• 천문학회지
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• 제40권4호
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• pp.161-164
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• 2007

We calculate the evolution of multiple supernova (SN) explosions inside a pre-exiting bubble blown up by winds from massive stars, using one-dimensional hydrodynamic simulations including radiative cooling and thermal conduction effects. First, the development of the wind bubble driven by collective winds from multiple stars during the main sequence is calculated. Then multiple SN explosion is loaded at the center of the bubble and the evolution of the SN remnant is followed for $10^6$ years. We find the size and mass of the SN-driven shell depend on the structure of the pre-existing wind bubble as well as the total SN explosion energy. Most of the explosion energy is lost via radiative cooling, while about 10% remains as kinetic energy and less than 10% as thermal energy of the expanding bubble shell. Thus the photoionization and heating by diffuse radiation emitted by the shock heated gas is the most dominant form of SN feedback into the surrounding interstellar medium.

• 천문학회보
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• 제22권
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• pp.27.2-27.2
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• 1997

• 한국전산유체공학회지
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• 제15권1호
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• pp.1-8
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• 2010

RCCS is a passive safety-related system that removes the decay heat of VHTR when normal decay heat removal systems are in failure. Understanding thermo-hydraulics of RCCS is important to design a safer VHTR. RCCS consists of 292 cooling panels, which are placed in the reactor cavity. The layout of RCCS gives an idea that, for CFD simulations, cooling panels can be assumed to be one annulus tube. This assumption can reduce significantly the computational time, especially for the unsteady simulation. To simulate RCCS in an axisymmetric manner, three models were suggested and compared. Each model has (1) the same outer radius, (2) the same cross-sectional area (3) the same pressure drop, respectively, as the RCCS cooling panels. The steady-state simulation was conducted with these three models and the DO radiation model. It is found that over 90% of the heat from the outer wall of the reactor pressure vessel is transported to the RCCS by radiative heat transfer. The simulation with the third model, which has the same pressure drop as the design, estimates the closest wall temperature profiles to a thermo-hydraulic code, GAMMA+, result.

• 한국환경과학회지
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• 제16권3호
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• pp.261-267
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• 2007

In this study, the Slab Ocean Model (SOM) is coupled with an Atmospheric General Circulation Model (AGCM) which developed in University of Kangnung based on the land surface model of Biosphere-Atmosphere Transfer Scheme (BATS). The purposes of this study are to understand radiative role of clouds considering of the atmospheric feedback, and to compare the Clouds Radiative Forcing (CRF) come from the analyses using the clear-cloud sky method and CGCM. The new CGCM was integrated by using two sets of the clouds with radiative role (EXP-A) and without radiative role (EXP-B). Clouds in this two cases show the negative effect $-26.0\;Wm^{-2}$ of difference of radiation budget at top of atmosphere (TOA). The annual global means radiation budget of this simulation at TOA is larger than the estimations ($-17.0 Wm^{-2}$) came from Earth Radiation Budget Experiment (ERBE). The work showed the surface negative effect with $-18.6 Wm^{-2}$ in the two different simulations of CRF. Otherwise, sensible heat flux in the simulation shows a great contribution with positive forcing of $+24.4 Wm^{-2}$. It is found that cooling effect to the surface temperature due to radiative role of clouds is about $7.5^{\circ}C$. From this study it could make an accurate of the different CRF estimation considering either feedback of EXP-B or not EXP-A under clear-sky and cloud-sky conditions respectively at TOA. This result clearly shows its difference of CRF $-11.1 Wm^{-2}$.

• 천문학회지
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• 제29권spc1호
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• pp.253-254
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• 1996

To understand the dynamical structures of stellar wind bubble, one and two-dimensional calculations has been performed. Using FCT Code with cooling effects and assuming constant mass loss rate and ambient medium density, we could divide stellar winds into the regime of slow and fast winds. The slow wind driven bubble shows initially radiative and becomes partially radiative bubble in which shocked stellar wind zone is still adiabatic. In contrast., the fast wind driven bubble shows initially fully adiabatic and becomes adiabatic bubbles with radiative outer shell. We also determine analytically the onset of thin-shell formation time in case of fast wind driven bubble with power-law energy injection and ambient density structure. We solve the line transfer problem with numerical results in order to calculate line profile of [OIII] forbidden line.

• 천문학회보
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• 제45권1호
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• pp.70.3-70.3
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• 2020

Previous numerical simulations on planet-disk interactions revealed a lot of interesting phenomena including the planetary migration and the formation of many sub-structures inside the disks. However, these simulations were limited to an isothermal or adiabatic equation of state which does not account for various heating and cooling processes in the disks. Recent studies showed that the behavior of the planet-disk interaction can be significantly influenced by the disk thermodynamics. We develop a radiative diffusion module based on the two-temperature flux-limited diffusion approximation accounting for viscous heating and the accretion feedback. In this presentation, we describe our radiative diffusion solver, present some test results, and discuss potential applications of the module to planet-disk interactions,

• 한국지리정보학회지
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• 제15권4호
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• pp.124-137
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• 2012

기후분석은 도시 쾌적도를 고려하는 도시계획에 있어 중요한 요소 중 하나이다. 도시지역의 기후는 종관규모보다 작은 국지규모의 기후 영향을 받는데, 본 연구에서는 도시 안에서의 야간 지면냉각과 찬공기 생성 및 유입의 효과를 분석함으로써 도시지역의 국지기후에 대한 영향을 정량화 하고자 하였다. 서울관측소 풍속에 미치는 종관 기상의 영향은 30%정도인 반면, 관측소 주변의 지형 건물 열적 현상의 영향은 70%정도인 것으로 나타났다. 또한 서울 은평구 뉴타운의 연구지역에 대하여 서울기후분석(CAS, Climate Analysis Seoul) 모델로 분석한 결과, 국지영향 기온편차 분포에서 토지피복률에 따라 도시 및 도시외곽 지역의 기온 특성이 함께 존재하고 있음을 보여주었다. 또한 고밀도 관측 자료로부터 각 지점들의 시간대별 열적반응이 국지영향 기온편차 분포와 일치함을 알 수 있었다. 관측지점들 중 실개천을 따라 설치된 지점들의 일변동은 유사하게 나타났는데, 인근 산으로부터 경사면을 따라 유입된 찬공기의 생성, 이동, 정체는 관측된 수직기온경도를 이용하여 표현되었다. 실개천의 입구에서 관측된 수직기온경도는 지면 냉각에 의한 것과 외부로부터의 찬공기 유입이라는 두 가지로 설명될 수 있다. 지면냉각은 풍속과 관계없이 존재하지만, 찬공기 유입에 의한 냉각효과는 풍속이 낮을 때만 일어났다. 풍속의 강약에 따른 회귀분석식을 이용하여, 찬공기 유입 냉각효과는 국지적인 지면 냉각의 84%였다는 것을 밝혔다. 본 연구를 통해 지역특성이 국지기후에 미치는 영향의 크기를 기존의 정적인 기온영향 분석에서 동적인 찬공기 유입분석으로 확장하였다. 이 연구를 바탕으로 앞으로의 기후분석에서는 도시민의 쾌적도를 지원하기 위한 도시개발계획의 찬공기 특성 변화를 분석할 수 있게 될 것이다.

• 한국추진공학회:학술대회논문집
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• 한국추진공학회 2003년도 제21회 추계학술대회 논문집
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• pp.83-88
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• 2003

케로신과 액체 산소를 추진제로 하며, 10톤을 설계 추력으로 하는 우주 발사체의 2단용 액 체로켓엔진의 재생 냉각 특성 에 대한 해석적 연구를 수행하였다. 또한 보조적인 냉각 방법으로서 노즐 확장부에는 대기로의 복사 방열에 의한 냉각을 적용하였다. 본 연구를 통해, 케로신을 연료로 하는 10톤 추력의 2단용 액체로켓 엔진에서 재생 냉각과 복사 냉각에 의한 냉각 기구만으로는 냉각 방법으로 적합하지는 않다는 것을 확인하였다. 따라서 새로운 냉각 방법으로서 막냉각 기법이 도입되었으며, 액체로켓엔진의 열적 불안정성을 제거하는데 효과적인 냉각방법임을 알 수 있었다.

• 한국농림기상학회:학술대회논문집
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• 한국농림기상학회 2001년도 춘계 학술발표논문집
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• pp.68-71
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• 2001

밝고 바람이 없는 저녁, 지표근처의 냉각은 많고 일출 전후에 최저기온이 나타난다(Nishiyama, 1985). 그리고 기온은 지표근처에서 가장 낮고 고도가 높아질수록 높아진다. 이러한 상태를 지표역전(surface inversion) 또는 지면역전(ground inversion)이라 한다. 지표 역전층은 지표근처에 강한 복사냉각(radiative cooling)에 의해 형성되고, 다른 하나는 차가운 공기의 drainage에 의해 이류(advection) 되어 지표근처에 축적된다.(중략)

• 한국환경과학회지
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• 제10권5호
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• pp.329-336
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• 2001

Characgcteristics of nocturnal boundary layer(NBL) were analyzed by the upper-air observations data using with the airsonde and pilot balloons from 1994 to 1999 in Kyungpook province. The automate weather boundary layer can become stably stratified when the surface is cooler than the air. Stable nocturnal boundary layer height were estimated from the top of surface stable layer where the vertical gradient of temperature and mixing ratio tend to zero or negative. The depth of the stable nocturnal boundary layer depended largely on the thermal effect rather than the wind effect at nighttime. The NBL was more developed on the land than on the coastal region. The stability index (bulk Richardson number) showed that the NBL was stable when the wind was weak and the vertical gradient of the temperature was strong. The heat budget in the NBL was studied by considering the effect of the radiative and the cooled by both the longwave radiative flux and the divergence of the heat flux, while NBL under the cloudy sky the longwave radiative flux played a role of the warming. It was noted that the heat was not conserved in both cases. To complete the heat budget in the NBL the warming/cooling by advection and subsidence must be considered.