• 대기
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• 제26권2호
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• pp.243-256
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• 2016

Total number concentration of aerosols larger than 10 nm ($N_{CN10}$), 3 nm ($N_{CN3}$), and cloud condensation nuclei ($N_{CCN}$) were measured during four different ship cruises over the Yellow Sea. Average values of $N_{CN10}$ and $N_{CCN}$ at 0.6% supersaturation were 6914 and $3353cm^{-3}$, respectively, and the minimum value of $N_{CN10}$ was $2000cm^{-3}$, suggesting significant anthropogenic influence even at relatively clean marine environment. Although $N_{CN10}$ and $N_{CN3}$ increased near the coast due to anthropogenic influence, $N_{CCN}$ was relatively constant and therefore $N_{CCN}/N_{CN10}$ ratio tended to decrease, suggesting that coastal aerosols were relatively less hygroscopic. In general $N_{CN10}$, $N_{CN3}$, and $N_{CCN}$ during the cruises seemed to be significantly influenced by wet scavenging effects (e.g. fog) and boundary layer height variation. Only one new particle formation (NPF) event was observed during the measurement period. Interestingly, the NPF event occurred during a dust storm event and spatial scale of the NPF event was estimated to be larger than 100 km. These results demonstrate that aerosol and CCN concentration over the Yellow Sea can vary due to various different factors.

• 천문학회보
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• 제36권2호
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• pp.117.1-117.1
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• 2011

We present the smoothness of mid-infrared sky brightness from the Japanese infrared astronomical satellite, AKARI observations. AKARI monitored the north ecliptic pole (NEP) during its cold phase with nine wavebands from 2.4 to 24 ${\mu}m$, out of which six mid-infrared bands are used in this study. Simple sinusoidal fit to the seasonal variation of the sky brightness shows that the mid-infrared brightness towards the NEP is not affected by small-scale features of the interplanetary dust cloud. We applied the power spectrum analysis to the images to search for the fluctuation of sky brightness. The fluctuation powers at 200 arcsecond are estimated to be at most $1.58{\pm}0.33\;nW\;m^{-2}sr^{-1}$ or 0.13% of the total brightness at $7{\mu}m$ and a tleast $0.64{\pm}0.11\;nW\;m^{-2}sr^{-1}$ or 0.02% at $18{\mu}m$. The residual fluctuations at a few arcminute scales at short mid-infrared wavelengths (7, 9, and 11 ${\mu}m$) are consistent with those expected from the diffuse galactic light. At long mid-infrared wavelengths (15, 18, and 24 ${\mu}m$) the measured fluctuations are comparable to or smaller than the one caused by photon noise and their sources are not identified. We conclude that the upper limit of the fluctuation in the zodiacal light is about 0.02% of the sky brightness.

• 천문학회지
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• 제48권6호
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• pp.343-355
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• 2015

There is much observational evidence that active star formation is taking place in the Hii regions Sh 2-255 – 257. We present a photometric study of this star forming region (SFR) using imaging data obtained in passbands from the optical to the mid-infrared, in order to study the star formation process. A total of 218 members were identified using various selection criteria based on their observational properties. The SFR is reddened by at least E(B −V ) = 0.8 mag, and the reddening law toward the region is normal (R_V = 3.1). From the zero-age main sequence fitting method it is confirmed that the SFR is 2.1 ± 0.3 kpc from the Sun. The median age of the identified members is estimated to be about 1.3 Myr from a comparison of the Hertzsprung-Russell diagram (HRD) with stellar evolutionary models. The initial mass function (IMF) is derived from the HRD and the near-infrared (J, J −H) color-magnitude diagram. The slope of the IMF is about Γ = −1.6 ± 0.1, which is slightly steeper than that of the Salpeter/Kroupa IMF. It implies that low-mass star formation is dominant in the SFR. The sum of the masses of all the identified members provides the lower limit of the cluster mass (169M_⊙). We also analyzed the spectral energy distribution (SED) of pre-main sequence stars using the SED fitting tool of Robitaille et al., and confirm that there is a significant discrepancy between stellar mass and age obtained from two different methods based on the SED fitting tool and the HRD.

• 천문학회보
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• 제41권1호
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• pp.37.2-37.2
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• 2016

There exist scaling relations that link the mass of supermassive black holes with both the velocity dispersion and the mass of the central stellar cusp of their host galaxies. This implies that galaxies co-evolve with their central black holes, potentially through the feedback from actively accreting supermassive black holes (AGN). We use integral field spectroscopy data from the 8.2m Gemini-North telescope to investigate ionized gas outflows in luminous local (z<0.1) Type 2 AGN. Our sample of 6 galaxies was selected based on their [OIII] dust-corrected luminosity (>$10^{42}erg/s$) and signatures of outflows in the [OIII] line profile of their SDSS spectra. These are arguably the best candidates to explore AGN feedback in action since they are < 1% of a large local type 2 AGN SDSS sample selected based on their [OIII] kinematics. Expanding on previously reported results concerning the kinematic decomposition and size determination of these outflows, here we report their photoionization properties and energetics. We find strong evidence that connect the extreme kinematics of the ionized gas with AGN photoionization. The kinematic component related to the AGN-driven outflow is clearly separated from other kinematic components, such as gravitation- or stellar-driven motions, on the velocity and velocity dispersion diagram. Our spatially resolved kinematic analysis reveals that up to 90% of the mass and kinetic energy of the outflow is contained within the central kiloparcec of the galaxy. The total mass and kinetic energy of the outflow correlate well with the AGN bolometric luminosity, resulting in energy conversion efficiencies between 0.01% and 1%. Intriguingly, we detect ubiquitous signs of ongoing circumnuclear star formation. Their small size, the centrally contained mass and energy, and the universally detected circumnuclear star formation cast doubts on the potency of these AGN-driven outflows as agents of negative feedback.

• 보존과학회지
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• 제28권4호
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• pp.297-303
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• 2012

안동 봉황사의 삼세불(三世佛)은 대웅전 후불탱화로 경상북도 유형문화재 406호로 지정되어 있다. 이들 탱화들은 조선시대 삼세불화 연구의 기준이 되는 작품으로 귀중한 의미를 지닌다. 본 연구에서는 이들 탱화가 그려진 바탕직물의 섬유에 대해 현미경 관찰 및 용해법과 감쇠 전반사이용 적외분광분석법, 주사전자현미경 등을 이용하여 섬유의 재질을 동정하였다. 실험을 위해 보존처리과정 중 수거된 약사불 시료 2점(A, B), 석가불 시료 1점(C), 아미타불 시료 1점(D)을 채취하여 사용하였다. 본 시료들에 대해 기존의 문화재 명칭에는 삼베로 기록되어 있었다. 열화가 심하고 두꺼운 먼지층을 형성하고 있어 육안으로는 감별이 어려웠으나 본 실험을 통하여 약사불 시료1점(A)을 제외하고는 모두 견직물임을 알 수 있었다.

• KEPCO Journal on Electric Power and Energy
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• 제6권4호
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• pp.455-460
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• 2020

In order to identify the characteristics of fine particle emissions from thermal power plants, this study conducted measurement of the primary emission concentration of TPM, PM₁₀ and PM_2.5 according to Korea standard test method (ES 01301.1) and ISO 23210 method (KS I ISO 23210). Particulate matters were sampled in total 74 units of power plants such as 59 units of coal-fired power plants, 7 units of heavy oil power plants, 2 units of biomass power plant, and 6 units of liquid natural gas power plants. The average concentration of TPM, PM₁₀, PM_2.5 by fuel are 3.33 mg/m³, 3.01 mg/m³, 2.70 mg/m³ in coal-fired plant, 3.02 mg/m³, 2.99 mg/m³, 2.93 mg/m³ in heavy oil plant, 0.114 mg/m³, 0.046 mg/m³, 0.036 mg/m³ in LNG plant, respectively. These results of TPM, PM₁₀ and PM_2.5 were satisfied with the standards of fine dust emission allowance in all units of power plants, respectively. Also, this study evaluated the characteristics of fine particle emissions by conditions of power plants including generation sources, boiler types and operation years and calculated emission factors and then evaluated fine particle emissions by sources of electricity generation.

• 융합신호처리학회논문지
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• 제19권4호
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• pp.167-173
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• 2018

빛이 부족하고 공기 순환이 원활하지 않은 실내에서 식물의 지상부와 지하부를 활용한 공기 정화 시스템을 제안한다. 제안된 시스템은 식물의 공기정화 효과를 극대화하고자 지상부는 청색과 녹색의 LED를 조합한 혼합광과 자연광에 가까운 고연색 LED를 각각 조사하고 지하부의 토양을 필터로 활용하고자 팬을 이용하여 강제 순환하였다. 광원과 팬이 결합된 실내공기정화 시스템이 식물만 배치된 경우보다 오염된 공기를 단시간에 가장 많이 제거하였다. 실내 공기정화 시스템의 혼합광과 고연색광 두 가지의 경우에서 식물만 배치된 경우보다 미세먼지는 각각 14%, 14.2%, TVOC는 7.5%, 9.4% 로 더 크게 감소하였다. 팬을 15분 동안만 가동한 실험에서도 TVOC가 97.8%로 크게 감소하였다. 식물의 광합성과 토양을 필터로 활용하는 것이 오염된 공기를 짧은 시간에 정화시킬 수 있었고 팬의 일시적인 가동으로도 지속적인 가동의 효과를 얻었다.

• 화약ㆍ발파
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• 제37권1호
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• pp.34-47
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• 2019

본 사례연구는 인천 학익동에 위치한 디씨알이 인천공장 발파해체 프로젝트에 관한 것이다. 대상건물은 건물내부에 위치한 굴뚝형태의 강구조 설비들이 가동 시 내뿜었던 수백도의 고열과 해풍 등의 영향으로 주요 구조체에 극심한 노후화가 진행되었다. 이로 인해 기둥과 보의 콘크리트들이 탈락하여 녹이 슨 철근들이 노출되어 있었고, 일부 슬래브들은 커다랗게 구멍이 뚫려있어 작업 인원의 접근도 힘들 만큼 구조물이 위험한 상태였다. 따라서 중장비가 건물 내부로 진입하여 작업하는 기계식 철거방법의 적용이 불가능하여 건물 내부의 설비구조물들을 그대로 두고 해체 할 수 있는 발파해체공법을 적용하였다. 발파순서는 (1)탄화탑 ${\rightarrow}$ (2)연돌 2 ${\rightarrow}$ (3)연돌 1의 순서로 진행되도록 계획하였다. 탄화탑과 연돌들에 설치된 폭약을 순차적으로 기폭시키는 데에는 총 406개의 전자뇌관(Unitronic 600)이 사용되었다.

• 한국보건간호학회지
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• 제33권1호
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• pp.5-19
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• 2019

Purpose: This study conducted to determine if people perceive differences in disaster preparedness, ego-resilience and disaster stress according to their perception of risk and disaster safety, safety of residence, disaster experience and disaster education experience. Methods: A total of 1,000 subjects voluntarily participated in a nationwide online survey. Data obtained were evaluated using the t-test and ANOVA. Results: The average scores were $2.66{\pm}0.73$, $2.64{\pm}0.81$, $2.89{\pm}0.85$, and $3.62{\pm}0.66$ out of 5 points for -the risk of disaster, disaster safety, safety of residence and interest in disaster, respectively. For 18.6% of the subjects who reported having experience with disaster, fine dust was the most common disaster experienced. Moreover, 50.1% of respondents reported earthquake was the most likely disaster. The disaster preparedness score was $4.91{\pm}3.75$ out of 16 points, ego resilience was $3.38{\pm}0.53$ out of 5 points, and disaster stress was $5.61{\pm}1.77$ out of 10 points. There were significant differences in disaster preparedness, ego-resilience and disaster stress depending on subjects' perception of safety or interest in disaster and their experiences or education regarding disaster. Conclusion: Our results suggest that it is necessary to increase awareness of disaster and to prepare a plan for persistent and systematic disaster education.

• Safety and Health at Work
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• 제12권1호
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• pp.114-118
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• 2021

Background: Exposure to particulate matter (PM) emitted from vehicle exhaust might disrupt systemic function and elevate the risk of cardiovascular disease. In this study, we examined the changes of cardiometabolic biomarkers among vehicle inspectors exposed daily to PM0.25 and components. Methods: This cross-sectional study was conducted at two vehicle inspection centers, Pulogadung and Ujung Menteng, located in East Jakarta, Indonesia. The exposed respondents were 43 workers from vehicle inspection centers, and the unexposed group consisted of 22 staff officers working in the same locations. Vehicle exhaust particulate matter was measured for eight hours using a Leland Legacy personal pump attached to a Sioutas Cascade Impactor. The used filters were 25 and 37-mm quartz filters. The particulate matter concentration was analyzed using a gravimetric method, whereas trace elements were analyzed using energy dispersive X-ray fluorescence. An EEL Smoke Stain Reflectometer analyzed black carbon. Results: The personal exposure concentrations of PM0.25 were 10.4-fold higher than those in unexposed groups. Calcium and sulfur were the major components in the obtained dust, and their levels were 3.3- and 7.2-fold higher, respectively, in the exposed group. Based on an independent-samples t-test, high-density lipoprotein, triglyceride, HbA1c, total immunoglobulin E, high-sensitivity C-reactive protein, tumor necrosis factor-alpha, and nitric oxide levels were significantly different between the groups. Conclusions: In summary, it was suggested that PM0.25 exposure from vehicle exhaust might affect cardiometabolic biomarkers change.