To harvest marketable cucumbers, high quality seedlings must be used. Producing seedlings in the greenhouse during the low radiation period decreases marketability due to insufficient light for growth. Supplemental lighting with artificial light of different quality can be used to improve low light conditions and produce high quality seedlings. Therefore, this study was conducted to select the appropriate supplemental light sources on the growth and seedling quality of grafted cucumber seedlings during the low radiation period. Three cultivars of cucumber were used as scions for grafting; ‘NakWonSeongcheongjang’, ‘Sinsedae’, and ‘Goodmorning baekdadagi’. Figleaf gourd (Cucurbita ficifolia) ‘Heukjong’ was used as the rootstock. The seeds were sown on January 26, 2023, and grafted on February 9, 2023. After graft-taking, cucumbers in plug trays were treated with RB light-emitting diodes (LED, red and blue LED, red:blue = 8:2), W LED (white LED, R:G:B = 5:3:2), and HPS (high-pressure sodium lamp), respectively. Non-treatment was used as the control. Supplemental lighting was applied 2 hours before sunrise and 2 hours after sunset for 19 days. The stem diameter and fresh and dry weights of roots did not differ significantly by supplemental light sources. The plant height and hypocotyl length were decreased in W LED. However, the leaf length, leaf width, leaf area, and fresh and dry weights of shoots were the highest in the RB LED. Seedling qualities such as crop growth rate, net assimilation rate, and compactness were also increased in RB LED and W LED. After transplanting, most of the growth was not significant, but early yield of cucumber was higher in LED than non-treatment. In conclusion, using RB LED, W LED for supplemental light source during low radiation period in grafted cucumber seedlings improved growth, seedling quality, and early yield of cucumber.

고품질의 작물을 재배하기 위해 광은 필수적인 환경조건이 다. 겨울철에는 다른 계절에 비해 일사량이 저조하므로 보광 처리를 이용해 작물의 생육과 수확량을 증대시킬 수 있다. 본 연구는 약광기 동안 고추 온실재배를 위한 경제적인 보광 광 원을 선발하기 위해 수행되었다. 풋고추(Capsicum annuum ‘Super Cheongyang’)는 2019년 9월 5일에 정식하였다. 보광 처리는 2020년 1월 1일부터 2020년 3월 31일까지 수행되었 다. White LED(R:G:B = 5:3:2, W LED), RB LED(red:blue = 7:3, RB LED), 고압나트륨등(high pressure sodium lamp, HPS)을 광원으로 사용하였다. 무처리를 대조구로 사용하였 다. 고추의 초장, SPAD, 마디 수는 보광 광원에 따른 유의적인 차이가 없었다. 그러나 분지 수는 RB LED 광원에서 가장 많 았다. 또한 보광은 고추의 광합성을 증가시켰으며, 특히 RB LED에서 보광기간 동안 가장 높은 광합성률을 보였다. 또한 고추의 수확량은 보광처리에서 증가하였고, RB LED는 다른 광원에 비해 가장 높은 수확량을 보였다. 소비전력은 W LED 가 가장 높았고 HPS 조명이 가장 낮았다. 경제적인 측면에서 RB LED를 이용한 보광처리는 다른 광원에 비해 높은 경제성 을 가졌다. 결론적으로 이러한 결과는 고추 온실에서 약광기 동안 보광 광원으로 RB LED를 사용하는 것이 수확량과 경제 성을 향상시킬 수 있을 것으로 판단된다.

본 연구는 HPS (high-pressure sodium lamp, 고압나트륨등, 700W)와 PLS (Plasma Lighting System, 플라즈마 등, 1,000W) 램프를 이용하여 겨울재배 오이의 보광재배 효과를 구명하고자, 양지붕형 유리온실 3동에 무보광을 대조구로 하여 오이(‘후레쉬’ 품종)를 2015년 11월 2일에 정식하여 2016년 3월 15일까지 재배하였다. 보광은 2015년 11월 20일부터 2016년 3월 15일까지 약 4개월 동안 명기를 14시간/일(일몰 전 약 30분에 점등 개시)으로 정하여 실시하였고, 낮동안의 일사량이 100W·m2 이하일 경우 자동으로 점등이 되도록 제어하였다. 분광투과특성은 PLS의 경우 광합성유효광(400-700nm)이 전반적으로 고르게 분포하나 HPS는 400-550nm 광량이 매우 적은 반면, 550-650nm 광원이 PLS보다 많이 분포되었다. 330-1,100nm 광은 HPS가 PLS에 비해 6% 많았고 UV와 적색광은 비슷하였다. 광합성유효광(400-700nm)은 HPS에 비해 PLS가 12.6% 많았고, 근적외선(700-1,100nm)은 HPS에 비해 PLS가 12.6% 적었으며, R/FR은 HPS가 높았다. 오이의 초장, 엽수, 마디수, 건물중 등의 생육은 무보광에 비해 두 보광등에서 비슷한 수준으로 높았다. 광합성능력은 두 광원 간에 유의적인 차이가 없었다. 오이의 주당 과실 개수(무게)는 무보광 21.2개(2.9kg)에 비해 PLS가 38.7개(5.5kg), HPS가 40.4개(5.6kg)로 1.8~1.9배 많았다. 보광등의 설치비와 전기 에너지 비용을 고려하여 오이 보광재배의 경제성을 분석한 결과, PLS와 HPS 보광등은 각각 37%와 62%의 소득증대효과가 있었다.

Modern society attaches great important to state of the technology, but, unconscious desire and subconscious are also discussed in an important value. In the social background of such madness is acting as an artistic inspirational to the many people. At such a time, fashion photographs also being used medium which speak for people's desire. Editorial fashion photographs with unusual stories or including experimental visual elements unlike fashion advertising have increasing. The subject of this study is the formative characteristics in recognition of madness from ancient times until now and find out new meaning of the unusual and informal form of editorial fashion photographs showed in Vogue Italia since 2000. The analysis data of this study, we used 36 photographs of editorial fashion photographs taken by Steven Meisel, Tim Walker and Miles Aldriege. The final process of analysis made in with agreement of 10 major people. We used photograph's basic visual elements as analysis to avoid arbitrary interpretations. The content of this study is drawing in editorial fashion photographs from the viewpoint of Michael Foucault's Madness theory, Deleuze and Felix Guattari's Madness as the aspects of desire. The madness images in the editorial fashion photographs were showed as Decadence, Blindness, Violence and Grotesque based on the analysis results from above. The formative characteristics of editorial fashion photographs enabled the awareness on the value and importance of madness in modern society. These editorial fashion photographs can be the source of our wider perspectives for changing recognition of madness.

KASI (Korea Astronomy and Space Science Institute) is developing the near-infrared camera system named KASINICS (KASI Near-Infrared Camera System) which will be installed at the 60cm f/13.5 Ritchey-Chretien telescope of the Sobaeksan Optical Astronomy Observatory (SOAO). The camera system is optimized for JHKL bands and has a 6 arcmin FOV. The optical system consists of two spherical mirrors and a 8-position filter wheel. With the exception for the dewar window, all optical elements are cooled inside cryogenic dewar. Since the Offner system is adopted to prevent thermal noises from outside of the telescope primary mirror, the secondary mirror of the Offner system acts as a cold Lyot stop. The optical performance does not change by temperature variations because the Aluminum mirrors contract and expand homogeneously with its mount. We finished the design and fabrication of the optical parts and are now aligning the optical system. We plan to have a test observation on 2006 January.

We tested the characteristics of the BOAO Medium Dispersion Spectrograph (MDS) such as the CCD capabilities, wavelength shift by gravity direction variation, slit illumination function and efficiency. Then we calculated the appropriate exposure time to obtain the given S/N ratio for several given magnitudes. Also the remaining problems to be improved were discussed.