• 천문학회보
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• 제40권1호
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• pp.78.2-78.2
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• 2015

Powered by a supermassive black hole, active galactic nuclei (AGNs) are characterized by prominent emission lines including Blamer lines. The unification scheme of AGNs requires the existence of a thick molecular torus that may hide the broad emission line region. In this configuration, it is expected that the far UV radiation from the central engine can be Raman scattered by neutral hydrogen to reappear around Balmer lines which can be identified observationally with broad Balmer wings. Another mechanism that can form Balmer wings is considered by invoking a fast moving medium around the central engine. In this presentation, we produce Balmer wings that are formed through Raman scattering and also those expected from a fast moving emission flow. It is noted that Raman Balmer wings exhibit stronger red part whereas the opposite behavior is seen in the Balmer wings obtained from a fast moving emission flow.

• 한국가스학회지
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• 제8권3호
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• pp.24-30
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• 2004

본 연구에서는 개선된 view cell 실험 장치를 통하여 가스 하이드레이트 생성 과정을 관찰하고 이의 동특성을 고찰하였다. 순수한 물과 촉진제로 음이온계 계면활성제를 미량 첨가한 물에 천연가스를 넣어 가스 하이드레이트를 생성 과정을 관찰하였다. 본 실험에서 사용한 276.65 K, 6 MPa 조건 상태에서는 충분한 지체 지연 시간이후 물에 순간 교반을 줌으로써 형성자 생성을 쉽게 유도할 수 있었다. 가스 하이드레이트 필름의 생성은 정적상태에서 가스와 접촉된 물의 표면에 생성되었다. 이는 육안으로 구분하기 어려운 매우 얇은 막이 수초 안에 물의 표면 전체를 덮는 선행과정과 이후 다시 육안관찰이 쉬운 필름층이 재생성되었다. 순수한 물에는 짧고 굵은 섬유 다발의 형태로 끝 부분이 둥글게 말려서 결정이 형성된 모습인 반면 촉진제를 넣은 경우 작은 섬유 다발 형태로 길게 생성되었고 다른 다발과 접촉되어 엉킨 결정 상상을 보였다.

• 한국입자에어로졸학회지
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• 제9권1호
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• pp.7-21
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• 2013

Twelve-hour size-resolved atmospheric aerosols were measured to determine size distributions of water-soluble organic carbon(WSOC) during daytime and nighttime, and to investigate sources and formation pathways of WSOC in individual particle size classes. Mass, WSOC, ${NO_3}^-$, $K^+$, and $Cl^-$ at day and night showed mostly bimodal size distributions, peaking at the size range of $0.32-0.55{\mu}m$(condensation mode) and $3.1-6.2{\mu}m$(coarse mode), respectively, with a predominant condensation mode and a minor coarse mode. While ${NH_4}^+$ and ${SO_4}^{2-}$ showed unimodal size distributions which peaked between 0.32 and $0.55{\mu}m$. WSOC was enriched into nuclei mode particles(< $0.1{\mu}m$) based on the WSOC-to-mass and WSOC-to-water soluble species ratios. The sources and formation mechanisms of WSOC were inferred in reference to the size distribution characteristics of inorganic species(${SO_4}^{2-}$, ${NO_3}^-$, $K^+$, $Ca^{2+}$, $Na^+$, and $Cl^-$) and carbon monoxide. Nuclei mode WSOC was likely associated with primary combustion sources during daytime and nighttime. Among significant sources contributing to the condensation mode WSOC were homogeneous gas-phase oxidation of VOCs, primary combustion emissions, and fresh(or slightly aged) biomass burning aerosols. The droplet mode WSOC could be attributed to aqueous oxidation of VOCs in clouds, cloud-processed biomass burning aerosols, and small contributions from primary combustion sources. From the correlations between WSOC and soil-related particles, and between WSOC and sea-salt particles, it is suggested that the coarse mode WSOC during daytime is likely to condense on the soil-related particles($K^+$ and $Ca^{2+}$), while the WSOC in the coarse fraction during nighttime is likely associated with the sea-salt particles($Na^+$).

• 한국가축번식학회지
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• 제18권1호
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• pp.39-46
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• 1994

This experiment was carried out to develop an in vitro culture system for rabbit embryos. The zygotes or 2-cell embryos were collected from the oviducts of the superovulated and mated does with D-PBS/10% FCS at 24 hours after hCG injection. The in vitro developmental rate of blastocyst formation and the number of nuclei in the embryos were examined under the following treatments; 1) TCM-199 with 10% FCS, 2) EBSS with 10% FCS, 3) rabbit vitreous humor(VH), 4) TCM-199 with 10% FCS＋BOEC, 5) TCM-199 with 10% FCS＋ROEC, 6) EBSS with 10% FCS＋BOEC and 7) EBSS with 10% FCS＋ROEC. For a comparative study of in vivo and in vitro development, the fresh blastocysts, which were developed in vivo for 96 hours after hCG injection, were collected from the uterus and their numbers of nuclei were counted. 1. The zygotes or 2-cell embryos developed to the blastocyst stage in TCM-199, EBSS and VH at the rates of 93, 92 and 89%, respectively. 2. The higher developmental rates 95~98% of blastocyst formation was achieved when the embryos were co-cultured with a monolayer of bovine or rabbit oviductal epithelial cells in TCM-199 or EBSS. No significant difference in developmental rates was shown between bovine and rabbit oviductal epithelial cells. 3. In a comparative study of in vivo and in vitro development, the total numbers of nuclei were significantly less in the in vitro cultured embryos(104~224) than the in vivo developed embryos(1, 0090 at 96 hours after hCG injectin. 4. The mean cell cycle numbers in the embryos cultured for 72 hours in TCM-199 with 10% FCS, EBSS with 10% FCS, TCM-199 with 10% FCS＋BOEC, TCM-199 with 10% FCS＋ROEC, EBSS with 10% FCS＋BOEC and in vivo was 7.38, 6.63, 7.76, 7.69, 7.01 and 9.92, respectively. From these results, it can be suggested the optimal culture system for in vitro culture of rabbit embryos is a co-culture system with bovine or rabbit oviductal epithelial cells in TCM-199 with 10% FCS. Considering the significant reduction in total numbers of nuclei in the in vitro cultured embryos, the advanced research on development of in vitro culture system for rabbit embryos is expected.

• 한국결정성장학회지
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• 제30권4호
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• pp.136-142
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• 2020

아연결정유약은 결정생성의 요건을 맞추기 위해서는 조핵제의 생성 - 조핵제의 양 조절 - 결정의 성장 등의 까다로운 소성과정을 거쳐야 한다. 소성온도 폭이 좁고 아연의 상태에 따라 결정에 영향을 미치는 등 사용이 용이하지 않다. 아연결정생성을 촉진시켜 이를 Frit화하여 폭넓은 소성조건에서 안정적으로 재결정화도록 하여 상용유약으로 유약을 개발할 수 있다.

• 천문학논총
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• 제32권1호
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• pp.337-341
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• 2017

This paper reviews the requirements for far-infrared astronomy in the period following the SPICA satellite in the late 2020's. We take a very long view of the state of FIR astronomy and what facilities will be required in a twenty year timeframe. We show that spatial resolution to match that of observatories operating in the optical and mid-infrared and the radio will be a necessity. Moreover this high spatial resolution must be combined with high spectral and photometric sensitivity to provide the data required to further our understanding of planetary formation mechanisms, the history of star formation through cosmic time and the feedback between active galactic nuclei and their host galaxies in controlling star formation. We review three possible conceptual mission scenarios and comment on the possibility of realising them in the coming deades.

• 대기
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• 제27권4호
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• pp.499-509
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• 2017

Possible links among cosmic ray, cloud, and climate have scientific uncertainties. The reputed topics have been highly controversial during several decades. A link between the atmospheric ionization by galactic cosmic rays (GCR), which is modulated by solar activities, and global cloud cover was firstly proposed in 1997. Some researchers suggested that the GCR can stimulate the formation of cloud condensation nuclei (CCN) in the atmosphere, and then the higher CCN concentrations may lead to an increase of cloud cover, resulting in a cooling of the Earth's climate, and vise versa. The CLOUD (Cosmic leaving outdoor droplets) experiment was designed to study the effect of GCR on the formation of atmospheric aerosols and clouds under precisely controlled laboratory conditions. A state-of-the-art chamber experiment has greatly advanced our scientific understanding of the aerosol formation in early stage and its nucleation processes if the GCR effect is considered or not. Many studies on the climate-GCR (or space weather) connection including the CLOUD experiment have been carried out during the several decades. Although it may not be easy to clarify the physical connection, the recent scientific approaches such as the laboratory experiments or modeling studies give some implications that the research definitively contributed to reduce the scientific uncertainties of natural and anthropogenic aerosol radiative forcing as well as to better understand the formation processes of fine particulate matters as an important parameter of air quality forecast.

• 천문학회지
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• 제36권3호
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• pp.105-110
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• 2003

Recent observations of galaxy clusters in radio and X-ray indicate that cosmic rays and magnetic fields may be energetically important in the intracluster medium. According to the estimates based on theses observational studies, the combined pressure of these two components of the intracluster medium may range between $10\%{\~}100\%$ of gas pressure, although their total energy is probably time dependent. Hence, these non-thermal components may have influenced the formation and evolution of cosmic structures, and may provide unique and vital diagnostic information through various radiations emitted via their interactions with surrounding matter and cosmic background photons. We suggest that shock waves associated with cosmic structures, along with individual sources such as active galactic nuclei and radio galaxies, supply the cosmic rays and magnetic fields to the intracluster medium and to surrounding large scale structures. In order to study 1) the properties of cosmic shock waves emerging during the large scale structure formation of the universe, and 2) the dynamical influence of cosmic rays, which were ejected by AGN-like sources into the intracluster medium, on structure formation, we have performed two sets of N-body /hydrodynamic simulations of cosmic structure formation. In this contribution, we report the preliminary results of these simulations.