• 감성과학
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• 제17권3호
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• pp.3-14
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• 2014

2009년 아이폰의 국내 출시 이후 스마트폰의 보급이 급격히 증가하여 기존에 다양한 장비로 수행되어 오던 작업이 스마트폰으로 대체되었다. 이 과정에서 스마트폰의 작은 화면을 통하여 글자를 읽는 과제를 수행하는 비중이 상당히 증가하였다. 본 연구에서는 일상적인 스마트폰 사용 환경에서 디스플레이 요인(화소 밀집도, 화소 하부구조, 휘도)과 환경 요인(조명 조도)이 글자를 읽을 때의 가독성 관련 불편감에 어떤 영향을 미치는지를 확인하였다. 그 결과 지각된 가독성 관련 불편감에 영향을 미치는 것은 주로 화소 밀집도로, 화소 밀집도가 300 PPI미만인 경우 글자를 읽는데 불편함을 느낀다는 것을 확인하였다. 조명 조도는 제한적인 영향을 보였다. 참가자들은 조명 조도가 변화 할 때 변화하지 않을 때 보다 더 큰 가독성 관련 불편감을 보고하였다. 화소 하부구조와 밝기는 가독성 관련 불편감에 영향을 미치지 않았다. 이 결과를 바탕으로 가독성을 고려할 때 다양한 크기를 가지는 스마트 기기(스마트 폰, 태블릿 컴퓨터)에서 가독성을 해치지 않는 해상도의 하한선을 제안하였다.

• 한국정보디스플레이학회:학술대회논문집
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• 한국정보디스플레이학회 2006년도 6th International Meeting on Information Display
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• pp.49-51
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• 2006

A new data line reduction driving method was developed for high pixel density LCoS microdisplays. Its pixel structures and its corresponding gate line waveform were proposed, too. This idea can fulfill the increasing demand for higher resolution LCoS. In this method, no additional AC power is dissipated, and no more horizontal line time is needed. So this method can be applied to the high resolution microdisplay devices. It prefers being applied to the reflective liquid crystal on silicon microdisplays because of the pixel structure asymmetry and PMOS transistor switches used.

• 대한원격탐사학회지
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• 제23권3호
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• pp.153-160
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• 2007

Forest cover density studies using high resolution satellite data and object oriented classification are limited in India. This article focuses on the potential use of QuickBird satellite data and object oriented classification in forest density mapping. In this study, the high-resolution satellite data was classified based on NDVI/pixel based and object oriented classification methods and results were compared. The QuickBird satellite data was found to be suitable in forest density mapping. Object oriented classification was superior than the NDVI/pixel based classification. The Object oriented classification method classified all the density classes of forest (dense, open, degraded and bare soil) with higher producer and user accuracies and with more kappa statistics value compared to pixel based method. The overall classification accuracy and Kappa statistics values of the object oriented classification were 83.33% and 0.77 respectively, which were higher than the pixel based classification (68%, 0.56 respectively). According to the Z statistics, the results of these two classifications were significantly different at 95% confidence level.

• 천문학회보
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• 제44권2호
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• pp.53.4-53.4
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• 2019

We reconstruct the underlying dark matter (DM) density distribution of the local universe within 20Mpc/h cubic box by using the galaxy position and peculiar velocity. About 1,000 subboxes in the Illustris-TNG cosmological simulation are used to train the relation between DM density distribution and galaxy properties by using UNet-like convolutional neural network (CNN). The estimated DM density distributions have a good agreement with their truth values in terms of pixel-to-pixel correlation, the probability distribution of DM density, and matter power spectrum. We apply the trained CNN architecture to the galaxy properties from the Cosmicflows-3 catalogue to reconstruct the DM density distribution of the local universe. The reconstructed DM density distribution can be used to understand the evolution and fate of our local environment.

• 한국정보디스플레이학회:학술대회논문집
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• 한국정보디스플레이학회 2005년도 International Meeting on Information Displayvol.II
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• pp.867-872
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• 2005

High-pixel-density displays are now under development to meet the needs of next-generation mobile devices; methods to more efficiently build such displays are described. Displays based on subpixel rendering and RGBW technologies, known as PenTile $Matrix^{TM}$ RGBW, are shown to offer the best approach to meeting the demanding requirements of low manufacturing cost, high brightness, and low power.

• 한국정보디스플레이학회:학술대회논문집
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• 한국정보디스플레이학회 2005년도 International Meeting on Information Displayvol.I
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• pp.21-25
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• 2005

In order to implement high pixel density in AMLCDs, high aperture ratio is a very important design factor. We have implemented VGA panels with IPS and TN modes. IPS mode is a very attractive solution to meet the requirement for mobile phone displays. It provides much higher aperture ratio as well as wider viewing angle at extremely high pixel density over 400 ppi.

• KSII Transactions on Internet and Information Systems (TIIS)
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• 제11권12호
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• pp.5998-6016
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• 2017

In thin-film transistor liquid-crystal displays (TFT-LCDs), which are most commonly used in mobile devices, the backlight accounts for about 70% of the power consumption. Therefore, most low-power-related studies focus on realizing power savings through backlight dimming. Image compensation is performed to mitigate the visual distortion caused by the backlight dimming. Therefore, popular techniques include pixel compensation for brightness recovery and contrast enhancement, such as histogram equalization. However, existing pixel compensation techniques often have limitations with respect to blur owing to the pixel saturation phenomenon, or because contrast enhancement cannot adequately satisfy the human visual system (HVS). To overcome these, in this study, we propose a novel dimming technique to achieve both power saving and HVS-awareness by combining the pixel compensation and histogram specifications, which convert the original cumulative density function (CDF) by designing and using the desired CDF of an image. Because the process of obtaining the desired CDF is customized to consider image characteristics, histogram specification is found to achieve better HVS-awareness than histogram equalization. For the experiments, we employ the LIVE image database, and we use the structural similarity (SSIM) index to measure the degree of visual satisfaction. The experimental results show that the proposed technique achieves up to 15.9% increase in the SSIM index compared with existing dimming techniques that use pixel compensation and histogram equalization in the case of the same low-power ratio. Further, the results indicate that it achieves improved HVS-awareness and increased power saving concurrently compared with previous techniques.

• International Journal of Computer Science & Network Security
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• 제22권11호
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• pp.308-318
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• 2022

Noise is a serious issue. While sending images via electronic communication, Impulse noise, which is created by unsteady voltage, is one of the most common noises in digital communication. During the acquisition process, pictures were collected. It is possible to obtain accurate diagnosis images by removing these noises without affecting the edges and tiny features. The New Average High Noise Density Median Filter. (HNDMF) was proposed in this paper, and it operates in two steps for each pixel. Filter can decide whether the test pixels is degraded by SPN. In the first stage, a detector identifies corrupted pixels, in the second stage, an algorithm replaced by noise free processed pixel, the New average suggested Filter produced for this window. The paper examines the performance of Gaussian Filter (GF), Adaptive Median Filter (AMF), and PHDNF. In this paper the comparison of known image denoising is discussed and a new decision based weighted median filter used to remove impulse noise. Using Mean Square Error (MSE), Peak Signal to Noise Ratio (PSNR), and Structure Similarity Index Method (SSIM) metrics, the paper examines the performance of Gaussian Filter (GF), Adaptive Median Filter (AMF), and PHDNF. A detailed simulation process is performed to ensure the betterment of the presented model on the Mini-MIAS dataset. The obtained experimental values stated that the HNDMF model has reached to a better performance with the maximum picture quality. images affected by various amounts of pretend salt and paper noise, as well as speckle noise, are calculated and provided as experimental results. According to quality metrics, the HNDMF Method produces a superior result than the existing filter method. Accurately detect and replace salt and pepper noise pixel values with mean and median value in images. The proposed method is to improve the median filter with a significant change.

• 천문학회보
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• 제44권1호
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• pp.43.3-43.3
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• 2019

Magnetic fields play an important role in supporting molecular clouds against gravitational collapse. The measured magnetic field strengths in molecular clods enable us to see the effect of magnetic fields in star-forming regions. People have used the Chandrasekhar and Fermi (CF) method to estimate magnetic field strength from observational quantities of molecular cloud density, turbulent velocity and polarization angle dispersion. However, previous studies obtained just one magnetic field strength over the quite large region of a molecular cloud by using the CF method. We here suggest a way to estimate magnetic field strength distribution in Orion A region. We used 450 and 850-micron polarization data of James Clerk Maxwell Telescope (JCMT). Magnetic field strengths were estimated in two wavelengths with 4 pixel resolutions of 16, 20, 24 and 28". Through statistical analysis, we proved the difference of magnetic field strengths between two wavelengths were caused by the difference of their beam sizes. Additionally, we calculated the radii of curvature of polarization segments to select a best pixel resolution for estimating the magnetic field distribution. The pixel resolution should be larger than a radius of curvature. We selected that 20 or 24" pixel resolutions are good choices towards Orion A region.

• 한국결정성장학회지
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• 제27권2호
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• pp.75-79
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• 2017

고밀도 플라즈마 식각 및 lift-off 두 가지 공정으로 honeycomb 형상의 Ag-grid 투명전극층을 제작하였고 제조 공법에 따른 광학적 및 전기적 특성을 비교하였다. 플라즈마 식각 조건 선정을 위하여 Ag 박막의 $10CF_4/5Ar$ 유도결합 플라즈마 식각특성을 조사하였다. 비교적 낮은 ICP source power 또는 rf chuck power 영역에서는 power 증가에 따라 Ag 식각속도가 증가하였고, 높은 power 조건에서는 $Ar^+$ 이온 에너지 감소 또는 $Ar^+$ 이온에 의한 F radical 제거로 인해 식각속도가 감소하였다. $10CF_4/5Ar$ 플라즈마 식각 공정에 의해 제작된 Ag-grid 전극층은 lift-off 공정으로 제작된 전극층에 비해 grid 패턴 형상의 왜곡이나 단절이 없는 더 우수한 grid 패턴 전사 효율과 가시광선 영역에서 더 높은 83.3 %(pixel 크기 $30{\mu}m$/선폭 $5{\mu}m$)와 71 %(pixel 크기 $26{\mu}m$/선폭 $8{\mu}m$)의 광투과율을 각각 나타내었다. 반면에 lift-off 공정으로 제작된 Ag-grid 전극층은 플라즈마 식각 공정 시편보다 더 우수한 $2.163{\Omega}/{\square}$(pixel 크기 $26{\mu}m$/선폭 $8{\mu}m$)과 $4.932{\Omega}/{\square}$(pixel 크기 $30{\mu}m$/선폭 $5{\mu}m$)의 면저항 특성을 나타내었다.