The aim of this study was to examine the promoting effect of herbal extracts on hair regrowth in C3H/HeJ mice. The herbal extracts were obtained from the Damo-cosmetics Inc. There were four experimental groups including distilled water (D. W., negative control), 20% ethanol (EtOH, vehicle control), 3% minoxidil (MXD, positive control), and herbal extract (Ext). The herbal extract included the mixture of water and alcohol extract from Pleuropterus multflorus, Lonicera japonica Thunberg, Phellinus linteus, and Phaseolus radiatus. Test compounds were applied to the shaved dorsal skin of mice mouse for 3 weeks. The photograph of hair regrowth was taken at day 0, 4, 7, 10, 14, 17, and 21. The herbal extract group showed faster hair regrowth than negative control group or 20% EtOH groups after 10 and 14 days of treatments. The elongation of hair follicles in MXD and the herbal extract groups were observed. The activities of alkaline phosphatase (ALP) and γ-glutamyl transpeptidase were sfanificantly (γ-GT) increased in MXD and herbal extract groups compared with negative control group (p＜0.05). The expression of epidermal growth factor (EGF) and vascular endothelial growth factor (VEGF) were also sfanificantly hfaher in MXD and herbal extract group than negative control group (p＜0.05), althouah there were no sfanificant differences amoularhe groups of 20% EtOH, MXD, and herbal extract. These results suagest that the herbal extract used in this study may have grpromoting effect on hair regrowth by increasing activities of ALP and γ-GT and expression of EGF and VEGF.

흰목이버섯 균주와 공생균을 수집하고 ITS 5.8S rDNA sequencing을 하여 유전자 서열을 분석하였다. Gene Bank Data homology search 결과 분리된 균의 rDNA 서 열이 이 Tremella fuciformis AF042409의 rDNA 서열 과 99% 일치하는 것으로 확인되었다. 그리고 함께 분리 된 공생균은 같은 방법으로 Annulohhypoxylon stygium 으로 확인하였다. 분리된 T. fuciformis KG 103과 A. stygium KG 201 균주는 PD배지에서 각각 14 ㎜/14 days과 85 ㎜/14 days의 균사생육을 나타내었다. T. fuciformis KG 103 균주의 생육최적온도는 25℃ (14mm/14days) 이었으며, 35℃이상 고온과 15 이하 저 온에서 균사 생장이 억제되었다. A. stygium KG 201은 흰목이버섯균과 유사한 최적온도를 나타내었다. T. fuciformis KG 103 균의 생육 최적 pH는 5.0이었으며, A. stygium KG 201도 pH 5.0에서 생육이 가장 왕성하였다. 흰목이버섯 종균용 최적 배지로 참나무톱밥 77.5%, 미 강 20%, 석고 1.5%, 황백당 1% 가 선정되었다. T. fuciformis KG 103과 A. stygium KG 201혼합 종균을 제조하고 흰목이버섯 자실체생산을 위한 병속재배 방법 을 확립하였다. 콘코브(Corn cob) (77%와 52%)가 사용 한 재료 중 최적의 자실체 성장률을 나타냈으며, 콘코브 함량을 줄일수록 생육이 저조하였다. 면실박과 참나무톱 밥은 단독 사용시 생육이 저조하였고, 콘코브를 첨가시 수 율이 증대되었다. 최적수분농도는 55%로 결정되었다 .

We have preliminarily designed two infrared optical systems of the multi-purpose infrared camera system (MIRIS) which is the main payload of STSAT-3. Each optical system consists of a Cassegrain telescope, a field lens and a 1:1 re-imaging lens system that is essential for providing a cold stop. The Cassegrain telescope is identical for both of two infrared cameras, but the field correction lens and re-imaging lens system are different from each other because of different bands of wavelength. The effective aperture size is 100mm in diameter and the focal ratio is f/5. The total length of the optical system is 300mm and the position of the cold stop is 25mm from the detector focal plane. The RMS spot size is smaller than 40μm over the whole detector plane.

The detection and measurement of faint features in cometary image is generally troublesome due to the high value of the ratio of the brightness of the nucleus to the tail, the large size and low surface brightness of the coma and tail and the disturbing presence of field stars trails. The image processing is based on background removal by median filtering. Sample results are shown for the case study of comet 73P/Schwassmann-Wachmann 3.

We present the sensitivity calculation results for observing the Cosmic Infrared Background (CIRB) by the Multi-purpose IR Imaging System (MIRIS), which will be launched in 2010 as a main payload of the Science and Technology Satellite 3 (STSAT-3). MIRIS will observe in I ( 0.9∼1.2um) and H (1.2∼2.0um) band with a 4×4 degree field of view to obtain the large scale structure ( ∼3 degree) of the CIRB. With the given specifications of the MIRIS, our sensitivity calculation results show that the MIRIS has a detection limit of ∼9nWm−2sr−1 (I band) and ∼6nWm−2sr−1 (H band), which is appropriate to observe the large scale structure of CIRB.