• 천문학회지
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• 제47권1호
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• pp.15-39
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• 2014

Polarization is a basic property of light and is fundamentally linked to the internal geometry of a source of radiation. Polarimetry complements photometric, spectroscopic, and imaging analyses of sources of radiation and has made possible multiple astrophysical discoveries. In this article I review (i) the physical basics of polarization: electromagnetic waves, photons, and parameterizations; (ii) astrophysical sources of polarization: scattering, synchrotron radiation, active media, and the Zeeman, Goldreich-Kylafis, and Hanle effects, as well as interactions between polarization and matter (like birefringence, Faraday rotation, or the Chandrasekhar-Fermi effect); (iii) observational methodology: on-sky geometry, influence of atmosphere and instrumental polarization, polarization statistics, and observational techniques for radio, optical, and $X/{\gamma}$ wavelengths; and (iv) science cases for astronomical polarimetry: solar and stellar physics, planetary system bodies, interstellar matter, astrobiology, astronomical masers, pulsars, galactic magnetic fields, gamma-ray bursts, active galactic nuclei, and cosmic microwave background radiation.

• 한국태양에너지학회 논문집
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• 제33권4호
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• pp.101-110
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• 2013

The propose of this study is to understand the phenomenon of radiation and comparison of analysis of two methods. One is analysis method of same-time data and the another is analysis method of rank data. We confirmed that two methods of correlation analysis had the effectiveness and suitability. The followings are main results from this study. 1) The seasonal correlation coefficient of long and short-wave radiation is higher in winter than in summer because of high humidity in the summer season can makes easily cloud in the sky locally. 2) According to analysis method, there is big difference in correlation coefficient from 0.494(Analysis method of same-time data) to 0.967(Analysis method of rank data) with short-wave radiation by the location during summer. These results have significant value in solar radiation research and analysis. It has explored a new way for solar radiation research of analysis method as well.

• Ecology and Resilient Infrastructure
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• 제7권1호
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• pp.43-52
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• 2020

본 연구는 컴퓨터 모델링의 결과를 실측자료 보정없이 이용하였을 때의 문제점을 조사하기 위해, 작은 도시공원을 대상으로 실측자료와 컴퓨터 모델링 결과를 비교 분석하여 보았다. 컴퓨터 모델링 결과는 실측자료에 비해 미기후 요소인 기온과 풍속에서는 과소예측을 보였으며, 상대습도와 평균복사온도에서는 과대예측을 하는 것으로 나타났다. 그 차이는 인간 열환경지수인 PMV와 UTCI에서 최대 2.3 PMV와 4℃ UTCI의 차이를 보였다. 그러므로, 인간 열환경지수 (열쾌적성) 연구에서 컴퓨터 모델링을 이용할 때는 반드시 실측자료를 이용한 결과보정 과정을 거쳐 도시와 조경계획 및 디자인에 적용되어야 할 것이다.

• 한국항공우주학회지
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• 제33권9호
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• pp.89-96
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• 2005

이 논문에서는 주간 항법용 별센서의 실제 활용을 목적으로 주간 대기 조건과 주간 별 감지 가능성을 논한다. 주간동안의 대기 자료를 구하기 위해 표준 대기 모델(LOWTRAN 7)을 사용했으며 그 모델로부터 배경하늘에 대한 복사와 대기투과도를 구하였다. 대기 복사량을 감소시키기 위해 광학 필터를 장착한 별센서를 가정했으며 태양 복사 효과를 나타내기 위해 별센서와 태양 사이의 다양한 분리각을 설정하였다. 별센서의 FOV에 대한 고려로서, 하늘 배경 복사의 변화와 감지가능한 별의 개수 밀도를 분석하였다. 또한 요구되는 신호 대 잡음비를 얻기 위한 노출시간과 별센서의 주간 활용 한계로서 작용하는 CCD의 복사에 의한 전자 수를 계산하였다.

• 한국태양에너지학회 논문집
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• 제23권3호
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• pp.23-28
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• 2003

The purpose of this study is to procure basic data to be used for solar power plant and concentrating collector designs. Site elevation is one of the major factors which influences the incoming insolation to the earth surface. Because the nonpermanent gases such as ozone, water vapor are unmixed components of the atmosphere and their concentrations are the function of height, the site elevation effects the relative proportion of the atmospheric constituents. We have measured solar radiation on Jiri Mt. (1,400m) and in Gurye area(115m) at the near same latitude. These values were then compared to obtain their characteristics and to investigate the potential for the solar utilization for both high and low elevated areas. From the experimental results, we concluded that 1) Daily mean horizontal global radiation and normal beam radiation on Mt. Jiri are 9.5%, and 35.3% higher than Gurye area respectively for a clear day. 2) A significant difference in atmospheric clearness index is observed between Mt. Jiri and Gurye areas.

• 천문학논총
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• 제32권1호
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• pp.63-65
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• 2017

The zodiacal light emission is the thermal emission from the interplanetary dust and the dominant diffuse radiation in the mid- to far-infrared wavelength region. Even in the far-infrared, the contribution of the zodiacal emission is not negligible at the region near the ecliptic plane. The AKARI far-infrared all-sky survey covered 97% of the whole sky in four photometric bands with band central wavelengths of 65, 90, 140, and $160{\mu}m$. AKARI detected the small-scale structure of the zodiacal dust cloud, such as the asteroidal dust bands and the circumsolar ring, in far-infrared wavelength region. Although the most part of the zodiacal light structure in the AKARI far-infrared all-sky image can be well reproduced with the DIRBE zodiacal light model, there are discrepancies in the small-scale structures. In particular, the intensity and the ecliptic latitude of the peak position of the asteroidal dust bands cannot be reproduced precisely with the DIRBE models. The AKARI observational data during more than one year has advantages over the 10-month DIRBE data in modeling the full-sky zodiacal dust cloud. The resulting small-scale zodiacal light structure template has been used to subtract the zodiacal light from the AKARI all-sky maps.

• 한국우주과학회:학술대회논문집(한국우주과학회보)
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• 한국우주과학회 2004년도 한국우주과학회보 제13권2호
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• pp.356-359
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• 2004

Prelaunch thermal analysis of the KSLV (Korea Space Launch Vehicle)-I PLF (Payload Fairing) was performed to predict maximum/minimum liftoff temperatures and to evaluate of air conditioning performance. Prelaunch thermal analysis includes internal air conditioning effect, external convective heating/cooling, radiation exchange with the ground and sky, radiation between spacecraft and PLF, and solar radiation incident on PLF. Analysis was performed at two extreme conditions, hot day condition and cold day condition. The results showed that the maximum liftoff temperature was $53^{\circ}C$ and the minimum liftoff temperature was $-3.8^{\circ}C$. It was also found that conditioned air supplying, in $20{\pm}2^{\circ}C\;and\;1200\;m^3/hr$, is sufficient to keep the internal air in required temperature range.

• 토지주택연구
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• 제12권1호
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• pp.129-137
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• 2021

외부 차양장치는 대표적인 여름철 일사조절 장치이다. 특히 냉방부하가 높은 업무용 건물에 적합한 기술로 인식되어왔다. 그러나 본 연구에서는 차양장치의 냉방부하 저감뿐만 아니라 난방부하 저감 효과를 검증하기 위한 실험을 수행하였다. 이를 위해 겨울철 야간 천공복사냉각에 따른 영향을 중심으로 일반 창호, 롤 블라인드, 외부 차양장치를 대상으로 실험을 수행하였으며, 그 결과는 다음과 같다. 외부 차양장치가 적용된 경우 유리 내·외표면 온도차는 평균 11.8℃로 차양장치가 없는 경우의 14.6℃ 보다 평균 2.8℃ 낮은 온도차를 나타냈으며, 이는 천공복사에 의한 열교환으로 차양 표면온도가 외기온도보다 낮은 시간때에 발생한다. 한편, 롤 블라인드는 내부 중공층의 평균온도보다 0.8℃ 낮은 온도를 나타냈으며 이 또한 투과체를 통과한 천공복사가 롤 블라인드 표면과 열교환이 이뤄졌기 때문이다. 유리 외부 표면온도만을 고려하면 약 3℃ 이상의 온도 상승이 예상된다. 그리고 차양장치가 없는 경우 일반적인 온도구배를 나타내고 있었다. 한편 남동향과 남서향에 외부 차양장치가 설치되었을 때 남서향의 외측 유리 표면온도가 더 낮게 나타나는 특징이 있다. 이 결과는 천공복사에 의한 냉방 저감 효과를 정량화할 수는 없지만 적어도 타당성은 확인할 수 있었다. 향후 연구에서는 천공복사 냉각과 에너지 소비 사이의 상관관계를 조사하고 외부 차양장치의 난방에너지 절감 효과에 대한 독립 챔버 실험을 진행할 계획이다.

• Advances in Energy Research
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• 제8권2호
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• pp.111-123
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• 2022

Solar Energy is the energy of solar radiation carried by them in the form of heat and light. It can be converted into electricity. Solar potential depends on the site's atmosphere; the solar energy distribution depends on many factors, e.g., turbidity, cloud types, pollution levels, solar altitude, etc. We estimated solar radiation with the help of the Ashrae clear-sky model for three locations in Pakistan, namely Pasni, Gwadar, and Jiwani. As these locations are close to each other as compared to the distance between the sun and earth, therefore a slight change of latitude and longitude does not make any difference in the calculation of direct beam solar radiation (BSR), diffuse solar radiation (DSR), and global solar radiation (GSR). A modified formula for declination angle is also developed and presented. We also created two different models for Ashrae constants. The values of these constants are compared with the standard Ashrae Model. A good agreement is observed when we used these constants to calculate BSR, DSR, GSR, the Root mean square error (RMSE), Mean Absolute error (MABE), Mean Absolute percent error (MAPE), and chisquare (χ²) values are in acceptance range, indicating the validity of the models.

• 천문학논총
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• 제27권4호
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• pp.217-218
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• 2012

Among the AKARI all-sky survey data, the $9{\mu}m$ diffuse map is crucial to study the polycyclic aromatic hydrocarbon (PAH) emission features on large spatial scales, while the $18{\mu}m$ map is useful to trace hot dust emission. To utilize these advantages, we have improved the AKARI mid-infrared (MIR) all-sky survey diffuse maps. For example, we have established special methods to remove the effects of the ionizing radiation in the South Atlantic Anomaly (SAA) and of the scattered light from the moon. Using improved diffuse map data, we study the properties of PAHs and dust in the Galactic center region associated with high-energy phenomena.