• Title/Summary/Keyword: Infra Red

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Heating of a coronal loop by the evolution of the fine-scale magnetic discontinuity in the photosphere

  • Song, Donguk;Chae, Jongchul;Park, Soyoung;Ahn, Kwangsu;Cao, Wenda
    • The Bulletin of The Korean Astronomical Society
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    • v.40 no.1
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    • pp.84.3-85
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    • 2015
  • We report a small-scale EUV bright loop associated with the evolution of the fine-scale magnetic discontinuity in the photosphere. Our analysis was carried out by using the high spatial resolution data taken with InfraRed Imaging Magnetograph (IRIM) and the Fast Imaging Solar Spectrograph (FISS). As a result, an extremely narrow dark lane of the intense horizontal magnetic field (width ~ 300 km) is detected parallel to the boundary of the magnetic pore, which is one of the footpoints of the small-scale bright coronal loop. We find that the variation of the net linear polarization inside the dark lane is closely related to the intensity variations of the coronal loop. Based on our results, we suggest that small-scale atmospheric heating such as bright coronal loop seen above the complex pore group may be strongly affected by the evolution of the fine-scale magnetic discontinuity in the photosphere. This is a nice example of solar atmospheric heatings associated with the fine-scale magnetic discontinuity in the photosphere.

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User-Calibration Free Gaze Tracking System Model (사용자 캘리브레이션이 필요 없는 시선 추적 모델 연구)

  • Ko, Eun-Ji;Kim, Myoung-Jun
    • Journal of the Korea Institute of Information and Communication Engineering
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    • v.18 no.5
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    • pp.1096-1102
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    • 2014
  • In remote gaze tracking system using infra-red LEDs, calibrating the position of reflected light is essential for computing pupil position in captured images. However, there are limitations in reducing errors because variable locations of head and unknown radius of cornea are involved in the calibration process as constants. This study purposes a gaze tracking method based on pupil-corneal reflection that does not require user-calibration. Our goal is to eliminate the correction process of glint positions, which require a prior calibration, so that the gaze calculation is simplified.

Implementation and Validation of Earth Acquisition Algorithm for Communication, Ocean and Meteorological Satellite

  • Park, Sang-Wook;Lee, Young-Ran;Lee, Byoung-Sun;Hwang, Yoo-La;Lee, Un-Seob
    • Journal of Astronomy and Space Sciences
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    • v.28 no.4
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    • pp.345-354
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    • 2011
  • Earth acquisition is to solve when earth can be visible from satellite after Sun acquisition during launch and early operation period or on-station satellite anomaly. In this paper, the algorithm and test result of the Communication, Ocean and Meteorological Satellite (COMS) Earth acquisition are presented in case of on-station satellite anomaly status. The algorithms for the calculation of Earth-pointing attitude control parameters including those attitude direction vector, rotation matrix, and maneuver time and duration are based on COMS configuration (Eurostar 3000 bus). The coordinate system uses the reference initial frame. The constraint calculating available time-slot to perform the earth acquisition considers eclipse, angular separation, solar local time, and infra-red earth sensor blinding conditions. The results of Electronics and Telecommunications Research Institute (ETRI) are compared with that of the Astrium software to validate the implemented ETRI software.

NORTH ECLIPTIC POLE WIDE SURVEY

  • Lee, Hyung Mok;Kim, Seong Jin;NEP-Wide Team, NEP-Wide Team
    • Publications of The Korean Astronomical Society
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    • v.27 no.4
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    • pp.129-134
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    • 2012
  • The North Ecliptic Pole (NEP) Wide survey covered about 5.4 $deg^2$, a nearly circular area centered on the NEP, using nine passbands of InfraRed Camera (IRC). We present the photometric properties of the data sets, and the nature of the sources detected in this field. The number of detected sources varied according to the filter band: with about 109,000 sources in the NIR, about 20,000 sources in the MIR-S, and about 16,000 sources seen in the MIR-L channel. The $5{\sigma}$ detection limits are about 21 mag in the NIR and 19.5 - 18.5 mag in the MIR bands in terms of the AB magnitude. 50% completeness levels are about 19.8 mag at $3{\mu}m$, 18.6 mag at $9{\mu}m$, and 18 mag at $18{\mu}m$ band (in AB magnitude), respectively. In order to validate the detected sources, all of them are confirmed by matching tests with those in other bands. The 'star-like' sources, defined by the high stellarity and magnitude cut from the optical ancillary data, appear statistically to have a high probability of being stars. The nature of the various types of extragalactic sources in this field are discussed using the color-color diagrams of the NIR and MIR bands with the redshift tracks of galaxies providing useful guidelines.

A Study on Analysis of Infrared Rotating Lovell Reticle Seeker and an Efficient Counter-countermeasure Algorithm (적외선 회전 Lovell 레티클 탐색기의 성능 분석 및 효율적인 반대응 알고리즘에 대한 연구)

  • Kim, Sun-Kook;Han, Sung-Hyun;Hong, Hyun-Ki;Choi, Jong-Soo
    • Journal of the Korean Institute of Telematics and Electronics S
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    • v.35S no.11
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    • pp.166-175
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    • 1998
  • The previous simulation models of infra-red (IR) reticle seekers were performed in a static situation. However, in this paper, we develop a new simulation tool which is applicable in various cases, and propose an efficient counter-countermeasure (CCM) in the presence of countermeasures (CM) such as flares. The developed tool analyzes performance of rotating Lovell reticle seeker, and gives tracking performances in various scenarios. The simulation results show that our counter-countermeasure algorithm makes an efficient target tracking in the presence of flares.

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DC pulse sputter로 제작한 단열필름 컬러화에 대한 연구

  • Lee, Dong-Hun;Park, Eun-Mi;Seo, Mun-Seok;Kim, Hye-Jin;Ha, In-Ho;Jo, Eun-Seon;Han, Geon-Hui
    • Proceedings of the Korean Vacuum Society Conference
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    • 2016.02a
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    • pp.167.2-167.2
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    • 2016
  • 태양에너지는 전자기파로써 파장에 따라 여러 부분으로 나뉜다. 파장이 780nm 이상인 부분의 영역을 IR (infra Red) 즉 적외선으로 불린다. 이 부분이 열선에 해당하는 부분인데 대부분의 창문에 설치된 커튼이나 vertical 등은 빛을 차단하는 수단일 뿐, 유입되는 열 (적외선)을 차단시킬 수는 없다. 열은 결국 실내의 온도를 높이기 때문에 난방비 등 에너지 손실을 막긴 어렵다. 단열필름은 커튼이나 vertical과 달리 실내로 유입되는 열 (적외선)을 다시 실외로 반사시켜 실내로 유입되는 열을 최소화 한다. 본 연구는 IR 차폐를 목적으로 연구 되었고, 거기서 한 발 나아가 실내 분위기 등을 고려하여 소비자의 구호에 맞는 제품에 더 맞추기 위해 연구되었다. 기존 제품들과 차별된 점은 색상을 위한 추가적인 작업없이 굴절률과 두께 factor 등을 변화시켜 바로 7가지 색을 구현한다는 장점을 가지고 있다. 따라서 가격 경쟁력에서도 우위를 점 할 수 있는 중요한 기술이라 할 수 있겠다. 박막제조 장비로는 DC pulse In-line Sputter를 사용하였으며, 굴절률과 광학적인 두께 측정을 위한 ellipsometer, 그리고 UV-vis 를 통한 Transmittance 측정으로 제품 능력을 확인하였다.

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Review of Clinical Studies on Korean Medicine and Complementary and Alternative Medicine Treatment for Allergic Rhinitis in the Korean Literature (알레르기성 비염의 한의학 및 보완대체의학적 치료에 대한 국내 임상 연구 동향)

  • Koo, Eun Jin;Han, Jae Kyung;Kim, Yun Hee
    • The Journal of Pediatrics of Korean Medicine
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    • v.29 no.4
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    • pp.77-89
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    • 2015
  • Objectives The purpose of this study is to analyze Korean clinical studies in Korean medicine and complementary and alternative medicine for allergic rhinitis and to propose for better methods of clinical studies and effective treatments on allergic rhinitis. Methods Electronic researches were performed with NDSL, RISS, KISTI, KISS, OASIS by keyword 'Allergic rhinitis'. Results The treatments used in 36 studies were herbal medicines, acupuncture, pharmacopuncture, moxibustion, cupping, inject medicine to nasal cavity, aroma therapy, ointment, nasal cleansing solution, laser treatment, infra-red therapy, oxygen nebulizer, diet treatment, moxa-pellet treatment, mindfulness meditation and space-spine manipulation techniques. The most common acupoints were LI4 and LI20 (Large Intestine Meridian). The most common methods of assessment is subjective nasal symptoms. All studies using subjective nasal symptoms and quality of life as assessment methods to show valid results on the improvement of allergic rhinitis. Conclusions This study shows that Korean medicine and complementary and alternative medicine on allergic rhinitis are effective. It will be expected to use that various methods for allergic rhinitis and more clinical studies for allergic rhinitis and pediatric patients needed in the future.

The Wormicidal Sibstance of Fresh Water Fishes on Clonorchis sinensis(VI) - Struture Identification of Purified Clonorchicidal Sudstance from Epidermal Mucus of Cyprinus carpio nudus (간흡충에 대한 살충성물질에 관한 연구 (VI) - 향어 체표면 점액내 살충성물질의 구조 확인)

  • 이재구;김평길;안병준
    • YAKHAK HOEJI
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    • v.31 no.1
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    • pp.33-39
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    • 1987
  • In order to elucidate the defence mechanism of Cyprinus carpio nudus to Clonorchis sinensis, clonorchicidal substance in the epidermal mucus of this fish was isolated by silica gel column and thin layer chromatography and analyzed for its chemical nature by UV, IR and NMR-spectroscopy. The epidermal mucus of the fish was extracted by ethyl ether and separated into 2 fractions by column chromatography using petroleum ether/chloroform(30/70,v/v) as first solvent and methanol as second solvent. The second fraction with greyish white colour showed clonorchicidal effect. The second was again fractionated into greyish white precipitate and clonorchicidal greenish yellow supernatant fraction, by adding petroleum ether and standing the mixture for 5 days at $5^{\circ}C$. The latter was divided into 7 fractions in column chromatography with acetone/ benzene (10/90, v/v) as carrier. The fraction on equivalent to the spot of Rf. 0.225 value among them disclosed the strongest clonorchicidal effect. By this purification procedure, clonorchicidal substance was purified 154-fold with 0.9% yield from the mucus of the fish, and 10mg of the final fraction killed tne metaceicariae in 22 min. Infra red, nuclear magnetic resonance and ultraviolet spectrometric analysis of the purified substance revealed that the substance is linoleic acid. According to the results of the present studies it seemed that this fish could not be proper intermediate host of Clonorchis sixensis, and that defence mechanism of this fish to the worm seems to be correlated with clonorchicidal substance in epidermal mucus.

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Influence of 1st,2rd Sustain Pulse Width on AC-PDP Driving (Sustain 초단 펄스가 AC-PDP 의 구동에 미치는 영향)

  • Kim, S.S.;Cho, T.S.;Ahn, J.C.;Choi, M.C.;Jeoung, J.M.;Leem, J.Y.;Jeoung, Y.H.;Kim, T.Y.;Chong, M.W.;Choi, S.H.;Kim, S.B.;Ko, J.J.;Cho, K.S.;Choi, E.H.
    • Proceedings of the Korean Institute of Electrical and Electronic Material Engineers Conference
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    • 2000.04a
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    • pp.152-154
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    • 2000
  • Electro_optical characteristics in AC-PDP are confined by a lots of parameters. especially driving pulse shape is very important to improve AC-PDP's luminosity and efficiency. In that experiment measure the luminosity, IR(Infra Red) peak value and response time as the increase of 1st, 2rd sustain pulse width. The VDS(Versatile Driving Simulator -developed by kwangwoon university-) was used to make driving pulse shape. It is found that IR response time after displacement current, Luminosity and IR peak value are changed on account of 1st,2rd sustain pulse width.

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Influence of frequency and duty ratio on electro-optical characteristics in AC-PDP (AC-PDP에서의 주파수 및 duty비의 영향에 따른 전기광학적 특성)

  • Kim, T.Y.;Cho, T.S.;Ahn, J.C.;Choi, M.C.;Jeoung, J.M.;Leem, J.Y.;Jeoung, Y.H.;Kim, S.S.;Chong, M.W.;Choi, S.H.;Kim, S.B.;Ko, J.J.;Cho, K.S.;Choi, E.H.
    • Proceedings of the Korean Institute of Electrical and Electronic Material Engineers Conference
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    • 2000.04a
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    • pp.139-142
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    • 2000
  • Influence of frequency and duty ratio on electro-optical characteristics are experimentally investigated in surface AC plasma display panels(AC-PDPs) by using the VDS(Versitile Driving Simulator)., in which electrode gap and width are 100 ${\mu}m$ and 260 ${\mu}m$, respectively. The filling gas is Ne-Xe gas mixture, and total pressure 400 Torr. It is found that the response time gets to be fast from 450 ns to 150 ns as pulse-off time of the sustain pulse decreases from 2 ${\mu}s$ to 0.2 ${\mu}s$. Also it is found that the IR(Infra Red) intensity and the luminous decreases as pulse-off time of the sustain pulse increases from 0.2 ${\mu}s$ to 2 ${\mu}s$.

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