• 한국항행학회논문지
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• 제10권1호
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• pp.13-19
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• 2006

본 논문에서는 FCC의 방사 스펙트럼 제한 규정에 따라 5 GHz-WLAN 주파수 대역을 억제한 DS-UWB 가우시안 임펄스 생성기를 제안하고, 이를 실험적으로 구현하였다. 단극 구형파를 가우시안 임펄스로 변환하기 위해 SRD를 이용한 첫 번째 임펄스 생성기와 반도체 레이저의 이득 스위칭을 이용한 두 번째 임펄스 생성기로 구성된 2단 구조의 임펄스 생성기를 사용하였다. 출력된 가우시안 임펄스의 폭은 약 180 psec로 매우 짧다. 또한 WLAN 주파수 대역을 제거하기 위해 4단 링 공진기 구조의 고차 미분 가우시안 필터를 설계 및 제작하여 최종적으로 WLAN 신호 대역은 약 25 dB의 억제 효과를 갖는 DS-UWB 신호의 발생기를 실험적으로 구현하였다.

• 천문학논총
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• 제30권3호
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• pp.811-819
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• 2015

The e-CALLISTO is a network of CALLISTO (Compact Astronomical Low-frequency, Low-cost Instrument for Spectroscopy in Transportable Observatories) spectrometers which detect solar radio bursts 24 hours a day in frequency range 45-870 MHz. The number of channels per spectrum is 200 and the time resolution of whole spectrum is 0.25 second. The Korean e-CALLISTO station was developed by Korea Astronomy and Space Science Institute (KASI) collaborating with Swiss Federal Institute of Technology Zurich (ETH Zurich) since 2007. In this paper, we report replacement of the tracking mount and development of the control program using Visual C++/MFC. The program can make the tracking mount track the Sun and schedule CALLISTO to start and to finish its observation automatically using the Solar Position Algorithm (SPA). Daily tracking errors (RMSE) are 0.0028 degree in azimuthal axis and 0.0019 degree in elevational axis between 2014 January and 2015 July. We expect that the program can save time and labor to make the observations of solar activity for space weather monitoring, and improve CALLISTO data quality due to the stable and precise tracking methods.

• 천문학회보
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• 제37권1호
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• pp.90.2-90.2
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• 2012

Geosynchronous electron flux dropouts are most likely due to fast drift loss of the particles to the magnetopause (or equivalently, the "magnetopause shadowing effect"). A possible effect related to the drift loss is the radial diffusion of PSD due to gradient of PSD set by the drift loss effect at an outer L region. This possibly implies that the drift loss can affect the flux levels even inside the trapping boundary. We recently investigated the details of such diffusion process by solving the diffusion equation with a set of initial and boundary conditions set by the drift loss. Motivated by the simulation work, we have examined observationally the energy spectrum and pitch angle distribution near trapping boundary during the geosynchronous flux dropouts. For this work, we have first identified a list of geosynchronous flux dropout events for 2007-2010 from GOES satellite electron measurements and solar wind pressures observed by ACE satellite. We have then used the electron data from the Time History of Events and Macroscale Interactions during Substorms (THEMIS) spacecraft measurements to investigate the particle fluxes. The five THEMIS spacecraft sufficiently cover the inner magnetospheric regions near the equatorial plane and thus provide us with data of much higher spatial resolution. In this paper, we report the results of our investigations on the energy spectrum and pitch angle distribution near trapping boundary during the geosynchronous flux dropout events and discuss implications on the effects of the drift loss on the flux levels at inner L regions.

• 한국동물학회지
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• 제13권3호
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• pp.75-84
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• 1970

蛋白質의 放射線分解의 기작을 밝히는 연구의 일환으로, 특히 peptide 結合의 분해의 기작을 구명하기 위하여 Glycylglycylglycine의 水溶液과 固體를 酸素의 존재하에서와 無酸素하에서 r 線을 조사하여 分解生成物을 여지크로마토그라프로 분리하였고, carbonyl 化合物과 amide를 각각 分光光度法과 微凉摘定法으로 정량하였으나 放射線障害를 평가하기 위하여 赤外線 spectrum과 紫外線 spectrum을 얻어 검토하였다. 水溶液과 固體에 있어서의 peptide 結合의 분해기작은 근본적인 차이가 있는 것으로 여겨지며, 전자에서는 월등하게 분해가 많이 일어난데 반해서 후자에서는 무시할 정도에 지나지 않았다. 한편, 水溶液의 경우 酸素의 유무에 따라 현저한 영향은 보이지 않았으나 無酸素하에서는 遊離基의 再結合이 일어나는 점이 특기할만 하였다. 水溶液에 있어서의 peptide 結合의 분해기구는 Garrison 一派가 주장한 기작에 의해서 일어나는 것이 분명하여 脫水素反應에 뒤이어 加水分解反應에 의해서 amide 와 carbonyl 이 생성되는 것으로 보이며, 固體의 경우도 $\\alpha$-炭素의 부위가 방사선의 공격을 가장 많이 받는 것으로 추정되나 그 정도는 미미한 것에 지나지 않는 것으로 생각되었다.

• 천문학회지
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• 제36권2호
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• pp.55-60
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• 2003

In Lee, Kang & Byun (2001) the discovery of Raman scattered 6545 A feature was reported in symbiotic stars and the planetary nebula M2-9. The broad emission feature around 6545 A is formed as a result of Raman scattering of He II n = 6 $\to$ n = 2 photons by atomic hydrogen. In this paper, we introduce a method to compute the equivalent width of He II $\lambda$ 1025 line and present an optical spectrum of the symbiotic star RR Telescopii as an example for a detailed illustration. In this spectrum, we pay attention to the broad H$\alpha$ wings and the Raman scattered He II 6545 feature. The broad Ha wings are also proposed to be formed through Raman scattering of continuum around Ly$\beta$ by Lee (2000), and therefore we propose that the equivalent width of the He II $\lambda$ 1025 emission line is obtained by a simple comparison of the strengths of the 6545 feature and the broad H$\alpha$ wings. We prepare a template H$\alpha$ wing profile from continuum radiation around Ly$\beta$ with the neutral scattering region that is supposed to be responsible for the formation of Raman scattered He II 6545 feature. Isolation of the 6545 feature that is blended with [N II] $\lambda$ 6548 is made by using the fact that [N II] $\lambda$ 6584 is always 3 times stronger than [N II] $\lambda$ 6548. We also fit the 6545 feature by a Gaussian which has a width 6.4 times that of the He II $\lambda$ 6527 line. A direct comparison of these two features for RR Tel yields the equivalent width $EW_{Hel025} = 2.3{\AA}$ of He II $\lambda$ 1025 line. Even though this far UV emission line is not directly observable due to heavy interstellar extinction, nearby He II lines such as He II $\lambda$ 1085 line may be observed using far UV space instruments, which will verify this calculation and hence the origins of various features occurring in spectra around H$\alpha$.

• 한국농업기계학회:학술대회논문집
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• 한국농업기계학회 1996년도 International Conference on Agricultural Machinery Engineering Proceedings
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• pp.334-343
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• 1996

Quality evaluation for food and agricultural products have always been one of the most elusive problems associated with the handling , processing and marketing in a food plant production. In order to detect physical foreign materials in food and agricultural products, non-destructive techniques have been developed for many years. Application of X-ray system to detect physical foreign materials in food and agricultural products could be considered to be a high potential method. Especially , it is impossible to detect internal physical foreign materials by visual inspections. In this study, it was tried to be applied for two different X-ray devices. Soft X-ray system with CdTe sensor and X-ray CT scanner were evaluated for advantage of the detection of non-meltallic foreign materials in food and agricultural products . Though the soft X-ray is not a high energy radiation, it is possible to detect small different density in a material. The CdTe sensor has a high resolution for t e soft X-ray energy region. The density characteristics of foods and foreign material were expressed region. The density characteristics of foods and foreign materials were expressed as a soft X-ray energy spectrum. The energy spectrum was analyzed by a personal computer with a multi-channel analyzer. X-ray CT scanner can provide visual image and analyze by three dimensional information inside food and agricultural products. The X-ray CT scanner using as a medical equipment was used to detect a foreign material. The density characteristics of food and foreign materials in food were tried to be detected by the threshold value on the basis of the CT numbers. The soft X-ray absorption characteristics for acrylin plates and distilled water were obtained and could be found the possibility of detecting a small physical foreign materials such as a plastic wrapping film , a stone and grasshopper in food and agricultural products.

• 한국방사선학회논문지
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• 제8권5호
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• pp.249-254
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• 2014

의료용 선형가속장치는 1952년에 개발된 이후 방사선 치료에 사용되어 왔으며 그 활용도가 더욱 증가하고 있다. 현재는 6 MeV 이상의 광자 에너지를 사용하는 고 에너지 방사선치료가 보편화되어 사용되고 있으나, 광핵반응에 의한 중성자의 생성으로 환자 및 술자에 대한 피폭이 문제가 되고 있다. 이에 본 연구에서는 MCNPX를 사용하여 의료용 선형가속장치에서 발생되는 6~24 MV 광자선의 스펙트럼을 분석하고, 평균에너지 및 텅스텐의 중성자 생성 임계에너지인 7.41 MeV 이상의 광자 개수를 평가하였다. 그 결과 8 MV를 시작으로 24 MV에서는 전체 검출 광자 수에 비해 0.59%의 비율로서 광핵 반응을 일으킬 수 있는 광자수가 증가함을 알 수 있었다.

• 한국자기학회지
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• 제19권4호
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• pp.152-155
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• 2009

Ba-ferrite 단결정을 제조하여 자기적 성질을 $M\"{o}ssbauer$ 분광법으로 연구하였다. 단결정 시료를 c-축 방향으로 얇게 절단하고 그 면에 감마선을 조사한 결과 Fe 이온의 스핀방향이 c-축과 일치하였고 시료 전체에 걸쳐 단일 결정체임을 확인하였다. 특히 감마선이 스핀과 나란한 경우 $M\"{o}ssbauer$ 흡수선 중에서 결정 내에 존재하는 Fe의 5개 자리 중에서 단지 4개 자리에서만 공명흡수선이 존재하였고 2b 자리에서는 전혀 공명흡수가 일어나지 않았다. 2b 자리에서의 공명흡수가 일어나지 않는 이유는 대칭성이 있는 2개의 우물 형 위치에너지의 중심 사이를 Fe 이온이 매우 빠른 속도로 c-축을 따라 진동하는 것으로 설명할 수 있다.

• 천문학회보
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• 제37권2호
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• pp.141.1-141.1
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• 2012

CIBER (Cosmic Infrared Background ExpeRiment) is a sounding-rocket borne experiment which is designed to find the evidence of the First stars (Pop.III stars) in the universe. They are expected to be formed between the recombination era at z ~ 1100 and the most distant quasar (z ~ 8). They have never been directly detected due to its faintness so far, but can be observed as a background radiation at around $1{\mu}m$ which is called the Cosmic Near-Infrared Background (CNB). The CIBER is successfully launched on July 10, 2010 at White Sands Missile Range, New Mexico, USA. It consists of three kinds of instruments. One of them is a LRS (Low Resolution Spectrometer) which is a refractive telescope of 5.5 cm aperture with spectral resolution of 20 ~ 30 and wavelength coverage of 0.7 to $2.0{\mu}m$ to measure the spectrum of the CNB. Since LRS detects not only CNB but also stellar components, we can study their spectral features with the broad band advantage especially at around $1{\mu}m$ which is difficult at ground observations because of the atmospheric absorption by water vapor. I identified around 300 stars from observed six fields. If we can classify their spectral types with SED fitting, we can study their physical conditions of the stellar atmosphere as well as making a stellar catalogue of continuous stellar spectrum.

• 조명전기설비학회논문지
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• 제20권6호
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• pp.75-80
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• 2006

산업현장에서 많이 사용되고 있는 전력기기에 결함이 발생하면 치명적인 사고로 진전되어 경제적, 인적 손실이 발생될 수가 있다. 본 논문은 GIS에 사용되는 절연가스인 $SF_6$의 압력 변화에 따른 부분방전을 모의하고, 발생되는 부분방전 신호를 절연 진단 방법 중 하나인 UHF법을 이용하여 부분방전 시 방사되는 방사전자파의 스펙트럼을 분석해 금속 이물질이 $SF_6$가스 부분방전에 미치는 영향을 측정하였다. 이러한 연구는 현장 GIS 및 $SF_6$가스절연 전력설비에서 내부압력 변화 시 금속 이물질에 의해 발생되는 절연파괴 사고의 방지에 중요한 역할을 할 것으로 사료된다.