• 천문학논총
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• 제19권1호
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• pp.17-20
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• 2004

In this paper, the intensity ratio of [O I] $\lambda6300$ and $H_\alpha$ lines, which plays an important role in the study of warm (or diffuse) ionized interstellar medium, is calculated assuming collisional ionization equilibrium (or coronal equilibrium). The calculated ratio is compared with the previous works, and with the observations, obtained by Reynolds (1989) and Reynolds et al. (1998) with the Wisconsin Ha Mapper facility, toward the directions that sample the faint interstellar emission-line background. The comparison confirms that most of the Ha originates from nearly fully ionized regions along the lines of sight rather than from partially ionized H I clouds or layers of H II on the surfaces of H I clouds.

• Journal of Nutrition and Health
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• 제22권6호
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• pp.476-484
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• 1989

An epidemiological survey was made on dietary calcium intake, serum total calcium and ionized calcium ion, and serum lipid compositions. Compared with 120 normotensive controls, 101 hypertensive subjects were significantly higher in the levels of serum cholesterol and triglyceride, but lower in HDL-cholesterol and higher in the ratio of total choesterol/HDL-chol Hypertensive subjects were also significantly lower in the relative amount of fatty acids C18:2 but higher in those of C20:0, C20:2 and total amount of saturated fatty acids(longer than C14:0) than control serum. Patients were significantly lower in serum total calcium and ionized calcium ion concentrations and significantly less calcium ingestion from milk and dairy produces by feeding frequency test.

• 한국전기전자재료학회:학술대회논문집
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• 한국전기전자재료학회 1999년도 추계학술대회 논문집
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• pp.617-620
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• 1999

To reduce the consumption of chemicals and ultra pure water(UPW) in cleaning process used in device manufacturing, we proposed wet processes that use electrolytic ionized water(EIW), which is generated by electrolysis of a diluted electrolyte solution or UPW and systemically investicate the EIW\`s characteristics. EIW\`s pH values are increased in cathode chamber and decreased in anode chamber according to the electrolysis time and its varied ratio is reduced with time increasement. The variation of pH and ORP is increased accordin to the applied voltage until critical voltage. But more than that voltage, the variation is decreased because of ion\`s scattering effect. When electrolyte is added, the effects of electrolysis is increased because electrolyte acts as catalyst. But when the density of electrolyte is increased more than critical value, ion\`s flowage is obstructed and the effects of electrolysis is decreased.

• 천문학회지
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• 제9권1호
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• pp.1-6
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• 1976

The translational and reactive parts of thermal conductivity of a partially ionized solar magneto-plasma gas have been calculated based on Yun and Wyller's formulation (1972) along with Devoto's theory(1968). The computed results are presented as functions of temperature and pressure for given magnetic field strengths. The results of the calculations show that for most photospheric conditions the magnetic field does not play any important role in characterizing thermal properties of the ionized gas. However, when the gas pressure is low(e.g., P<10 dynes/$cm^2)$) the field becomes extremely effective even if its strength is quite small (e.g., B<0.1 gauss). The reactive part of the thermal transport is found to be very important when the gas is undertaking active ionization.

• 대한전기학회논문지
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• 제39권5호
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• pp.516-518
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• 1990

We have derived the equation which involves the variation of electron energy with time in a lowly ionized plasma when a low alternating electric field is applied. We consider only elastic collisions between electrons and neutral atoms. This equation is solved using the 4th-order Runge-Kutta method, and applied to argon gas discharge which is driven by source frequency of 100, 1K, 10K, 100K, and 1M (Hz). The results show that the variation of electron energy becomes flat with higher frequencies.

• 한국진공학회지
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• 제13권1호
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• pp.43-43
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• 2004

• 천문학회보
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• 제40권2호
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• pp.32.3-33
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• 2015

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 these two components grow in tandem. Feedback from actively accreting supermassive black holes (AGN), in the form of multi-phase gas outflows, has been argued to be the agent of this co-evolution. Here we employ the powerful GMOS integral field spectroscopy unit on the 8.2m Gemini-North telescope to investigate ionized gas outflows of luminous Type 2 AGN in the local Universe (z<0.1). Our sample of 6 galaxies is drawn from the Sloan Digital Sky Survey (SDSS) and was selected based on their [OIII] dust-corrected luminosity (>1042 erg/s) and signatures of outflows in the [OIII] line profile of their spatially integrated 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. We combine a careful spectral decomposition of the [OIII] and $H{\alpha}$ line profiles with spatial information on ~0.5kpc scales to understand the outflow kinematics and energetics in these objects. We find clear evidence for strong outflows in [OIII] and occasionally $H{\alpha}$ that are clearly driven by the ionizing radiation of the AGN. We kinematically and spatially decompose outflowing and rotating ionized gas components. We find [OIII] to be a better tracer of AGN outflows, while $H{\alpha}$ appears to be strongly affected by both stellar rotation and outflows induced by ongoing star formation. The observed kinematics and spatial distribution of the ionized gas imply a large opening angle for the outflow. Finally, we find the projected outflow velocity to decrease as a function of distance, while its dispersion shows a more complex structure with a potentially initially increasing trend (out to 0.5-1kpc distances).

• 한국진공학회지
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• 제9권4호
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• pp.394-399
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• 2000

Underlayer의 종류 및 두께가 Al 박막의 texture 및 면저항 변화에 미치는 영향을 연구하였다. Al의 underlayer로는 ionized physical vapor deposition(I-PVD)에 의해 제조된 Ti와 I-PVD Ti 위에 metalorganic chemical vapor deposition(MOCVD)에 의해 제조된 TiN을 적층한 구조가 사용되었으며, 각각에 대해 두께를 변화시키면서 Al 박막의 배향성, 면저항을 조사하고, $400^{\circ}C$, $N_2$분리기에서 열처리하면서 면저항의 변화를 조사하였다. I-PVD Ti만을 Al의 underlayer로 사용한 경우, Ti두께가 5 nm이어도 Al 박막이 우수한 <111> 배향성을 나타내었으나, Al-Ti반응 때문에 열처리 후 Al 배선의 면저항이 크게 상승하였다. I-PVD 와 Al 사이에 MOCVD TiN을 적용함에 의해 Al <111> 배향성의 큰 저하없이 Al-Ti 반응에 의한 면저항의 증가를 억제할 수 있었으며, MOCVD TiN의 두께가 4 nm 이하일 때 특히 우수한 Al <111> 배향성을 나타내었다.

• 천문학회보
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• 제41권1호
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• pp.35.2-35.2
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• 2016

We present a census of AGN-driven gas outflows based on the kinematics of ionized gas and stars, using a large sample of ~11,000 emission line galaxies at z < 0.3, selected from SDSS. First, a broad correlation between gas and stellar velocity dispersions indicates that the bulge gravitational potential plays a main role in determining the ionized gas kinematics. However, the velocity dispersion of the [OIII] emission line is larger than stellar velocity dispersion by a factor of 1.3-1.4, suggesting that the non-gravitational (non-virial) component, i.e., outflows, is almost comparable to the gravitational component. Second, gas-to-stellar velocity dispersion ratio increases with both AGN luminosity and Eddington ratio, suggesting that non-gravitational kinematics are clearly linked to AGN accretion. The distribution in the [OIII] velocity - velocity dispersion diagram dramatically expands toward large values with increasing AGN luminosity, implying that the launching velocity of gas outflows increases with AGN luminosity. Third, the fraction of AGNs with a signature of the non-gravitational kinematics, steeply increases with AGN luminosity and Eddington ratio, while the majority of luminous AGNs presents the non-gravitational kinematics in the [OIII] profile. These results suggest that ionized gas outflows are prevalent among type 2 AGNs. On the other hand, we find no strong trend of the [OIII] kinematics with radio luminosity, once we remove the effect of the bulge gravitational potential, indicating that ionized gas outflows are not directly related to radio activity for the majority of type 2 AGNs. We will discuss the implication of these results for AGN feedback in the local universe.

• 한국화재소방학회논문지
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• 제33권1호
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• pp.23-29
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• 2019

리튬이온 배터리와 같은 충전식 배터리는 에너지의 저장장치로서 최근의 에너지 이용의 변화에 따라 크게 주목받고 있을 뿐 아니라 실제로 다양한 소형 전기기기 및 전기 자동차의 전기에너지 저장시스템으로 폭넓게 적용되고 있다. 하지만 리튬이온 배터리는 화재나 폭발 등의 위험성이 항상 존재하여 사용의 폭을 제한시키고 있다. 배터리화재가 일반적인 화재와의 다른 특성은 여러 가지가 있지만 그 중에 가연물질이 전해질에서 이온화 되어있다는 특성이다. 본 연구에서는 배터리 화재를 이해하기 위해서 양이온과 전자 등으로 이온화된 메탄 제트화염에서의 연소특성을 실험적으로 관찰하였다. 화염 형상 및 화염안전성은 현재의 실험조건에서는 연료 이온화 효과가 없었고, 제트화염 후류에서 측정한 CO와 NOx의 농도가 이온화연료에서 모두 감소하는 것을 확인할 수 있었다. 또한 이온화 메탄 연소특성의 파라미터 연구를 위하여 수치해석의 반응기구를 수소첨가의 형태로 단순화하여 이온화연료의 연소특성을 모사할 수 있는지에 대한 모델링 검토를 수행하였다. 연료 이온화의 영향으로 수소의 농도는 증가시키되 반응 후 온도는 일정함을 가정하여 모델링하면 실험결과와 일치하는 결과를 얻을 수 있었다.