In this study, occurrence of aflatoxin M₁ (AFM₁) in domestic milk and milk products was determined. The level of AFM₁ in market milk (0.047 ppb) was lower than that in raw milk (0.083 ppb) but this looks like that is due to dilution in collecting process rather than the effect of sterilization. In the case of nonfat dry milk, level of AFM₁ appeared high by 0.24 ppb but it is thought to be not different from market milk actually because nonfat dry milk is diluted at intake. In the case of ice cream, finished products were contaminated with AFM₁ of 0.020 ppb and also have the possibility of the contamination of AFB₁ due to secondary raw material such as nuts and alinond. On the basis of the results of this study and previous studies, Monte-Carlo simulation is conducted to estimate the contamination level of AFM₁ in domestic market milk. To consider uncertainty and variability fitting procedure was passed through. And we used beta distribution to estimate the prevalence and triangular distribution to estimate the concentration level of AFM₁ in milk. As a result, the 5%, 50% and 95% points of the distribution of the probability of AFM₁ contamination level in milk is 0.0214, 0.0946 and 0.1888 ppb, respectively. Also we estimate that AFM₁ in almost milk was low more than 0.5 ppb that is American acceptable level but 80.4% exceeded far 0.05 ppb that is European standard.

The emission line objects such as planetary nebulae, symbiotics, gaseous nebulae, HII regions, novae, supernovae, SNRs, nearby spiral galaxies, dIrr, dE, and nearby active galactic nuclei, would be goldmines for us to dig with the 1.8m bohyunsan optical (BOAO) telescope. We discussed the importance of strategically important diagnostic lines and atomic constant calculation for a study of Galactic and extragalactic emission objects. The scientific background on a spectrometer development history is briefly presented and spectroscopic research areas other than the emission objects are also summarized.

We installed windscreen at the BOAO 1.8m telescope dome, in order to reduce the degradation of image Quality under strong wind larger than 8m/sec. The windscreen was designed on the basis of that installed at the MSSSO 2.3m telescope dome in Australia. We developed control system (remote control and user program) of the windscreen, being able to operate the windscreen at observation room. We tested the performance of the windscreen under strong wind of 6-15m/see. Tracking error of the telescope, especially in altitude-axis, was greatly decreased when the windscreen was used. Standard deviation of the error was estimated to be less than 0.3arcsec, which has little effect on image quality.

Y0.8Ta0.2O1.7-MO(M=Ba, Sr, Ca 및 Mg) 계에서의 형석구조의 생성과 이와 관련된 구조에 관하여 연구하였다. BaO또는 SrO를 4mol% 첨가한 조성에서는 결함형석구조 이외에 입방정 perovskite형 규칙구조인 Ba2YTaO6 및 Sr2YTaO6와 입방정 Y2O3가 관찰되었다. CaO를 첨가한 경우에는 8mol%이상을 첨가한 조성에서부터 단사정 Ca2YTaO6와 Y2O3의 2차상이 나타났다. MgO의 경우에는 12mol% MgO를 첨가한 조성까지는 형석구조의 단일상을 나타내어 MgO가 형석구조에 고용되는 것을 알수 있었으며, 16 mol%조성부터는 2차상으로 MgO가 관찰되었다. 그러므로 위의 계에서 형석구조의 생성은 A2(B'B")O6의 생성과 첨가된 양이온의 크기에 영향을 받는 것으로 생각된다.생각된다.

1.0Cr-1.0Mo-0.25V강 용접부의 크립 파단 시험시 파단 발생 원인에 관한 연구가 시행되었다. 파괴는 Intercritical Heat Affected Zone에서 발생하였으며 파단면에서 구상의조대한 M6C탄화물이 발견되었다. 모재는 molybdenum 주성분의 M2C, vanadium 주성분의 M4C3 및 chromium 주성분의 M23C6와 M7C3 탄화물이 존재하였다. 모의 실험 결과 준안정 상태인 M2C 탄화물은 850˚C, 10oh에서 안정한 M6C탄화물로 변태하였다. M6C 탄화물은 주변의 molybdenum 농도를 떨어뜨려 강도의 저하를 가져오며 크립 기공의 발생 원인을 제공하였다.

We propose the development and test result of new optical axis alignment system for the interchangeable F/8 secondary mirror of the BOAO 1.8m telescope system. Since the original system was not equipped with a suitable optical alignment facility, the whole alignment process was performed by hand. It was necessary at least three persons working more than 2 nights and the altitude of the telescope could not exceed 10 degrees, in such altitude the alignment quality was not so good by atmospheric effect. The new system adopts position readable motorized system and remote control operation by the computer installed in observation room, which reduces the number of workers to only one and eliminates the altitude restriction. The defocused CCD image pair obtained at higher altitude makes the aberration estimates more accurately and the number of required alignment loops is reduced from 10 to 4. The system has been installed on September 1, and performed alignment three times. The test results show that the system is stable and accurate, gives better optical performance of the telescope under F/8 focus. We hope to emphasize the fact that the new system will increase observation time of the telescope by about 20 nights per year assuming one alignment in every month.

(Pb0.63Ca0.37)ZrO3 세라믹에 MgO와 SrO를 첨가하여 Ca를 Mg와 Sr 이온으로 치환하였을 때의 고주파 유전특성에 대해 연구하였다. Ca 이온의 일부를 Mg 이온으로 치환시킨 경우에는 A-O결합에 의한 분극의 증가로 인하여 유전상수는 직선적으로 증가하지만 품질계수는 감소한다. 또한 Ca 이온을 Sr 이온으로 치환시킨 경우에는 결합길이의 증가로 인해 분극이 감소되어 유전상수와 품질계수가 감소한다. 고주파용 유전재료의 설계에 있어서 관용인자와 이온결합성의 평가가 중요하다.

We present test results of time-series CCD photometry to investigate the photometric precision of the BOAO (Bohyunsan Optical Astronomy Observatory) 1.8m telescope. A well-known field of the old open cluster M67, which includes two pulsating blue stragglers and two W UMa type binaries, was monitored for 3.5 hours on February 22, 1996. We have collected 148 V frames and 3 B frames. Photometric noises which consist mainly of photon noise and scintillation noise, were lowered down to about 1.9 mmag for stars of 10.m5 in M67 with exposure time of 20 seconds. From the C-M diagram for M67, a number of observational properties were derived; E(B-V) = 0.03, (V-Mv)o = 9.6, Age = 4 Gyr. We obtained light curves for four known variable stars and confirmed their variational characteristics. The pulsating blue stragglers show a low amplitude (about 0.01 mag) of light variation.

Mn((Cu0.66AI0.34)1-x(Bi0.3Sb0.7)x) 및 Mn((Fe0.66AI0.34)1-x(Bi0.3Sb0.7)x) 합금계의 상의 변화와 자기적 특성을 조사하였다. Mn((Cu, SI)(Bi, Sb)) 합금계는 Bi상, MnSb상, MnBi상, k-상, Heuser상, Mn2Sb 및 β-Mn상의 혼합상으로 이루어졌으며 x가 증가함에 따라 Bi상과 Mn2Sb상이 증가하고 K-상, Heusler상 및 β-Mn상이 줄어들거나 사라졌다. 자기적 성질은 자성을 띄는 MnSb상, MnBi상, Mn2Sb상, k-상 및 Hseusler상과 비자성인 Bi상과 β-Mn상의 상대적 분율에 의해 결정됨을 알 수 있었고, 150K-200K 부근에서 그 이하로 온도가 감소함에 따라 자화값이 급격히 감소하는 현상이 나타났다. Mn((Fe, AI)(Bi, Sb))합금계는 Bi상, MnSb상, MnBi상, MnBi상,β-Mn상, k-상 및 Mn2Sb상의 혼합상으로 나타났으며, 자기적 성질은 조사한 전 조성에서 강자성을 띄고 있음을 알 수 있었다.

The antifungal effects of polyphosphates on the growth and T-2 toxin production of Fusarium sporotrichioides M-1-1 were investigated. The growth of the strain was significantly inhibited in the potatoes dextrose agar medium treated with 1.5% polyphosphates or more. When we checked T-2 toxin by the indirect competitive ELISA, the strain produced 11.25 ug/ml and 10.90 g/ml levels of T-2 toxin in rice and corn containing 50% moisture contents, respectively. However, T-2 toxin was little detected in rice medium and corn medium with 1.5% polyphosphates addition for short(14 days) and prolonged incubation time(45 days). We also observed the destruction of cell wall and outflow of cell ingredients with 1% polyphosphates treatment to the strain. Therefore, moisture and polyphosphates greatly effected on the growth and T-2 toxin production of the strain.

30KV 전자빔리소그래피 장치를 사용하여 PMMA 3000Å/P(MMA/MAA) 6000Å의 이중구조에서 foot width 0.1μm이하, head width 0.4μm의 T-gate를 형성하였다. PMMA/P(MMA/MAA)/GaAS 구조에 대한 Monte Carlo 시뮬레이션 결과, 산란반경 0.1μm에서 전방산란전자와 후방산란전자의 에너지 비는 19.5:1로 나타났다. 전자빔리소그래피 공정에 필요한 PMMA 및 P(MMA/MMA)의 열처리 조건, 설게 선폭에 대한 패턴감도를 구하였다. MIBK : IPA = 1 : 1 현상액에 대한 PMMA 및 P(MMA/MAA)의 감마값(gamma value)은 2.3이었다. 광 및 전자빔리소그래피 장치의 혼합사용(mix-and-match) 결과 층간정렬도 (alignment accuracy)는 0.1μm(3σ) 이하를 얻었다.