• Journal of the Korean Chemical Society
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• v.54 no.1
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• pp.71-76
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• 2010

The densities and viscosities of 2-bromopropane-methanol binary mixtures had been determined using an digital vibrating U-tube densimeter and Ubbelohde capillary viscometer respectively from (298.15 to 318.15) K. The dependence of densities and viscosities on temperature and concentration had been correlated. The excess molar volume and the excess viscosity of the binary system were calculated from the experimental density and viscosity data. The excess molar volumes were related to compositions by polynomial regression and regression parameters and total RMSD deviations were obtained; the excess viscosities was related to compositions by Redlich-Kister equation and regression coefficients and total RMSD deviation of the excess viscosity for 2-bromopropane and methanol binary system were obtained. The results showed that the model agreed very well with the experimental data.

• Journal of Conservation Science
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• v.1 no.1 s.1
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• pp.27-39
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• 1992

Metallurgical studies of the bronze artifacts excavated from Miruksa Temple were performed by chemical analysis and metallographic observation. Alloy systems of the bronze artifacts were classified into two groups of Cu-Sn and Cu-Sn-Pb, according to the items. The contents of impurities such as Sb, As, Ni and Fe in bronze artifacts are within the limiting range of the mod ern standard bronze castings. Chemical compositions of the kitchen utensils such as bronze vessels and dishes in the Unified Silla dynasty, are in the follow ing range, Cu : 74.8-79.4% and Sn : 18.6-21.1%. Chemical composition of the Buddha-image in Koryo dynasty are 820Cu-7.0Sn-10.3Pb, showing increased Pb content and decreased Sn content. The results of chemical analysis suggest that the chemical compositions were good controlled. Any casting defects such as voids and shrinkage holes are not found microscopically, indicating high casting skill. Zinc atoms are not contained in the all bronze artifacts of Miruksa Temple site. This is the common facts founded in the east asian bronze artifacts of Korea, China and Japan. It is comparable with the European bronze of Cu-Sn-Pb-Zn system, after the Middle Age.

• Proceedings of the KWS Conference
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• 1997.05a
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• pp.157-158
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• 1997

• 한국기계연구소 소보
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• s.13
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• pp.45-52
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• 1984

• Korean Journal of Materials Research
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• v.5 no.8
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• pp.1013-1019
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• 1995

The thin plate of Co-Ni-P was deposited on the polyester film by the electroless plating method. Through present experiments, deposition rates and metal compositions of the plates were determined according to compositions of solution, pH and temperature. Also, magnetic properties of plates were examined according to metal compositions. Considering magnetic properties and deposition rates of electroless plating, the best condition was obtained as pH of 8.5 and 90℃. It was observed that metal compositions were evidently varied by the pH of solutions and the concentration of complex agents. However. they were not affected by other factors. At the optimum condition, the composition of the plate was Co(78%), Ni(16%), and P(6%). Also, it was found that the coercive force was 370 Oe, and squareness was 0.65 at this condition. Magnetic properties (hard or soft) of thin plates were determined by metal compositions. Therefore. the plate became soft magnetic plate as the composition of nickel increased over 30 per cents. The crystal structure of the soft magnetic plate was found to be amorphous in which it was strongly oriented to the (111)phahe of nickel. On the ohter hand, the hard magnetic place was found to be hcp crystalline of α-cobalt which was oriented to the (101)phase of cobalt and the (100)phase of cobalt.

• Korean Journal of Food Science and Technology
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• v.29 no.4
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• pp.657-662
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• 1997

An attempt was made to investigate the chemical compositions of green pumpkin, edible flesh and seed of ripened pumpkin (Cucurbita moschata Duch.). The proximate compositions were moisture 9.34%, 11.98%, protein 12.70%, 13.38%, lipid 11.31%, 0.85%, carbohydrate 64.32%, 62.18%, fiber 6.31%, 4.54% and ash 6.05%, 7.76% in green and ripened pumpkin, respectively. The compositions of free sugar were glucose, fructose, sucrose, lactose and maltose in green and ripened pumpkin, respectively. During flesh growth, glucose, maltose and lactose was increased but sucrose and fructose was decreased in pumpkin. Pattern of 15 amino acid compositions in green and ripened pumpkin was shown to be of similarity. Major amino acids were glutamic acid, aspartic acid and alanine in green pumpkin and edible flesh of ripened pumpkin. And major amino acid in seed of ripened pumpkin were glutamic acid, arginine, aspartic acid and leucine. The predominant fatty acids were palmitic acid, linolenic acid, linoleic acid and oleic acid in green and ripened pumpkin, respectively. And those in seed of ripened pumpkin were linoleic acid, palmitic acid and oleic acid. The richest mineral contained in the green and ripened pumpkin was shown to be K and followed by Ca, Mg, Na and Fe in order.

• Journal of the Mineralogical Society of Korea
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• v.13 no.3
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• pp.147-163
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• 2000

The mineralogy and chemical composition of reddish to brownish yellow residual soils, so called "Hwangto" have been examined according to representative host rocks. The result of the study indicates that Hwangto consists of 40-80% clay minerals and various minerals such as quartz, feldspar, hornblende, goethite, and gibbsite. Clay minerals include kaolinite, halloysite, illite, hydroxy interlayered vermiculite (HIV), mica/vermiculite interstratifield mineral and chlorite. The mineralogical constituents and contents of Hwangto were different depending on the types of host rocks. Moreover, the Jurassic granitic rocks contain relatively more kaolin minerals, whereas the Cretaceous granitic rocks contain more HIV and illite. In addition, reddish Hwangto contains relatively more kaolinite and HIV, and yellowish Hwangto contains more illite and halloysite. It is suggested that feldspars and micas of host rocks were chemically weathered into illite, halloysite, illite/vermiculite interstratified minerals, and HIV, and finally into kaolinite. Compared with their host rocks, the major chemical compositions of Hwangto tend to contain more $Al_2O_3,\;Fe_2O_3,\;H_2O$ in amount and less Ca, Mg, and Na. Hwangto contains relatively high amount of trace elements, P, S, Zr, Sr, Ba, Rb, and Ce including considerable amount of Li, V, Cr, Zn, Co, Ni, Cu, Y, Nb, La, Nd, Pb, Th in excess of 10 ppm. Relatively high amount of most trace elements were detected in the Hwangto. The major and minor chemical compositions of the Hwangto were different depending on the types of host rocks. However, their difference was in the similar range compared with the compositions of host rocks.

• Journal of Conservation Science
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• v.32 no.1
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• pp.63-73
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• 2016

This study defined material and characteristics of 24 glass fragments and 26 whole glass beads. The feature of glass beads shape are divided into 5 types following color, size, weathering condition and manufacturing techniques. Through the chemical composition, the first and second type is soda glass, the third type is potash glass, the fourth and fifth type is lead barium glass. This site showed the aspect that the chemical composition is changed according to the feature of glass shape and was found that various chemical compositions. Looking at the flow of glass culture, the tomb that are lead barium glass IItype and potash glass I, IItype is relatively preceding period and the tomb that are soda glass and lead barium glass IIItype is following period.

• Journal of the Korean Society of Food Science and Nutrition
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• v.30 no.4
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• pp.717-720
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• 2001

Chemical compositions and physiological activities of Platycodon grandiflorum roots grown for 4 and 24 years were investigated. Chemical compositions of P. grandiflorum roots grown for 24 years were moisture 82.7%, crude protein 1.6%, crude lipid 2.1% crude ash 0.7%. total sugar 6.0% total dietary fiber 2.3% crude saponin 3.4mg% and ascorbic acid 3.0 mg%. Contents of each components in 24 years old roots were higher than that in 4 years old roots and the most abundant mineral was potassium being 879.9mg/kg. Physiological activities of solvent extract from P. grandiflorum roots grown for 4 and 24 years were high in order of ethanol methanol and water extract. The electron-donating abilities and nitrite-scavenging effect of solvent extract of 24 years were high in order of ethanol methanol and water extract. The electron-donating abilities and nitrite-scavenging effect of solvent extract of 24 years old roots were higher than those of 4 years of old roots in the range of 10~40% respectively.

• The Bulletin of The Korean Astronomical Society
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• v.46 no.2
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• pp.66.3-67
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• 2021

Low-mass stars form by the gravitational collapse of dense molecular cores. Observations and theories of low-mass protostars both suggest that accretion bursts happen in timescales of ~100 years with high accretion rates, so called episodic accretion. One mechanism that triggers accretion bursts is infalling fragments from the outer disk. Such fragmentation happens when the disk is massive enough, preferentially activated during the embedded phase of star formation (Class 0 and I). Most observations and models focus on the gas structure of the protostars undergoing episodic accretion. However, the dust and ice composition are poorly understood, but crucial to the chemical evolution through thermal and energetic processing via accretion burst. During the burst phase, the surrounding material is heated up, and the chemical compositions of gas and ice in the disk and envelope are altered by sublimation of icy molecules from grain surfaces. Such alterations leave imprints in the ice composition even when the temperature returns to the pre-burst level. Thus, chemical compositions of gas and ice retain the history of past bursts. Infrared spectral observations of the Spitzer and AKARI revealed a signature caused by substantial heating, toward many embedded protostars at the quiescent phase. We present the AKARI IRC 2.5-5.0 ㎛ spectra for embedded protostars to trace down the characteristics of accretion burst across the evolutionary stages. The ice compositions obtained from the absorption features therein are used as a clock to measure the timescale after the burst event, comparing the analyses of the gas component that traced the burst frequency using the different refreeze-out timescales. We discuss ice abundances, whose chemical change has been carved in the icy mantle, during the different timescales after the burst ends.