• 대한원격탐사학회지
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• 제36권2_1호
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• pp.155-165
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• 2020

본 연구에서는 복사전달모델을 사용하여 다양한 변수환경(파장 (340 nm, 477 nm), 에어로솔 종류(스모크, 황사, 황산염), AOD (aerosol optical depth), 지표면 반사도, 관측기하)에 따라 에어로솔 유효 고도(aerosol peak height; APH)에 대한 O₄ 대기질량인자(air mass factor; AMF)의 민감도를 조사하였다. 전반적으로, 477 nm의 O₄ AMF 가 340 nm 보다 APH에 대한 민감도가 크고 안정적으로 산출 가능한 것으로 확인하였다. AOD가 높을 때 APH에 대한 O₄ AMF의 민감도가 커지는 것을 확인하였다. 477 nm에서는 340 nm 보다 지표면 반사도의 영향이 큰 것으로 나타났다. 태양천정각 증가에 따라 340 nm에서의 O₄ AMF가 감소하는 추세를 발견하였으며, 이러한 경향은 태양천정각 40°인 환경에서 높은 Rayleigh 및 Mie 산란에 의한 장벽효과로 인해 O₄ 흡수가 발생하는 광경로 길이가 줄어들기 때문인 것으로 사료된다. 477 nm에서는 태양천정각이 증가함에 따라 Rayleigh 및 Mie 산란에 의한 다중산란이 일부 발생하여 O₄ AMF가 비선형함수 형태로 증가하는 경향을 보였다. 마지막으로, AOD의 불확실성이 APH 산출오차에 미치는 영향을 조사하였다. 황산염 타입에 대한 APH 산출 시, AOD의 불확실성으로 인한APH 산출오차가 다른 에어로솔 타입보다 크게 나타났으며, 황사의 경우 AOD 불확실성에 대한 APH 산출오차에 대한 영향이 미미하게 나타났다. 이러한 결과는 각 에어로솔 타입의 흡수 산란 특성이 다양하기 때문에, 에어로솔 타입이 APH 산출 오차에 영향을 미칠 수 있음을 의미한다.

• 한국지구과학회지
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• 제26권8호
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• pp.790-799
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• 2005

본 연구에서는 충청남도 공주시에 위치한 공주대학교 자연과학대학 옥상에 설치된 분광복사측정기의 일종인 스카이라디오미터(Sky-radiometer)로 측정된 직달 및 산란 일사량을 이용하여 간접적으로 공주지역의 에어로솔의 광학적 특성을 분석하였다. 분석기간은 2004년 1월부터 12월까지이며 에어로솔의 광학적 특성의 분석에 활용된 알고리즘은 Skyrad.pack.3(Nakajima et al., 1996)이다. 주요 분석요소는 에어로슬의 광학두께(AOT), 단일 산란알베도(SSA), 옹스트롬 지수${\alpha}$ 및 에어로솔의 크기별 분포이며 분석결과의 질을 높이기 위하여 초기 관측 자료의 품질검사를 수행하였다. 공주지역의 연평균 AOT, ${\alpha}$ 및 SSA는 각각 0.46, 1.14, 그리고 0.91이며 계절 및 기상현상에 따라 큰 시간변동을 보이고 있다. 크기별 입자분포에서는 미세입자와 조대입자에서 최대치가 나타나는 쌍봉(bi-modal) 형태를 보이고 있으며 황사(Asian dust) 기간인 봄에는 조대입자의 총 부피가 크게 증가하고 여름에는 반대로 미세입자의 부피가 증가하는 계절변동을 보이고 있다. 이러한 현상은 봄철동안에 AOT와 SSA가 각각 크게 증가하고 감소하는 점에서도 확인되고 있다. 또한 공주지역의 에어로솔의 광학적 특성은 계절에 따라서 변화가 크게 나타나고 있으나 풍향의 영향은 거의 받지 않는 것으로 나타나고 있다.

• 한국입자에어로졸학회지
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• 제13권1호
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• pp.25-31
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• 2017

This paper offer the characteristics for the detection and classification of biological and non-biological aerosol particles in the air by using laser-induced-fluorescence (LIF) based Bio-aerosol Detection System (BDS). The BDS is mainly consist of an optical chamber, in-outlet nozzle system, 405 nm diode laser, an avalanche photo detector (APD) for scattering signal and photomultiplier tubes (PMT) for fluorescence signals in two different wavelength range ; F1, 510-600 nm and F2, 435-470 nm. The detection characteristics, especially ratio of fluorescence signal intensity were examined using well-known components : polystylene latex (PSL), fluorescence PSL, $2{\mu}m$ of SiO2 micro sphere, dried yeast, NADH, ovalbumin, fungicide powder and standard dust. The results indicated that the 405 nm diode laser-based LIF instrument can be a useful bio-aerosol detection system for unexpected biological threaten alter in real-time to apply for dual-use technology in military and civilian fields.

• 천문학회보
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• 제39권2호
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• pp.81.2-81.2
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• 2014

We have analyzed the archival data of far ultraviolet (FUV) observations made for the region of GSH 006-15+7, a large shell-like structure discovered by Moss et al. (2012) from the H I velocity maps. FUV emission is seen enhanced in the lower supershell region and is believed to originate from dust scattering of interstellar photons. A corresponding Monte Carlo simulation indicates that the supershell is located at a distance of $1250^{+750}{_{-500}}$ pc, similar to the previous estimation of 1.5{\pm}0.5 kpc based on kinematic considerations. The spectrum obtained for the lower supershell exhibits molecular hydrogen fluorescence lines: a simulation model for this candidate photodissociation region (PDR) yields a rather high total hydrogen density of $n_H{\sim}30cm^{-3}$ with H2 column density of $N(H_2){=}^{1017.5-20.0}cm^{-2}$. It is argued that the region is in a transition stage from a warm to a cool neutral phase. Strong C IV emission is also seen in the spectrum, but it is not believed to be associated with the supershell as the corresponding spectral map shows a broad region of enhancement both inside and outside the supershell.

• KIEAE Journal
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• 제11권1호
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• pp.3-8
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• 2011

Sound absorbing materials used for lightweight panels and interior material are mainly made of fibroid material such as glass wool or rock wool. However these fiber type sound absorbing materials have some problems such that sound absorption could be decreased as time goes by because of durability. In addition, dust scattering from fiber type material can cause another problem in health. In this point of view, this study aims to develop environment friendly sound absorbing material using Hwangto(so called loess or yellow soil), a traditional housing material. Hwangto is natural housing material in Korea and generally known for improving indoor air quality. Hwangto panel is made to construct on the floor, wall and ceiling, and expected that there is not enough absorption. Present study tried to develop environment friendly sound absorbing material that has high sound absorption performance with good environment performance in terms of air quality. Pore rate was designed to maximize the absorption in the specific frequency bands, and two kinds of backing space were applied in order to see the effect of backing space. As a result peak frequency that has maximum absorption is going high as the pore rate is increased. The backing space provides more absorption and makes the peak frequency down to low.

• 천문학회보
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• 제43권1호
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• pp.59.3-59.3
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• 2018

With a recent observational study of extended Lyman-alpha halos around individual high-z star-forming galaxies by Leclercq et al. (2017) using MUSE, we perform radiative transfer calculations to see if Lyman-alpha scattering can explain the spatial extents of the halos together with their spectra. We adopt a spherically-symmetric halo model in which Lyman-alpha sources and neutral hydrogen (HI) medium have exponential density distributions. The HI medium is set to have outflowing motion based on a momentum-driven wind scenario in a gravitational potential well. We run our Lyman-alpha radiative transfer code, LaRT, upon this halo model for various sets of parameters regarding the HI medium such as temperature, optical depth, density scale radius, outflow velocities, and dust content. We analyze simulation results to see the impact of each parameter on Lyman-alpha spectra and surface brightness profiles, and degeneracies between the parameters. We also find a parameter set that best reproduces simultaneously the observed spectra and surface brightness profiles of the MUSE Lyman-alpha halos.

• 한국정보처리학회:학술대회논문집
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• 한국정보처리학회 2017년도 추계학술발표대회
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• pp.1258-1261
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• 2017

1급 발암물질인 미세먼지 중 44.3%를 차지하고 있는 도로 비산먼지는 효과적인 미세먼지 농도 저감 대책의 방안 중 하나이다. 도로 비산먼지 제거는 일반적으로 특수 차량을 이용, 정해진 경로와 주기에 따라 운행된다. 이러한 운행방식은 도로의 오염 현황에 따른 효과적 경로 선정 및 운영이 어렵다. 본 논문에서는 도로 비산먼지 제거의 효율적인 경로 제안을 위해 대구지역에 분포된 KISTI 이동형 도시센싱 테스트베드에서 수집되는 고해상도의 실시간 지역별 오염 현황 데이터를 활용하여 실시간 오염도를 분석하고, LSTM(LONG SHORT-TERM MEMORY) 알고리즘을 활용하여 미래의 미세먼지 농도를 예측하였다. 기존 연구와 달리 지역별 상황을 고려한 데이터를 사용하여 선형 회귀 분석을 수행하였다. 실험 결과, 시간 속성을 고려한 LSTM이 MLP 보다 평균 제곱근 오차 값이 경우에 따라 최대 30% 더 작음을 확인했다. 본 연구를 기반으로 고해상도 사물 데이터 기반 예측 연구의 가능성을 보였으며, 미세먼지 예측 결과를 활용 유연하고 효과적인 도로 청소차량의 운행 경로를 설정에 활용될 수 있을 것으로 기대한다.

• 한국환경과학회지
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• 제7권2호
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• pp.185-190
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• 1998

$PM_{10}$ concentrations were measured In underground stores located In 4 major cities, Chunchon, Wonju, Donghae and Sockcho, In Kangwon-Do using scattering light Integated type digital dust indicator. Per- sonal exposure to $PM_{10}$ for two women(housekeeper and gaduate students and a man(undergraduate student) were measured also. The dimensional conversion factors for mass concentrations(K) showed some difference among un- derground stores which were 2.0, 2.7, 3.4, 2.6 mg/$m^2$.CPM In chunchon, Wonju, Donghae and Sockcho, respectively. Average PMlo concentrations at underground stores were 178mg/$m^2$ in Chunchon, 141mg$m^2$ in Wonju, 125 mg/$m^2$ Donghe and 59mg/$m^2$) Sockcho. The portion of $PM_{10}$ In total suspended particles was about 50~60% as deight The exposure of graduate student, housekeeper and undergraduate to $PM_{10}$ during 12 hours were 1004. 3 (mg/$m^2$) .hr, 907.0 (mg/$m^2$) hr and 691.2 (mg/$m^2$) hr, respectively. Personal exposure to $PM_{10}$ showed very different according to heP activity pattern and they had more than 90 % of their $PM_{10}$ exposure at Indoor environment.

• 한국지하수토양환경학회지:지하수토양환경
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• 제16권1호
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• pp.71-81
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• 2011

Cause of contamination in the study area nearby Jang Hang Refinery is dust scattering in refinery stack, and soil washing treatment is one of the proper technologies for soil remediation in this area. Site conditions frequently limit the selection of a treatment process. A treatment technology may be eliminated based on the soil classification or physicochemical characteristics of soil. This study was assessed the soil washing efficiency by conducting of soil characteristic analysis in the vicinity of Jang Hang Refinery Stack within a 2 km radius. Also, it was decided about remedial range with comparative analysis of As in soil by Korean Standard Test Method before/after revision, whereupon As concentration in soil showed a increasing tendency after revision. As a result, the soil washing using the size separation of soil was determined through identifying of As species in the soil. In this site, only particle size distribution and water content of soil can provide the initial means of screening for the potential use of soil washing.

• 천문학회보
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• 제44권2호
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• pp.37.1-37.1
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• 2019

We perform Lyα radiative transfer calculations for reproducing Lyα properties of star-forming galaxies at high redshifts. We model a galaxy as a halo in which the density distributions of Lyα sources and HI plus dust medium are described with exponential functions. We also consider an outflow of the medium that represents a momentum-driven wind in a gravitational potential well. We demonstrate that this outflowing halo model with Lyα scattering can successfully reproduce both the spectrum and the surface brightness profile of eight star-forming galaxies at z=3-6 observed with MUSE. The best-fit model parameters (i.e., the outflowing velocity and optical depth) for these galaxies are in good agreement with other studies. We also demonstrate benefits of using spectrum and surface brightness profile simultaneously to the constraints on model parameters and thus spatial/kinematic distributions of medium. We examine the impacts of individual model parameters and intrinsic spectrum on emerging spectrum and surface brightness profile. Further investigations on the escape fraction, spatially resolved spectra, and the spatial extent of Lyα halos are presented as well.