• 한국추진공학회지
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• 제11권2호
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• pp.47-53
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• 2007

본 논문에서는 초음속유동장 내에 분사된 2차 분사유동과 주유동의 상호작용에 의한 2차 분사노즐 주변에서의 열전달 현상을 관찰하였다. 벽면에는 등열유속조건을 주었다. 제트 자유유동간 운동량비(Jet to Freestream Momentum Ratio, J)에 따라 2차 분사를 초음속 유동장에 분사시켰으며, 적외선 카메라를 이용하여 2차 분사노즐 주변 벽면온도를 측정하였고, 이를 통하여 대류 열전달계수를 제시하였다.

• 한국멀티미디어학회논문지
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• 제22권3호
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• pp.357-365
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• 2019

In this paper, we suggest the tracking method of moving multi-objects in maritime environments. The image acquisition is conducted using IR(InfraRed) camera sensors on an airborne platform. Under the circumstance of maritime, the qualities of IR images can be significantly degraded due to the clutter influence, which directly gives rise to a tracking loss problem. In order to reduce the effects from the clutters, we introduce a technical approach under Man-In-The-Loop(MITL) system for enhancing the tracking performance. To demonstrate the robustness of the proposed approach based on VTG(Valid Tracking Gate), the simulations are conducted utilizing the airborne IR video sequences: Then, the tracking performances are compared with the existing Kalman Filter tracking techniques.

• 전자통신동향분석
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• 제37권1호
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• pp.10-20
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• 2022

A drone without attaching guns or bombs can be a dangerous weapon, since its motor speed is greater than 3000 rpm, which is similar to that of a mower powered by a LiPo battery. The anti-drone system is the only means of detecting and neutralizing drone attacks. Many defense companies around the world provide solutions using various types of equipment (for example, radar, cameras, jamming guns, and net guns). ETRI has also developed a Low-Altitude Drone Detection (LADD) system consisting of Ku-band radar and an Electro-Optical/Infra-Red (EO/IR) camera. In this paper, we summarize recent technical advances in anti-drone systems around the world and introduce the features and describe the performance of the LADD system.

• 천문학회보
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• 제35권1호
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• pp.39.2-39.2
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• 2010

In this paper, I present the domestic development of near infrared camera systems for the ground telescope and the space satellite. These systems are the first infrared instruments made for astronomical observation in Korea. KASINICS (KASI Near Infrared Camera System) was developed to be installed on the 1.8m telescope of the Bohyunsan Optical Astronomy Observatory (BOAO) in Korea. KASINICS is equipped with a $512{\times}512$ InSb array enable L band observations as well as J, H, and Ks bands. The field-of-view of the array is $3.3'{\times}3.3'$ with a resolution of 0.39"/pixel. It employs an Offner relay optical system providing a cold stop to eliminate thermal background emission from the telescope structures. From the test observation, limiting magnitudes are J=17.6, H=17.5, Ks=16.1 and L(narrow)=10.0 mag at a signal-to-noise ratio of 10 in an integration time of 100 s. MIRIS (Multi-purpose InfraRed Imaging System) is the main payload of the STSAT-3 in Korea. MIRIS Space Observation Camera (SOC) covers the observation wavelength from $0.9{\mu}m$ to $2.0{\mu}m$ with a wide field of view $3.67^{\circ}{\times}3.67^{\circ}$. The PICNIC HgCdTe detector in a cold box is cooled down below 100K by a micro Stirling cooler of which cooling capacity is 220mW at 77K. MIRIS SOC adopts passive cooling technique to chill the telescope below 200K by pointing to the deep space (3K). The cooling mechanism employs a radiator, a Winston cone baffle, a thermal shield, MLI of 30 layers, and GFRP pipe support in the system. Opto-mechanical analysis was made in order to estimate and compensate possible stresses from the thermal contraction of mounting parts at cryogenic temperatures. Finite Element Analysis (FEA) of mechanical structure was also conducted to ensure safety and stability in launching environments and in orbit. MIRIS SOC will mainly perform the Galactic plane survey with narrow band filters (Pa $\alpha$ and Pa $\alpha$ continuum) and CIB (Cosmic Infrared Background) observation with wide band filters (I and H) driven by a cryogenic stepping motor.

• 한국식품저장유통학회지
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• 제23권3호
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• pp.422-431
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• 2016

일부 소스류 제품에 사용된 스탠딩 파우치에서 전자레인지 가열조리 시 열변형이 발견되어 이의 원인을 규명하고자 온도 변화 패턴을 조사하였다. 전자레인지로 포장된 식품을 가열 시 포장재의 온도 변화는 식품 자체의 온도보다 높고 국소적인 온도 측정 기술을 요한다. 공시 시료로 매운맛 닭 소스와 인도카레의 전자레인지 가열 시 포장재와 시료의 온도를 열화상 카메라, 온도센서 테이프 및 광섬유 온도계를 이용하여 측정하였다. 스탠딩 파우치 형태의 포장은 전자레인지 가열 조리 시 내용물의 불균일한 가열이 관찰되어 특정 부위, 특히 액위선 상단과 측면 sealing layer에 열이 집중되는 현상이 발생하였다. 열화상 카메라를 이용한 온도 측정 방법은 식품의 표면 온도를 측정하는 제약이 있고 실제 식품의 온도보다 낮게 측정되는 경향을 보였다. 온도센서 테이프를 이용할 경우 $200^{\circ}C$까지 온도까지 측정되어 전자레인지 가열 과정 중 포장재 변형 현상이 야기될 수 있는 가능성을 확인할 수 있었다. 그리고 전자레인지 가열 시 포장재 표면의 온도 변화를 기존 광섬유 온도계로 측정할 경우 실제 온도보다 낮게 측정되는 결과가 초래되므로, 좁은 범위에서의 hot spot의 온도 변화를 감지할 수 있는 방법으로 GaAS crystal 센서를 사용함으로서 기존 센서보다 더 민감하고 정확한 온도 측정이 가능하였다.

• 스마트미디어저널
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• 제2권4호
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• pp.60-65
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• 2013

본 논문에서는 Time-of-Flight (TOF) 원리를 이용하여 획득한 저해상도 깊이 영상을 고해상도의 색상 영상에 정합하는 방법을 소개한다. 거리 정보 기반의 3차원 렌더링에서 깊이 영상은 렌더링 결과에 큰 영향을 끼치지만, 기존의 스테레오 정합은 색상 영상의 특성에 따라 성능이 크게 변하고, 깊이 정보를 획득하지 못하는 영역이 존재한다. 반면에 TOF 카메라는 적외선 센서를 통해 카메라로부터 물체까지의 거리를 직접 측정하여 영상으로 출력하기 때문에, 장면의 깊이 정보를 실시간으로 획득 할 수 있고 높은 정확도를 가지는 장점이 있다. 하지만 출력 영상의 해상도가 너무 작아 3차원 응용에 직접 이용하기가 어렵다. 또한, 색상 영상과 다른 카메라를 이용하기 때문에 두 영상의 3차원적 위치와 특성이 서로 다르다는 문제점을 갖는다. 따라서 해상도를 증가시키고 다른 두 카메라로 부터 찍힌 영상을 정합시키는 방법이 필요하다. 본 논문에서 제안하는 방법은 깊이 카메라에서 획득한 저해상도 깊이 정보를 고해상도 색상 정보를 이용하여 두 영상간의 정합이 이루어지도록 한다. 향상된 깊이 영상을 사용하여 3차원으로 복원한 실험을 통해, 제안하는 방법이 효과적으로 장면의 변위 정보를 생성함을 알 수 있다.

• 천문학논총
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• 제27권3호
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• pp.39-47
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• 2012

MIRIS, Multi-purpose Infra-Red Imaging System, is the main payload of STSAT-3 (Korea Science & Technology Satellite 3), which will be launched in the end of 2012 (the exact date to be determined) by a Russian Dnepr rocket. MIRIS consists of two camera systems, SOC (Space Observation Camera) and EOC (Earth Observation Camera). During a shock test for the flight model stability in the launching environment, some lenses of SOC EQM (Engineering Qualification Model) were broken. In order to resolve the lens failure, analyses for cause were performed with visual inspections for lenses and opto-mechanical parts. After modifications of SOC opto-mechanical parts, the shock test was performed again and passed. In this paper, we introduce the solution for lens safety and report the test results.

• 천문학논총
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• 제27권4호
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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.

• 천문학회보
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• 제38권2호
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• pp.69.1-69.1
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• 2013

We describe a survey of quasars in the early universe beyond z=5, which is one of the main sciences of the Infrared Medium-deep Survey (IMS) performed by the Center for the Exploration of the Origin of the Universe (CEOU). We use multi-wavelength archival data such as SDSS, CFHTLS, UKIDSS, and SWIRE, which provide deep images over wide areas sufficient enough for searching high redshift quasars. In addition, we carried out a J-band imaging survey at the United Kingdom InfraRed Telescope (UKIRT) with a depth of ~23 AB and survey area of ~100 $deg^2$, which makes IMS the most suitable survey for finding high redshift quasars at z~7. Also for the quasar candidates at z~5.5, we are conducting observations with the Camera for QUasars in EArly uNiverse (CQUEAN), which are efficient for selecting robust quasar candidate samples in this redshift range. We used various color-color diagrams suitable to the specific redshift ranges, which can reduce the contaminating sources such as M/L/T dwarfs, low redshift galaxies, and instrumental defects. The high redshift quasars we are confirming can provide us with clues to the growth of super massive black holes since z~7. Also by expanding the quasar sample at 5

• 천문학논총
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• 제32권1호
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• pp.321-326
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• 2017

We analyzed spectral data of the astrophysical diffuse emission obtained with the low-resolution spectroscopy mode on the AKARI InfraRed Camera (IRC) in the $1.8-5.3{\mu}m$ wavelength region. Advanced reduction methods specialized for slit spectroscopy of diffuse sky spectra have been developed, and a catalog of 278 spectra of the diffuse sky covering a wide range of Galactic and ecliptic latitudes was constructed. Using this catalog, two other major foreground components, the zodiacal light (ZL) and the diffuse Galactic light (DGL), were separated and subtracted by taking correlations with ZL brightness estimated by the DIRBE ZL model and with the $100{\mu}m$ dust thermal emission, respectively. The isotropic emission was interpreted as the extragalactic background light (EBL), which shows significant excess over the integrated light of galaxies at <$4{\mu}m$.