The models include polarizations due to both dust scattering and dichroic extinction which is responsible for the observed interstellar polarization in the Milky Way. It is found that the magnetic fields in edge-on galaxies are in general vertical (or poloidal) except the central part, where the magnetic fields are mainly toroidal. We also find that the polarization level is enhanced if the clumpiness of the interstellar medium, and the dichroic extinction by vertical magnetic fields in the outer regions of the dust lane are included in the radiative transfer model. The predicted degree of polarization outside the dust lane was found to be consistent with that (ranging from 1% to 4%) observed in NGC 891.

• 대한기계학회:학술대회논문집
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• 대한기계학회 2003년도 추계학술대회
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• pp.115-120
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• 2003

In this study, smoke movement in tunnel fires was investigated with various aspect ratio(0.5, 0.667, 1.0, 1.5, 2.0) of tunnel cross section. Reduced-scale experiments were carried out under the Froude scaling using 8.27 kW ethanol pool fire. Temperatures were measured under the ceiling and vertical direction along the center of the tunnel. Smoke front velocity and temperature decrease rate were reduced as higher aspect ratio of the tunnel cross-section. Smoke movement was evaluated by analysis of vertical temperature distribution 3 m downstream from the fire source. Elevation of smoke interface according to N percent rule was under about 60% of tunnel height.

• 한국철도학회논문집
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• 제12권5호
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• pp.732-737
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• 2009

본 연구에서는 고속주행 시 팬터그래프에 가해지는 공기역학적 특성을 평가하기 위하여 고속철도차량용 실모형 팬터그래프에 대한 풍동시험을 수행하였다. 시험에 사용된 풍동은 공군사관학교의 중형아음속풍동으로서 폭 3.5m $\times$ 높이 2.45m $\times$ 길이 8.8m의 시험부를 가지며, 시험 모형은 하단의 차체부착용 브라켓에서 50cm의 수직 스트럿을 통해 풍동 바닥면에 지지되어 자유류가 시험부 바닥을 지나면서 성장하는 경계층의 영향을 제거하였다. 시험모델은 표준높이와 최소높이 및 풍동의 시험부를 고려한 최대높이에 대하여 정상주행방향 및 역방향 시의 조건을 바꾸어가며 수행되었다. 각각의 조건에 대해서 팬터그래프가 가선에 미치는 압상력을 측정하였으며, 시험 조건에 따른 압상력의 변화에 대하여 분석하였다.

• 한국지반신소재학회논문집
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• 제16권4호
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• pp.119-127
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• 2017

보강토체 상부에 작용하는 상재하중과 보강재의 인장강도 및 포설 단수가 보강토옹벽의 변형거동에 미치는 영향을 평가하기 위해 7종류의 축소모형 보강토옹벽을 축조하여 상재하중 재하실험을 수행하였다. 축소모형 보강토옹벽은 $100cm{\times}140cm{\times}100cm$ 크기의 모형토조 내에서 1m 높이로 축조하였으며, 인장강도가 상이한 3종류의 보강재를 사용하여 포설 단수를 5단, 7단, 9단으로 변화시키고, 5종류(50, 100, 150, 200, 250kPa)의 상재하중을 단계적으로 재하하면서 전면벽체의 수평변위와 보강재의 인장변형률 및 보강토체 저면의 수직응력 등을 측정하여 분석하였다. 분석 결과, 전면벽체의 수평변위는 보강토옹벽 하단부에서 가장 작고 보강토옹벽 하단으로부터 0.7H (H : 옹벽 높이) 지점에서 가장 큰 비선형적인 형태를 보여주며, 상재하중이 작고 보강재의 인장강도가 클수록 보강재의 상대적인 보강효과가 크게 발현되어 보강토체 하부의 수직응력이 작게 나타남을 알 수 있었다.

• 한국지리정보학회지
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• 제16권2호
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• pp.141-151
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• 2013

본 연구에서는 MODIS 인공위성으로 분석된 에어러솔 광학두께 자료와 지상에서 관측된 시정거리 자료를 이용하여 에어러솔 연직분포 모델링을 수행하였다. 위성과 지상관측자료로부터 에어러솔의 척도 고도를 구할 수 있었으며, 그 결과는 복사전달 모델에서 사용되고 있는 표준대기 모델과 비교에서 만족할 만한 수준의 근사치를 보였다. 그리고 실제 사례로서 대기가 청명한 경우(${\tau}_{MODIS}=0.12{\pm}0.07$, 시정거리=$21.13{\pm}3.31km$)와 혼탁한 경우(${\tau}_{MODIS}=1.71{\pm}0.85$, 시정거리 =$13.33{\pm}5.66km$)에 대해서 적용하여 척도 고도를 산정한 결과는 각각 전국 평균값으로서 $0.63{\pm}0.33km$와 $1.71{\pm}0.84km$로 나타났다. 그리고 이 결과를 바탕으로 대기 에어러솔 소산계수의 연직분포를 구할 수 있었으며, 최종적으로 KML 형식으로 코딩되어 관심 영역의 대기 환경 특성 변화를 감시하는데 도움이 될 것으로 기대된다.

• 한국농공학회논문집
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• 제48권4호
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• pp.33-40
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• 2006

In present study, the principal stress condition needed to conduct cubical large-scale triaxial test which can reflect three dimensional stress condition (or plain strain condition) in a dam was investigated by performing model test and numerical analysis and the principal stress ratio varying with the height of CFRD was examined. Also, the principal stress ratio in CFRD body was investigated from the monitoring results of horizontal and vertical earth pressure gages, installed in the center zone and lower part of transition zone of the dam body, respectively, in order to consider the principal stress condition in the large-scale triaxial test to model the behavior of CFRD. The result of the study indicated that the principal stress ratio decreased gradually from the lower to the upper part in the dam body for its center axis and was about 0.5 and 0.2 in the lower and upper part, respectively.

• 한국소음진동공학회:학술대회논문집
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• 한국소음진동공학회 2001년도 추계학술대회논문집 II
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• pp.647-652
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• 2001

A noise reduction of noise barrier for high speed train was measured by using scale down model test. A selected types of noise barriers were simple vertical barrier, interference type barrier with plate, interference type barrier with cylindrical pipes. On experiment, in order to make similar present test lane condition, reduced train model and multiple noise sources were considered. As a result. interference type noise barrier with cylindrical pipes is most effective than other barriers. A present height of noise barrier which is established in a test lane is not high enough for reducing patograph noise.

• 천문학회보
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• 제43권2호
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• pp.52.3-53
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• 2018

We compare vertical profiles of the extraplanar $H{\alpha}$ emission to those of the UV emission for 38 nearby edge-on late-type galaxies. It is found that detection of the "diffuse" extraplanar dust (eDust), traced by the vertically extended, scattered UV starlight, always coincides with the presence of the extraplanar $H{\alpha}$ emission. A strong correlation between the scale heights of the extraplanar $H{\alpha}$ and UV emissions is also found; the scale height at $H{\alpha}$ is found to be ~0.74 of the scale height at FUV. Our results may indicate the multiphase nature of the diffuse ionized gas and dust in the galactic halos. The existence of eDust in galaxies where the extraplanar $H{\alpha}$ emission is detected suggests that a larger portion of the extraplanar $H{\alpha}$ emission than that predicted in previous studies may be caused by $H{\alpha}$ photons that originate from H II regions in the galactic plane and are subsequently scattered by the eDust. This possibility raise an advantage in studying the extraplanar diffuse ionized gas. We also find that the scale heights of the extraplanar emissions normalized to the galaxy size correlate well with the star formation rate surface density of the galaxies. The properties of eDust in our galaxies is on a continuation line of that found through previous observations of the extraplanar polycyclic aromatic hydrocarbons emission in more active galaxies known to have galactic winds.

• 한국환경과학회지
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• 제7권3호
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• pp.335-348
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• 1998

The intensive meteorological observations including pibal balloon at Ungcheon, airsonde and 10m meteorological tower observations at Gulup-Do, where are located In the western coastal region, are taken to Investigate the characteristics of the upper and lower atmospheric structure and the local circulation pattern during the period of 17 to 22 September 1996. The diurnal variations of weather elements(i.e. air temperature, humidity, pressure, and Und speeds at Gulup-Do are analyzed and discussed with those at four inland meteorological stations. The vertical profiles of wind vector, ortho- gonality(Ω), and shear obtained from the pibal obsenrations are also presented to examine the change of wand structure according to the synoptic-scale pressure system's movement. The diurnal temperature changes at Gulup-Do are more sensitive than that of Inland meteorological stations In case of the mow of southwesterlies but are not dominant due to the ocean effect under the Influence of relatively cold northerlies. A well defined mixed layer Is developed from the 500m to the maximum 1700m with a significant capping Inversion layer on the top of it. It can be found from the vertical profiles of wind vector that the wind become generally strong at the interface heights between cloud lay- ers and non-cloud layers. The maximum Und shear Is appeared at the bel각t where the varlauon of wand direction Induced by the passage of synoptic-scale pressure system Is accompanied with the In- crease of Und speed. Based on the wind orthogonality, the change of wind direction with height is more complicated In cloudy day than In clear day. In case of a fair weather, the change of wand direction is showed to be at around 2km.