• 천문학회보
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• 제46권1호
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• pp.51.1-51.1
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• 2021

Spiral arms greatly affect gas flows and star formation in disk galaxies. We use local 3D simulations of vertically-stratified, self-gravitating, gaseous disks under a stellar spiral potential to study the effects of spiral arms on galactic star formation as well as formation of gaseous spurs/feathers. We adopt the TIGRESS framework to handle radiative heating and cooling, star formation, and ensuing supernova (SN) feedback. We find that more than 90% of star formation takes place inside spiral arms. The global star formation rate (SFR) in models with spiral arms is enhanced by less than a factor of 2 compared to the no-arm counterpart. This supports the picture that spiral arms do not trigger star formation but rather redistribute star-forming regions. Correlated SN feedback produces interarm feathers in both magnetized and unmagnetized models. These feathers live short, have parallel magnetic fields along their length, and are bounded by SN feedback in the lateral direction, in contrast to instability-induced feathers formed in our previous isothermal simulations.

• 해양환경안전학회지
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• 제12권4호
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• pp.267-272
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• 2006

버터플라이 밸브는 선박에서 냉각수와 유류 계통 등에 범용으로 널리 사용되고 있다. 이 연구에서는 유량조정에 따른 배관계통의 버터플라이밸브 후류 유동특성을 규명하기 위하여 입자영상 유속측정장치를 이용하여 밸브개도에 따른 유선과 속도벡터 분포에 관한 정량적인 데이터를 확보하였다. 또한 밸브 주위 유동장의 압력성분을 고찰하기 위하여 개폐각도를 6가지 경우로 변화시켜 정압을 측정하였다. 그 결과 실험관 벽면에서 측정된 압력의 분포는 디스크가 전개 상태인 $0^{\circ}$에서 $45^{\circ}$까지는 입구 압력은 일정한 상태로 거의 변화하지 않았으나 약 $60^{\circ}$ 이상에서부터 압력 상승과 점차 급격한 변동현상이 나타났다. 특히, $75^{\circ}$ 부근에서는 상류에서 급격한 압력 상승 경향을 보인 반면 하류 측은 압력변동이 적게 나타났다.

• Journal of Welding and Joining
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• 제31권3호
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• pp.66-75
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• 2013

In this study, the effect of coating thickness($20{\mu}m$ and $30{\mu}m$) on microstructure and tensile properties in Yb:YAG disk laser welds of Al-Si-coated boron steel (1.2mmt) was investigated. In the case of as welds, the quantity of ferrite was found to be higher in base metal than that in HAZ (Heat Affected Zone) and fusion zone, indicating, fracture occurrs in base metal, and the fracture position is unrelated to the coating thickness. Furthermore, yield strength, tensile strength of base metal and welded specimens showed similar behavior whereas elongation was decreased. On the other hand, base metal and HAZ showed existence of martensite after heat treatment, the fusion zone indicated the presence of full ferrite or austenite and ferrite during heat treatment ($900^{\circ}C$, 5min), After water cooling, austenite was transformed to martensite, and the quantity of ferrite in fusion zone was higher as compared with in base metal, resulting in sharply decrease of yield strength, tensile strength and elongation, which leads to fracture occured at fusion zone. In particular, results showed that because the concentration of Al was higher in 30um coating layer specimen than that of 20um coating specimen, after heat treatment, producing a higher quantity of ferrite was higher after heat treatment in the fusion zone; howevers, it leads to a lower tensile property.

• 한국광학회지
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• 제22권2호
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• pp.96-101
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• 2011

본 논문에서는 930 nm 대역 광섬유 결합 레이저 다이오드 여기광을 0.8 mm 두께의 얇은 디스크형 Yb:YAG 결정에 조사하여 레이저 발진 특성을 연구하였다. 구멍이 있는 구리판 사이에 레이저 결정을 고정시켜 발생된 열을 접촉 냉각시키는 구조를 채택하였고, 구리판 구멍 크기에 따른 조사 지점의 온도 변화를 발진 피크 스펙트럼 이동으로부터 조사하였다. 광섬유 결합 LD 여기 광에 대해 발진 레이저 출력은 기울기 효율 42.2%, 광변환 효율 34.8%로 높게 구현되었다. LD 여기 전류 및 구리판 구멍 크기가 증가함에 따라 여기광이 조사된 지점의 온도가 증가하였다. 구리판 구멍 크기가 결정 두께에 비해 상당히 큰 경우, 높은 여기광의 세기에서는 온도 상승이 선형 변화로부터 벗어남을 확인하였다.

• 한국추진공학회:학술대회논문집
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• 한국추진공학회 2004년도 제22회 춘계학술대회논문집
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• pp.165-172
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• 2004

LE-7A is the main engine of the H-IIA launch vehicle. Under its development, the nozzle suffered from two troubles during startup and shutdown transients of the engine. One is a large side load, which damages the actuator of the nozzle, and the other is damage on regenerative cooling tubes due to high heat load. It has been considered that these problems are caused by a peculiar separation pattern called Restricted Shock Separation (RSS). RSS is observed in several rocket nozzles, for example, LE-7A nozzle, Vulcain nozzle and so on. Their contours are not conventional truncated perfect (TP) nozzle - LE-7A nozzle is a compressed truncated perfect (CTP) nozzle and Vulcain nozzle is a thrust optimized (TO) nozzle. Although it is believed that the occurrence of RSS is affected by the nozzle contour, the mechanisms are not clarified sufficiently yet. In the present paper, a parametric numerical study is carried out to investigate the mechanisms of the occurrence of RSS in CTP nozzles during startup transient. The results show that RSS is caused by the adverse pressure gradient downstream of the Mach disk. The adverse pressure gradient is caused by the interaction of the pressure wave and Mach disk. The method to avoid the occurrence of RSS is also examined. A small step inside the nozzle affects the position of the separation point and prevents RSS. The result shows that the possibility that RSS can be suppressed by controlling the position of the separation point.

• 대한기계학회논문집A
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• 제39권1호
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• pp.89-94
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• 2015

본 연구의 목적은 열처리 전 후의 보론강 레이저 용접성을 비교하는 것이다. 일반적으로 보론강이 핫스탬핑 공정에 사용되고 있으며, 핫스탬핑 공정은 강판을 오스테나이트 온도까지 가열한 후 성형과 동시에 냉각하는 방법이다. 열처리후 보론강은 1500 MPa 이상의 고강도를 가진다. 따라서 본 연구에서는 보론강 및 핫스탬핑강의 레이저 용접성을 조사한 후 비교하였다. CW 디스크 레이저를 이용하여 레이저 출력 및 용접속도를 변화시켜가며 맞대기 및 겹치기 용접을 실시하였다. 맞대기 용접 결과, 핫스탬핑강에서 완전 용입을 얻을 수 있는 임계냉각속도가 보론강보다 낮았으며, 겹치기 용접결과 완전 관통이 일어난 용접 조건에서는 접합부 폭은 용접속도와 관계없이 거의 유사하였다.

• 천문학회지
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• 제29권spc1호
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• pp.171-172
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• 1996

We present the results of an rocket-borne observation of far-infrared [CII] line at 157.7 ${\mu}m$ from the diffuse inter-stellar medium in the Ursa Major. We also introduce a part of results on the [CII] emission recently obtained by the IRTS, a liquid-helium cooled 15cm telescope onboard the Space Flyer Unit. From the rocket-borne observation we obtained the cooling rate of the diffuse HI gas due to the [CII] line emission, which is $1.3{\pm}0.2 {\times} 10^{-26}$ $ergss^{-1} H^{-1}_{atom}$. We also observed appreciable [CII] emission from the molecular clouds, with average CII/CO intensity ratio of 420. The IRTS observation provided the [CII] line emission distribution over large area of the sky along great circles crossing the Galactic plane at I = $50^{\circ}$ and I = $230^{\circ}$. We found two components in their intensity distributions, one concentrates on the Galactic plane and the another extends over at least $20^{\circ}$ in Galactic latitude. We ascribe one component to the emission from the Galactic disk, and the another one to the emission from the local interstellar gas. The [CII] cooling rate of the latter component is $5.6 {\pm} 2.2 {\times}10$.

• 한국가스학회지
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• 제17권4호
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• pp.1-8
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• 2013

본 연구에서는 벌크 중합법을 이용한 폴리스티렌 중합공정의 폭주반응에 대한 열적 위험성을 가속속도열량계(ARC)와 소규모 반응열량계(MM)를 이용하여 평가하였다. 당해 중합공정은 반응온도 $120^{\circ}C{\sim}130^{\circ}C$로 운전되어져야 하며, $130^{\circ}C$ 이상의 반응온도에서는 반응 생성물의 급격한 점도 증가로 인하여 반응기의 온도제어 실패에 따른 폭주반응의 위험성이 존재하였다. 또한 당해 중합공정의 반응온도($120^{\circ}C{\sim}130^{\circ}C$)에서 공정운전 초기에 반응기의 냉각실패가 발생할 경우 폭주반응으로 인해 반응기의 온도와 압력이 각각 30 ~ 50분 이내에 약 $340^{\circ}C$, 5.3 bar 까지 급격히 상승하여 반응기의 파열판이 파열되거나 반응기가 폭발할 수 있는 열적 위험성이 높게 나타났다.

• 치위생과학회지
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• 제19권2호
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• pp.107-112
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• 2019

Background: Good oral health is important for systemic body health and quality of life. Spray oral cleansers are increasingly preferred because of their convenience of carrying and the ease of oral hygiene management. In addition, many kinds of oral cleanser products containing various ingredients with antibacterial, washing, and moisturizing effects are being manufactured. However, concerns about the safety and side effects of oral sprays are increasing, and there is very little information regarding the use and care of oral sprays is available to consumers. This study aimed to investigate the effects of oral spray on oral bacteria and tissue to elucidate the factors that need to be considered when using oral sprays. Methods: The effects of oral spray on the growth of dental plaque bacteria was assessed using disk diffusion assays. Cytotoxicity and morphological changes in oral epithelial cells were observed by microscopy. The effects of oral spray on dental plaque growth were also confirmed on specimens from permanent incisors of bovines by Coomassie staining. Results: The pH of spray products, such as Perioe Dental Cooling, Cool Sense, and Dentrix, were 3.65, 3.61, and 6.15, respectively. All tested spray products showed strong toxicity to dental plaque bacteria and oral epithelial cells. Compared with those on the control, dental plaque bacteria deposits on the enamel surface increased following the use of oral spray. Conclusion: Three types of oral spray, namely Perioe Dental Cooling, Cool Sense, and Dentrix, strongly inhibited the growth of dental plaque bacteria and oral epithelial cells. The oral spray ingredient enhanced dental plaque growth on the enamel surface. Users should be informed of precautions when using oral sprays and the need for oral hygiene after its use.

• 천문학회지
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• 제38권2호
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• pp.125-128
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• 2005

In this paper, we argue that the gigahertz peaked spectrum (GPS) quasars are special blazars, blazars in dense and dusty gas enviornment. The ROSAT detection rate of GPS quasars is similar to that of flat spectrum radio quasars (FSRQs), suggesting that the relativistic jets in GPS quasars are oriented at small angle to the line of sight. Due to strong inverse Compton scattering off infrared photons from dense and dusty nuclear interstellar media in GPS quasars, most of them may have significant soft gamma-ray and X-ray emission, which is consistent with ASCA X-ray observations. Because Compton cooling in GPS quasars is stronger than that in FSRQs, synchrotron emission in GPS quasars may less dominate over thermal emission of the accretion disk and hot dust, hence most GPS quasars show low optical polarization and small variability, consistent with observations. We suggest that it is the significant radio emission of electron/positron pairs produced by the interaction of gamma-rays with the dense gas and dust grains in GPS quasars that makes GPS quasars show steep radio spectra, low radio polarization, and relatively faint VLBI/VLBA cores. Whether GPS quasars are special blazars can be tested by gamma-ray observations with GLAST in the near future, with the detection rate of GPS quasars being similar to that of FSRQs.