• 제목/요약/키워드: 3D Gap Element

검색결과 87건 처리시간 0.029초

임플란트 지대주나사의 조임회전력이 연결부 안정성에 미치는 영향에 관한 3차원 유한요소해석 연구 (Effect of Tightening Torque on Abutment-Fixture Joint Stability using 3-Dimensional Finite Element Analysis)

  • 엄태관;서승우;전계록;신정욱;정창모
    • 대한치과보철학회지
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    • 제47권2호
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    • pp.125-135
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    • 2009
  • 연구목적: 임플란트 치료에서 흔히 발생하는 기계적인 문제점을 하나가 지대주나사의 풀림과 파절이다. 일반적으로 나사 연결의 안정성을 위해서는 지대주나사의 조임회전력에 의한 전하중을 나사의 탄성한계까지 증가시킬 필요가 있다. 그러나 저작운동에 의한 기능부하는 전하중이 가해진 지대주나사에 추가적인 인장력을 가하게 되어 나사의 풀림이나 파절의 가능성을 높인다. 이러한 풀림이나 파절을 방지하면서 동시에 최대의 결합 강도를 가지는 조임회전력을 찾는 연구가 필요하다. 본 연구는 지대주나사의 조임회전력이 임플란트-지대주 연결부 안정성에 미치는 영향을 3차원 유한요소 분석을 통하여 확인하고자했다. 연구 재료 및 방법: External butt joint를 가진 임플란트를 기반으로 3차원 유한요소 해석모형을 설계하였다. 조임회전력에 따른 지대주나사의 전하중을 이론치, 실험치 및 해석치를 비교하여 해석모형을 검증하였다. 검증한 해석모형에서 대해 조임회전력을 10 Ncm, 20 Ncm, 30 Ncm, 그리고 40 Ncm로 각각 적용하고 지대주에 30도 경사지게 250 N의 외부하중을 가하여 유산요소 해석을 실시하였다. 그 결과를 통해 지대주나사의 최대 등가응력을 계산하고 고정체와 지대주 연결부의 응력분포 및 이개거리(gap distance)를 산출하였다. 결과 및 결론: 본 연구조건 하에서 다음과 같은 결과를 얻었다. 1. 전하중은 조임회전력이 클수록 증가하였다. 2. 조임회전력 적용 후 최대 등가응력은 지대주나사 경부에서 발생하였으며, 나사산 체결부에서는 주로 경부쪽 네 개의 나사산에 응력이 집중되었다. 3. 외부하중을 가했을 때에도 조임회전력을 적용했을 때와 동일하게 최대 등가응력은 주로 지대주나사 경부에서 발생하였으나, 10 Ncm의 조임회전력을 적용한 경우에서는 지대주나사 두부밑면에서 발생하였다. 4. 외부하중을 가했을 때 10 Ncm와 20 Ncm의 조임회전력을 적용한 경우에서는 연결부 이개(joint opening) 현상이 관찰 되었다. 5. 조임회전력이 40 Ncm인 경우에는 경사하중에 의해 지대주나사의 경부에 발생하는 최대등가응력이 나사의 소재인 티타늄 합금의 허용응력을 초과하였다. 이상의 결과로 볼 때, 조임회전력은 고정체와 지대주 연결부의 안정성에 영향을 미치는 것이 확인되었다. 임플란트 지대주나사는 임상에서 발생하는 기능 하중을 고려하여 고정체와 지대주 연결의 안정성을 유지할 수 있는 적정 조임회전력의 크기가 제안되어야 한다.

트랜섬 파이프 간격이 동력대차-견인전동기간 강체 모드 공진응답에 미치는 영향에 관한 연구 (The influence of transom pipe gap on the resonance response in motorized bogie and traction motor system)

  • 김재환;송시엽;임효석
    • 한국음향학회지
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    • 제38권3호
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    • pp.340-343
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    • 2019
  • 본 논문은 동력차에서 견인전동기 기진 주파수와 견인전동기 강체 모드 공진 문제로 인해 발생할 수 있는 현상에 대해 소개하고, 이를 제어하는데 효과적인 설계인자를 해석적으로 검토해보았다. 회전 속도가 변하는 회전기기의 경우, 공진 문제를 해결하기 위해서는 공진주파수 대역을 상용 운전 범위 바깥으로 이동시키거나 동강성을 크게 하는 등의 방법을 통하여 공진 응답이 낮아지도록 하는 방안이 있다. 견인전동기의 운전 범위는 일반적으로 0 r/min ~ 4800 r/min으로 대차모드가 이 운전 영역대를 벗어나게 설계하는 것은 현실적으로 불가능 하다. 따라서 공진 응답에 영향을 주는 설계 인자를 찾아 이를 적절하게 조정하여야 한다. 유한요소 해석 검토 결과, 견인전동기 강체모드 공진 응답에 영향을 주는 설계인자는 트랜섬파이프 간격으로 간격이 지나치게 넓게 설계될 경우 견인전동기 기진력과 강체 모드 간 공진 시 과도한 진동이 발생될 수 있음을 파악하였다.

원동 마그마계 : 암석화학적 진화 (The Wondong magmatic system : its petrochemical evolution)

  • 황상구
    • 암석학회지
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    • 제6권3호
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    • pp.166-184
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    • 1997
  • 원동칼데라는 칼데라 내외부에 외류응회암이 보존되어 있고 함몰후 관입체, 용암과 응회암, 소생관입체와 후기관입체를 노출시킨다. 원동 마그마계의 암석단위는 함몰후에도 상호 점이적인 조성관계를 나타낸다. 이 암체를 정치순서대로 나열하면 원동 마그마계로서 석영반암맥, 반상유문암 용암, 회류응회암, 세립질 화강섬록암 암주, 각섬석 흑운모 화강암 암주와 규장암맥 등이 있고 후기 관입체로서 조면반암 플러그와 염기성암맥이 있다. 석영반암맥은 원동응회암의 유문암성분으로부터 유문대사이트 성분으로의 연속적인 조성변화를 나타낸다. 반상유문암 용암, 회류응회암, 각섬석 흑운모 화강암과 세립질 화강섬록암은 중규산 유문암에서 저규산 유문암, 유문대사이트, 그리고 안산암 성분까지의 연속직인 조성변화를 나타낸다. 이 연속적인 조성변화는 함몰후와 소생시에 마그마챔버에서 지붕에서 하부로 유문암, 유문대사이트, 안산암 성분 순으로 누대 되었음을 지시하고, 상한 성분은 함몰후 마그마 챔버에서 지붕근처의 조성대를 지시하고 하한 성분은 가장 깊은 출조 심도를 지시한다. 이 조상누대와 동위원소 초기치는 원동 마그마계의 화성암류가 마그마챔버에서 칼크알카리 마그마로부터 주로 분별결정작용에 의한 분화를 겪고 챔버지붕이나 챔버벽 근처에서 벽암과 동화작용에 의한 지각혼염이 수반되는 진화과정을 겪었음을 지시한다. 그러나 조면반암 플러그와 염기성암맥은 화학적 성질, 변화트랜드와/혹은 동위원소 초기치의 차별성에 의하면 각각 원동 마그마계의 형성 이후에 다른 마그마 배취로부터 유래 되었을 것으로 생각된다.)의 비대칭 습곡(F2 습곡)을 형성시켰다. 그 결과, 서쪽으로 침강하는 원래의 L1방향은 F2 습곡의 하위 날개(역전된 날개)부에서 북서쪽으로 침강하는 L1으로 재배열되었다. 세 번째 변형(D3 변형)은 $45^{\circ}/265^{\circ}$ 방향의 습곡을 갖는 셰브론(chevron)형 습곡(F3 습곡)으로, 남북 방향의 압축작용에 의해 형성된다. 그 결과, 원래의 L2 방향($20~45^{\circ}/210~230^{\circ}$방향)은 주로 $35~45^{\circ}/260~280^{\circ}$방향과 부수적으로 $30~45^{\circ}/135~165^{\circ}$ 방향의 L2로 재배열된다. D3 변형 이후, 동서 방향의 압축작용으로 형성된 남북 주향에 고각 경사의 습곡축면과 준 수평적인 습곡축을 갖는 열린(open)습곡이 관찰된다.변화는 본역의 화산암이 안산암으로부터 일연의 분별결정작용 산물임을 암시하며, 또한 $Al_2O_3$와 CaO 함량의 관계도, Th/Yb 비에 대한 Ta/Yb 비의 관계도, $Ce_N/Yb_N$$Ce_N$의 관계도에 따른 판별에서도 분별결정작용의 경향을 따르고 있다. 본역의 화산암은 $K_2O$, $Na_2O$, CaO 삼각도에서 도호의 영역에, Ba/La비, La/Th비에 의한 판별도에서 조산대의 high-K suite에 속한다. Rb 대

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Dynamic response of functionally gradient austenitic-ferritic steel composite panels under thermo-mechanical loadings

  • Isavand, S.;Bodaghi, M.;Shakeri, M.;Mohandesi, J. Aghazadeh
    • Steel and Composite Structures
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    • 제18권1호
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    • pp.1-28
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    • 2015
  • In this paper, the dynamic response of functionally gradient steel (FGS) composite cylindrical panels in steady-state thermal environments subjected to impulsive loads is investigated for the first time. FGSs composed of graded ferritic and austenitic regions together with bainite and martensite intermediate layers are analyzed. Thermo-mechanical material properties of FGS composites are predicted according to the microhardness profile of FGS composites and approximated with appropriate functions. Based on the three-dimensional theory of thermo-elasticity, the governing equations of motionare derived in spatial and time domains. These equations are solved using the hybrid Fourier series expansion-Galerkin finite element method-Newmark approach for simply supported boundary conditions. The present solution is then applied to the thermo-elastic dynamic analysis of cylindrical panels with three different arrangements of material compositions of FGSs including ${\alpha}{\beta}{\gamma}M{\gamma}$, ${\alpha}{\beta}{\gamma}{\beta}{\alpha}$ and ${\gamma}{\beta}{\alpha}{\beta}{\gamma}$ composites. Benchmark results on the displacement and stress time-histories of FGS cylindrical panels in thermal environments under various pulse loads are presented and discussed in detail. Due to the absence of similar results in the specialized literature, this paper is likely to fill a gap in the state of the art of this problem, and provide pertinent results that are instrumental in the design of FGS structures under time-dependent mechanical loadings.

열해석을 이용한 자기부상자석의 설계 (Design of Levitation Magnet with Thermal Analysis)

  • 배덕권;성호경;윤용수;배준한;조정민;김동성
    • 대한전기학회:학술대회논문집
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    • 대한전기학회 2007년도 제38회 하계학술대회
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    • pp.1185-1186
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    • 2007
  • The UTM-01 developed in 1998 was the first maglev vehicle in Korea for the urban transit maglev (UTM) system. Through the improvement of UTM-01 and development of UTM02, the commercialization of the UTM system is being prepared now. In order to prepare for the commercialization of maglev, it is necessary that an optimal design of the levitation magnet should be provided for the safe operation of the vehicle. The levitation force is formed through the function of magnetic flux density on the top of magnet poles and gap between magnet pole and guide rail. To generate a magnetic field that is high enough to levitate the vehicle, ferromagnetic materials, such as pure iron for magnet pole and SS400 for guide rail, were used. The heat generated by $I^2R$ loss of magnet conductor makes the thermal convection on the surface of magnet including coil and poles. As these two characteristics are nonlinear phenomena, this paper deals with the nonlinear analysis on the magnetic and thermal properties of the U-type levitation magnet by using 3-D finite element method (FEM). Base on the analysis results, a small scale U-type magnet was designed, manufactured, and tested and it was verified that the magnet manufactured was satisfactory to all the design specifications.

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THEORETICAL STUDY ON OBSERVED COLOR-MAGNITUDE DIAGRAMS

  • Lee, See-Woo
    • 천문학회지
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    • 제12권1호
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    • pp.41-70
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    • 1979
  • From $B\ddot{o}hm$-Vitense's atmospheric model calculations, the relations, [$T_e$, (B-V)] and [B.C, (B-V)] with respect to heavy element abundance were obtained. Using these relations and evolutionary model calculations of Rood, and Sweigart and Gross, analytic expressions for some physical parameters relating to the C-M diagrams of globular clusters were derived, and they were applied to 21 globular clusters with observed transition periods of RR Lyrae variables. More than 20 different parameters were examined for each globular cluster. The derived ranges of some basic parameters are as follows; $Y=0.21{\sim}0.33,\;Z=1.5{\times}10^{-4}{\sim}4.5{\times}10^{-3},\;age,\;t=9.5{\sim}19{\times}10^9$ years, mass for red giants, $m_{RG}=0.74m_{\odot}{\sim}0.91m_{\odot}$, mass for RR Lyrae stars, $m_{RR}=0.59m_{\odot}{\sim}0.75m_{\odot}$, the visual magnitude difference between the turnoff point and the horizontal branch (HB), ${\Delta}V_{to}=3.1{\sim}3.4(<{\Delta}V_{to}>=3.32)$, the color of the blue edge of RR Lyrae gap, $(B-V)_{BE}=0.17{\sim}0.21=(<(B-V)_{BE}>=0.18),\;[\frac{m}{L}]_{RR}=-1.7{\sim}-1.9$, mass difference of $m_{RR}$ relative to $m_{RG},(m_{RG}-m_{RR})/m_{RG}=0.0{\sim}0.39$. It was found that the ranges of derived parameters agree reasonably well with the observed ones and those estimated by others. Some important results obtained herein can be summarized as follows; (i) There are considerable variations in the initial helium abundance and in age of globular clusters. (ii) The radial gradient of heavy element abundance does exist for globular clusters as shown by Janes for field stars and open clusters. (iii) The helium abundance seems to have been increased with age by massive star evolution after a considerable amount (Y>0.2) of helium had been attained by the Big-Bang nucleosynthesis, but there is not seen a radial gradient of helium abundance. (iv) A considerable amount of heavy elements ($Z{\sim}10{-3}$) might have been formed in the inner halo ($r_{GC}$<10 kpc) from the earliest galactic co1lapse, and then the heavy element abundance has been slowly enriched towards the galactic center and disk, establishing the radial gradient of heavy element abundance. (v) The final galactic disk formation might have taken much longer by about a half of the galactic age than the halo formation, supporting a slow, inhomogeneous co1lapse model of Larson. (vi) Of the three principal parameters controlling the morphology of C-M diagrams, it was found that the first parameter is heavy clement abundance, the second age and the third helium abundance. (vii) The globular clusters can be divided into three different groups, AI, BI and CII according to Z, Y an d age as well as Dickens' HB types. BI group clusters of HB types 4 and 5 like M 3 and NGC 7006 are the oldest and have the lowest helium abundance of the three groups. And also they appear in the inner halo. On the other hand, the youngest AI clusters have the highest Z and Y, and appear in the innermost halo region and in the disk. (viii) From the result of the clean separations of the clusters into three groups, a three dimensional classification with three parameters, Z, Y and age is prsented. (ix) The anomalous C-M diagrams can be expalined in terms of the three principal parameters. That is, the anomaly of NGC 362 and NGC 7006 is accounted for by the smaller age of the order of $1{\sim}2{\times}10^9$ years rather than by the helium abundance difference, compared with M 3. (x) The difference in two Oosterhoff types I and II can be explained in terms of the mean mass difference of RR Lyrae variables rather than in terms of the helium abundance difference as suggested by Stobie. The mean mass of the variables in Oosterhoff type I clusters is smaller by $0.074m_{\odot}$ which is exactly consistent with Rood's estimate. Since it was found that the mean mass of RR Lyrae stars increases with decreasing Z, the two Oosterhoff types can be explained substantially by the metal abundance difference; the type II has Z<$3.4{\times}10^{-4}$, and the type I has higher Z than the type II.

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교사환경기준에 관한 연구 (A Study on Environmental Standards of School Building)

  • 홍석표;박영수
    • 한국학교ㆍ지역보건교육학회지
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    • 제1권1호
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    • pp.11-43
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    • 2000
  • The purpose of this study was, through analyzing the previous researches, to grasp the present status of environment of school building(ESB), research the sundry records of each element and, through comparative analysis of the standard of ESB in Korea, the United States, and Japan, select the normative standard of ESB, to clarify the point at issue presented in Regulation of Construction & facility Management for Elementary and and Secondary School in Korea, and to suggest an alternative preliminary standard of ESB. To carry out a research for this purpose, these were required: 1. to investigate the existing present status of ESB, 2. to make a comparative analysis of the standard of ESB in each country, 3. to suggest the normative standard of preliminary standard of ESB, 4. to analyze the controversial points of the standard of ESB in Korea, 5. to suggest an alternative preliminary standard of ESB. The conclusions were as follows: 1. Putting, through analyzing the previous researches, the existing present status of ESB together, it seemed that lighting environment, indoor air environment and noise environment were all in poor conditions. 2. In the result of a comparative analysis of the standard of ESB in Korea, Japan and the United States, in Korea the factors of each lighting and indoor air environment were not presented properly, in Japan, in lighting environment aspect, the standard on natural lighting and the factors on brightness were not presented., and in the USA the essential factors of each environment were throughly presented. In the comparison of the standards on each factor, Korea showed that the standard level presented was less properly prescribed than those of the USA and Japan but it also showed that the standard levels prescribed in the USA and in Japan were mostly similar to the standard levels in records investigated. 3. With the result of the normative standard selection on School Builiding environment factor of prescribed in this study, the controversial points of the standard of ESB in Korea were analyzed and the result was utilized to suggest new preliminary standard of ESB. 4. As the result of the analysis of the controversial points of the standard of ESB in Korea, it was found that the standard of ESB in Korea should be established on a basis of School Health Act and be concretely presented in School Health Regulation and School Health Rule. The factors of each environment was improperly presented in the existing standard of ESB in Korea. Moreover the standard of them was inferior to that of the records investigated and those of in the USA and in Japan and it also showed that the standard of it in Korea was improper to maintain Comfortable Learning Environment. 5. A suggested preliminary standard of ESB acquired through above study as follows: 1) In this study a new kind of preliminary standard of ESB is divided into lighting environment, indoor air environment, noise environment, odor environment and for above classification, reasonable factor and standard should be established and the controling way on each standard and countermeasures against it should be considered. 2) In lighting environment, the factors of natural lighting are divided into daylight rate, brightness, glare. In the standard on each factor, daylight rate should secure 5% of a mean daylight rate and 2% of a minimum daylight rate, brightness ratio of maximum illumination to minimum illumination should be under 10:1, and in glare there should not be an occurrence factor from a reflector outside of the classroom. And the factors of unnatural lighting are illumination, brightness, and glare. In the standard on each factor, illumination should be 750 lux or more, brightness ratio should be under 3 to 1, and glare should not occur. And Optimal reflection rate(%) of Colors and Facilities of Classroom which influences lighting environment should be considered. 3) In indoor air environment factors, thermal factors are divided into (1) room temperature, (2) relative humidity, (3) room air movement, (4) radiation heat, and harmful gases (5) CO, (6) $CO_2$ that are proceeded from using the heating fuel such as oval briquettes, firewood, charcoal being used in most of the classroom, and finally (7) dust. In the standard on each factor, the next are necessary; room temperature: $16^{\circ}C{\sim}26^{\circ}C$(summer : $E.T18.9{\sim}23.8^{\circ}C$, winter: $E.T16.7{\sim}21.7^{\circ}C$), relative humidity: $30{\sim}80%$, room air movement: under 0.5m/sec, radiation heat: under $5^{\circ}C$ gap between dry-bulb temperature and wet-bulb temperature, below 1000 ppm of ca and below 10ppm of $CO_2$, dust: below 0.10 $mg/m^3$ of Volume of dust in indoor air, and ventilation standard($CO_2$) for purification of indoor air : once/6 min.(about 7 times/40 min.) in an airtight classroom. 4) In the standard on noise environment, noise level should be under 40 dB(A) and the noise measuring way and the countermeasures against it should be considered. 5) In the standard on odor environment, odor level under Physical Method should be under 2 degrees, and the inspecting way and the countermeasures against it should be considered.

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