• 한국식품과학회지
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• 제16권2호
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• pp.223-227
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• 1984

$1980{\sim}1982$년의 3년간에 걸쳐 한국산(韓國産) 밀 166품종(品種) (또는 계통(系統))을 공시(供試)하여 단백질(蛋白質) 함량(含量), 침전가(沈澱價), Mixograph 및 제(製)빵적성(適性)을 조사하여 각 특성간의 관계를 검토하였다. 단백질함량(蛋白質含量)과 침전가(沈澱價) 또는 빵부피 및 침전가(沈澱價)와 빵부피는 고도(高度)의 정(正)의 상관(相關)이 있었으며, 이와갚은 현상은 연차간(年次間)의 관계에서도 유사한 경향을 보였다. 단백질(蛋白質) 함량(含量) 및 침전가(沈澱價)와 Mixograph흡수률(吸水率)은 정(正)의 유의관계(有意相關)이 있었으나 반죽시간이나 height와는 일정한 상관(相關)이 없었다. 각 품종(品種)의 반죽시간이나 height는 재배환경(栽培環境)이나 연차(年次)에 따라 변이(變異)가 있었으나 한 품종내(品種內)에서 Mixograph pattern은 환경(環境)이 달라도 품종고유(品種固有)의 모양을 보였다.

• The Korean Journal of Physiology and Pharmacology
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• 제2권3호
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• pp.395-401
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• 1998

We have synthesized new platinum(II) analogs containing 1,2-diaminocyclohexane (dach) as a carrier ligand, 1,3-bis(diphenylphosphino) propane (DPPP) /1,2-bis(diphenylphosphino)ethane (DPPE) as a leaving group and nitrates to improve solubility. In the present study, the cytotoxicity of $[Pt(trans-l-dach)(DPPP)]\;2NO_3$ (KHPC-001) and $[Pt(trans-l-dach)(DPPE)]\;2NO_3$ (KHPC-002) was evaluated and compared on various P-388 cancer cell lines and porcine kidney cell line ($LLC-PK_1$). The new platinum complexes demonstrated high efficacy on P-388 mouse leukemia cell line as well as cisplatin-resistant (P-388/CDDP) and adriamycin-resistant (P-388/ADR) P-388 cell lines. The intracellular platinum content was measured by a flame atomic absorption spectrophotometer (FAAS), and it was comparable to the results of $IC_{50}$ of the three complexes on $LLC-PK_1$ and P-388/S cells, while only DPPE compound was accumulated in high volume in P-388/ADR and P-388/CDDP cells. While the DNA-interstrand cross-links of KHPC-001, KHPC-002 and cisplatin were similar on P-388/S leukemia cells, these new platinum complexes were much less DNA cross-linking to a kidney derived cell line, $LLC-PK_1$. These results indicate that KHPC-001 and KHPC-002 are a third-generation platinum complexes with potent antitumor activity and low nephrotoxicity.

• 복식문화연구
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• 제30권6호
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• pp.880-897
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• 2022

The purpose of this study is to apply the traditional Chinese fretwork on the 'Faux Chenille' textile work method in a way of enhancing the decorative features of patterns and developing the fashion design. As for the method, it works on the historic background and advancement of the fretwork and it refers to the bibliographies pertinent to the traditional Chinese geometric pattern. The result are as follows. First, pure cotton and 100% rayon are mixed to make it feasible to produce the texture for the material to be tender and enhanced, and in the process of washing and drying the Faux Chenille textile. The Faux Chenille textile is an important material that is required to select materials with great absorption capability as the most effective material to re-visualize the lines and patterns by sustaining the diagonal lines. Second, the fretwork is designed to process the basic formation for 90° angle with the sense of unlimited extensive line and changes with straight line. It has been confirmed that, if the angle that controls the Faux Chenille textile and the tailoring interval are well aligned, the expression of traditional geometric pattern would be effective and it may be expressed in contemporary style. Third, through the fashion design application by utilizing the Faux Chenille textile of the fretwork, it is confirmed that the contemporary application of the traditional culture could be expressed uniquely and creatively while it is affirmed that the western technique and Asian culture can be blended in harmony.

• 천문학회보
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• 제46권1호
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• pp.50.2-51
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• 2021

Stars form exclusively in cold and dense molecular clouds. To fully understand star formation processes, it is hence a key to investigate how molecular clouds form out of the surrounding diffuse atomic gas. With an aim of shedding light in the process of the atomic-to-molecular transition in the interstellar medium, we analyze Arecibo HI emission and absorption spectral pairs along with TRAO/PMO 12CO(1-0) emission spectra toward 58 lines of sight probing in and around molecular clouds in the solar neighborhood, i.e., Perseus, Taurus, and California. 12CO(1-0) is detected from 19 out of 58 lines of sight, and we report the physical properties of HI (e.g., central velocity, spin temperature, and column density) in the vicinity of CO. Our preliminary results show that the velocity difference between the cold HI (Cold Neutral Medium or CNM) and CO (median ~ 0.7 km/s) is on average more than a factor of two smaller than the velocity difference between the warm HI (Warm Neutral Medium or WNM) and CO (median ~ 1.7 km/s). In addition, we find that the CNM tends to become colder (median spin temperature ~ 43 K) and abundant (median CNM fraction ~ 0.55) as it gets closer to CO. These results hints at the evolution of the CNM in the vicinity of CO, implying a close association between the CNM and molecular gas. Finally, in order to examine the role of HI in the formation of molecular gas, we compare the observed CNM properties to the theoretical model by Bialy & Sternberg (2016), where the HI column density for the HI-to-H2 transition point is predicted as a function of density, metallicity, and UV radiation field. Our comparison shows that while the model reproduces the observations reasonably well on average, the observed CNM components with high column densities are much denser than the model prediction. Several sources of this discrepancy, e.g., missing physical and chemical ingredients in the model such as the multi-phase ISM, non-equilibrium chemistry, and turbulence, will be discussed.

• 한국광학회지
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• 제19권1호
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• pp.54-59
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• 2008

적외선 영역에서 극초단 펄스 폭을 갖는 $Cr^{4+}$:YAG 레이저를 광자 결정 광섬유에 입사하여 초 연속 스펙트럼을 갖는 광원을 얻어냈다. 이 광원을 이용하여 광통신 파장 영역에서 많은 흡수 전이선을 갖는 아세틸렌($^{12}C_2H_2$) 및 시안화 수소($H^{13}C^{14}N$) 분자의 흡수 스펙트럼을 측정하였다. 초 연속 스펙트럼을 얻기 위해 펌핑 광원으로 모드 잠금된 $Cr^{4+}$:YAG 레이저를 사용하였다. 모드 잠금된 $Cr^{4+}$:YAG 레이저는 중심파장이 1510 nm 대역에서 반복률이 100 MHz이고, 펄스폭은 75 fs이다. 모드 잠금된 $Cr^{4+}$:YAG 레이저 출력을 20 m의 광자 결정 광섬유에 집속시켜 진폭변동이 ${\pm}5dB$이하에서 400 nm 이상의 평탄한 초 연속 스펙트럼을 얻었으며, 전체적으로 한 octave 이상의 초 광대역 광원을 얻었다. 이 광원을 이용하여 50개 이상의 흡수 전이선을 갖는 아세틸렌 분자($^{12}C_2H_2$)와 시안화 수소 분자($H^{13}C^{14}N$)의 흡수 스펙트럼을 측정하고, Voigt 곡선 맞춤을 이용하여 Lorentian 성분의 흡수 선폭을 각각 측정하였다. 이와 같은 초 광대역 광원의 스펙트럼을 이용하면 O, S, C, L 밴드와 같은 대역에 존재하는 분자의 흡수 스펙트럼 측정에 있어 유용하게 사용될 수 있다.

• 식물조직배양학회지
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• 제24권6호
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• pp.361-367
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• 1997

담배(Nicotiana tabacum cv. BY4)의 이배체식물과 담배의 약으로부터 유도된 반수체식물의 잎절편을 사용하여 2.4-D를 단독톄처리하여 캘러스를 유도하였다. 캘러스증식은 이배체에서는 2.0 mg/L 2.4-D와 1.0mg/L 카이네틴의 조합처리구에서, 반수체의 경우에 있어서는 2.0mg/L 2.4-D와 0.1mg/L BAP 조합처리구에서 실시하였으며, 현탁배양도 동일조건으로 실시하였다. 현탁배양 세포괴를 배양 15-20일째가 되면 0.8% low melting agarose와 혼합하여 카드a뮴이 0-2,000 $\mu$M의 농도로 처리된 선발배지에 평판배양하여 카드뮴저항성 colony(cell clump)를 조사관찰하였다. 그 결과 본 실험에서는 이배체는 세포의 성장에 있어서 최하저해농도(MIC : Minimum Inhibition Concentration)는 Cd$^{++}$ 300 $\mu$M이었으며 반수체는 Cd$^{++}$ 200 $\mu$M이었다. 이때 반수체 및 이배체의 MIC에서 선발된 세포주를 카드뮴 500, 1,000, 2,000 $\mu$M 농도로 옳겨 경화시킨 후 카드뮴저항성을 선발하였고 그 특성을 조사하였다. 그 결과 카드뮴 저항성을 띤 반수체 및 이배체유래 캘러스의 경우에는 각각 카드a뮴의 농도가 증가할수록 생중량은 감소하였으나, 건조중량은 오히려 증가하였다. 그리고 각각 선발된 세포주내의 카드뮴의 함량을 AAS를 사용하여 측정하였던 바, 카드뮴의 농도가 높을수록 캘러스에 축적된 카드뮴의 양이 높게 나타났다.

• Macromolecular Research
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• 제17권10호
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• pp.791-796
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• 2009

An electrochemically and photochemically polymerizable monomer, 2-((2,3-dihydrothieno[3,4-b] [1,4]dioxin-2-yl)methoxy)ethyl methacrylate (EDOT-EMA), was explored for patterning of poly(3,4-ethylenedioxythiophene) (PEDOT) via side chain cross-linking. The polymer from EDOT-EMA was deposited electrochemically to produce polymeric EDOT (PEDOT-EMA), which was directly photo-patterned by UV light as the side EMA groups of PEDOT-EMA were polymerized to give cross-linked EMA (PEDOT-PEMA). Absorption and FTIR studies of the UV-exposed film (PEDOT-PEMA) indicated that the photo-patterning mainly originated from the photo cross-linking of the methacrylates in the side-chain. After irradiation of the film, the conductivity of the irradiated area decreased from $5.6{\times}10^{-3}$ S/cm to $7.2{\times}10^{-4}$ S/cm, possibly due to bending of the conductive PEDOT channel as a result of the side chain cross-linking. The patterned film was applied to a solid state electrochromic (EC) cell to obtain micro-patterned EC cells with lines up to 5 ${\mu}m$ wide.

• 천문학논총
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• 제27권4호
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• pp.177-179
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• 2012

We present Spitzer IRS spectroscopy of $CO_2$ ice toward 19 young stellar objects (YSOs) with luminosity lower than $1L_{\odot}$. Pure $CO_2$ ice forms only at elevated temperatures, T > 20 K, and thus at higher luminosities. Current internal luminosities of YSOs with L < $1L_{\odot}$ do not provide such conditions out to radii of typical envelopes. Significant amounts of pure $CO_2$ ice would signify a higher past luminosity. We analyze $15.2{\mu}m$ $CO_2$ ice bending mode absorption lines in comparison to the laboratory data. We decompose pure $CO_2$ ice from 12 out of 19 young low luminosity sources. The presence of the pure $CO_2$ ice component indicates high dust temperature and hence high luminosity in the past. The sum of all the ice components (total $CO_2$ ice amount) can be explained by a long period of low luminosity stage between episodic accretion bursts as predicted in an episodic accretion scenario. Chemical modeling shows that the episodic accretion scenario explains the observed total $CO_2$ ice amount best.

• Bulletin of the Korean Chemical Society
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• 제31권2호
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• pp.315-326
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• 2010

This study examined the overlapping resonances in the systems involving 1 open and 2 closed channels using the phase-shifted version of multichannel quantum-defect theory (MQDT). The results showed that 21 patterns for the q reversals in the autoionization spectra are possible depending on the relative arrangements of the two simple poles and roots of the quadratic equations. Complete cases could be generated easily using the q zero planes determined using only 3 asymmetric spectral line profile indices. The transition of the spectra of the coarse interloper Rydberg series from the lines into a structured continuum by being dispersed onto the entire Rydberg series was found. The overall behavior of the time delays was found to be governed by the dense Rydberg series, which is quite different from the one of the autoionization cross sections that is governed by an interloper, indicating that different dynamics prevail for them. This is in contrast to the two channel system where both quantities behave similarly. The dynamics obtained in the presence of overlapping resonances is as follows. The absorption process is instant and dominated by a transition to the interloper line. This process is followed by rapid leakage into the dense Rydberg series, which has a longer residence time before ionization than that of the interloper state. This is because the orbiting period is proportional to $\upsilon^3$ so that an excited electron has a shorter lifetime in the interloper state belonging to a lower member of the Rydberg series.

• 천문학회지
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• 제27권1호
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• pp.31-44
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• 1994

The 4.8GHz formaldehyde absorption line in the dark clouds in M17 and NGC 2024 regions has been mapped. In both nebulae, we detected two $H_2CO$ line components. In M17, the 24km $S^{-1}$ cloud is closely associated with the HII region located in front of the radio continuum source, and the 19km $S^{-1}$ cloud is associated with the visual dark clouds with a larger extent which are closer to us. The 19km $S^{-1}$ cloud has a mass motion approaching to the HII region. In both clouds, a velocity gradient from the north-east to the south-west directions is observed. The linewidth has no variation indicating no collapsing motion. In NGC 2024, the 9km $S^{-1}$ feature is extended along the dark bar in front of the bright nebula and a weak second component at 13km $S^{-1}$ is confined to the immediate vicinity of the radio source. Indications are that the 9km $S^{-1}$ cloud is physically associated with the dark bar and the 13km $S^{-1}$ cloud is located behind the radio source. The angular extent, the column density, and the total mass of the clouds are derived. The radial velocities of other molecular lines observed in these clouds are compared.