We analyze the extinction law towards several B1V stars-members of our Galaxy, searching for possible discrepancies from the galactic average extinction curve. Our photometric data allow to build extinction curves in a very broad range: from extreme UV till infrared. Two-colour diagrams, based on the collected photometric data from the ANS UV satellite, published UBV measurements and on the infrared 2MASS data of the selected stars, are constructed. Slopes of the fitted straight lines are used to build the average extinction curve and to search for discrepant objects. The selected stars have also been observed spectroscopically from the Terskol and ESO Observatories; these spectra allow to check their Sp/L's. The spectra of only about 30% of the initially selected objects resemble closely that of HD144470, considered as the standard of B1 V type. Other spectra either show some emission features or belong clearly to another spectral types. They are not used to build the extinction curve. Two-colour diagrams, constructed for the selected B1 V stars, showing no emission stellar features, prove that the interstellar extinction law is homogeneous in the Galaxy. Both the shape of the curve and the total-to-selective extinction ratio do not differ from the galactic average and the canonical value(3.1) respectively. The circumstellar emissions usually cause some discrepancies from the average interstellar extinction law; the discrepancies observed in the extraterrestrial ultraviolet, usually follow some misclassifications.

이 연구의 목적은 기존의 학생들이 가지고 있던 기존이론과 일치하지 않는 공룡의 멸종 관련 불일치자료에 대한 중학생의 반응유형을 조사, 분류하는 것이다. ‘공룡의 멸종원인’이라는 지구과학 소재를 이용해 기존이론과 불일치자료에 해당하는 자료지를 구성하였다. 불일치자료에 대한 학생들의 반응유형을 분석한 결과, 거부, 재해석, 판단불확실, 신뢰감소, 부분적 이론변화, 이론변화 등 6가지로 분류할 수 있었다. 이러한 결과는 불일치자료를 이용한 개념변화 학습에서 불일치자료의 제시로 반드시 개념변화가 이루어지는 것이 아님을 보여준다. 따라서 교사는 학생들이 불일치자료에 대해 다양한 반응을 나타낼 수 있음을 인식하고, 구체적인 교수전략을 구상하여 처치함으로써 학생들의 개념변화를 도울 수 있을 것이다.

Detailed low spectral resolution observations of the spectrum have been made for three early spectral type standard stars, HR718, HR1544, HR3454, respectively, for the wavelength region 4,300 A to 7,500 A, using the Bohyunsan Optical Astronomy Observatory (BOAO) Middle- Dispersion Spectrograph. These standard stars were chosen from well-known bright northern standard stars. All of the observed long slit spectral data has been reduced and analyzed using the IRAF reduction procedure. The derived extinction coefficients are compared with the other observatory result. The derived value can be used in the determination of flux calibration of BOAO spectroscopic observation. However, until the high quality data are secured from a new series of observation in the blue region and are re-analyzed together, the extinction coefficients below the 4,000 A wavelength remains unknown.

We have made observations of the dark cloud, B5 in the transitions of H2CO, J = 1 10 ― 1 11, and 2 12 ― 1 11. We compared the H2CO result with the observational results of CO and with the visual extinction. There exists an overall correspondence of molecules and extinction. However, a detailed agreement is lacking. We discussed the kinematics and the spatial relationship of molecules and extinction in this cloud.

We mapped the 13CO line in the dark nebula L134 using the 14-m Taeduck radio telescope with a 57 arcsec beam and one beam spacing. The cloud has a spherical shape with an intensity peak ridge extended from the northwest to the southeast directions. The halfwidth and the radial velocity of the lines peak at the region of the cloud center. The radial velocity decreases from the cloud center towards the north and south directions. The integrated line intensity distributions in the space-velocity plane show some structure and a velocity gradient. The 13CO and H2CO clouds and dark clouds are closely related in space in shape, outer boundary, and intensity peak positions. The 13CO integrated line intensity is linearly proportional to the visual extinction.

We have compared the column densities of H 2 C O , 13 C O , C 18 O , 12 C O , CS, and H C O + to the visual extinctions derived from star counts in eight dark clouds, L1317, B1, L1551, L1535, L1544, L134, L134N, and B335. We examined the degree of correlation between molecules and extinctions. The contours of 13 C O , H 2 C O , and CS distributions show an excellent coincidence with those of the visual extinction. Even though the plots of molecule brightness temperature or column density as a function of the visual extinction show a considerable scatter, a good correlation is found between the two quantities. The turnover of the ratios of 13 C O and H 2 C O column densities to the visual extinction at high extinctions observed in several clouds is not apparent in this work. The ratios seem to maintain constant values within the range of A V we studied. The slopes of the relations between the molecule column density and extinction, and the threshold values of extinction for detection of molecules are comparable to the other works. The cause of the slope difference is discussed. We derived, for the first time, the relations of CS and H C O + column densities and the visual extinction. The ratio of CS column density to extinction is at least two orders of magnitude lower than the mean value for 13 C O , but the threshold for detection of CS is comparable to that of 13 C O . The ratio of the H C O + column density to extinction is one to two orders of magnitude lower than the mean ratio for H 2 C O .

We have observed 85 UBV standard stars(V<6) with SNU photoelectric photometer system and 24" Cassegrain reflector at Sobaeksan Observing Station during the period between January and May, 1980 in order to examine the photometer system and to determine atmospheric extinction coefficients. From five night observations, the following results were obtained: (1) The set of filters(V=2mm GG 495, B=2mm GG 385+1mm BG 12, U=2mm UG 2) is better than the other filter set used in our tests on the basis of linear instrumental calibrations for V and B filters. (2) The SNU detecting system is very stable within σ = 0.002 in magnitude in a night but the variation in its stability from night to night is not negligible. (3) The extinction coefficients were derived from two different methods and we have found no systematic seasonal variation in the extinction coefficients although the mean dispersion is considerable.

최근 공동주택은 편리한 교통이나 우수한 교육여건보다 풍부한 녹지와 주변 자연경관을 선호하는 경향으로 변화하고 있다. 공동주택에서 교목, 관목, 초본이 다양하게 혼식되어 풍부한 생태공간을 조성하기 위해서는 공동주택 건물에 의한 공간별 일조환경의 정확한 예측이 요 구된다. 본 연구는 다층구조식재를 위해 관목과 초본의 일조에 영향을 미치는 건물과 교목류 하부의 일조환경을 예측하기 위해 수종별 광 소멸계수를 도출하였다. 공동주택에 식재되는 대표적인 18종의 교목을 대상으로 180도 화각을 가진 어안렌즈로 측정한 영상자료를 Hemisfer 프로그램을 이용하여 식물의 엽면적 지수를 산출한 후 Goudriaan의 방정식으로 수종별 광소멸 계수를 산정하였다. 엽면적 지수 증가에 따른 광소멸계수는 꽃사과, 대왕참나무, 고로쇠나무가 유사한 패턴으로 가장 급격하게 감소하여 일사의 차이가 가장 큰 수종 그룹 으로 나타났다. 향후 정원 설계 및 유지관리용 소프트웨어 개발을 통한 공동주택 일조환경 분석에 필요한 기초데이터로 활용하고자 한다.

수분함량과 유기물 함량이 80% 이상으로 매우 높고, 염도가 높은 국내 음식물쓰레기는 저장 및 운송과정에서 쉽게 부패하는 문제가 있어 적정 처리에 대한 효과적 기술 개발 필요성이 증대되고 있다. 유기물질을 분해하는 미생물이 산소를 이용하는 호기성 퇴비화방법은 유기물을 안정화시키는 것으로 미생물이 음식물 쓰레기를 분해하여 부식질인 퇴비물질, 물과 이산화탄소로 전환시킨다. 본 연구에서는 음식물쓰레기 발효 소멸 시스템을 이용 음식물쓰레기를 처리 하여 음식물 쓰레기의 발효특성을 알아보았다. 이를 통해 운전 안정화를 위한 미생물 활성기반 제어인자를 도출 하고자 하였다. 수분 조절을 위한 통기 개량제는 우드칩이 사용되었고 교반기의 혼합은 3rpm으로 진행되었다. 반응온도는 가온없이 자체발열로 운전 하고 흡인송풍으로 공기가 공급되었다. 운전인자 도출을 위한 발효물질 분석은 공업분석, 원소분석 등이 수행되었고 pH, 함수율, 염도 등이 측정되었다.