• 한국대기환경학회지
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• 제30권4호
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• pp.311-318
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• 2014

The goles of this study were that we calculated the difference between the emission factors currently used officially and the emission factors that calculated by atmospheric dispersion modeling results and actual field measurements of dust concentrations and that we investigated how we applied to the emission factors appropriate to the reality in Korea. At the results, we calculated the Business As Usual ambient dust concentration concerning U.S. EPA method emissions, and we thought that the emission reduction efficiency had to be 99.7% if the ambient dust concentration that measured in this study could be satisfied. In other words, U.S. EPA dust emission calculation method is very overestimated than reality, so it is important that our country obtain reliable construction site dust emissions estimation methods by continuous researches.

• 한국정보디스플레이학회:학술대회논문집
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• 한국정보디스플레이학회 2002년도 International Meeting on Information Display
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• pp.658-661
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• 2002

Chemical species during growth of carbon nanotubes (CNTs) in direct current-plasma enhanced chemical vapor deposition were studied in details using $C_3H_4-NH_3$ and $CO-NH_3$ mixtures through optical emission spectroscopy (OES). In the $C_3H_4-NH_3$ system, the relative intensities of CN (388.3 nm) and CH (431.4 nm) decreased and that of $C_2$ (436 nm) increased, leading to $sp^2$-graphization into the CNT structure, leading to improvement of field emission property of CNTs. In the $CO-NH_3$ system, the trend is completely reversed. Attributing to the atomic oxygen for helping the graphitization of carbon, CNTs could be grown under the flow rate of CO (180 sccm)-$NH_3$ (10 sccm). Through these results, we suggest the growth mechanism in our system.

• 천문학회보
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• 제42권1호
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• pp.56.1-56.1
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• 2017

When turbulent motions perturb magnetic field lines and produce magnetic fluctuations, the perturbations leave imprints of turbulence statistics on magnetic field. Observation of synchrotron radiation is one of the easiest ways to study turbulent magnetic field. Therefore, we study statistical properties of synchrotron polarization emitted from media with magnetohydrodynamic (MHD) turbulence, using both synthetic and MHD turbulence simulation data. First, we obtain the spatial spectrum and its derivative with respect to wavelength of synchrotron polarization arising from both synchrotron radiation and Faraday rotation. The study of spatial spectrum shows how the spectrum is affected by Faraday rotation and how we can recover the statistics of underlying turbulent magnetic field as well as turbulent density of electrons from interferometric observations that incorporate the effects of noise and finite telescopic beam size. Second, we study quadrupole ratio to quantitatively describe the degree of anisotropy introduced by magnetic field in the presence of MHD turbulence. We consider the case that the synchrotron emission and Faraday rotation are spatially separated, as well as the situation that the sources of the synchrotron radiation and thermal electrons causing Faraday rotation exist in the same region. In this study, we demonstrate that the spectrum and quadrupole ratio of synchrotron polarization can be very informative tools to get detailed information about the statistical properties of MHD turbulence from radio observations of diffuse synchrotron polarization.

• 천문학회보
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• 제39권1호
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• pp.63.2-63.2
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• 2014

As a part of the "Dust, Ice, and Gas In Time" (DIGIT) key program on Herschel, we observed GSS30-IRS1, a Class I protostar located in Ophiuchus (d =125 pc), with Herschel/Photodetector Array Camera and Spectrometer (PACS). More than 70 lines were detected within a wavelength range from 50 ${\mu}m$ to 200 ${\mu}m$: CO lines from J = 14-13 to 41-40, several $H_2O$ lines of Eup = 100 K to 1500 K, 16 transitions of OH rotational lines, and two atomic [O I] lines at 63 and 145 ${\mu}m$. The [C II] line, known as a tracer of externally heated gas by the interstellar radiation field, is also detected at 158 ${\mu}m$. All lines, except [O I] and [C II], are detected only at the central spaxel of $9^{\prime\prime}.4{\times}9^{\prime\prime}.4$. The [O I] emission is extended along a NE-SW orientation, which is consistent with the known outflow direction, while the [C II] line is detected over all spaxels. One possible explanation of the detection of the [C II] line and no correlation of its spatial distribution with any other molecular emission is the existence of the enhanced ISRF nearby GSS30-IRS1. One interesting feature of GSS30-IRS1 is that the continuum emission is extended beyond the point-spread function (PSF), unlike the molecular line emission, indicative of significant external heating. The best-fit continuum model of GSS30-IRS1 with the physical structure including flared disk, envelope, and outflow shows that the internal luminosity is 11 $L_{\odot}$, and the region is also externally heated by a radiation field enhanced by a factor of 25 compared to the local standard interstellar field.

• 한국농공학회논문집
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• 제64권6호
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• pp.55-63
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• 2022

Odors emitted from pig houses have been a constant root of legal issues in pig farming. These gases are among the main causes of health and mental stresses to nearby communities, so policymakers and researchers continuously study to reduce the concentration of odorous gases from pig facilities. A continuous field experiment proved that the concentration of odor emissions inside the pig houses is highly dependent on ventilation rate, breeding details, and animal activities. However, the standard odor emission rate worldwide widely varies due to differences in pig house designs and ventilation requirements. Thus, this study aimed to measure the odor emission rates, considering the actual condition of selected Korean pig houses, through field measurement. The odor measurements were performed at three different pig production facilities without odor abatement technologies. The target experimental pig houses were buildings for weaning, growing, and fattening pigs. Results showed that the actual ventilation rate in target pig houses falls below the standard ventilation requirement of pigs, resulting in high odor concentrations inside the pig houses.

• 한국토양비료학회지
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• 제38권3호
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• pp.150-156
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• 2005

논토양에서 관개 깊이를 조절하여 온난화가스 배출특성을 구명하고, 그에 따른 온난화가스 배출량를 추정하여 온난화가스 배출 저감기술을 확립하고자 연구를 수행하였다. 볏짚시용후 담수 8 cm의 시기별 $CH_4\;flux$는 이앙 32일 경에 $23.9mg\;m^{-2}\;h^{-1}$로 가장 높았으며, 이앙 35일 이후부터 감소하기 시작하여 중간낙수 이후에는 $CH_4\;flux$가 급격히 감소하였다. 포화용수량 처리구의 시기별 $CH_4\;flux$는 이앙 32일에 $19.9mg\;m^{-2}\;h^{-1}$ 로 가장 높았으며, 전 생육시기 동안 담수 8 cm와 담수 4 cm에 비하여 $CH_4\;flux$는 적었다. 볏짚 무시용후 시기별 $CH_4\;flux$는 이앙 20일경 $2.2-3.8mg\;m^{-2}\;h^{-1}$의 범위를 보였으며 그 이후부터는 처리별 차이가 컸으나 이앙 50일 이후부터는 비슷한 경향을 보였다. 토양 Eh 변화는 벼 이앙후 20일부터 -100 mV로 낮아 졌으며, 중간낙수 이후인 이앙 60일경에는 50 mV로 상승하였고 논물 담수심이 낮을수록 토양 Eh는 높았다. 볏짚을 시용하지 않았던 구와 포화용수량 처리구에서의 토양 Eh변화는 볏짚 시용구에 비하여 벼 전 생육기간에 걸쳐서 높았다. 처리별 지구온난화지수는 볏짚 시용후 담수 8 cm 처리구가 $6,939kg\;CO_2\;ha^{-1}$, 담수 4 cm 처리구는 $6,431kg\;CO_2\;ha^{-1}$, 포화용수량 처리구는 $5,222kg\;CO_2\;ha^{-1}$ 이었다. 그리고 볏짚을 시용하지 않은 담수 8cm 처리구의 지구온난화지수는 $4,449kg\;CO_2\;ha^{-1}$, 담수 4 cm 처리구는 $3,702kg\;CO_2\;ha^{-1}$, 포화용수량 처리구는 $3,561kg\;CO_2\;ha^{-1}$ 이었다.

• 한국재료학회:학술대회논문집
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• 한국재료학회 1999년도 추계학술발표강연 및 논문개요집
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• pp.171-171
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• 1999

• 한국재료학회:학술대회논문집
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• 한국재료학회 1996년도 재료학회 춘계학술발표회
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• pp.85-85
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• 1996

• 한국진공학회:학술대회논문집
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• 한국진공학회 2005년도 제28회 학술발표회 초록집
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• pp.147-147
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• 2005

• 전자공학회지
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• 제22권3호
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• pp.51-60
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• 1995