• Bulletin of the Korean Chemical Society
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• 제16권12호
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• pp.1193-1203
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• 1995

In this work, we focused on the setup of the tools for the analysis of the final rotational state distribution of photofragments in vibrational predissociations of triatomic van der Waals molecules A-B2. We found that reflection principle used for the direct photodissociation processes can also be applied to find out the final rotational state distributions for indirect photodissociation processes. The quantity which represents the strength of rovibrational coupling between the quasi-bound state and the final state is reflected into the mirror of the classical angular momentum function, instead of the initial state before light absorption used in the reflection principle of direct processes. The sign change in the first derivative of the interaction potential with respect to the bond distance of B2 is found to be the source of the binodal structures in the final rotational distributions of photofragments in the model system studied in this work. In MQDT analysis, short range eigenchannel basis functions were found to be localized in angle, in the previous work [Lee, C.W. Bull. Korean Chem. Soc. 1995, 16, 957.] and may be called angle functions. Angle functions enjoy simple geometrical structures which have simple functional relations with the final state distributions of photofragments. Two processes take place along the angle functions which resemble the quasi-bound state and dominate over other processes. Two such angle functions are found to be not only localized angularly but also localized either one of ends of B2 in motions along the bond of B2. These dominating photodissociation processes, however, cancel each other. This cancellation causes photodissociation to depend sensitively on the interaction potential at other angles than the dominant one. Part of potential surface where much larger torque exists can now play an important role in photodissociation. MQDT also enables us to see which processes play important roles after cancellation. This is done by examining the amounts of time delayed by asymptotic eigenchannels.

• 한국운동역학회지
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• 제31권4호
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• pp.283-289
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• 2021

Objective: The aim of this study was to analyze the pattern of Kolman technique by five Korean top gymnasts including the three national athletes on horizontal bar. Method: Two digital high-speed camcorders were used with 90 frames/sec and their Kolman motions were filmed in sports science secondary school gymnasium at U city. After the kinematic and kinetic variables were carried out by Kwon3D 3.1 motion package during the whole phase, the optimized release motion was investigated by simulating the body COG path during the aerial phase. Results: Firstly, it was revealed that the average changes of hip, shoulder joint angle were 84 deg, 53 deg respectively during the functional sub-phase and the average swing phaseal time was 1.21 s. Secondly, it was revealed that the average body COG positions and velocities (Y, Z) at release were -0.65 m, 0.48 m, 1.65 m/s, 3.97 m/s respectively and the average release angle, peak height and flight time were 67 deg, 1.29 m, 0.79 s respectively. Thirdly, it was revealed that the directions of somersault of whole and lower body, tilt of lower body were counterclockwise, whereas the directions of tilt of whole body, twist of whole and lower body were clockwise at the ready for re-grasp. Lastly, it was revealed that the body COG paths were different from each other during the aerial phase followed by the different body COG velocities. Conclusion: Korean gymnasts of this study controlled their motions well in terms of the timing of hip·shoulder joint, body position, body angular momentum especially during the functional sub-phase, but their motions were different during the aerial phase. Nonetheless most of them made the adequate body position at the instant of re-grasp. It would be suggested that Korean gymnasts except S3 should increase the vertical velocity.

• 한국운동역학회지
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• 제29권3호
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• pp.129-135
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• 2019

Objective: The purpose of this study is to present the scientific and quantitative data by finding the common points and differences of the side-kick according to the height change through the difference of the side kick motion performance according to the three target height changes and the function of the lower limbs muscle in side kick motion of Taekwondo Poomsae. Method: For this, total 14 players were selected who were registered in Korea Taekwondo Association and skilled group 7 players who had a medal from national competition and 7 players who did not have Taekwondo experience from department of physics. 4 video cameras to the feature on side kick per target height, and the subjects' support foot was located on the ground reactor and the practice was conducted 3 times: waist, chest, and head as the target height. the basic materials were collected by using Kwon 3D XP program and the T-test was conducted to verify the statistic difference between groups (SPSS 24.0). At this time, the statistics significance level was set as .05 and the following conclusion was obtained. Results: The lower the proficiency and the higher the height, the more the joint coordination between the hip and the knee. Conclusion: Summary of the result shows a common point that the change of target's height makes the lower the proficiency and the higher the height, the more the joint coordination between the hip and the knee. Also, the higher the target's height became, the greater angular momentum of thighs, shanks, foot became in common.

• 한국항공우주학회지
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• 제47권6호
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• pp.438-445
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• 2019

본 논문에서는 MEMS 자이로스코프에서 발생하는 G-민감도 오차를 관성센서 오차 모델에 정의하고, 이를 분석하여 오차 성분을 추출하는 기법을 제안한다. 일반적으로 MEMS기반 자이로스코프는 스프링과 관성질량체를 갖는 진동형 방식으로 개발된다. 따라서 구조적으로 고기동 환경에서 인가되는 가속도에 비례하는 G-민감도 오차 특성을 갖게 된다. 이러한 G-민감도 오차는 외부에서 높은 가속도가 인가되지 않는 민수분야에서는 무시할 정도로 작다. 하지만 전술급 성능의 MEMS 관성측정기가 고가속 환경에서 외란과 가속도에 의해 G-민감도 오차가 발생하게 되면 항체의 유도조종을 위한 항법장치 성능에 큰 영향을 미치게 되므로 오차 분석과 보상은 필수적이다. 따라서 본 논문에서는 MEMS 자이로스코프에 발생하는 G-민감도 오차를 분석하고 정의하여 관성센서 오차모델에 적용한다. 새로 정의된 관성센서 오차모델을 분석하여, 오차 성분을 고가속도 시험환경이 아닌 FMS 시험만으로 정확히 추출하는 방법을 제안한다. 그리고 제안한 방법으로 얻은 오차를 보상하여 고가속도 시험을 수행하고 그 결과를 분석하여 성능과 신뢰성을 검증한다.

• 대한조선학회논문집
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• 제59권3호
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• pp.183-191
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• 2022

A design method for a propeller type rim-driven axial-flow turbine for a micro-hydropower system is presented. The turbine consists of pre-stator, impeller and post-stator, where the pre-stator plays a role as a guide vane to provide circumferential velocity to the on-coming flow, and the impeller as a rotational power generator by absorbing angular momentum of the flow. BEM(Blade Element Method), which is based on the turbine Euler equation, is employed to design the pre-stator and impeller blades. NACA 66 thickness form and a=0.8 mean camber line, which is widely accepted as a marine propeller blade section, is used for the pre-stator and turbine blade section. A CFD method, derived from the discretization of the RANS equations, is applied for the analysis of the designed turbine system. The design conditions of the turbine is confirmed by the CFD calculation. Turbine characteristic curve is calculated by the CFD method, in order to provide the performance characteristics at off-design operation conditions. The proposed procedures for the design of a propeller type rim-driven axial-flow turbine are established and confirmed by the CFD analysis.

• 천문학회보
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• 제40권1호
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• pp.73.2-74
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• 2015

The gas cloud G2 falling toward Sagittarius A* (Sgr A*), the supermassive black hole at the center of the Milky Way, is supposed to provide valuable information on the physics of accretion flows and the environment of the black hole. We observed Sgr A* with four European stations of the Global Millimeter Very Long Baseline Interferometry Array (GMVA) at 86 GHz on 1 October 2013 when parts of G2 had already passed the pericenter. We searched for possible transient asymmetric structure - such as jets or winds from hot accretion flows - around Sgr A* caused by accretion of material from G2. The interferometric closure phases (which are zero if the spatial brightness distribution of the target is symmetric, and deviate from zero otherwise) remained zero within errors during the observation time. We thus conclude that Sgr A* did not show significant asymmetric (in the observer frame) outflows in late 2013. Using simulations, we constrain the size of the outflows that we could have missed to ${\approx}2.5$ mas along the major axis, ${\approx}0.4$ mas along the minor axis of the beam, corresponding to approximately 232 and 35 Schwarzschild radii, respectively; we thus probe spatial scales on which the jets of radio galaxies are suspected to convert magnetic into kinetic energy. As probably less than 0.2 Jy of the flux from Sgr A* can be attributed to accretion from G2, one finds an effective accretion rate ${\eta}M{\leq}1.5{\times}10^9kg/s{\approx}7.7{\times}10^{-9}M_{earth}/yr$ for material from G2. Exploiting the kinetic jet power-accretion power relation of radio galaxies, one finds that the rate of accretion of matter that ends up in jets is limited to $M{\leq}10^{17}kg/s{\approx}0.5M_{Earth}/yr$ less than about 20% of the mass of G2. Accordingly, G2 appears to be largely stable against loss of angular momentum and subsequent (partial) accretion at least on time scales ${\leq}1$ year.

• 한국지구과학회지
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• 제25권6호
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• pp.402-408
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• 2004

이 연구의 목적은 중${\cdot}$고등학교 지구과학 전공 교들이 몇 가지 지구과학 개념에 대하여 가지고 있는 이해유형을 조사하는 것이다. 이 연구의 대상으로 선택한 개념은 저기압에서의 바람, 해류의 서안강화, 편서풍 파동, 온실효과, 오존층 그리고 대기압이며 중${\cdot}$고등학교 지구과학 전공교사 26명이다. 조사의 결과는 중${\cdot}$고등학교에서 교사들이 이들 개념을 학습지도할 때 필요하다고 생각되는 학습의 객관적 자료의 측면에서 분석하였고 그 결과는 다음과 같다. 지구과학 전공교사들도 이 연구에서 선정된 몇 가지 개념에 대하여 학생의 학습지도에 부족한 여러 가지 이해유형을 가지고 있으며 이들 유형 중에는 오개념들도 포함하고 있음을 알았다. 교사들은 저기압에서의 바람에 대하여 경도풍과 관련된 이해유형을, 서안강화에 대해서는 지구자전과 관련된 오개념을, 편서풍 파동에 대해서는 각운동량 보존과 관련된 오개념을, 온실효과에 대해서는 주된 온실기체와 관련된 오개념을, 오존층에 대해서는 지표부근의 오존기체 생성과 관련된 오개넘을, 그리고 대기압에 대해서는 대기압으로 인해 생기는 현상과 관련된 오개념을 가지고 있음을 발견하였다. 이 연구에서 발견된 교사의 여러 가지 이해유형은 지구과학개념의 힉습지도에서 유용하게 이용될 수 있을 것으로 생각한다.

• 한국지구과학회지
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• 제33권2호
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• pp.170-182
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• 2012

본 연구의 목적은 행성운동 법칙에 관한 케플러의 귀추적 사고를 도입한 학습자료를 개발하고 이를 고등학교 수업에 적용하여 학생들의 귀추적 추론을 밝히고자 하는 것이다. 이를 위하여 태양의 자기장, 피겨 스케이터의 각운동량 보존, 케플러의 정다면체 이론을 포함한 제시문과 과제문항을 개발하였다. 본 연구의 대상은 과학고등학교 학생 79명과 일반계 고등학교 학생 83명이었고 과제문항에 대한 응답을 비교 분석하여 학생들의 추론 전략 유형과 특성을 논의하였다. 본 연구의 결과, 학생들은 태양의 자기장에 대한 케플러의 생각을 근거로 화성의 운동에 대하여 불완전 유비귀추, 유비귀추, 자료의 재구성 전략을 사용하여 추론하였다. 케플러 제2법칙에 대한 귀추적 추론에서는 불완전 유비귀추, 유비귀추, 모델 구성 및 조작 귀추 등이 나타났다. 이와 관련하여 피겨 스케이터 유비 자체가 학습자들에게 대안개념을 유발할 수 있으므로 실제 수업에서 좀 더 구체적인 설명이 요구됨을 알 수 있었다. 또한 케플러 제3법칙에 대해서는 특히 정다면체 개념과 기존의 알고 있는 지식을 통합하는 개념적 결합 전략을 사용하여 추론한 경우도 나타났다. 적절한 유비귀추를 보여준 과학고 학생의 비율이 일반고 학생보다 여러 과제에서 더 높게 나타난 반면 일반고 학생은 과학고 학생에 비하여 불완전 유비귀추를 더 많이 보여주었다. 본 연구는 케플러의 귀추적 사고를 모델링하여 가설을 형성하는 과정에서 발휘되는 귀추전략을 밝힘으로써 이와 관련한 수업에서 구체적인 방안을 찾는데 근거 자료가 될 것이다.

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

• Nuclear Engineering and Technology
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• 제52권4호
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• pp.721-733
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• 2020

In nuclear engineering, the occurrence of critical heat flux (CHF) is complicated for rod bundle, and it is much more difficult to predict the CHF when it is in natural circulation under motion condition. In this paper, the dryout-type CHF is investigated for the rod bundle in a natural circulation loop under rolling motion condition based on the coupled analysis of subchannel method, a one-dimensional system analysis method and a CHF mechanism model, namely the three-fluid model for annular flow. In order to consider the rolling effect of the natural circulation loop, the subchannel model is connected to the one-dimensional system code at the inlet and outlet of the rod bundle. The subchannel analysis provides the local thermal hydraulic parameters as input for the CHF mechanism model to calculate the occurrence of CHF. The rolling motion is modeled by additional motion forces in the momentum equation. First, the calculation methods of the natural circulation and CHF are validated by a published natural circulation experiment data and a CHF empirical correlation, respectively. Then, the CHF of the rod bundle in a natural circulation loop under both the stationary and rolling motion condition is predicted and analyzed. According to the calculation results, CHF under stationary condition is smaller than that under rolling motion condition. Besides, the CHF decreases with the increase of the rolling period and angular acceleration amplitude within the range of inlet subcooling and mass flux adopted in the current research. This paper can provide useful information for the prediction of CHF in natural circulation under motion condition, which is important for the nuclear reactor design improvement and safety analysis.