본 연구는 달의 일주 운동에서 관찰되는 월면 무늬의 겉보기 회전 운동에 관해서 정량적으로 기술하고 관측 결과를 제시하여 지구과학 교과 관점에서 지구 자전 현상과의 연관성을 고찰하였다. 이러한 연구를 통하여 달의 일주 운동 관측이 지구과학 교과 영역에서 수행할 수 있는 탐구활동 소재 중의 하나로 구성될 수 있다는 것을 제시하고자 한다. 월면 무늬 회전은 지표면에 서 있는 관측자가 일주 운동하고 있는 달을 보고 있을 때 달 표면에 있는 어두운 무늬들이 지평선에 대해서 회전하고 있는 것처럼 보이는 현상이다. 이 현상은 육안으로도 쉽게 관측되므로 지구과학 탐구 요소로서 의문을 품어볼 만한 자연현상임에도 불구하고 이 현상을 지구 자전과 관련된 내용으로 소개하고 있는 지구과학 전공 영역 서적을 찾아보기가 쉽지 않다. 따라서 본 연구에서는 월면 회전 현상의 이론적인 원리를 수학적으로 상세히 유도하고, 실제관측을 통하여 이 현상이 지구과학 교과 영역의 탐구 소재로서 개발될 수 있는 가능성을 제시하였다. 또한 월면의 역회전 현상을 제시하고, 이를 수학적으로 증명하였으며 정성적인 이해가 가능하도록 설명 방법을 고안하여 소개하였다.

The purpose of this study was to identify the effect of the hip internal rotation on gluteal and erector spinae muscle electromyographic (EMG) activity during treadmill walking. Eleven healthy subjects were recruited. All subjects performed treadmill walking while maintaining the hip in neutral position (condition 1) and in internal rotation (condition 2). Surface EMG activity was recorded from four muscles (gluteus maximus (GM), gluteus medius (GMED), tensor fascia latae (TFL), and erector spinae (ES)) and the hip internal rotation angle was measured using a three dimensional motion analysis system. The gait cycle was determined with two foot switches, and stance phase was normalized as 100% stance phase (SP) for each condition using the MatLab 7.0 program. The normalized EMG activities according to the hip rotation (neutral or internal rotation) were compared using a paired t-test. During the entire SP of treadmill walking, the EMG activities of GM in condition 1 were significantly greater than in condition 2 (p<.05). The EMG activities of TFL and ES in condition 2 were significantly greater than in condition 1 (p<.05). The EMG activities of the GMED in condition 1 were significantly greater than in condition 1 (p>.05) except for 80~100% SP. Further studies need randomized control trials regarding the effect of hip internal rotation on the hip and lumbar spine muscle activity. Kinetic variables during gait or going up and down stairs are also needed.

이 논문에서는 단면성질을 나타내는 모멘트-곡률 관계에 토대를 둔 해석모델을 제안하였다. 기존의 제안된 해석방법에서는 모멘트-곡률 관계가 완전부착을 가정한 휨거동만을 주요한 거동으로 가정하여 구조물의 응답을 과소평가하고 강성을 과대평가한 것과는 달리 제안된 해석 방법에서는 접합부의 부착슬립에 의한 강체변형을 산정할 수 있는 알고리즘을 개발하였고 나아가 등가휨강성을 이용하여 부착슬립에 의한 강체변형을 고려한 철근콘크리트 구조물의 해석을 수행하였다. 또한 모멘트-곡률 관계를 철근의 항복점을 기준으로 두개의 직선으로 간편화 시킴으로써 해석의 효율성을 높이는 한편 고려해야 할 비선형 거동특성을 효과적으로 반영하였다. 마지막으로 철근콘크리트 구조물의 비선형 해석에 대한 제안된 모델식의 적용성을 검증하기 위하여 해석결과와 실험값들의 비교를 수행하였다.

Magnetic fields are an important ingredient of galaxy clusters and are indirectly observed on cluster scales as radio haloes and radio relics. One promising method to shed light on the properties of cluster wide magnetic fields is the analysis of Faraday rotation maps of extended extragalactic radio sources. We developed a Fourier analysis for such Faraday rotation maps in order to determine the magnetic power spectra of cluster fields. In an advanced step, here we apply a Bayesian maximum likelihood method to the RM map of the north lobe of Hydra A on the basis of our Fourier analysis and derive the power spectrum of the cluster magnetic field. For Hydra A, we measure a spectral index of -5/3 over at least one order of magnitude implying Kolmogorov type turbulence. We find a dominant scale of about 3 kpc on which the magnetic power is concentrated, since the magnetic autocorrelation length is ⋋B = 3 ± 0.5 kpc. Furthermore, we investigate the influences of the assumption about the sampling volume (described by a window function) on the magnetic power spectrum. The central magnetic field strength was determined to be ~ 7 ± 2μG for the most likely geometries.

The energy injection of galactic black holes (BH) into the intergalactic medium via extragalactic radio source jets and lobes is sufficient to magnetize the IGM in the filaments and walls of Large Scale Structure at < [B] > ~ 0.lμG or more. It appears that this process of galaxy-IGM feedback is the primary source of IGM cosmic rays(CR) and magnetic field energy. Large scale gravitational infall energy serves to re-heat the intergalactic magnetoplasma in localities of space and time, maintaining or amplifying the IGM magnetic field, but this can be thought of as a secondary process. I briefly review observations that confirm IGM fields around this level, describe further Faraday rotation measurements in progress, and also the observational evidence that magnetic fields in galaxy systems around z=2 were approximately as strong then, ~ 10 Gyr ago, as now.

The presence of magnetic fields in the intracluster medium in clusters of galaxies has been revealed through several different observational techniques. These fields may be dynamically important in clusters as they will provide additional pressure support to the intracluster medium as well as inhibit transport mechanisms such as thermal conduction. Here, we review the current observational state of Faraday rotation measure studies of the cluster fields. The fields are generally found to be a few to 10 $\mu$ 수식 이미지G in non-cooling core clusters and ordered on scales of 10 - 20 kpc. Studies of sources at large impact parameters show that the magnetic fields extend from cluster cores to radii of at least 500 kpc. In central regions of cooling core systems the field strengths are often somewhat higher (10 - 40 μG) and appear to be ordered on smaller scales of a few to 10 kpc. We also review some of the recent work on interpreting Faraday rotation measure observations through theory and numerical simulations. These techniques allow us to build up a much more detailed view of the strength and topology of the fields.

A frame element embedded normal to a shear wall or slab (shell element) is common in the structural systems. In that case there is a need for a membrane or shell element to have a normal rotation degree of freedom at each node in order to have a good result of stresses. Even if Many other people studied this area, All man, Cook and Sabir are representative investigators in this area. In this research paper, Sabir's methods of vertex rotation stiffness matrix in a membrane element are studied. New stiffness of vertex rotation are proposed by taking advantage of beam stiffness theory. Rectangular elements stiffness with rotational degree of freedom are compared in accuracy ratio each other.

본 연구는 파종기가 다른 추파호밀의 Feekes scale에 의한 생장발달을 분석하기 위하여 수행하였다. 시험배치는 10처리 3반복의 분할구배치로 주구에는 9월 30일과 10월 15일의 파종시기를, 세구로는 'Kodiak', 'Koolgrager', 'Danko', 'Homil22', 'Olhomil' 품종을 두었다. 초장은 조기파종이 만기파종보다 높았으며, 공시품종간에는 조생품종이 가장 높았다. 분얼경수는 조기파종시에 48.0개로 만기파종시의 24.3

본 연구의 목적은 지구의 운동에 대한 흥미와 학습양식이 서로 다른 고등학교 1학년 학생들을 대상으로 지구의 자전과 관련된 개념을 알아보는데 있다. 학생들의 지구의 자전에 대한 흥미와 시각-언어 학습 양식을 알아보기 위해, 흥미가 많고 시각-언어의 학습 양식을 모두 지닌 학생 1명, 흥미가 많고 시각적인 학습 양식을 지닌 학생 1명, 흥미가 적고 시각적 학습 양식을 지닌 학생 1명, 흥미가 적고 언어적 학습 양식을 지닌 학생 1명 등 4명을 연구 대상자로 선정하였다. 학생의 개념을 다방면으로 이끌기 위하여 말 이외에 몸 동작과 그림 등을 그리게 하였으며, 자료 분석은 면담 기록지를 통해 개인별로 분석하였다. 연구 결과 흥미가 많은 학생이 흥미가 적은 학생보다 지구의 자전에 관한 질문에 반응과 내용의 이해도가 높았으며 답변에 대한 이유를 논리적으로 설명하였다. 또한 흥미의 유무와는 달리 개인이 지닌 학습 양식에 따른 개념 형성 차이는 크게 나타나지 않았다. 학생들이 지닌 가장 대표적이 오개념 유형으로 태양의 이동 경로를 나타낼 때 오른쪽을 동쪽으로 생각하여 태양이 오른쪽에서 왼쪽으로 이동하며, 북쪽 하늘에서 별들은 시계 방향으로 이동한다는 것이다.

The accuracy of rotation of spindle unit could be defined as the stability of its spindle axis while rotating. The rotation in the rolling bearings causes the disturbing influence, which leads to the oscillation of a rotation axis. The main source of oscillation is the interaction between rolling bodies and rings’ races. The first oscillation source investigated was the out-of-shape imperfection of inner bearing ring. It was shown that it is possible to considerably decrease the radial runout of spindle if we can orient the inner rings in such a manner that oscillations caused by them would mutually compensate each other. Also the outer ring harmonics were explored as the second oscillation source. It was found that it is possible to reduce the runout by making the oscillation antiphased by mutually adjusting position of bearings on assembly stage.

회전(turning)은 보행 중 방향을 바꾸는 운동 기술(motor skill)이고, 회전 전략(turning strategy)은 회전을 완수하는데 사용되는 일반적 행동 전형(generalized movement pattern)이다. 회전에 대한 보행속도의 영향은 분명하지 않다. 이 연구의 목적은 보행속도의 돌기 전략에 대한 영향을 분석하고 보행속도의 하지 내외 회전(internal and external rotation)에 대한 영향을 분석하는 것이다

Curing reaction was carried out with the acrylic resin (ACR) [n-butyl acrylate/atyrene/2-hydroxyethyl methacrylate/acetoacetoxyethyl methacrylate (AAEM)] synthesized before and a curing agent, hexamethoxymethylmelamine (HMMM). With rotational rheometer, the effect of catalysts on curing rate of acrylic resin/melamine was examined. Among the four catalysts used, p-toluene sulfonic acid showed the highest reactivity, and the optimum amount of catalyst was 0.5 phr. It was observed that in the ACR/HMMM curing reaction, gelation point was lowered with the increasing the amount of AAEM and HMMM in the ACR.

We investigate the effects of planetary rotation on the exospheres of the earth and Mars with simple collisionless models. We develope a numerical code that computes exospheric densities by integrating velocity functions at the exobase with a 10 point Gauss method. It is assumed in the model that atoms above the exobase altitude move collisionlessly on an orbit under the planet's gravity. Temperatures and densities at the exobase over the globe are adopted from MSIS-86 for the earth and from Bougher et al's MTGCM for Mars. For both the earth and Mars, the rotation affects the exospheric density distribution significantly in two ways: (1) the variation of the exospheric density distribution is shifted toward the rotational direction with respect to the variation at the exobase, (2) the exospheric densities in general increase over the non-rotating case. We find that the rotational effects are more significant for lower thermospheric temperatures. Both the enhancement of densities and shift of the exospheric distribution due to rotation have not been considered in previous models of Martian exosphere. Our non-spherical distribution with the rotational effects should contribute to refining the hot oxygen corona models of Mars which so far assume simple geometry. Our model will also help in analyzing exospheric data to be measured by the upcoming Nozomi mission to Mars.

회전축계가 거동시 지진하중을 받을때의 응답 거동을 조사하였다. 지진과 기동으로 인하여 회전축계가 불안정하다면, 과다한 진동이 발생할 뿐만 이니라 회정지계의 회전자가 고정자와 부딪혀 기계 성능을 발휘하지 못하게 할 것이다. 그래서 면진장치를 갖춘 기초에 지진동이 작용할 때에, 회전축계의 응답을 모사하였다. 거동시 회전축계의 과도 응답을 얻기 위하여 우선 회전축계의 운동방정식을 유도 하였다. 유도한 운동방정식은 비선형이어서 Runge-Kutta 수치해석법을 이용하여 응답을 계산하였으며, 기동 운전모드에 따른 거동뿐만 아니라 면진스프링의 강성을 매개변수로 취하여 회전축계의 응답거동을 고찰하였다.

The purpose of this investigation was to examine the influence of head and neck(HN) position in the transverse plane on the static production of elbow extension force in the involved(paretic) upper extremity of patients with hemiparesis. On this study, thirty patients who had experienced a cerebrovascular accident were matched with neurologically intact subjects. Force of static elbow extension was tested with a hand-held dynamometer, twice with the HN rotated toward the paretic side and twice with the HN rotated toward the non-paretic side. Elbow extension force differed significantly with the HN in the two position in patients with hemiparesis but not in normal persons(=0.05). Results of this study support the conclusion that HN position in the transverse plane influences the production of static elbow extension force on the paretic side in patients with hemiparesis.