• 천문학회지
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• 제46권6호
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• pp.243-251
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• 2013

We present results on the intrinsic brightness temperature of a sample of compact radio sources observed at 86 GHz using the Global Millimeter VLBI Array. We use the observed brightness temperatures at 86 GHz and the observed superluminal motions at 15 GHz for the sample in order to constrain the characteristic intrinsic brightness temperature of the sample. With a statistical method for studying the intrinsic brightness temperatures of innermost jet cores of compact radio sources, assuming that all sources have the same intrinsic brightness temperature and the viewing angles of their jets are around the critical value for the maximal apparent speed, we find that sources in the sample have a characteristic intrinsic brightness temperature, $T_0=4.8^{+2.6}_{-1.5}{\times}10^9K$, which is lower than the equipartition temperature for the condition that the particle energy equals to the magnetic field energy. Our results suggest that the VLBI cores seen at 86 GHz may be representing a jet region where the magnetic field energy dominates the total energy in the jet.

• 천문학회보
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• 제39권2호
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• pp.57.1-57.1
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• 2014

We present results of our investigation of intrinsic brightness temperatures of compact radio jets at radio frequencies. The intrinsic brightness temperatures of about 100 compact radio jets at 2, 5, 8, 15, and 86 GHz are estimated based on large VLBI surveys conducted in 2001-2003 (or in 1996 for the 5 GHz sample). The multi-freqeuncy intrinsic brightness temperatures of the sample of the jets are determined with a statistical method relating the observed brightness temperatures with the maximal apparent jet speed, assuming one representative intrinsic brightness temperature for the sample at each observing frequency. With investigating the observed brightness temperatures at 15 GHz in multiple epochs, we found that the determination of the intrinsc brightness temperature for our sample is affected by variability of individual jets in flux density at the time scales of a few years. This implies an importance of contemporaneity of the multi-frequency VLBI observations for the statistical method. Since our analysis is based on the VLBI observations conducted in 2001-2003, the results are less affected by the flux density variability. We found that the intrinsic brightness temperature $T_0$ increases as $T_0{\propto}{\nu}^{\epsilon}$ with ${\epsilon}{\approx}0.7$ below a critical frequency ${\nu}_c{\approx}10GHz$ where energy losses begin to dominate the emission, and above the critical frequency, $T_0$ decreases with ${\epsilon}{\approx}-1.2$ supporting for the decelerating jet model.

• 천문학회지
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• 제47권6호
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• pp.303-309
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• 2014

We present results of our investigation of the radio intrinsic brightness temperatures of compact radio jets. The intrinsic brightness temperatures of about 100 compact radio jets at 2, 5, 8, 15, and 86 GHz are estimated based on large VLBI surveys conducted in 2001-2003 (or in 1996 for the 5 GHz sample). The multi-frequency intrinsic brightness temperatures of the sample of jets are determined by a statistical method relating the observed brightness temperatures with the maximal apparent jet speeds, assuming one representative intrinsic brightness temperature for a sample of jets at each observing frequency. By investigating the observed brightness temperatures at 15 GHz in multiple epochs, we find that the determination of the intrinsic brightness temperature for our sample is affected by the flux density variability of individual jets at time scales of a few years. This implies that it is important to use contemporaneous VLBI observations for the multi-frequency analysis of intrinsic brightness temperatures. Since our analysis is based on the VLBI observations conducted in 2001-2003, the results are not strongly affected by the flux density variability. We find that the intrinsic brightness temperature $T_0$ increases as $T_0{\propto}{\nu}^{\xi}_{obs}$ with ${\xi}=0.7$ below a critical frequency ${\nu}_c{\approx}9GHz$ where the energy loss begins to dominate the emission. Above ${\nu}_c$, $T_0$ decreases with ${\xi}=-1.2$, supporting the decelerating jet model or particle cascade model. We also find that the peak value of $T_0{\approx}3.4{\times}10^{10}$ K is close to the equipartition temperature, implying that the VLBI cores observable at 2-86 GHz may be representing jet regions where the magnetic field energy dominates the total energy in jets.

• International journal of advanced smart convergence
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• 제9권4호
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• pp.203-208
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• 2020

In this paper, we propose the design and implementation of a desktop LED stand and smart app that automatically adjusts color temperature and illuminance for optimal brightness and eye health by improving the structural problem of the LED stand. It is a tabletop LED stand that supports optimal brightness through color temperature control and heat transfer through infrared LED to relieve eye strain through blood circulation and muscle movement. The LED stand works with the smartphone to automatically adjust the optimal brightness and color temperature for the user's environment. In addition, the brightness of the infrared LED is adjusted to a living frequency of 4Hz to relax the eye muscles and reduce eye strain. This study implemented an effective measured data-based system of previous studies through the color temperature and illumination of LED lighting, and near-infrared rays, and presented meaningful results by conducting an experiment to prove the effect through subjects.

• 한국지리정보학회지
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• 제21권2호
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• pp.68-79
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• 2018

일반적으로 밝기온도는 대기온도와 밀접한 연관이 있으며, 밝기온도는 Landsat과 같은 지구관측위성의 열적외 센서를 활용하여 측정이 가능하다. Landsat-8 위성의 열적외 센서는 지표온도를 측정할 수 있는 두 개의 밴드 (Band 10과 Band 11)를 가지고 있다. 본 연구에서는 대한민국 서울지역의 기상관측센터에서 측정한 대기온도와 Band 10과 Band 11로부터 각각 측정한 밝기온도의 상관관계를 시기별(봄, 여름, 가을, 겨울)로 분석하였으며, 본 연구를 통해 다음과 같은 결과를 확인할 수 있었다. 첫째, 밝기온도와 대기온도의 상관관계는 봄, 가을, 겨울 및 여름 순으로 높았다. 둘째, 봄, 가을 및 겨울에서는 대기온도가 증가할수록 밝기온도도 증가하였으나, 여름에서는 대기온도가 증가할수록 밝기온도는 감소하였다. 셋째, Band 10을 활용하여 측정한 밝기온도가 Band 11을 활용하여 측정한 밝기온도에 비해 대기온도와 상관관계가 높았다.

• 한국안전학회지
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• 제27권4호
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• pp.13-19
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• 2012

The purpose of this study is to extract the major factors related to the deterioration mechanism of white organic light-emitting diodes(WOLED) by performing accelerated testing of temperature, voltage, time, etc., and to develop an accelerated life test(ALT) model. The measurement results of the brightness of the WOLED exhibited that their average brightness tended to increase as the operating voltage increased and that the half-life period of the brightness appeared after approximately 400 hours when the operating voltage was 20V and the ambient temperature was $85^{\circ}C$. It could be seen that although the WOLED showed comparatively the same brightness when the initial acceleration began after the operating voltage was applied to it, its brightness changed excessively after the WOLED's thermal storage had been made. In addition, it was observed that the half-life period was reduced as the ambient temperature and applied voltage increased. The strength of the WOLED which had been maintained in the range of visible light at the maximum load was reduced by the deterioration of the organic light emitting material due to the influence of the operating voltage and temperature, and the reduction of emitted light was small at low voltage and temperature. It could be seen that the failure of the WOLED during the ALT was caused by wear due to load accumulation over time, and that Weibull distribution was appropriate for the life distribution and acceleration was established between test conditions. From the WOLED analysis, it is thought that factors influencing the brightness deterioration are voltage, temperature, etc., and that comprehensive analysis considering discharge control, dielectric tangent margin, etc., would further increase the reliability.

• 한국항공우주학회지
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• 제48권12호
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• pp.977-985
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• 2020

2015년 발사된 다목적실용위성 3A호는 3.3~5.2㎛ 파장의 중적외선 영상을 제공한다. 다목적실용위성 3A호는 지상 물체의 밝기 온도를 추정하기 위한 고해상도 영상을 제공하지만 기존 자연 과학 목적으로 개발된 위성과 차이가 있다. 다목적실용위성 3A호의 단일 채널의 중적외선 영상으로 지표 밝기 온도를 추정하기 위해서는 대기 보정 과정이 필수적이다. 하지만 대기 보정 이후에도 여러 요인으로 인하여 밝기 온도 추정 오차가 존재한다. 본 논문에서는 다목적실용위성 3A호 카메라의 물리적인 특성으로부터 영상 처리까지 신호 흐름을 추적하여 밝기 온도 추정 오차 요인을 분석하였다. 또한, 천리안위성 2A호를 이용하여 다목적실용위성 3A호와 밝기 온도 편향 오차 개선 가능성을 연구하였다. 큰 편향 오차를 가지고 있는 야간 영상에 대하여 편향 오차를 보상한 이후 다목적실용위성 3A호와 천리안위성 2A호의 지표 밝기 온도가 상관성이 있음을 확인하였다. 다목적실용위성 3A호 중적외선 밝기 온도 편향 오차를 개선하는데 천리안위성 2A호 영상이 도움이 될 것으로 예상된다.

• 대한원격탐사학회:학술대회논문집
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• 대한원격탐사학회 2007년도 Proceedings of ISRS 2007
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• pp.282-285
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• 2007

Satellite observed brightness temperature simulation using a radiative transfer model (here after, RTM) is useful for various fields, for example sensor design and channel selection by using theoretically calculated radiance data, development of satellite data processing algorithm and algorithm parameter determination before launch. This study is focused on elaborating the simulation procedure, and analyzing of difference between observed and modelled clear sky brightness temperatures. For the CMDPS (COMS Meteorological Data Processing System) development, the simulated clear sky brightness temperatures are used to determine whether the corresponding pixels are cloud-contaminated in cloud mask algorithm as a reference data. Also it provides important information for calibrating satellite observed radiances. Meanwhile, simulated brightness temperatures of COMS channels plan to be used for assessing the CMDPS performance test. For these applications, the RTM requires fast calculation and high accuracy. The simulated clear sky brightness temperatures are compared with those of MTSAT-1R observation to assess the model performance and the quality of the observation. The results show that there is good agreement in the ocean mostly, while in the land disagreement is partially found due to surface characteristics such as land surface temperature, surface vegetation, terrain effect, and so on.

• 전자공학회논문지
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• 제53권5호
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• pp.163-167
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• 2016

본 논문은 밀리미터파 라디오미터를 이용한 의료응용의 한 분야인 인체 내부의 밝기온도 측정에 관한 연구이다. 밀리미터파 대역 중에서 Ka - band의 주파수 영역에서 동작하는 렌즈, 직접 검출 수신기, 캘리브레이션 소스 등을 설계 제작하여 라디오미터 시스템을 구성하였다. 밀리미터파 렌즈 초점에 수신안테나를 스캔하는 방식을 통하여 미약한 신호를 수신하였으며, 렌즈 수차를 감소시키기 위해 광선 추적 방법을 사용하여 비구면 렌즈를 설계 하였다. 직접 검출 수신기는 Dicke 타입 수신기 형태로 설계되었으며, 제작된 수신기의 잡음지수는 3.3 dB, 온도감도는 0.1 K으로 측정되었다. 라디오미터의 수신기 교정은 밀리미터파 대역에서 사용가능한 새로운 형태의 블랙바디(Black body)를 제작하여 물체의 등가 잡음온도와 출력전압의 관계를 도출하였다. 제작된 시스템을 이용하여 1.7 m 거리에서 인체의 상반신을 측정하여 약 $38^{\circ}$[C]의 밝기온도를 측정하였다. 적외선 영상과 라디오미터 영상의 비교를 통해 상반신의 밝기온도 영상을 통하여 밀리미터파 라디오미터의 의료응용 가능성을 제시하였다.

• 한국정밀공학회:학술대회논문집
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• 한국정밀공학회 2005년도 춘계학술대회 논문집
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• pp.1609-1612
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• 2005

The effects of injection molding conditions on the uniformity and brightness of light guide plate(LGP) with micro-patterns were investigated in the present study. An injection molding system for stampers with mirco-pattern was designed and manufactured to perform experiment. Variations of injection molding speed, mold and melt temperature for LGP were considered in this work. Also, injection molding characteristics of LGP were investigated by numerical analysis using plastic injection molding commercial code. It was shown that injection molding conditions such as injection speed, melt temperature and mold temperature can have an effect on the uniformity and brightness of light guide plate.