• 대한기계학회논문집
• /
• 제18권1호
• /
• pp.101-112
• /
• 1994

The measurement of residual stress distribution of $Si_3N_4/SUS304$ joint was performed on 23 specimens with the same joint condition using PSPC type X-ray stress measurement system and the two-dimensional elastoplastic analysis using finite element method was also attempted. As results, residual stress distribution near the interface on the ceramic side of the joint was revealed quantitatively. Residual stress on the ceramic side of the joint was turned out to be tensional near the interface, maximum along the edge, varying in accordance with the condition of the joint and variance to be most conspicuous for the residual stress normal to the interface characterized by the stress singularities. In the vicinity of the interface, the high stress concentration occurs and residual stress distributes three-dimensionally. Therefore, the measured stress distribution differed remarkably from the result of the two-dimensional finite-element analysis. Especially at the center of the specimen near the interface, the residual stress, $\sigma_{x}$ obtained from the finite element analysis was compressive, whereas measurement using X-ray yielded tensile $\sigma_{x}$. Here we discuss two dimensional superposition model the discrepancy between the results from the two dimensional finite element analysis and X-ray measurement.

• 디지털콘텐츠학회 논문지
• /
• 제8권4호
• /
• pp.459-465
• /
• 2007

본 논문에서는 다중 벽면 구조의 실내 환경에서 전파의 전달특성을 모델링하기 위해 ray-launching 기반의 광선추적법을 이용한 2차원 ray-tracing 시뮬레이터를 구현하였고, 이를 통해 ray의 전파 경로를 분석하고 평가하였다. 실험 결과, 구현된 광선추적법의 경로 패턴 및 시간지연 분포는 동일한 무선 환경에서 수행된 이전의 실험 결과와 비슷한 결과가 나타남을 확인하였으며, 송수신 거리 및 방사각에 따른 수신반경의 조정이 타당함을 확인하였다. 특히 비가시거리 송수신 환경에서 다중 벽면을 투과한 ray가 반사와 투과를 형성하여 수신기에 도달할 때까지의 ray의 impulse response는 기존 연구의 실험 결과와 대부분 일치하였으며, 송신기에서 발사되는 ray의 방사각을 $1^{\circ}$에서 $7^{\circ}$까지 달리하여 실험한 경우 도출된 channel profile이 서로 유사함을 확인하였다.

• 대한방사선기술학회지:방사선기술과학
• /
• 제20권2호
• /
• pp.34-43
• /
• 1997

There are 4 types of equipment in diagnostic radiography. These are single phase, three phase, inverter type and condenser type X-ray generators. It is very confusing to make an adequate exposure factor and to know the usage of different type of X-ray generators. In this experiment, I explored a comparative study of outputs in 4 different type of X-ray units. I expect that this experiment could be helpful for manufacturer to make both the X-ray equipment better, In terms of Ideal exposure factors, thereby reducing the patient dose. Experimental results are as follow : 1) X-ray output The ratio of X-ray output of single, three phase and inverter type of X-ray generator was 1 : 1.6 : 2 without absorber and 1 : 2 : 2.6 with 20 mm aluminium absorber. 2) Beam quality The X-ray beam quality of single phase generator was proved to be softer than three phase and inverter type of generators by 0.4 mmAL and 0.55 mmAl HVL respectively. 3) Reproducibility Linearity of X-ray output Retroducibility of X-ray output met the regulation below CV 0.05 and linearity also met the regulation below 0.1 in 4 types of diagnostic X-ray generators. 4) The comparison of incident dose Three phase X-ray generator was 20% higher than two other X-ray generators in radiation dose to make same film density.

• 대한토목학회논문집
• /
• 제28권2D호
• /
• pp.277-285
• /
• 2008

엑스선 영상은 의료분야에서 많이 활용되고 있으며 특히 인간의 골격형성 과정에서 발생할 수 있는 척추만곡의 변형을 파악하는 데 아주 효율적이다. 본 연구에서는 엑스선 영상의 사진기 검정과 엑스선 영상을 이용한 대상물의 3차원 좌표 결정에 중점을 두었다. 엑스선 사진기를 이용한 대상물의 좌표결정 과정은 엑스선 사진기 검정을 위해서 방사선이 투과되지 않게 제작된 쇠볼이 배치된 1차 검정대상물을 이용하여 엑스선 영상의 내부표정요소와 외부표정요소를 결정하고 이로 부터 엑스선에 교차하게 아크릴로 제작된 두 면을 가지고 있는 엑스선 검정장의 3차원 좌표를 결정하는 2단계 과정을 거쳤다. 사진측량기법에 의해 결정된 엑스선 검정장의 3차원 좌표값은 정밀하게 관측된 CMM과의 비교를 통하여 그 정확도를 평가하였으며 엑스선의 진행방향(X축)에 대한 오차가 Y축과 Z축에 비해 상대적으로 높게 나타났으나 Y축과 Z축에 대한 위치오차는 수 mm의 정확도를 나타내었다. 본 연구를 통해서 사진측량기법은 환자의 3차원 위치결정이나 의료용 교정기기를 제작하는데 도움을 줄 수 있을 것으로 사료된다.

• 한국통신학회논문지
• /
• 제41권12호
• /
• pp.1876-1883
• /
• 2016

본 논문에서는 고속의 공용데이터링크(common data link, CDL)를 위한 새로운 채널 모델을 제안한다. 송신기의 고도가 수km ~ 수십km이고 통달거리가 수백km인 경우 지구 곡률에 의해 송신신호가 수신기의 앞 쪽에서 지면에 반사되어 들어오는 Two-ray 채널이 발생할 가능성이 크다. 송수신기의 빔포밍(beamforming) 각도와 안테나 방사 패턴(radiation pattern)에 따라 반사 경로로 들어오는 신호의 최대 지연 시간(maximum delay)과 전력 지연 프로파일(power delay profile)을 추정하여 Two-ray 채널을 모델링한다. 제안하는 채널 모델에서는 통달거리가 길기 때문에 전력 지연 프로파일이 최대 지연 시간보다 신호 대 잡음비(signal to noise ratio, SNR)에 대한 비트 오류율(bit error rate, BER)에 더 큰 영향을 미친다.

• Journal of Astronomy and Space Sciences
• /
• 제33권1호
• /
• pp.1-11
• /
• 2016

Over the last few years, the data obtained using the Large Area Telescope (LAT) aboard the Fermi Gamma-ray Space Telescope has provided new insights on high-energy processes in globular clusters, particularly those involving compact objects such as MilliSecond Pulsars (MSPs). Gamma-ray emission in the 100 MeV to 10 GeV range has been detected from more than a dozen globular clusters in our galaxy, including 47 Tucanae and Terzan 5. Based on a sample of known gammaray globular clusters, the empirical relations between gamma-ray luminosity and properties of globular clusters such as their stellar encounter rate, metallicity, and possible optical and infrared photon energy densities, have been derived. The measured gamma-ray spectra are generally described by a power law with a cut-off at a few gigaelectronvolts. Together with the detection of pulsed γ-rays from two MSPs in two different globular clusters, such spectral signature lends support to the hypothesis that γ-rays from globular clusters represent collective curvature emission from magnetospheres of MSPs in the clusters. Alternative models, involving Inverse-Compton (IC) emission of relativistic electrons that are accelerated close to MSPs or pulsar wind nebula shocks, have also been suggested. Observations at >100 GeV by using Fermi/LAT and atmospheric Cherenkov telescopes such as H.E.S.S.-II, MAGIC-II, VERITAS, and CTA will help to settle some questions unanswered by current data.

• 천문학회보
• /
• 제41권1호
• /
• pp.36.1-36.1
• /
• 2016

The physical scenario describing the origin of quasar winds remains largely unsettled due to our failure to account for X-ray weak BAL quasars. We approach this problem by studying the relation between the inner part of the outflow which is likely to be shielding the X-ray emission and thereby helping to drive the UV winds characterised by broad absorption lines (BALs). In particular, we aim to probe the wind-shield connection in the highly X-ray variable BAL quasar PG 2112+059, which has exhibited periods of X-ray weakness and X-ray normality in the past. A set of two 20 ks Chandra observations and two contemporaneous HST observations, separated by at least eight months, combined with a nearly simultaneous archival Chandra-HST observation from 2002, afford us a unique opportunity to study the connection between the shield (which is thought to be responsible for the X-ray absorption) and the ionisation state of the wind (observed as UV BAL features; e.g., C IV and O VI lines) over various timescales.

• 천문학회보
• /
• 제37권2호
• /
• pp.77.2-77.2
• /
• 2012

We have studied the physical properties of X-ray point sources in galaxy clusters for years based on the archival observations using the most sophisticated space X-ray observatory, Chandra X-ray Observatory. Because the ultimate goal of the study is comparing the physical properties of X-ray point sources found in galaxy clusters to those in X-ray blank fields; blank fields are the regions in the sky where any noticeable cosmic diffuse X-ray emission is not observed, an important key issue regarding this study is picking out the point sources related with galaxy clusters. However we do not have red-shift information of all the X-ray point sources. Therefore as a first order approximation we will consider the point sources with smaller projected cluster-centric distance than the adopted size of galaxy clusters. As a first step of this study we perform X-ray surface photometry of ~600 galaxy clusters based on ~800 Chandra ACIS observations. We carefully investigate the radial structures of diffuse X-ray emission in 3 different energy bands. Based on the highly accurate surface photometry we determine the characteristic size of diffuse X-ray emission (i.e., the boundary of X-ray emission). We also investigate the cosmological evolution of this characteristic size of galaxy clusters. General discussion regarding the two dimensional morphology of galaxy clusters will be presented.

• 한국감성과학회:학술대회논문집
• /
• 한국감성과학회 2000년도 추계학술대회 논문집
• /
• pp.105-112
• /
• 2000

The conventional model did not take momentum conservation into consideration when the electron absorbs and emits the photons. II-ray provides momentum conservations on any directions of the entering photons, and also the electrons have radial momentum conservations and fully elastic bouncing between two atoms, in the new atom model. Conventional atom model must be criticized on the following four points. (1) Natural motions between positive and negative entities are not circular motions but linear going and returning ones, fur examples sexual motion, tidal motion, day and night etc. Because the radius of hydrogen atom's electron orbit is the order of 10$^{-11}$ m and the radia of the nucleons in the nucleus are the order of 10$^{-l4}$m and then the converging $\pi$-gamma rays to the nucleus have so great circular momentum, the electron can not have a circular motion. We can say without doubt that any elementary mass particle can have only linear motion, because of the $\pi$-rays' hindrances, near the nucleus. (2) Potential energy generation was neglected when electron changes its orbit from outer one to inner one. The h v is the kinetic energy of the photo-electron. The total energy difference between orbits comprises kinetic and potential energies. (3) The structure of the space must be taken into consideration because the properties of the electron do not change during the transition from outer orbit to inner one even though it produces photon. (4) Total energy conservation law applies to the energy flow between mind and matter because we daily experiences a interconnection between mind and body. Any magnet absorbs n-rays to S pole and sends out the $\pi$-rays from N pole. Proton are constructed with the closed n-rays quantum-mechanically. The crystallizing n-bonding makes two $\pi$-far infrared rays of one wave length between two protons if two $\pi$-rays are supplied to each proton. It is easily done for a $\pi$-ray to be absorbed to a proton if there is a parallel magnetic flow to the blood flow because a $\pi$-ray advances axially under a magnetic field and a proton looks like a sphere. A axially advancing disk-like $\pi$-ray can meet more easily the coming spheres than from the other directions. The blood crystals stimulate the autonomous nerves on the blood vessels during the flow by their mechanical sliding collisions. SM n-ray meridian therapy and SMACN $\pi$-ray meridian therapy show the stimulation of blood flow and also combinational experiment between SM $\pi$-ray meridian therapy and n-ray psycho-physics acupuncture shows more clearly that magnet is forcing to make $\pi$-rays absorbed to the nucleons.s.ons.

• Journal of Information Display
• /
• 제9권3호
• /
• pp.33-38
• /
• 2008

A simple ray tracing model is developed to establish the relationship between the distributions of observed visible light and the excited Xe species in a PDP cell. The ray tracing model can obtain the density distribution of the excited Xe species. It shows the two independent discharge modes created during a single period of sustaining discharge. The maximum density of excited Xe species is located about $148{\mu}m$ away from the center of the gap between two sustaining electrodes. We also found the loss rate of VUV photons by comparing the luminance profile predicted in our theoretical model from experimental results. According to calculations based on our model, only about 22 percent of the photons can impinge the phosphor layer.