• 천문학논총
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• 제11권1호
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• pp.75-90
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• 1996

The vertical distribution of HCN, $HC_3N$ and $C_2N_2$ have been determined from a sequence of Voyager 1 IRIS limb tangent measurements over Titan's north polar region. This sequence yields gas distributions with ${\sim}200\;km$ altitude resolution over the 50-400 km range. The derived mixing ratios of HCN, $HC_3N$ and $C_2N_2$ are $5{\times}10^{-7}$, $7{\times}10^{-8}$ and $8{\times}10^{-9}$, respectively, at 120 km with a factor of 3 uncertainty.

• Bulletin of the Korean Chemical Society
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• 제15권10호
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• pp.821-824
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• 1994

• 설비공학논문집
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• 제27권11호
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• pp.559-566
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• 2015

The main objective of this work is to experimentally investigate the effect of angle variation on the distribution of two-phase flow at header-channel junctions. The cross-sections of the header and the channels were fixed at $16mm{\times}16mm$ and $12mm{\times}1.8mm$, respectively. Air and water were used as the test fluids. Four different header-channel positions were tested : Vertical header with Horizontal channels (case VM-HC), Horizontal header with Horizontal channels (case HM-HC), Horizontal header with Vertical Downward channels (case HM-VDC), and Horizontal header with Vertical Upward channels (case HM-VUC). In all cases, liquid flow distribution tended to decrease gradually in the upstream header region. However, in the downstream region, different trends could be seen. The reason for these different tendencies were identified by flow visualization in each case. The standard deviations for the liquid and gas flow distribution in each case were calculated, and the case of VM-HC had the lowest values compared to other cases because of the symmetrically distributed liquid film and strong flow recirculation near the end plate.

• 한국자동차공학회논문집
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• 제11권3호
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• pp.39-47
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• 2003

UEGI (Unburned Exhaust Gas Ignition) is an alternative method for fast light-off of a catalyst. It ignites the unburned exhaust mixture using two glow plugs installed in the upstream of the close-coupled catalysts. In addition, a hydrocarbon adsorber was applied to the UEGI, for more effective reduction of HC emission. Engine bench tests show that the CCC reaches the light-off temperature laster than the baseline exhaust system and HC and CO emissions are reduced significantly during the cold start. From the vehicle test, it was observed that a few amount of HC emission was reduced even the catalysts were aged. It is expected to develop a solution kit applicable to a new vehicle or used one, to meet the emission regulation

• 대한치과의사협회지
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• 제11권1호
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• pp.45-52
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• 1973

Ketamine HC1(Phencyclidine derivative) is a white, crystalline substance with melting point 259℃. It is soluble in water to a 20% clear, colorless solution. a 10% aqueous solution has a pH 3.5. The chemical structure is 2-(O-chlorophenyl)-2-(methylamino) cyclohexanone hydrochloride. It is a rapid acting, nonhypnotic, nonbarbiturate drug with a wide safety margin. The author used the anesthetic ketamine hydrochloride for oral surgery procedure in 16 patients(2 to 33 years). Anesthesia was achieved with a single intramuscular injection by introduction of manufacture. Result obtained as follows : 1. It was easily administered. 2. Onset time was rapid and duration was short. 3. The mild cardiac stimulation resulted in moderate increase in the blood pressure and pulse. 4. There was no significant respiratory depression. 5. The airway can be maintained without artificial support or endotracheal intubation. 6. All protective reflex maintained, which was important in oral surgery. 7. The best results were achieved in pediatric patients than adults.

• 한국버섯학회지
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• 제14권4호
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• pp.191-196
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• 2016

버섯 세균갈성색무늬병원균인 Pseudomonas agarici에 대한 길항미생물로 보고된 Alcaligenes sp. HC12 균주의 배양적 특성과 대량 배양을 위한 최적배양 조건을 설정하였다. HC12균주의 생육온도는 $20{\sim}40^{\circ}C$, pH는 6.0 이상에서 왕성한 생육을 보였다. 대량배양을 위한 효율적인 영양원 선발을 위하여 기본배지에 탄소원 fructose 등 18종, 무기질소원 $NH_4Cl$ 등 6종, 유기질소원 peptone 등 6종 그리고 아미노산 asparagine 등 11종을 각각 1%씩 첨가하였고, 무기염류 13종을 첨가하여 각각에 대한 생육에 미치는 영향을 조사하였다. 또한 선발된 각각의 영양성분들에 대한 최적 농도를 조사하기 위하여 각각의 성분을 최소 0.1%에서 최대 4.0%까지 배지에 첨가하여 배양 후 생육정도를 조사하였다. 그 결과, 대량배양을 위한 생육최적조건은 온도 $30^{\circ}C$, pH 9, 탄소원 0.5% dextrine, 유기질소원 1.5% yeast extract, 무기질소원 1.0% $NaNO_3$, 아미노산 1.5% asparagine 그리고 무기염류는 0.5% $KH_2PO_4$에서 왕성한 생육을 보였다.

• 한국융합학회논문지
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• 제11권10호
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• pp.53-61
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• 2020

최근 코로나19 바이러스로 인하여 언컨텍트 서비스가 본격적으로 활성화됨에 따라 비대면 접촉 원격 의료 서비스를 제공하기 위한 시스템 개발의 필요성이 증가하게 되었다. 본 연구에서는 원격진료를 지원하기 위한 스마트 헬스케어 시스템인 Rm_She(Remote Medical Smart Healthcare System)을 제안한다. Rm_She는 IoT를 기반으로 생체신호를 감지하는 다양한 헬스케어 제품을 하나의 애플리케이션으로 연결하여 여러 가지의 생체신호 정보를 수집 및 관리할 수 있다. 스마트 폰에 실행되는 헬스체크 앱(HC_app)을 이용하여 여러 종류의 생체신호 측정 장치와 무선랜으로 연결하고, 생체신호 값을 HC_app에서 전송 받아, 사용자에게 측정된 생체신호를 출력하고, 해당 정보를 헬스케어관리서버로 전송한다. 헬스케어 서버에서는 측정값을 전송 받아 데이터베이스에 저장하고, 저장된 측정값은 의료진들이 원격에서 실시간으로 모니터링 할 수 있도록 웹서비스로 제공한다.

• 대한기계학회논문집
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• 제11권5호
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• pp.819-827
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• 1987

본 연구에서는 예혼합화염에 물을 촘가하였을 때의 물/연료 체적비에 따른 화 염온도, 불완전가스농도(CO, THC, H$_{2}$), soot 농도를 측정하여 물이 연소효율에 미치는 영향을 고찰하고자 한다.

• Asian-Australasian Journal of Animal Sciences
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• 제13권9호
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• pp.1201-1204
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• 2000

We examined expression patterns of imc-415 gene in mammary gland and in HC11 mammary epithelial cells in culture. mRNA levels of imc-415 gene were higher at pregnancy and involution stages of mouse mammary gland compared with lactation period. Expression of imc-415 gene was induced with serum starvation or treatment with Fas monoclonal antibody in HC11 mammary epithelial cells in culture.

• 천문학회지
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• 제24권2호
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• pp.217-271
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• 1991

We have observed dense core around young stellar objects, DR21, S140, Orion-KL, and L1551 using four millimeter-wave transitions of $HC_3N\;J$=4-3, J=5-4, J=10-9, and J=12-11. The spatial distribution of $HC_3N$ emission closely resembles the morphology of the previous CS observations that trace high density gas. These observations reveal the existence of $HC_3N$ dense cores around central IR source, elliptical in shape and almost perpendicular to the CO bipolar outflow axis. Small differences can be explained by that $HC_3N$ molecular line is more optically thin and is seen to be more detailed structure in the neighborhood of central IR sources. In S140 and Orion-KL, massive(${\sim}10\;M_{\odot}$), slowly rotating dense cores lie near at the central IR sources of bipolar outflows. The velocity channel maps of DR21 show that the bipolar outflow gas may have a correlation with the dense core of DR21. We analyzed intensities of the four lines to derive physical conditions in dense core from two methods, LTE and LVG. The column density of $HC_3N$, $N(HC_3N)$, between LTE and LVG calculations agree well with each other. The abundances of $HC_3N$ in each observing source have been estimated using the average values of $n(H_2)$ and $N(HC_3N)$ and assuming the size of dense core. The fractional $HC_3N$ abundances in massive dense cores of DR21, S140, and Orion-KL have a range of $(2-7){\times}10^{-10}$, while that of low mass dense core, L1551, has one order of magnitude greater value of $2{\times}10^{-9}$. This should be considered good agreement with the result by Morris et al.(1976). It may be considered that dense cores of DR21, S140, and Orion-KL may have almost same stage of chemical evolution, and their abundances have a small values relative to that of L1551. The column density $N(HC_3N)$ decreases with increasing distance from the densest part of the cloud, the central infrared source, and have the relation of $N(HC_3N){\varpropto}R^{\alpha}$, where a has a range of 0.65 to 0.89. The values of $n(H_2)$ are not varied with increasing distance from the dense core, and have almost same values. Therefore, it is considered that the dense cores in these regions probably consist of dense clumps in diffuse molecular gas medium, and $n(H_2)$ of each clump is ${\sim}10^5\;cm^{-3}$. Levels in the $T_{ex}$ increases with $n(H_2)$. It is considered that the $HC_3N$ dense cores are not completely thermalized. We examine the relationships between the luminosity of central infrared sources versus mass of the dense cores, and the luminosity of central infrared sources versus molecular hydrogen column density. Luminosities of the central IR sources show good correlation with mass and hydrogen column density of the dense core. Same has been found from CS observations. However, mass and size derived from $HC_3N$ observations are one order of magnitude smaller than those from CS. It can be interpreted that we see more central part of the cloud cores in $NC_3N$ lines than CS lines.