• 한국유기농업학회지
• /
• 제25권4호
• /
• pp.737-747
• /
• 2017

This experiment was carried out to determine the optimal concentration of agricultural organic materials using sulfur and oil for the insect pest control in pepper and cherry tomato cultivation. The control value of aphids and Oriental tobacco budworm (OTB) was examined one day after spraying with sulfur preparation (SP) (0.33~0.17%), oil preparations (OP) (2.00~0.33%), SP+OP, OP+ginkgo leaf extracts (GLE), SP+OP+GLE on the "Super Manidaa"pepper. The aphid control in pepper was complete by applications of SP+OP (0.25+1.00%) in the early growth stage and the control value was above 98.1% by the application of OP+GLE (1.00+1.00 %), SP+OP+GLE (0.25+1.0+1%), SP+OP+GLE (0.25+1.0+0.5%) in the middle to late growth stage while showing 0% in the control treatment. The OTB was completely controlled by the 3 times application with the high concentration of SP+OP (0.25+1.00%) in pepper cultivation. This result indicates that the oil and the sulfur preparations should be applied at low concentration before insect pests do not appeared, and then sprayed at the high concentration after they appear at pepper plant. The greenhouse whitefly in 'Minichal' tomatoes was completely controlled by three times application of SP (0.25~0.33), OP (1.0~2.00%). and all the treatment of SP+OP. However, continuous control with intervals of 1~3 days was considered favorable in the tomato plant. By the periodical control with agricultural organic materials using sulfur and oil, the greenhouse whitefly, which is a high-temperature insect pest, several moths of OTB did not occur at all. In conclusion, SP+OP (0.17%+0.33%) treatment was the most economical combination to control the aphid, OTB, and greenhouse whitefly in pepper and tomato cultivation when considering operating cost. In addition, we recommend that SP should not be sprayed on the plant shoots during the day time from July to August because of high temperature.

• Journal of Astronomy and Space Sciences
• /
• 제33권3호
• /
• pp.185-196
• /
• 2016

New multiband BVRI light curves of NSVS 1461538 were obtained as a byproduct during the photometric observations of our program star PV Cas for three years from 2011 to 2013. The light curves indicate characteristics of a typical W-subtype W UMa eclipsing system, displaying a flat bottom at primary eclipse and the O'Connell effect, rather than those of an Algol/b Lyrae eclipsing variable classified by the northern sky variability survey (NSVS). A total of 35 times of minimum lights were determined from our observations (20 timings) and the SuperWASP measurements (15 ones). A period study with all the timings shows that the orbital period may vary in a sinusoidal manner with a period of about 5.6 yr and a small semi-amplitude of about 0.008 day. The cyclical period variation can be interpreted as a light-time effect due to a tertiary body with a minimum mass of 0.71 M_⊙. Simultaneous analysis of the multiband light curves using the 2003 version of the Wilson-Devinney binary model shows that NSVS 1461538 is a genuine W-subtype W UMa contact binary with the hotter primary component being less massive and the system shows a low mass ratio of q(m_c/m_h)=3.51, a high orbital inclination of 88.7°, a moderate fill-out factor of 30 %, and a temperature difference of ΔT=412 K. The O'Connell effect can be similarly explained by cool spots on either the hotter primary star or the cool secondary star. A small third-light corresponding to about 5 % and 2 % of the total systemic light in the B and V bandpasses, respectively, supports the third-body hypothesis proposed by the period study. Preliminary absolute dimensions of the system were derived and used to look into its evolutionary status with other W UMa binaries in the mass-radius and mass-luminosity diagrams. A possible evolution scenario of the system was also discussed in the context of the mass vs mass ratio diagram.

• 한국산업보건학회지
• /
• 제26권3호
• /
• pp.324-333
• /
• 2016

Objectives: We aimed to compare the sampling performance of different flow-based impactor samplers for collecting fungal spores and bacteria and to explore the association of the level of bioaerosols with activity patterns of occupants in daycare center settings. Methods: For comparison of sampling performance, two different flow-based samplers (greater than 100 L/min or not) were selected; a low flow-based sampler (one-stage Andersen sampler) and two high flow-based samplers (DUO SAS SUPER 360 sampler, BUCK bio-culture sampler). We collected airborne mold and bacteria in 30 daycare centers with various levels of contaminated air. Three repeat samplings per each sampler were performed. Mold and bacteria were grown for 96 hours at $25{\pm}1^{\circ}C$ and 48 hours at $35{\pm}1^{\circ}C$, respectively. The Andersen and SAS samplers were used for investigating the association between the level of bioaerosols and the activity patterns of occupants in daycares. Particular matters 10($PM_{10}$), temperature, and relative humidity were monitored as well. Samplings were carried out with one-hour interval from 9 to 5 O'clock. For statistical comparisons, Kruskal-Wallis test, Wilcoxon's signed rank test, and multiple regression analysis were carried out. Results: The airborne level of molds by the low flow-based sampler were significantly higher than that of high flow-based samplers (indoor, P=0.037; outdoor, P=0.041). However, no statistical difference was observed in the airborne level of bacteria by each sampler. Also the level of bioaerosols varied by the time, particularly with different activity patterns in daycare centers. The higher level of mold and bacteria were observed in play time in indoor. Similarly, the concentrations of $PM_{10}$ were significantly associated with the level of bioaerosols (P<0.05). Conclusions: Our findings indicate that the flow rate of sampler, rather than total air volume, could be able to affect the results of sampling. Also, the level of airborne mold and bacteria vary behavior patterns of occupants in indoor of daycare settings. Therefore, different samplers with other flow rate may be selected for mold or bacteria sampling, and activity patterns should be considered for bioaerosol sampling as well.

• 한국자동차공학회논문집
• /
• 제22권5호
• /
• pp.20-28
• /
• 2014

The high velocity oxygen fuel spraying (HVOF) is a kind of surface modification process technology to form the sprayed coating layer after spraying the powder to molten or semi-molten state by the ultra-high speed at the high-temperature heat source and conflicting with a substrate. It is desirable to melt completely the thermal spray powder in order to produce the coating layer with an optimal adhesion, however, because a semi-molten powder in a spray process has the low efficiency and become a factor that degrades the mechanical property by the inducement of pore-forming within the coating layer. To improve the wear resistance, corrosion resistance and heat resistance, in this study, the plungers of high-speed and ultra-high pressure reciprocating hydraulic pumps for oil and water used in ironwork are produced with $420J_2$ and the coating layers of plungers are formed by the powders of WC-Co-Cr and WC-Cr-Ni including the high hardness WC. The surface of these plungers is modified by the super-mirror face grinding machine using variable air pressure developed in this laboratory, and then the characteristics of cross-sectional microstructure, and surface roughness and hardness values between no operation and 100 days-operation are examined and made a comparison. The fine tops and bottoms on surface roughness curve of oil-hydraulic pump plunger sprayed by WC-Cr-Ni are molded more and higher than those of water-hydraulic pump sprayed by WC-Co-Cr because the plunger diameter of oil-hydraulic pump is 0.4 times smaller than that of water-hydraulic pump and the pressure of oil-hydraulic pump exerted on the plunger is operated with the 70 bars higher than that of water-hydraulic pump. As a result, it is found that the values of centerline average surface roughness and maximum height for oil-hydraulic pump plunger are bigger than those of water-hydraulic pump plunger.

• 동력기계공학회지
• /
• 제11권2호
• /
• pp.5-11
• /
• 2007

액화천연가스(LNG : Liquified Natural Gas)는 연료로 사용하기 위하여 기화하는 과정을 거치게 되는데 기화하는 방식에는 해수에 의한 기화와 공기에 의한 기화의 두 가지 방식으로 나뉘게 된다. 해수에 의한 기화는 LNG 인수기지에서 대량의 LNG를 NG로 기화하기 위하여 사용하며, 공기에 의한 기화는 LNG 위성기지에서 사용처에 적합한 온도를 얻기 위해서 일반적으로 많이 사용하고 있는 공기식 기화기를 이용하여 기화를 하는 방식을 취하고 있다. LNG가 NG로 기화하는 과정에서 1kg당 200kcal의 냉열을 외부로 방출하고 있으며, 이러한 냉열의 방출로 인하여 공기식 기화기의 표면에 결빙현상을 발생시킨다. 또한 현재 사용하고 있는 기화기는 $2{\sim}3$개의 기화기를 연결하여 사용하고 있어 그 비용의 손실이 크다고 할 수 있다. 그리하여 본 연구는 최근 사용빈도가 증가하고 있는 공기식 기화기에 관한 것으로 작동유체는 실제 LNG와 특성이 비슷한 초저온 액화가스인 $LN_2$를 사용하였다. 이번 연구에 사용된 변수는 다음과 같다. 첫째, 각각의 기화기의 길이를 4000mm, 6000mm, 8000mm으로 하였고 핀의 type을 finless, 4fin, 8fin으로 하여 적용하였다. 두 번째는 봄, 여름, 가을, 겨울철에 따른 기화기의 성능을 알고자 각각의 계절별 온도와 습도를 적용하였다. 마지막으로 계절별 풍속과 실험을 하는 시간 동안의 유량을 알고자 압력을 1 bar로 적용하였다. 그리하여 이번 연구의 목적으로는 각각의 변수를 통하여 실험을 진행 한 후 vaporizer type과 길이에 대한 최적의 성능을 가지는 기화기에 대한 자료를 제시하고자 한다.기성분은 균주에 따른 약간의 차이가 있었으나 경향은 비슷하게 나타났다. 이상의 결과 알코올 발효 균주에 따른 참다래 와인의 이화학적 품질특성에는 큰 차이가 없었으나 고급알코올함량을 비교하였을 때 Sacch. cerevisiae Wine 3이 와인제조에 가장 적합한 것으로 평가되었다.장 낮은 값을 나타내었으며, 홍국의 함유량이 증가할수록 유의적으로 증가하였다. b값은 CSB가 가장 낮은 값을 나타내었으며, 홍국의 함유량이 증가할수록 유의적으로 증가하였다. 물성측정 결과 경도와 응집성은 각 시료들 간의 유의적인 차이가 나타나지 않았다. 탄력성과 부서짐성은 CSB가 가장 낮았으며, 홍국의 함유량이 증가할수록 증가하였다. 점착성은 SDB1이 가장 낮았으며, 홍국의 함유량이 증가할수록 증가하였다. 관능검사 결과 기공의 균일성은 SDB1이 가장 균일한 것으로 나타났으며, 색은 홍국의 함유량이 증가할수록 높게 나타났다. 경도, 탄력성, 단맛 및 신맛 등은 홍국 함유량이 증가할수록 증가하는 것으로 나타났다. 이취는 SDB1이 가장 적게 나는 것으로 나타났으며, 전반적인 기호도는 SDB1이 가장 높았다. 따라서 홍국을 10% 첨가한 sourdough starter를 3일 동안 발효한 후 반죽에 첨가하여 sourdough bread를 제조할 때 품질이 가장 우수한 제품을 얻을 수 있었다.생수와 여러 물질의 혼합용액의 온도가 장에 끼치는 자극에 차이가 있지 않나 추측되며 이에 관한 추후 연구가 요망된다. 총대장통과시간의 단축은 결장 분절 모두에서 줄어들어 나타났으나 좌측결장 통과시간의 감소 및 이로 인한 이 부위의 통과시간 비율의 저하가 가장 주요하였다. 이러한 결과는 차가운 생수 섭취가 주로 결장 근위부를 자극하는 효과를 발휘하는 것이 아닌가

• 마이크로전자및패키징학회지
• /
• 제8권2호
• /
• pp.31-36
• /
• 2001

Plasma Polymerization를 이용하여 Teflon-like 불화 유기 박막을 Si, $SiO_2$, Al, TEOS 위에 증착하였다. Difluoromethane $(CH_2F_2$)에 Ar, $O_2$, 그리고 $CH_4$를 첨가하여 첨가 가스에 따른 불화 유기 박막의 특성을 평가하였다. 각각의 첨가가스에 대하여 압력, 온도, 그리고 첨가가스의 비율을 변화시켜 박막을 증착하여 정접촉각 통한 표면의 친수성 (hydrophilicity)과 소수성(hydrophobicity) 정도를 관찰하였다. Ar을 첨가한 경우 Ar 첨가량과 power의 증가에 따라 정접촉각의 감소를 관찰하였다. 그러나 증착압력이 증가함에 따라 정접촉각이 증가하였다. Ar 첨가시 2 Torr이상의 증착압력에서 분말형태의 초소수성 불화 유기박막을 얻을 수 있었다. $O_2$를 첨가한 경우, $O_2$의 첨가량과 증착압력이 증가함에 따라 정접촉각은 감소하였다. 약 100W까지의 power에서는 정접촉각은 일정하였지만 power의 증가에 따라 정접촉각은 감소하여 200W에서는 천수성표면을 얻을 수 있었다. $CH_4$를 첨가하여 불화유기박막을 증착하였을 경우 $CH_4/CH_2F_2$비율이 5까지 급격한 증가를 나타내었고, 비율이 5이상인 경우에서는 일정한 정접촉각을 나타내었다. 화학기상증착에 의해 제조된 박막보다 plasma polymerization으로 제작된 불화유기박막이 히스테리시스(hysteresis)가 낮은 불화유기박막을 형성하였다.

• 한국식품영양과학회지
• /
• 제2권1호
• /
• pp.55-59
• /
• 1973

닭고기의 가공특성(加工特性)을 알고, 가공방법(加工方法)을 개선(改善)하기 위하여 폐계와 육계(肉鷄)를 각(各) 20수(首)씩을 5군(群)으로 나누어(whole carcass, skinned carcass, debonned carcass, thigh muscle, breast muscle) 마쇄하여 실험(實驗)하였다. 그 결과를 요약(要約)하면 다음과 같다. 1. 폐계와 육계(肉鷄)의 도체률(屠體率)은 각(各) $64.32{\pm}2.11,\;67.96{\pm}1.16$이었고, 흡수증체률(吸水增體率)은 $105.43{\pm}1.9,\;104.13{\pm}0.2$이었다. 2. 화학성분(化學成分)은 육계(肉鷄)가 폐계보다 수분(水分)이 많고, 지방(脂肪)이 다소(多少) 적었다. 시료별(試料別)로는 폐계, 육계(肉鷄) 공(共)히 whole carcass ground meat가 thigh m., breast m보다 수분이 적고 지방과 회분의 많았다. 3. Relative WHC와 water retention은 thigh m. breast m. 과 skinned carcass가 높고, whole carcass가 가장 낮았다. 4. 가열감량률(加熱減量率)은 각군(各群) 모두 온도(溫度)가 상승할수록 높고 whole carcass가 가장 높았다. 5. Relative WHC, water retention과 가열감량률(加熱減量率)은 폐계와 육계(肉鷄) 사이의 유의성(有意性)은 전혀 인정(認定)되지 않았다.

• 한국작물학회지
• /
• 제12권
• /
• pp.31-36
• /
• 1972

조춘 저온기에 혼반용대두(풋콩)을 조기재배하는 경우 다수가능한 재식거리 및 질소질비료 시비적량을 구명하기 위하여 온상내에서 단일처리(1일 11시간)를 하고 오개수준의 재식거리 및 4개수준의 질소시비량(각 구 공히 인산과 가리는 표준시비량 시용)을 조합 적용하였다. 품종은 조생종인 북해일호를 공시하였으며 그 시험 결과를 요약하면 다음과 같다. (1) 일주당 협수, 입수, 및 분지수를 많이 착생시키기 위해서는 재식거리를 50cm$\times$10cm 및 30cm$\times$20cm 등 비교적 넓게 하는 것이 효과적이었으나 단위면적당 꼬투리 및 알맹이의 증수를 위해서는 오히려 평당주수가 월등히 많은 50cm$\times$5cm 및 30cm$\times$10cm 등 재식거리를 좁게 하는 것이 효과적이었다. (2) 단위면적당 꼬투리 및 알맹이의 다수를 위한 질소질비료의 시비적량은 표준시비량만으로 충분하다는 사실을 인정하였다.

• 천문학논총
• /
• 제30권2호
• /
• pp.559-563
• /
• 2015

Monitor of All-sky X-ray Image (MAXI) is a Japanese X-ray all-sky surveyer mounted on the International Space Station (ISS). It has been scanning the whole sky since 2009 during every 92-minute ISS rotation. X-ray transients are quickly found by the real-time nova-search program. As a result, MAXI has issued 133 Astronomer's Telegrams and 44 Gamma-ray burst Coordinated Networks so far. MAXI has discovered six new black holes (BH) in 4.5 years. Long-term behaviors of the MAXI BHs can be classified into two types by their outbursts; a fast-rise exponential-decay type and a fast-rise flat-top one. The slit camera is suitable for accumulating data over a long time. MAXI issued a 37-month catalog containing 500 sources above a ~0.6 mCrab detection limit at 4-10 keV in the region ${\mid}{b}{\mid}$ > $10^{\circ}$. The SSC instrument utilizing an X-ray CCD has detected diffuse soft X-rays extending over a large solid angle, such as the Cygnus super bubble. MAXI/SSC has also detcted a Ne emission line from the rapid soft X-ray nova MAXI J0158-744. The overall shapes of outbursts in Be X-ray binaries (BeXRB) are precisely observed with MAXI/GSC. BeXRB have two kinds of outbursts, a normal outburst and a giant one. The peak dates of the subsequent giant outbursts of A0535+26 repeated with a different period than the orbital one. The Be stellar disk is considered to either have a precession motion or a distorted shape. The long-term behaviors of low-mass X-ray binaries (LMXB) containing weakly magnetized neutron stars are investigated. Transient LMXBs (Aql X-1 and 4U 1608-52) repeated outbursts every 200-1000 days, which is understood by the limit-cycle of hydrogen ionization states in the outer accretion disk. A third state (very dim state) in Aql X-1 and 4U 1608-52 was interpreted as the propeller effect in the unified picture of LMXB. Cir X-1 is a peculiar source in the sense that its long-term behavior is not like typical LMXBs. The luminosity sometimes decreases suddenly at periastron. It might be explained by the stripping of the outer accretion disk by a clumpy stellar wind. MAXI observed 64 large flares from 22 active stars (RS CVns, dMe stars, Argol types, young stellar objects) over 4 years. The total energies are $10^{34}-10^{36}$ erg $s^{-1}$. Since MAXI can measure the spectrum (temperature and emission measure), we can estimate the size of the plasma and the magnetic fields. The size sometimes exceeds the size of the star. The magnetic field is in the range of 10-100 gauss, which is a typical value for solar flares.

• Journal of Periodontal and Implant Science
• /
• 제42권2호
• /
• pp.59-63
• /
• 2012

Purpose: This study evaluated the surface characteristics and bond strength produced using a novel technique for coating hydroxyapatite (HA) onto titanium implants. Methods: HA was coated on the titanium implant surface using a super-high-speed (SHS) blasting method with highly purified HA. The coating was performed at a low temperature, unlike conventional HA coating methods. Coating thickness was measured. The novel HA-coated disc was fabricated. X-ray diffraction analysis was performed directly on the disc to evaluate crystallinity. Four novel HA-coated discs and four resorbable blast medium (RBM) discs were prepared. Their surface roughnesses and areas were measured. Five puretitanium, RBM-treated, and novel HA-coated discs were prepared. Contact angle was measured. Two-way analysis of variance and the post-hoc Scheffe's test were used to analyze differences between the groups, with those with a probability of P<0.05 considered to be statistically significant. To evaluate exfoliation of the coating layer, 7 sites on the mandibles from 7 mongrel dogs were used. Other sites were used for another research project. In total, seven novel HA-coated implants were placed 2 months after extraction of premolars according to the manufacturer's instructions. The dogs were sacrificed 8 weeks after implant surgery. Implants were removed using a ratchet driver. The surface of the retrieved implants was evaluated microscopically. Results: A uniform HA coating layer was formed on the titanium implants with no deformation of the RBM titanium surface microtexture when an SHS blasting method was used. Conclusions: These HA-coated implants exhibited increased roughness, crystallinity, and wettability when compared with RBM implants.