The main objective of this paper is to analyze the r('ctangular stiffened plates with two opposite ends elasti cally restrained and t he others simply supported subjected to in-plane bending by Finite Element κ1ethod. Another objecti ve is to develope Classical Method analyzing the unstiffened rectangular plates with the above boundary conditions. In order to validate finite element and classical methods, the buck , ling strengths of the rectangular plates with four simply supported ends, and with two simply supported and the others fixed ends by fini te element method and classical method are compared with those of references. In finite element method, elas tically restrained ends can be obtained as considering torsional and warping rigidities of end stiffeners. The buckling strengths of the rectangular plates with elastically restrained ends by finit e element and classical methods are calcu lated and compared with each other.In case of stiffened plates, to validate finite elernent rnethod, the buckling strengths of the rectangular stiffened plates with four sirnply supported ends, and with two sirnply supported and the others fixed ends are also cornpared with those of references. The buckling strengths of the rectangular stiffened plates with elastically restrained ends by finite elernent rnethod are calculated as solving eigenvalue problerns which are obtained as assernbling rectangular plate elernents and bearn elernents considered torsional and warping rigidities. The buckling strengths of rectangular stiffened plates according to various positions of rectangular intermediate stiffener, J and 1" of end stiffeners are also obtained, which are cornpared to deterrnine the efficient position of interrnediate stiffener.

We present UBVRI CCD photometry of the Type Ie supernova SN 19941 in M51 which was discovered on April 2, 1994 (UT). UBVRI CCD photometry of SN 1994 I were obtained for the period of the first two months from April 4, 1994, using the Seoul National University Observatory 60 cm telescope. The light curves of SN 19941 show several interesting features: (a) SN 19941 reaches the maximum brightness at B-band on April 8.23 (B = 13.68 mag), at V-band on April 9.10 (V = 12.89 mag), and at I-band on April 10.32 (I = 12.48 mag); (b) The light curves around the maximum brightness are much narrower than those of other types of supernovae; (c) The light curves after the peak decline more steeply than those of other types of supernovae; and (d) The colors get redder from (V-R) ≈ 0.2 mag ((V - I) ≈ 0.3 mag, (B - V) ≈ 0.7 mag) on April 4 to (V-R)≈ 0.6 mag ((V-1) ≈0.9 mag, (B-V) ≈ 1.3 mag) on April 18. Afterwards (V - R) colors get bluer slightly (by ~0.005 mag/day), while (V-I) colors stay almost constant around (V-1) ≈ 1.0 mag. The color at the maximum brightness is (B-V)=0.9 mag, which is ~1 mag redder than the mean color of typical Type la supernovae at the maximum brightness. The light curves of SN 1994I are similar to those of the Type Ie supernova SN 1962L in NGC 1073. Adopting the distance modulus of (m-M)0 = 29.2 mag and the reddening of E(B - V) = 0.45 mag [Iwamoto et al. 1994, preprint for ApJ], we derive absolute magnitudes at the maximum brightness of SN 1994I, Mv(max) = -17.7 mag and MB(max) = -17.4 mag. This result shows that SN 1994I was ~2 mag fainter at the maximum brightness compared with typical Type Ia supernovae. A narrower peak and faster decline after the maximum in the light curve of SN 1994I compared with other types of supernovae indicate that the progenitor of SN 1994I might be a lower mass star compared with those of other types of supernovae.

One of the problems facing international companies is the question of whether to use standardized international advertising or to adapt advertising messages in each country. This paper provides empirical evidence for whether or not to be able to use standardized advertising based on a comparison of evaluative criteria for automobiles and toothpaste among American, Japanese, and Korean consumers. There appears to be a similar pattern among respondents of the three countries in rank of attribute importance. Especially, the result of toothpaste shows an almost identical pattern. The findings do support the idea that international advertising can be standardized due to the similarities among world-wide consumers.

Slow seedling growth rate and nodulation failure of white clover (Trifolium repens L.) has been limited its good establishment to pastures. The experiment was done to determine the effect of removal of cotyledon and unifoliolate on the shoot, root growth,

Two perforated plates(a square plate and a rectangular plate having an as야ct ratlO 1.57(L,=11, L,= 7)) are taken as analysis examples. Each of these plates is given some changes in the boundary ∞nditions. The size of cutouts as well as their locations are also changed in order to examine the variation of two eigenvalues corresponding to the fundamental mode. The relationship between two eigenvalues is estab!ished by changing the magnitude of edge thrust

2차원인 유한요소들을 각 절점에서 6개의 자유도를 갖는 3차원언 업체호 결함함으로서， 횡하중을 받 고있는 합성 젤 구조를 해석할 수 있는 프로그랩 [MSSLL]을 개발하였다. 전체 구조물이 여러개의 반복 되는 Substructure들로 이루어졌을 때에는， 인력의 소모를 극소화 하고 계산시간을 절약할 수 있도록 해석과정에 Substructuring 기법을 본 프로그램에 도입하였다. 프로그램의 신뢰도를 확인하기 위하여 본 프로그램에 의한 해석결과와 다른 방법에 의한 결과를 비교분석 하였으며， 지진력을 받고있는 8 개의 개별 원추뜰로 구성된 웰 구조의 거동에 대한 높이-경간비의 영향을 규명하기 위하여 변수연구를 수 행하였다.

According to the star formation rate and metal enrichment rate given by the disk-halo model of Lee and Ann (1981), the two different forms of time-dependent initial mass function (IMF) and the present day mass function (PDMF) of nearby stars have been examined. It was shown that the constraint for the initial rapid metal enrichment requires the time-dependence of IMF at the very early phase ( t ≲ 5 × 10 8 yrs) of the solar neighborhood. The computed PDMF's show that the PDMF is nearly independent of any specific functional form of IMF as long as the latter includes a Gaussian distribution of log m. This result is due to the very small fractional mass ( × 5 of stars formed at the very early period during which the IMF is time-dependent. The computed PDMF suggests the presence of more numerous low mass stars than shown in Miller and Scalo's (1979) PDMF, supporting the possibility of the existence of low-velocity M dwarfs. According to the number distribution of stars with respect to [Fe/H], the mean age of these low mass star must be very old so as to yield the mean metal abundance ¯ [ F e / H ] ≈ − 0.15 for the stars in the solar neighborhood.

Although Serkowski used a single value K=1.15 in representing all the observed interstellar linear polarization curves by his empirical relation p ( λ ) / P m a x =exp (-K 1 n 2 ( λ m a x / λ ) ), where p m a x is the maximum polarization at wavelength λ m a x , we have noticed a meaningful variation in K from observations of 72 stars. By comparing K's with P m a x / E B − V a n d w i t h λ m a x , we have examined how the shape of the polarization curve is related with the degree of grain alignment on one hand, and with grain sizes on the other. We have shown that correlations between K, P m a x / E B − V a n d w i t h λ m a x , are consistent with the idea of Davis-Greenstein mechanism for grain alignment.

This study is conducted to investigate the effects of growth characteristics (GC) and DPPH radical scavenging activity (DRSA) of the heading lettuce ‘Fidel’ depending on four concentrations of activated mineral groups (AMG: 1.6% active minerals and 0.03% CaO) added to basic nutrient solutions (diluted by 0, 0.05, 0.1, and 0.2%) and on four different light-emitting diodes (LED; B:R:W ratio = 0:1:12, 0:1:9, 0:5:5, and 2:3:5). Both 0.1 and 0.2% AMG showed better GC of lettuce in plant width, plant length, leaf width, leaf length, and the number of leaves than those of other AMG, while leaf thickness and chlorophyll value did not show significant difference among all AMG. Moreover, 0.1 and 0.2% AMG showed heavier shoot fresh weights than those of other AMG. As for the combinations of AMG and LED, B0:R5:W5 showed the best lettuce GC regardless of AMG compared to other AMG and LED combinations. As shown in the above results of LED, although there was a difference in lettuce growth by LED, the differences of lettuce growth by AMG were statistically significant. The DRSA was the highest at 82.8% in B2:R3:W5, followed by B0:R5:W5 at 77.8%. LED showed differences but AMG did not affect DRSA. Therefore, the optimal conditions in plant factory for GC and DRSA of the lettuce were 0.1% AMG and B0:R5:W5.

유방촬영장치(mammography equipment, ME)을 이용한 유방검사(mammography, MG)의 경우 유방암의 조기진단을 위해 가장 일반적으로 시행되고 있는 검사방법으로 유방 내 섬유화 조직, 미소석회화 및 종양덩어리의 발견과 진단은 유방촬영장치의 품질관리(quality management, QM)에 의해 크게 영향을 받게 된다. 특히, 유방검사에서 품질관리란 장치와 연관된 문제점들이 임상영상에서 영상의 질(image quality, IQ) 저하로 진단영역 축소를 초래할 수 있는 발생가능한 모든 문제점을 사전에 파악하여 교정함으로써 항상 일정 수준의 영상의 질을 유지하고 영상을 획득할 수 있게 하는 행위를 의미한다. 이에 본 연구진은 유방촬영장치를 이용한 유방검사의 품질관리에 대한 일반적인 내용을 요약하여 보고 한다.

본 연구에서는 CT영상기반 3차원 고관절모델을 이용한 컴퓨터시뮬레이션을 통해서 고관절의 운동범위 (Range of Motion)를 측정하는 방법을 제시하였다. 본 연구에서는 그 측정방법에 대한 기술적인 사항을 제시하고, 그 기술이 재현성 있게 실현할 수 있도록 대퇴골두 중심점의 결절, 대퇴골 외전(Abduction)/내전(adduction)회전축, 굽힙(flexion)/신전(extension) 회전축을 정의하고 측정하는 명확한 방법을 제시하였다. 외전각은 해부학적인 시상면(Sagittal plane)상의 Anterior-Posterior축에 대해 아래쪽(Inferior)면으로부터 Lateral 쪽으로의 회전각으로 정의된다. 최대외전각은 대퇴골두가 엉덩이뼈(Pelvis)의 절구(Acetabulum)의 테두리와 겹치지 않고 Anterior-Posterior축을 중심으로 회전할 수 있는 최대 외전각으로 결정된다. 굴곡각은 해부학적인 관상면(Coronal plane)상의 Medial-Lateral축에 대해 아래쪽(Inferior)면으로부터 회전각으로 정의된다. 최대굴곡각은 대퇴골이 Medial-Lateral축을 중심으로 엉덩이뼈(Pelvis)의 절구(Acetabulum)의 테두리와 겹치지 않고 회전할 수 있는 최대 굴곡각으로 결정된다. 정상고관절에 비해 인공고관절술을 받은 해당 환자의 경우, 외전에서는 60도 정도, 굽힘에서는 4도 정도 운동범위가 줄어들 수 있다는 예측이 나왔다. 본 연구에서 행한 시뮬레이션을 해보고 외전의 경우 운동범위의 감소가 예측되므로, 대퇴골두를 조금 큰 것을 고르거나 대퇴골목부의 길이 (femoral neck offset)를 길게 시술해야 할 필요가 있음을 의미한다.