The researcher inquired drying characteristics by reflecter shape. Near infrared ray (NIR) is very useful in various drying field. The researcher compared and investigated, temperature about reflecter's shape with numerical analysis method and experimental method. The researcher also investigated about distance between a lamp and a drying target plate using experimental method. As far as a experimental method is concerned, the researcher used the thermal image processing system for changing distance between a lamp and a drying target plate into H=500mm, 600mm and 700mm. Also presented experimental results are compared about thermal image for temperature distribution at each cases. As a result, the researcher has come to the H=700mm about best result in this study.

본 연구의 목적은 축우용 TMR 사용이 점차 증가하고 있으나 TMR의 영양성분을 측정하고자 할 경우 실험실 분석에 의존하므로 많은 비용과 시간이 소요되어 농가 현장에서 활용하기가 어려움에 따라 NIRS(Near InfraRed Spectroscopy, 근적외선분광분석기)을 이용하여 TMR에 대한 신속하고 간편하게 사료가치를 평가하기 위한 검량선을 작성하기 위하여 실시하였다. 근적외선 분광분석법은 친환경 분석으로서 시약의 사용이 전혀 없고, 폐수 및 유해

본 연구는 청예용 사초의 질을 신속하고 정확하게 측정할 수 있는 대안을 모색하기 위하여수행하였다. 근적외선분광분석법을 이용한 사초의 분석가능성을 타진하기 위해 2002년부터 2007년에 거쳐 생산된 각종 사초 258점을 시료로 사용하였다. 즉 시료는 조단백질, 조섬유, NDF, ADF 그리고 건물소화율을 분석하였으며, 또한 NIR System으로 사이의 파장을 얻었다. 그리고 파장과 습식분석치를 이용하여 중회귀식을 만들고 이것을 사용하여 미지의 시료를

We present optical and near-infrared imaging and long-slit spectroscopy for the blue compact dwarf galaxy (BCD) Mrk 49 in the Virgo Cluster. The surface brightness distribution analysis shows that Mrk 49 consists of an off-centered blue bright compact core of r = 10′′ and a red faint outer exponential envelope. The Hα image and color difference suggest that these two components have different stellar populations: a high surface brightness population of massive young stars and an underlying low surface brightness population of older stars. The redder near-infrared colors of the inner most region suggest that the near-infrared flux of Mrk 49 originates from evolved massive stars associated with the current star-forming activity. The total apparent magnitude is BT = 14.32 mag and the mean effective surface brightness is μeff (B) = 21.56 mag arcsec−2. Long-slit spectroscopy shows that Mrk 49 rotates apparently as a solid body within r = 10′′ in a plane at position angle 55 degrees with an amplitude of about 20 km sec−1. The measured radial velocity of Mrk 49 was derived as 1,535 km sec−1; and the total mass of stars and gases is in the range of 3 to 6 × 109 M⊙. The mass-to-light ratios for the central region of Mrk 49 in I and B band are estimated 1.0 and 0.5, respectively. The upper limit of the dark matter to visible matter ratio seems to be < 5. The oxygen abundance is 12 + log(O/H) = 8.21 ± 0.1 which is about one quarter of the solar value while the relative helium abundance appears to be similar to that of the sun.

We present wide-field JHKs-band photometric observations of the three compact H II regions G48.9-0.3, G49.0-0.3, and G49.2-0.3 in the active star-forming region W51B. The star clusters inside the three compact H II regions show the excess number of stars in the J-Ks histograms compared with reference fields. While the mean color excess ratio (EJ-H/EH-Ks) of the three compact H II regions are similar to ~2.07 the visual extinctions toward them are somewhat different ~17 mag for G48.9-0.3 and G49.0-0.3; ~23 ≤ 2 Myr The inferred total stellar mass,~1.4x104M⊙, of W51B makes it one of the most active star forming regions in the Galaxy with the star formation efficiency of ~10%.

We present JHKS near-infrared CCD photometric study for the Galactic open clusters NGC 1641 and NGC 2394. These clusters have never been studied before, and we provide, for the first time the cluster parameters; reddening, distance, metallicity and age. NGC 1641 is an old open cluster with age 1.6 ± 0.2 Gyr, metallicity [Fe/H]= 0.0 ± 0.2 dex, distance modulus(m-M)0=10.4 ± 0.3 mag(d=1.2 ± 0.2 kpc), and reddening E(B-V)=0.10±0.05 mag. The parameters for the other old open cluster NGC 2394 are estimated to be age=1.1±0.2 Gyr, [Fe/H]=0.0±0.2 dex, (m-M)0=9.1±0.4 mag(d=660±120 pc), and E(B-V)=0.05±0.10 mag. The metallicities and distance values for these two old open clusters are consistent with the relation between the metallicities and the Galactocentric distances of other old open clusters. We find the metallicity gradient of 53 old open clusters including NGC 1641 and NGC 2394 to be Δ[Fe/H]/ΔRgc=-0.067 ± 0.009 dex kpc-1.

We present JHK-band near-infrared photometry of the star clusters in the dwarf irregular galaxy IC 5152. After excluding possible foreground stars, a number of candidate star clusters are identified in the near-infrared images of IC 5152, which include young populations. Especially, five young star clusters are identified in the(J-H, H-K) two color diagram and the total extinction values toward these clusters are estimated to be Av=2-6 from the comparison with the theoretical values given by the Leitherer et al.(1999)'s theoretical star cluster model.

본 연구는 시료 및 스펙트럼의 전처리 방법이 근적외선 분광법을 이용한 옥수수 사일리지의 화학적 조성분의 예측능력에 미치는 영향을 평가하기 위해 수행되었다. 시료의 전처리 방법은 건조하여 분쇄하는 방법(Oven Dried Grinding), 액화 질소처리 후 분쇄하는 방법(Liquid Nitrogen Grinding) 그리고 생사일리지(Intact Fresh)처리로 하였으며 4개의 스펙트럼의 수처리(1,4,4, 2,6,4, 2,10,5) 방법을 이용하여