• 한국콘텐츠학회논문지
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• 제9권6호
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• pp.247-255
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• 2009

국내 방사선 및 방사성 동위원소 신고사업장 피폭실태를 조사하여 안전보건 관리방안 수립을 위한 기초자료를 제시한다. 153개 사업장 근로자를 surveymeter로 선량률(작업공간, 작업자위치)을 측정하였고, 27개 사업장은 thermal luminescence dosimeter(TLD)로 개인노출 농도(표층선량, 심부선량)를 측정하였다. Surveymeter에 의한 업종별[소방방재업(n=10), 금융보험업(n=3), 기타사업장(n=140)] 측정결과, 세 군 간에 차이가 있었다(p<0.000). 소방방재업과 금융보험업의 작업자위치 선량률은 허가사업장 기준인 10.0 ${\mu}Sv$/hr보다 높았고, 기타업종과 비교하여 109.3배(p<0.000), 187.5배(p<0.000) 각각 높게 나타났다. TLD 심부선량 농도[소방방재업(n=10), 기타 사업장(n=17)]는 소방방재업이 기타업종과 비교하여 높게 나타났다(p<0.05). Surveymeter와 TLD 측정결과 간의 관련성 분석에서는, 작업공간과 작업자위치 선량률(r=0.406, p<0.05), 작업자위치 선량률과 표층선량(r=0.453, p<0.05), 작업자위치 선량률과 심부선량(r=0.553, p<0.01), 표층선량과 심부선량(r=0.927, p<0.001)간에 각각 관련이 있었다. 방사선 및 방사선동위원소 신고사업장인 소방방재업과 금융보험업은 법적 관리구역 재설정을 통한 허가사업장으로의 전환은 방사선 취급 종사자의 안전보건을 위하여 매우 시급하다.

• 대한전자공학회논문지
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• 제27권12호
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• pp.1900-1905
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• 1990

In this study, the thermal neutron effects on optical fiber are examined theoretically. Also, the induced loss by thermal neutron irradiation in optical fibers is measured at the optical wavelengths of 0.85 and 1.3\ulcorner, respectively, and the results are analyzed. Thermal neutrons cause nuclear reaction with fiber compositions. So secondary ionizing radiations of high energy are generated. Color centers formed by these secondary ionizing rasiations increase transmission loss of optical fiber by absorbing propagating light in fiber core. As a result of experiment, owing to Ge, P, and B doping effects, the induced loss in multimode fibers has been 5 tmes larger than that in single mode fibers at 1.3 \ulcorner wavelengh. In case of multimode fibers, the loss at 0.8 \ulcorner wavelength region more suceptible for radiations has been twice higher than at 1.3\ulcorner.

• 천문학회지
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• 제29권spc1호
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• pp.247-248
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• 1996

In order to study the X-ray radiations from solar type strong interacting binary stars, we have collected X-ray data of 44i Bootis (P=0.2678 days, SP=G2+G2) from the EXOSAT data archive. Preliminarly analysis of a part of these data has been already reported by Vilhu & Heise (1986). In this paper, however, we present a more complete light curve in LE region than the previous work, and some unpublished X-ray light curves and spectrums. Using these new materials a new attempt to find the physical explanation about. some observational characteristic figures in the X-ray light curves and spectrums has been made.

• Journal of Photoscience
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• 제9권3호
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• pp.37-40
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• 2002

Astronauts are constantly exposed to space radiation at a low-dose rate during long-tenn stays in space. Therefore, it is important to determine correctly the biological effects of space radiation on human health. Space radiations contain various kinds of different energy particles, especially high linear energy transfer (LET) particles. Therefore, we have to study the relative biological effectiveness (RBE) of space radiation under microgravity environment which may change RBE from a stress for cells. Furthermore, the research about space radiation might give us useful information about birth and evolution of life on the earth. We also can realize the importance of preventing the ozone layer from depletion by use of exposure equipment to sunlight at International Space Station (ISS).

• Radiation Oncology Journal
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• 제2권2호
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• pp.271-280
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• 1984

The peripheral dose, defined as the dose outside therapeutic photon fields, which is responsible for the functional damage of the critical organs, fetus, and radiation. induced carcinogenesis, has been investigated for $^{60}Co\;\gamma$ ray and 10 MV Xray. It was measured by silicon diode controlled by semiautomated water phantom without any shielding or with lead plate of HVL thickness put horizontally or vertically to shield stray radiations. Authors could obtain following results. 1. The peripheral dose was larger than $0.7\%$ of central axis maximum dose even at 20cm distance from field margin. That is clinically significant, so it should be reduced. 2. Even for square fields of 10 MV Xray, radial peripheral dose distribution did not coincide with transverse distribution, because of the position of collimator jaws. 3. Between surface and $d_m$, the peripheral dose distributions show a pattern of the dose distribution of electron beams and the maximum doss was approximately proportional to the length of a side of square field. 4. The peripheral doses depended on radiation quality, field size, distance from field margin and depth in water. Distance from field margin was the most important factor. 5. Except for near surface, the peripheral dose from phantom was approximately equal to that from therapy unit. 6. To reduce the surface dose outside fields, therapist should shield stray radiations from therapy unit by lead plate of at least one HVL for 10 MV X-ray and by bolus equivalent to tissue of 0.5cm thickness for $^{60}Co$. 7. To reduce the dose at depth deeper than $d_m$, it is desirable to shield stray radiations from therapy unit by lead.

• Journal of Photoscience
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• 제9권2호
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• pp.170-173
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• 2002

Space is full of energetic events emitting high-energy radiations which may be fatal to all living things unless protected. The present paper briefly describes high-energy photons and particles incident on Earth surface and their common properties toward living things. Role of radiation played in evolution of life and earth environment will be presented.

• 천문학회보
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• 제34권2호
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• pp.55.1-55.1
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• 2009

• 한국광학회:학술대회논문집
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• 한국광학회 2008년도 하계학술발표회 논문집
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• pp.235-236
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• 2008

• 한국자기학회:학술대회 개요집
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• 한국자기학회 2014년도 자성 및 자성재료 국제학술대회
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• pp.103-103
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• 2014

• 천문학회지
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• 제36권spc1호
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• pp.29-36
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• 2003

Quiescent solar radiation, at microwave spectral regime, is dominated by gyroresonant and thermal Bremsstrahlung radiations from hot electrons residing in solar active region corona. These radiations are known to provide excellent diagnostics on the coronal temperature, density, and magnetic field, provided that spatially resolved spectra are available from observations. In this paper we present an imaging spectroscopy implemented for a bipolar active region, AR 7912, using the multifrequency interferometric data from the Owens Valley Solar Array (OVSA), as processed with a new imaging technique, so-called Spatio-Spectral Maximum Entropy Method (SSMEM). From the microwave maps at 26 frequencies in the range of 1.2-12.4 GHz at both right- and left-circular polarizations, we construct spatially resolved brightness spectra in every reconstructed pixel of about 2 arcsec interval. These spectra allowed us to determine 2-D distribution of electron temperature, magnetic field of coronal base, and emission measure at the coronal base above the active region. We briefly compare the present result with existing studies of the coronal active regions.