• 정보보호학회논문지
• /
• 제10권4호
• /
• pp.3-11
• /
• 2000

본 논문에서는 몽고메리 알고리즘을 사용하여 모듈러 곱셈을 빠르게 수행하는 선형 시스톨릭 어레이를 설계하고, 이 곱셈기와 LR 이진 제곱 곱셈 알고리즘을 사용하여 n 비트 메시지 블록에 대해 모듈러 지수 연산을 수행하는 지수 연산 프로세서를 설계한다 이 프로세서는 제어장치, 입출력 시프트 레지스터, 지수 연산 장치 등 3개의 영역으로 나 누어진다. 설계된 지수 연산 프로세서의 동작을 검증하기 위해 VHDL를 사용하여 모델링하고 MAX+PLUS II를 사용하여 시뮬레이션 한다. 메시지 블록의 길이 n=512일 때 설계된 지수 연산 프로세서의 지연 시간은 59.5ms이다. 설계된 모듈러 지수 연산 프로세서는 RSA 칩(chip)에 이용될 수 있을 것이다.

• Current Photovoltaic Research
• /
• 제9권4호
• /
• pp.137-144
• /
• 2021

In this study, the microstructure of the CVD-fabricated Cu(In,Ga)Se₂ (CIGSe) absorber layer by simulating the stacking sequence used in a co-evaporation method, and changes solar cell performance were investigated. The absorber layer prepared by stacking CuSe and (In,Ga)Se between InSe is separated into Ga-free CuInSe₂ and Ga-rich CIGSe, and transformed to CIGSe by selenization heat treatment with slight improvement in the the solar cell efficiency. However, in CVD, since the supply of liquid Cu-Se is not as active as in the co-evaporation method, the nanoocrystalline layer containing a large amount of Ga remained independently in the absorption layer, which acted as a cause of the loss of J_SC and FF. Therefore, by using a precursor structure in which CuGa is sputter-deposited on a single layer of InSe deposited by CVD, performance parameters of V_OC, J_SC, and FF could be greatly improved.

• 융합신호처리학회논문지
• /
• 제11권1호
• /
• pp.47-52
• /
• 2010

암호화 시스템에서 대부분의 선형시스템은 쉽게 해석될 수 있기 때문에 비선형성은 매우 중요하다. 비선형 함수인 bent함수와 유사한 특성을 갖고 C.Bracken, Z.Zha 등에 의하여 제안된 APN(Almost Perfect Nonlinear) 함수를 이용하여 두 종류의 새로운 부호계열 발생 알고리즘을 제안하였다. 이를 이용하여 GF(2)상에서 발생된 부호계열의 자기상관함수 $R_{ii}(\tau)$, ${\tau}\;{\neq}\;0$와 상호상관함수 $R_{ik}(\tau)$의 값은 {-1, $-1-2^{n/2}$, $-1+2^{n/2}$}을 가진다. 이 개념을 확장한 GF(p), $p\;{\geq}\;3$상에서 발생된 비 이원부호계열의 자기상관함수 $R_{p,ii}(\tau}$, ${\tau}\;{\neq}\;0$와 상호상관함수 $R_{p,ik}(\tau)$의 값은 {$-1+p^{n-1}$, $-1-p^{(n-1)/2}+p^{n-1}$, $-1+p^{(n-1)/2}+p^{n-1}$} 로 역시 3종류 값을 가짐을 보였다. 이 분석결과로부터 발생된 부호계열의 상관함수가 Gold 부호계열과 유사한 특성을 가짐을 확인하였다.

• Journal of Electrical Engineering and Technology
• /
• 제13권6호
• /
• pp.2545-2552
• /
• 2018

$SF_6$ has been widely used in high voltage power equipment, such as gas insulated switchgear (GIS) and gas insulated transmission line (GIL), because of its excellent insulation and arc extinguishing performance. However, $SF_6$ faces two environmental problems: greenhouse effect and high liquefaction temperature. Therefore, to find the $SF_6$ substitute gases has become a research hotspot in recent years. In this paper, the liquefaction characteristics of $SF_6$ substitute gases were studied. Peng-Robinson equation of state with the van der Waals mixing rule (PR-vdW model) was used to calculate the dew point temperature of the binary gas mixtures, with $SF_6$, $C_3F_8$, $c-C_4F_8$, $CF_3I$ or $C_4F_7N$ as the insulating gas and $N_2$ or $CO_2$ as the buffer gas. The sequence of the dew point temperatures of the binary gas mixtures under the same pressure and composition ratio was obtained. $SF_6/N_2$ < $SF_6/CO_2$ < $C_3F_8/N_2$ < $C_3F_8/CO_2$ < $CF_3I/N_2$ < $CF_3I/CO_2$ < $c-C_4F_8/N_2$ < $C_4F_7N/N_2$ < $c-C_4F_8/CO_2$ < $C_4F_7N/CO_2$. $SF_6/N_2$ gas mixture showed the best temperature adaptability and $C_4F_7N/CO_2$ gas mixture showed the worst temperature adaptability. Furthermore, the dew point temperatures of the $SF_6$ substitute gases at different pressures and the upper limits of the insulating gas mole fraction at $-30^{\circ}C$, $-20^{\circ}C$ and $-10^{\circ}C$ were obtained. The results would supply sufficient data support for GIS/GIL operators and researchers.

• Journal of Astronomy and Space Sciences
• /
• 제28권3호
• /
• pp.163-172
• /
• 2011

An intensive analysis of 185 timings of WZ Cep, including our new three timings, was made to understand the dynamical picture of this active W UMa-type binary. It was found that the orbital period of the system has complexly varied in two cyclical components superposed on a secularly downward parabola over about 80y. The downward parabola, corresponding to a secular period decrease of $-9.{^d}97{\times}10^{-8}y^{-1}$, is most probably produced by the action of both angular momentum loss (AML) due to magnetic braking and mass-transfer from the massive primary component to the secondary. The period decrease rate of $-6.^{d}72{\times}10^{-8}y^{-1}$ due to AML contributes about 67% to the observed period decrease. The mass flow of about $5.16{\times}10^{-8}M_{\odot}y^{-1}$ from the primary to the secondary results the remaining 33% period decrease. Two cyclical components have an $11.^{y}8$ period with amplitude of $0.^{d}0054$ and a $41.^{y}3$ period with amplitude of $0.^{d}0178$. It is very interesting that there seems to be exactly in a commensurable 7:2 relation between their mean motions. As the possible causes, two rival interpretations (i.e., light-time effects (LTE) by additional bodies and the Applegate model) were considered. In the LTE interpretation, the minimum masses of $0.30M_{\odot}$ for the shorter period and $0.49M_{\odot}$ for the longer one were calculated. Their contributions to the total light were at most within 2%, if they were assumed to be main-sequence stars. If the LTE explanation is true for the WZ Cep system, the 7:2 relation found between their mean motions would be interpreted as a stable 7:2 orbit resonance produced by a long-term gravitational interaction between two tertiary bodies. In the Applegate model interpretation, the deduced model parameters indicate that the mechanism could work only in the primary star for both of the two period modulations, but could not in the secondary. However, we couldn't find any meaningful relation between the light variation and the period variability from the historical light curve data. At present, we prefer the interpretation of the mechanical perturbation from the third and fourth stars as the possible cause of two cycling period changes.

• 천문학회지
• /
• 제49권5호
• /
• pp.209-223
• /
• 2016

We present analyses of ~1250 variable sources identified in a 20 square degree field toward NGC 2784 by the KMTNet Supernova Program. We categorize the variable sources into three groups based on their B-band variability. The first group consists of 31 high variability sources with their B-band RMS variability greater than 0.3 magnitudes. The second group of medium variability contains 265 sources with RMS variability between 0.05 and 0.3 magnitudes. The remaining 951 sources belong to the third group of low variability with an RMS variability smaller than 0.05 magnitudes. Of the entire ~1250 sources, 4 clearly show periods of variability greater than 100 days, while the rest have periods shorter than ~51 days or no reliable periods. The majority of the sources show either rather irregular variability or short periods faster than 2 days. Most of the sources with reliable period determination between 2 and 51 days belong to the low-variability group, although a few belong to the medium-variability group. All the variable sources with periods longer than 35 days appear to be very red with B - V > 1.5 and V - I > 2.1 magnitudes. We classify candidates of 51 Cepheids, 17 semi-regular variables, 3 Mira types, 2 RV(B) Tauri stars, 26 eclipsing binary systems and 1 active galactic nucleus. The majority of long-term variables in our sample belong to either Mira or semi-regular types, indicating that long-term variability may be more prominent in post-main sequence phases of late-type stars. The depth of the eclipsing dips of the 26 candidates for eclipsing binaries is equivalent to ~0.61 as the average relative size of the two stars in the binary system. Our results illustrate the power of the KMTNet Supernova Program for future studies of variable objects.

• 천문학회지
• /
• 제49권5호
• /
• pp.199-208
• /
• 2016

We present photometric results of the δ Sct star V1162 Ori, which is extensively monitored for a total of 49 nights from mid-December 2014 to early-March 2015. The observations are made with three KMTNet (Korea Microlensing Telescope Network) 1.6 m telescopes installed in Chile, South Africa, and Australia. Multiple frequency analysis is applied to the data and resulted in clear detection of seven frequencies without an alias problem: five known frequencies and two new ones with small amplitudes of 1.2-1.7 mmag. The amplitudes of all but one frequency are significantly different from previous results, confirming the existence of long-term amplitude changes. We examine the variations in pulsation timings of V1162 Ori for about 30 years by using the times of maximum light obtained from our data and collected from the literatures. The O − C (Observed minus Calculated) timing diagram shows a combination of a downward parabolic variation with a period decreasing rate of (1/P)dP/dt = −4.22 × 10⁻⁶ year⁻¹ and a cyclic change with a period of about 2780 days. The most probable explanation for this cyclic variation is the light-travel-time effect caused by an unknown binary companion, which has a minimum mass of 0.69 M_⊙. V1162 Ori is the first δ Sct-type pulsating star of which the observed fast period decrease can be interpreted as an evolutionary effect of a pre-main sequence star, considering its membership of the Orion OB 1c association.

• Molecules and Cells
• /
• 제37권10호
• /
• pp.719-726
• /
• 2014

The ${\gamma}$-Aminobutyric acid (GABA) that is found in prokaryotic and eukaryotic organisms has been used in various ways as a signaling molecule or a significant component generating metabolic energy under conditions of nutrient limitation or stress, through GABA catabolism. Succinic semialdehyde dehydrogenase (SSADH) catalyzes the oxidation of succinic semialdehyde to succinic acid in the final step of GABA catabolism. Here, we report the catalytic properties and two crystal structures of SSADH from Streptococcus pyogenes (SpSSADH) regarding its cofactor preference. Kinetic analysis showed that SpSSADH prefers $NADP^+$ over $NAD^+$ as a hydride acceptor. Moreover, the structures of SpSSADH were determined in an apo-form and in a binary complex with $NADP^+$ at $1.6{\AA}$ and $2.1{\AA}$ resolutions, respectively. Both structures of SpSSADH showed dimeric conformation, containing a single cysteine residue in the catalytic loop of each subunit. Further structural analysis and sequence comparison of SpSSADH with other SSADHs revealed that Ser158 and Tyr188 in SpSSADH participate in the stabilization of the 2'-phosphate group of adenine-side ribose in $NADP^+$. Our results provide structural insights into the cofactor preference of SpSSADH as the gram-positive bacterial SSADH.

• 한국멀티미디어학회논문지
• /
• 제12권7호
• /
• pp.929-940
• /
• 2009

본 논문에서는 컨투어렛 변환 영역 상에서 저작권 보호, 인증 및 변형 검출 등을 위한 다중 목적의 워터마킹 기법을 제안한다. 컨투어렛 변환은 웨이블릿 변환보다 다방향성의 에지 및 부드러운 윤곽선 검출 성능이 보다 우수하여 제안한 방법에서는 4레벨 라플라시안 피라미드와 2 레벨 방향성 필터 뱅크를 이용한 컨투어렛 변환 영역 상에서 워터마크를 삽입한다. 먼저 제안한 방법의 첫 번째 단계에서는 저작권 보호를 위한 강인성 워터마킹 기법으로 워터마크 비트에 따라 원 패턴의 시퀀스를 생성하여, 이들 시퀀스 형태로 방향성 고주파 대역의 평균 계수 대역 내에 투영한다. 그리고 투영된 계수들의 분산 분포에 워터마크 비트를 각각 삽입한다. 그리고 두 번째 단계에서는 인증 및 변형 검출을 위한 준연약성 워터마킹 기법으로써, 최상위 레벨의 저주파 대역 내에 이진 워터마크 영상을 적응적 양자화기에 의하여 삽입한다. Checkmark 2.1를 이용한 평가 실험에서 제안한 방법이 기존의 방법에 비하여 강인성 및 비가시성이 보다 우수함을 확인하였다.

• 대한전자공학회논문지SP
• /
• 제38권5호
• /
• pp.509-517
• /
• 2001

전역탐색알고리즘(full-search algorithm, FSA)은 탐색영역의 범위가 커짐에 따라 방대한 양의 계산을 필요로 하기 때문에 이에 따른 알고리듬의 처리시간이 커지고, 하드웨어로 구현했을 때 회로가 복잡해진다는 문제점을 안고 있다. 본 논문에서는 이러한 문제점을 개선하기 위한 방안으로 비트플레인 정합에 의한 움직임 추정기의 VLSI 구조를 제안한다. 제안된 움직임 추정기에서는 비트 플레인 정합기준을 이용하여 기존의 전역 탐색 알고리즘을 하나의 이진영상으로 적용함으로써 움직임 추정에 소요되는 연산의 양을 크게 줄이면 서도 전역탐색 알고리듬과 유사한 움직임 추정 성능을 갖도록 하였으며, 제안된 VLSI 구조에서는 두 개의 프로세싱 코어를 채택하여 데이터 흐름을 시스톨릭 (systolic) 어레이의 형태로 제어하여, 시스템 내부의 SRAM을 제거하여 동작 속도 상의 이득뿐만 아니라, 메모리 공정을 필요로 하지 않는 저가의 공정을 사용 가능하게 함으로써 제작상의 비용을 절감할 수 있는 해결책을 제시하였다. 구현된 하드웨어는 VHDL을 이용하여 설계하고, 기능 검증을 수행한 후 0.6-μm three-metal CMOS 공정을 이용하여 8.15 X 10.84㎟의 크기로 집적하였다.