• The Journal of Asian Finance, Economics and Business
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• 제4권2호
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• pp.75-80
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• 2017

Hand phones are standard paraphernalia among university students. Factors that motivate them to own the gadget would be of interest to both the students as well as marketers. Hand phone usage is an unexamined field in academic literature, this exploratory study attempts to investigate student purchasing motives in cellular phone markets. It also intends to know the student's satisfaction with the different services and its future impact on socio economic changes. In this study, undergraduates (n=336) were requested to specify their purchase criteria of hand phone. The instrument used in the study to collect feedback from the respondents contains a combination of open-ended and scaled questions, and some background demographics. The study employed content analysis, Pearson's correlation, and t-tests as the primary tools to analyze the responses. Results show that brand was rated as the most important factor in student purchase decisions. Other factors, arranged in decreasing order of importance comprise price, product quality, features, durability, availability, promotion, and post purchase service. Brand and price correlated significantly. It is also observed that there is very little difference regarding preference between brand and price in purchasing a hand phone. Marketers may formulate suitable strategies out of the findings to promote hand phones to university undergraduates in Malaysia by emphasizing at brands and price.

• 한국인터넷방송통신학회논문지
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• 제20권4호
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• pp.87-92
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• 2020

GPGPU(General-Purpose GPU)는 수만 단위의 스레드들을 병렬적으로 수행하여 성능을 최대화시킬 수 있지만, 실질적으로는 스레드들을 그룹화하여 스레드블록(Thread Block) 단위로 작업을 정의하고 GPGPU 하드웨어 자원의 할당 단위로 활용한다. 이러한 역할을 담당하는 스레드블록 스케줄러는 GPGPU내에 하드웨어적으로 구현되어 있으며, 스레드블록들을 하드웨어 자원들에게 라운드로빈 방식으로 할당한다. 그런데, 라운드로빈 정책은 단순 순차 할당 방식으로서 GPGPU 하드웨어 자원의 활용도에 최적화되어 있지 않다. 본 논문에서는 다양한 스레드블록 스케줄링 방식의 성능을 정량적으로 분석할 수 있는 스레드블록 스케줄러 모델을 제안하고, 구현된 시뮬레이터의 성능 결과를 통해 기존 GPGPU의 스레드블록 스케줄링 방식이 작업 부하가 높은 경우에는 적합하지 않음을 보이고자 한다.

• 천문학회보
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• 제41권1호
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• pp.39.4-40
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• 2016

We aim to investigate formation of satellite sub-galactic structures around isolated dwarf galaxies using cosmological hydrodynamic zoom simulations. For this, we modify a cosmological hydrodynamic code, GADGET-3, in a way that includes gas cooling down to T~10K, gas heating by universal reionization when z < 8.9, UV shielding for high density regions of $n_{shield}$ > $0.014cm^{-3}$, star formation in the dense regions ($n_H$ > $100cm^{-3}$), and supernova feedback. To get good statistics, we perform three different simulations for different target galaxies of the same mass of ${\sim}10^{10}M_{sun}$. Each simulation starts in a cubic box of a side length of 1Mpc/h with 17 million particles from z = 49. The mass of dark matter (DM) and gas particle is $M_{DM}=4.1{\times}10^3M_{sun}$ and $M_{gas}=7.9{\times}10^2M_{sun}$, respectively, thus each satellite sub-galactic structure can be resolved with more than hundreds or thousands particles. We analyze total 90 sub-galactic structures that have formed outside of the main halos but infall the main halos. We found that 1) mini halos that interact more with the other mini halos tend to accrete the more mass, 2) mini halos that interact more before the reionization tend to form more stars, 3) mini halos with the more interaction tend to approach closer to the galactic center and have the lower orbital circularity, 4) survivals even in the strong tidal fields evolve baryon dominated system, such as globular clusters.

• 천문학회보
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• 제36권1호
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• pp.61.1-61.1
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• 2011

NGC5929는 북동방향으로 0.5' 떨어진 NGC5930의 기조력 영향을 받는 활동성은하이다. 우리는 NGC5930이 NGC5929와의 상호작용에 따라 NGC5929의 활동성을 어떻게 유발하는지 수치실험을 알아보고자 한다. NGC5929의 적경, 적위는 (15h 26m, $41^{\circ}$40')이고, 크기는 $1'.14{\times}$ 0'.89이다. 지구로부터 거리는 36.5Mpc(적색편이는 $0.00836{\pm}0.00007km/s$)이다. 관측 자료에서 보인 NGC5929는 원반 모양의 은하 오른쪽 위쪽의 가스는 접근성, 왼쪽 아래 부분은 멀어지는 운동학적 특성이 보인다. 호스트 은하 원반이 기울어져 장축 방향이 $PA=85^{\circ}$, 단축이 $PA=45^{\circ}$ 은하의 구조임을 알 수 있다. 이 연구를 위해 우리는 하와이 CFHT 3.6m의 OASIS로 관측한 NGC5929의 중심부를 MR1, MR2로 관측한 영상을 참고하여, 이 영상에서 보이는 활동성 즉, 15*12 arcsec의 OASIS field 영역의 관측 자료에 나타난 $H{\beta}$영상이나, [O III]에 나타난 제트 형태와 방출방향에 대해 조사하였다. CFHT OASIS의 분석으로 우리는 continuum, [O III], $H{\beta}$ 선을 통한 영상을 조사하였고, 특히 [O III]영상에서 에서 강한 활동은하의 성격이 보인다. 이 방출선의 특성이 별의 UV, 행성상 성운 주변, 블랙홀 주위, 충격파 중 어느 영향이 가장 강한지 조사하였고, [O III]이미지에서 보인 제트의 형성조건에 동반은하 NGC5930의 영향이 어떠한 역할을 하였는지 조사하고, $H{\beta}$영상에 나타난 starburs지역도 살펴보고자 한다. 우리는 관측 자료에서 보인 활동성의 근원을 알기 위해 Gadget, Magalie를 사용하여 두 은하의 운동학적 및 은하의 구조에 대해 조사하려고 한다.

• 한국산업융합학회 논문집
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• 제23권6_2호
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• pp.949-956
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• 2020

It's important to measure fuel consumption of vehicles. It's possible to monitor green house gas from vehicles for various traffic conditions with the measured data. It's effective to eco-drive for drivers with fuel consumption data also. There's a display of fuel consumption in the modern vehicles, but it's not useful to get the data from the display. An estimating method for fuel consumption of a vehicle is suggested in the study. It's a simple but an effective method using GPS data. The GPS data(speed, acceleration, road slope) and vehicle data(weight, frontal area, model year, certified fuel economy) is necessary to estimate the fuel consumption for the method. It calculates driving resistance force to estimate engine power. Then it estimates the necessary fuel consumption to maintain the engine power with fuel-power conversion factor. The conversion factor is corrected with certified fuel economy, model year and rated power. The precision of the methods is checked with road test data. The test driving data was measured with GPS and OBD. The error of the estimated fuel consumption for the measured one is about 1.8%. But the error is large for the 1000 and 100 data number from the total data number of about 10,000. The error is from the larger change range of the GPS data than the one of the measured fuel consumption data. But the proposed estimating method is useful to percept the fuel consumption change for better fuel economy with simple gadget like smart phone or other GPS instruments.

• Safety and Health at Work
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• 제14권1호
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• pp.66-70
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• 2023

Background: Online teaching and learning extend the duration of using gadgets such as mobile phones and tablets. A prolonged usage of these gadgets in a static position can lead to musculoskeletal disorders (MSD). Therefore, this study aims to identify the risk factors related to musculoskeletal symptoms while using gadgets during work from home due to the COVID-19 pandemic. Method: A cross-sectional survey with online-based questionnaires was collected from the University of Indonesia, consisting of lecturers, students, and managerial staff. The minimum number of respondents was 1,080 and was defined by stratified random sampling. Furthermore, the dependent variable was musculoskeletal symptoms, while the independent were age, gender, job position, duration, activity when using gadgets, and how to hold them. Result: Most of the respondents had mobile phones but only 16% had tablets. Furthermore, about 56.7% have used a mobile phone for more than 10 years, while about 89.7% have used a tablet for less than 10 years. A multivariate analysis found factors that were significantly associated with MSD symptoms while using a mobile phone, such as age, gender, web browsing activity, work, or college activities. These activities include doing assignments and holding the phone with two hands with two thumbs actively operating. The factors that were significantly associated with MSD symptoms when using tablets were gender, academic position, social media activity, and placing the tablet on a table with two actively working index fingers. Conclusion: Therefore, from the results of this study it is necessary to have WFH and e-learning policies to reduce MSD symptoms and enhance productivity at work.

• 천문학회보
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• 제44권2호
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• pp.48.4-48.4
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• 2019

We studied the metal-distribution of isolated Milky-way mass galaxy using various hydrodynamic solvers and investigated the difference of the result between AMR and SPH codes. In particle-based codes, physical quantities like mass or metallicity defined in each particle are conserved unless being injected explicitly by the effect of the supernova, whereas in the Eulerian codes the diffusion is simply accomplished by hydro-equation. Therefore, without including explicit physics of diffusion on the SPH- codes, the metal mixing in the galaxy or CGM only can be accomplished by the direct motion of the particles, however, the standard-SPH codes depress the instability of the turbulent fluid mixing. In this work, we simulated under common initial conditions, common gas-physics like cooling-heating models, and star-formation feedback using ENZO(AMR) GIZMO and GADGET-2 codes. We additionally included a metal-diffusion algorithm on the SPH-codes, which follows the subgrid-turbulent mixing model investigated by Shen et al. (2010) and compared the effect of the metal-outflow on the halo region of the galaxy in different hydro-solvers. We also found that for the implementation of the diffusion scheme in the SPH-codes, the existence of a sufficient number of the gas-particles, which is the carrier of the metals, is necessary. So we tested a new initial condition for proper implementation of the diffusion scheme on the SPH simulations. By comparing the metal-contamination of the circumgalactic medium with different hydrodynamics models, we quantify the diffusion strength of AMR codes using diffusion parameterization of the SPH codes and also suggest the calibration solutions in the different behavior of codes in metal-outflow.

• International Journal of Internet, Broadcasting and Communication
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• 제16권1호
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• pp.17-28
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• 2024

As listed as one of the most important requirements for Post-Quantum Cryptography standardization process by National Institute of Standards and Technology, the resistance to various side-channel attacks is considered very critical in deploying cryptosystems in practice. In fact, cryptosystems can easily be broken by side-channel attacks, even though they are considered to be secure in the mathematical point of view. The timing attack(TA) and the simple power analysis attack(SPA) are such side-channel attack methods which can reveal sensitive information by analyzing the timing behavior or the power consumption pattern of cryptographic operations. Thus, appropriate measures against such attacks must carefully be considered in the early stage of cryptosystem's implementation process. The Montgomery multiplier is a commonly used and classical gadget in implementing big-number-based cryptosystems including RSA and ECC. And, as recently proposed as an alternative of building blocks for implementing post quantum cryptography such as lattice-based cryptography, the big-number multiplier including the Montgomery multiplier still plays a role in modern cryptography. However, in spite of its effectiveness and wide-adoption, the multiplier is known to be vulnerable to TA and SPA. And this paper proposes a new countermeasure for the Montgomery multiplier against TA and SPA. Briefly speaking, the new measure first represents a multiplication operand without 0 digits, so the resulting multiplication operation behaves in a very regular manner. Also, the new algorithm removes the extra final reduction (which is intrinsic to the modular multiplication) to make the resulting multiplier more timing-independent. Consequently, the resulting multiplier operates in constant time so that it totally removes any TA and SPA vulnerabilities. Since the proposed method can process multi bits at a time, implementers can also trade-off the performance with the resource usage to get desirable implementation characteristics.

• 천문학회지
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• 제46권1호
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• pp.1-32
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• 2013

We construct several Milky Way-like galaxy models containing a gas halo (as well as gaseous and stellar disks, a dark matter halo, and a stellar bulge) following either an isothermal or an NFW density profile with varying mass and initial spin. In addition, galactic winds associated with star formation are tested in some of the simulations. We evolve these isolated galaxy models using the GADGET-3 N-body/hydrodynamic simulation code, paying particular attention to the effects of the gaseous halo on the evolution. We find that the evolution of the models is strongly affected by the adopted gas halo component, particularly in the gas dissipation and the star formation activity in the disk. The model without a gas halo shows an increasing star formation rate (SFR) at the beginning of the simulation for some hundreds of millions of years and then a continuously decreasing rate to the end of the run at 3 Gyr. Whereas the SFRs in the models with a gas halo, depending on the density profile and the total mass of the gas halo, emerge to be either relatively flat throughout the simulations or increasing until the middle of the run (over a gigayear) and then decreasing to the end. The models with the more centrally concentrated NFW gas halo show overall higher SFRs than those with the isothermal gas halo of the equal mass. The gas accretion from the halo onto the disk also occurs more in the models with the NFW gas halo, however, this is shown to take place mostly in the inner part of the disk and not to contribute significantly to the star formation unless the gas halo has very high density at the central part. The rotation of a gas halo is found to make SFR lower in the model. The SFRs in the runs including galactic winds are found to be lower than those in the same runs but without winds. We conclude that the effects of a hot gaseous halo on the evolution of galaxies are generally too significant to be simply ignored. We also expect that more hydrodynamical processes in galaxies could be understood through numerical simulations employing both gas disk and gas halo components.

• 전자공학회논문지CI
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• 제47권5호
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• pp.50-60
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• 2010

지난 반세기 동안 컴퓨터 시스템의 발전으로 개인용 컴퓨터와 소프트웨어 산업은 유래 없는 호황을 누렸다. 21세기에 들어서는 이러한 흐름이 모바일 기기로 점차 이동하면서 임베디드 시스템 시장이 폭발적으로 증가하였다. 휴대전화, 내비게이션 시스템, PMP 등의 휴대용 멀티미디어 기기들은 시장에 쏟아져 나온 반면에 대부분의 산업용 제어시스템은 여전히 단순제어 시스템에 의존하여 제품이 개발되고 있다. 실제로 이를 첨단 하드웨어와 소프트웨어의 기술로 전환하려고 해도 그 수요가 모바일 시장에 비해 낮아 부품수급이 어렵고 가격이 상승하는 문제를 안고 있으며 기술개발 시 발생하는 많은 비용과 인력은 기업 입장에서는 투자 부담이 될 수밖에 없다. 그러나 미래 고객들에게 제품에 대한 기업 이미지를 끌어올리기 위해서는 고성능 시스템의 하드웨어와 소프트웨어 플랫폼 개발이 반드시 필요하다. 본 논문에서는 이러한 문제점들을 해결하기 위해서 네트워크 임베디드 시스템의 최적화된 하드웨어 플랫폼과 소프트웨어 플랫폼을 개발하였다. 개발된 플랫폼은 멀티미디어 기능을 추가하여 고급형 제품을 위한 플랫폼으로 제작하였다. 멀티미디어 기능을 구현하기 위해서 텔레칩스 사의 멀티미디어 프로세서인 TCC8300을 기반으로 개발하였으며 프로세서 내부의 다양한 병렬하드웨어 기능을 이용함으로써 회로상의 부품의 수를 최소화 하고 성능 향상과 더불어 전력소모량을 최소화하였다. 그리고 소프트웨어의 기술비용(로열티)을 없애기 위해서 오픈소스 기반의 운영체제인 임베디드 리눅스와 오픈소스 기반의 그래픽 라이브러리인 TinyX와 GTK+를 이용하여 GUI(Graphic User Interface)를 구현하였다. 또한 개발된 플랫폼을 이용하여 여러 가지 방식의 YUV2RGB 프레임 변환 실험 및 측정을 통해서 성능 및 프레임별 변환 시에 소모되는 전력량을 계산하였고 플랫폼의 각 부분별 동작에 대한 전력소모량 측정을 통해서 플랫폼 구성 시 필요한 전력과 성능을 예측할 수 있도록 하였다. 응용제품을 개발할 때 주어진 기능 및 성능 그리고 저전력 등의 사양이 구현 가능한지 분석하고 절충할 때 사용할 수 있는 모델식을 개발하였고 이를 활용하여 직접 제작해 봄으로써 신뢰성을 입증하였다. 이 때, 하드웨어 부품들은 휴대폰 생산 시에 사용되는 부품들을 사용함으로써 저가의 부품을 안정적으로 수급하여 대량생산을 용이하게 하였다.