• 한국자동차공학회논문집
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• 제21권5호
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• pp.82-86
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• 2013

The automotive weather strip has the functions isolating of dust, water, noise and vibration from outside. The core of weather strip is made of steel with stiffness. By using the wire formed as the core of weather strip, weight can be reduced as much as 35% by comparing with existing steel core. For this reason, forming wire is necessary to keep the zigzag shape as it is. The deformation which is occurred during forming process can be predicted and it can be used in case of manufacturing dies through CAE. In this paper, rolling process conditions are deduced and the springback amount is predicted after rolling process by using the simulation. The springback amount of product is measured by using optical microscope, and measurement result is compared with the simulation result of springback as the same condition. The suitable gap between dies to compensate springback after rolling process is predicted through simulation and it is used for manufacturing dies.

• Journal of Preventive Medicine and Public Health
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• 제27권2호
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• pp.274-285
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• 1994

The effects of resin on the respiratory health have been investigated in 309 workers from four iron and steel foundries and the results compared with those from 122 workers who were not significantly exposed to resin gas and silica dust at the same industries. Phenol-formaldehyde resin was used in the core making and molding processes and workers were exposed to their decomposition products as well as to silica dust containing particulates. The subjects were grouped according to formaldehyde, dust and other gas exposures, and smoking habits were considered also in thi analysis. Standardized respiratory symptom questionnaire was administered by trained interviewers. Chest radiograph, pulmonary funtion tests, and methacholine challenge tests were done. Environmental measurements at the breathing zone were carried out to determine levels of formaldehyde, respiable dust and total dust. Foundry workers had a higher prevalence of symptoms of chronic bronchitis with chronic phlegm and chronic cough when exposed to dust. Exposure to gas was significantly associated with lowered $FEV_1$ and obstructive pulmonary function changes. Exposure to formaldehyde and phenol gas was associated with wheezing symptom among workers, but $FEV_1$ changes after methacholine challenge were not significantly different among different exposure groups. When asthma was defined as the presence of bronchial hyperreactivity with more than 20% decrease in $FEV_1$ after methacholine challenge, 17 workers out of 222 tested had asthma. Fewer asthmatic welters were found among groups exposed to formaldehyde, gas and dust, which indicates a healthy worker effects ill a cross-sectional study. The concentration of formaldehyde gas ranged from 0.24 to 0.43 ppm among studied foundries. The authors conclude that formaldehyde and phenol gas from combusted resin is probably the cause of asthmatic symptoms and also a selection force of those with higher bronchial reactivity away from exposures.

• 한국결정성장학회지
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• 제13권4호
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• pp.199-204
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• 2003

전기로 더스트, 석탄회, 석분 등 폐기물을 재활용한 소성벽돌의 미세구조 및 조성분포를 SEM과 EBS로 분석하였다. 소성벽돌 시편 중 일부에서 갈색 매트릭스 위에 노란색 영역이 발견되었고 내부에는 갈색 영역 외에 흑색 black-core 영역이 존재하였다. 표면의 노란색 영역은 Zn이 주성분이었으며 흑색 black-core 영역은 매트릭스와 조성차이는 보이지 않았다. 소성벽돌 시편의 전 부분에 걸쳐 1$\mu\textrm{m}$ 크기의 mullite 결정상이 분포하고 있었으며 유리질에 의해 둘러싸여져 있었다. 이는 고령토와 석탄회 내의 alumino-silicate 화합물이 소성과정에서 meta-kaolinite를 거쳐 mullite로 전이된 것으로 사료된다. 시편 외부는 산화분위기가 조성되나 내부는 석탄회 및 더스트에 함유되어 있는 미연탄소분에 의해 환원분위기가 조성 되면서 발생한 가스에 의해 발포되어 흑색 black-core 영역에서는 수십 fm 크기의 구형 기공이 발견되었다. 벽돌 내부는 Al과 Si가 주성분이었고 소량의 Fe, K, Ca, Na를 포함하고 있었다 특히 Fe는 비정질상 표면에 원판형 Fe-rich 결정상으로 석출되어 존재하고 있었다. 시편 내부에서는 상대적으로 적은 양의 Zn이 발견되었고 외부에서는 내부에 있던 Zn이 환원되면서 표면으로 확산되어 Zn-rich 결정상을 표면에 형성하여 노란색 표피층을 형성하였다.

• 과학기술학연구
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• 제18권1호
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• pp.129-175
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• 2018

이 논문은 한국석면운동의 지식 정치적 측면을 검토한다. 2008년 본격적으로 시작된 석면운동은 석면오염을 한국 사회의 중요한 안전보건의제로 만드는 데 앞장서 왔다. 석면오염 측정은 특히 석면오염이 광범위하고 심각한 환경보건문제라는 주요 주장을 펼치는 데 매우 중요했다. 이 활동의 특징은 공정시험방법이 아닌 '먼지 분석법'을 활용했다는 것이다. 이 논문에서는 석면운동가들의 오염 조사 보고서와 삼성 본관 주변 석면오염 논란을 통해 먼지 분석법이 대항 지식으로서 권력을 획득하는 과정을 분석한다. 석면운동가들은 먼지 분석으로 얻은 측정 데이터를 활용해 그들의 주장에 언론의 이목을 집중시키고, 정책적 변화에 필요한 자원을 동원할 수 있었다. 그러나 규제기관을 중심으로 한 전문가 집단은 먼지 분석법이 신뢰할 수 있는 석면오염 측정방법이라는 석면운동가들의 주장에 동의하지 않았다. 이와 같은 결론을 내리는 데 측정 과정에서 표준적 방법의 사용 여부와 측정 데이터의 해석적 맥락이 중요한 기준으로 작용하였다. 먼지 분석법의 권위는 부분적으로 획득되었다. 그러나 먼지 분석법은 규제과학이 내포하는 가정들을 드러내고 사회적 토론의 대상으로 전환시켰다는 점에서, 사회 운동과 과학을 결합하여 규제기관과 전문가 집단의 측정에 도전한 석면운동의 특성을 잘 보여준다.

• 천문학회보
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• 제43권1호
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• pp.44.2-44.2
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• 2018

G33.92+0.11, classified as a core-halo UC HII region at a distance of 7.1 kpc, contains several sub-clumps (~20-200 solar masses) as identified by dust continuum emission. This source shows very complicated features associated with vigorous massive star-forming activities with a nearly face-on projection. The ambient gas is still accreting to the massive molecular clumps dynamically, while the whole cloud is under disruption by newly formed stars. Using the recent high resolution (< 0.2") ALMA observations, we investigate the detailed structure associated with the star-forming activities by comparing different chemical tracers. The sub-clumps having extremely complex morphologies still preserve cold dense gas together with the turbulent and dense warm gas resulted by newly formed stars and interaction with accreting gas. The accretion of the ambient gas may have occurred episodically to this source. Most recent star formation, which probably the third generation of star formation in this region, is taking place in the northern part (A5 clump). The relatively small mass (~ 1/3 of A1 or A2) and the lack of turbulent gas of this star-forming core may suggest that this core was formed already during the overall collapse of the whole cloud for the first star formation. We think that gravitational collapse of these sub-clumps appears as sequential star formation of this region. The later interaction with accreting gas may have not been a direct cause of the star formation activities of this source.

• 한국해양학회지:바다
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• 제26권2호
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• pp.135-144
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• 2021

동해 남한국대지 IODP Site U1430 시추 퇴적물 쇄설성 성분의 입도 자료에 대한 구성 성분 분해 결과 황사 입자와 화산재 입자를 대표하는 4개 구성 입도 집단이 구별되었다. 이 중 화산재 입자를 대표하는 2개 구성 입도 집단은 다양한 형태의 세립 및 조립 유리질 샤드들로 이루어져 있으며, 전체 입도 분포에서 0-82% 범위의 비율을 차지하고 있다. 분석된 입도 자료 중 화산재 유입 영향을 받은 자료를 제거하고 황사 입경 변화의 경향을 추출하기 위한 기준으로 화산재 구성 입도 집단 비율 33%가 적정한 것으로 판단된다.

• 자원리싸이클링
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• 제24권6호
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• pp.24-30
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• 2015

본 연구에서는 페로망간 제조공정에서 발생한 집진분의 황산침출에 대하여 조사하였다. 황산의 농도, 반응온도, 교반속도, 입자크기 및 고-액비가 집진분 중의 Mn과 Fe의 침출에 미치는 영향에 대하여 검토하였다. Mn과 Fe의 침출속도는 황산의 농도가 높고 반응온도가 높을수록 높아졌다. 실험결과를 입자수축모델을 이용하여 검토한 결과 침출반응은 입자표면에서의 화학반응에 의해서 율속되는 것으로 생각된다. Mn과 Fe 침출반응의 활성화에너지는 각각 79.55 kJ/mol과 77.48 kJ/mol로 계산되었다.

• 천문학회보
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• 제36권1호
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• pp.88.1-88.1
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• 2011

We present the FIMS/SPEAR FUV continuum map of The Taurus - Auriga - Perseus (TPA) complex, which is one of the largest local association of dark clouds located in (l,b)~([152,180],[-28,0]). We also present the result of FUV dust scattering simulation, which is based on Monte Carlo Radiative Transfer(MCRT) technique. Before the simulation we generate the model cloud using Hipparcos 77834 stars and the calculation of their E(B-V). From the density-integrated image and the cross section image of the modeled cloud we confirmed that the Taurus cloud is located in ~130pc. The cloud north of the California nebula is known for its two layered structure and we confirm that using the cross section image of the modeled cloud. In our modeled cloud, that two clouds are located at ~130pc and at ~300pc, respectively. Over the whole region the result image of simulation is well correlated with the diffuse FUV observed with FIMS/SPEAR. The dense core of the Taurus cloud, however, is not revealed completely in the map.

• 천문학회보
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• 제45권1호
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• pp.58.4-59
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• 2020

We present preliminary results of 1.1 and 1.3 mm dust continuum and 12CO (J=2-1) line data obtained with the Submillimeter Array toward six cores harboring Class 0/I objects in the λ Orionis cloud. They are located in bright rimmed clouds, which are exposed to the far-ultraviolet radiation field by the O-type star λ Ori. Compact dust continuum emission is observed from all six cores. Among the six cores, only one core G196.92-10.37 shows a signature of binarity with separation of 4000 AU. The numbers of singles and binaries in our sample are five and one, respectively and the derived multiplicity frequency (MF) is 0.17. This value is lower than those found in the binary surveys toward Class 0/I objects, which may be a hint for negative feedback by the nearby massive star, lambda Ori. The derived excitation temperature (Tex) using 12CO emission shows a lower median value (20 K) than those of triggered star-forming regions (30 K). The lower MF and Tex support our previous study that star formation was not triggered in the λ Orionis cloud. We aim to further investigate whether the Class 0/I YSOs in the λ Orionis cloud have less circumstellar materials and smaller accretion rates than in other filamentary clouds (e.g., Orion A & B), which might be attributed to negative feedback from the massive star in limiting accretion of protostars.

• 한국제4기학회지
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• 제19권2호
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• pp.55-58
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• 2005

A 120-cm core recovered from Lake Hovsgol, the northern Mongolia provides evidence for climate variability since the Marine Isotope Stage 3, representing a sharp lithological change. The lowermost part of the core consists of diatom-barren calcareous silty clay without coarse sands, framboidal pyrite, and biogenic components deposited during the MIS 3. Following the last glacial maximum, in-situ moss is included in the sediments, as lake-level was retreated by cold and dry environment with low precipitation. The AMS radiocarbon ages of the plant fragments match a marked lithologic boundary between 14,060 and 14,325 $^{14}C$ yr BP. The contents of coarse sands abruptly increase, indicating probably wind-derived sandy dust or coarse grains contributed from floating icebergs. And abundant framboidal pyrite grains were deposited in an anoxic environment, as reflected by high accumulation of organic matters at a low lake stand. During the deglaciation, quantities of coarse sands, ostracod, shell fragments, framboidal pyrite, and diatom markedly varies by regional and global scale climate regimes. Some allochthonous coarse sands were probably ice-rafted debris derived from floating icebergs. A rapid increase in diatom productivity probably marked the onset of Bolling-Allerod warming. Subsequent high concentration of framboidal pyrite probably represents a dry and cold condition, such as Younger Drays events. Consistent warm period with high precipitation at Holocene is documented by diatomaceous clayey ooze without framboidal pyrite, coarse sands, and ostracod.