• 천문학회지
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• 제35권4호
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• pp.159-174
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• 2002

Cosmological hydrodynamic simulations of large scale structure in the universe have shown that accretion shocks and merger shocks form due to flow motions associated with the gravitational collapse of nonlinear structures. Estimated speed and curvature radius of these shocks could be as large as a few 1000 km/s and several Mpc, respectively. According to the diffusive shock acceleration theory, populations of cosmic-ray particles can be injected and accelerated to very high energy by astrophysical shocks in tenuous plasmas. In order to explore the cosmic ray acceleration at the cosmic shocks, we have performed nonlinear numerical simulations of cosmic ray (CR) modified shocks with the newly developed CRASH (Cosmic Ray Amr SHock) numerical code. We adopted the Bohm diffusion model for CRs, based on the hypothesis that strong Alfven waves are self-generated by streaming CRs. The shock formation simulation includes a plasma-physics-based 'injection' model that transfers a small proportion of the thermal proton flux through the shock into low energy CRs for acceleration there. We found that, for strong accretion shocks, CRs can absorb most of shock kinetic energy and the accretion shock speed is reduced up to $20\%$, compared to pure gas dynamic shocks. For merger shocks with small Mach numbers, however, the energy transfer to CRs is only about $10-20\%$ with an associated CR particle fraction of $10^{-3}$. Nonlinear feedback due to the CR pressure is insignificant in the latter shocks. Although detailed results depend on models for the particle diffusion and injection, these calculations show that cosmic shocks in large scale structure could provide acceleration sites of extragalactic cosmic rays of the highest energy.

• 대한화학회지
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• 제18권3호
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• pp.180-188
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• 1974

Layer silicate 에 지지된 陽이온상에서의 일어난 acetaldehyde, acrolein, 그리고 crotonaldehyde의 吸着機構에 對하여 IR과 X-ray로서 硏究하였다. $1720∼1580㎝^{-1}$의 범위에서 일어난 4個의 특성적인 吸捉 band를 分析한 結果 $130㎝^{-1}$程度로 shift한 carbonyl band 는 >C=O${\cdots}$M형 complex 形成에 基因하는 것이었고, acetaldehyde는 $1722㎝^{-1}$에서, 다른 알데히드는 $1690㎝^{-1}$에서 sharp하게 나타난 carbonyl band는 >C=O와 surface -O-H와의 interaction에서 일어난 것이었다. 그리고 1710∼1660㎝-1에서 나타난 broad한 band는 >C=O와 陽이온 -O-H와의 사이에 일어난 水素結合에 依한 것이었다. 그리고 $1640∼1660㎝^{-1}$사이에 나타난 弱한 band는 carbonyl group 의 强한 吸着에 依하여 誤起된 >C=C< 二重結合에 依한 것이었다. 이 사실들은 X-ray 廻折에 依하여 다시 確認하였다.

• Bulletin of the Korean Chemical Society
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• 제21권6호
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• pp.588-594
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• 2000

Structural changes of an iron phthalocyanine (FePC) monolayer induced by adsorption and externally applied potential on high area carbon surface have been investigated in situ by iron K-edge X-ray absorption fine structure (XAFS) in 0.5 M $H_2S0_4.$ Fine structures shown in the X-ray absorption near edge structure (XANES) for microcrystalline FePC decreased upon adsorption and further diminished under electrochemical conditions. Fe(II)PC(-2) showed a 1s ${\rightarrow}$ 4p transition as poorly resolved shoulder to the main absorption edge rather than a distinct peak and a weak 1s ${\rightarrow}$ 3d transition. The absorption edge position measured at half maximum was shifted from 7121.8 eV for Fe(lI)PC(-2) to 7124.8 eV for $[Fe(III)PC(-2)]^+$ as well as the 1s ${\rightarrow}$ 3d pre-edge peak being slightly enhanced. However, essentially no absorption edge shift was observed by the 1-electron reduction of Fe(Il)PC(-2), indicating that the species formed is $[Fe(II)PC(-3)]^-$. Structural parameters were obtained by analyzing extended X-ray absorption fine structure (EXAFS) oscillations with theoretical phases and amplitudes calculated from FEFF 6.01 using multiple-scattering theory. When applied to the powder FePC, the average iron-to-phthalocyanine nitrogen distance, d(Fe-$N_p$) and the coordination number were found to be 1.933 $\AA$ and 3.2, respectively, and these values are the same, within experimental error, as those reported ( $1.927\AA$ and 4). Virtually no structural changes were found upon adsorption except for the increased Debye-Wailer factor of $0.005\AA^2$ from $0.003\AA^2.$ Oxidation of Fe(II)PC(-2) to $[Fe(III)PC(-2)]^+$ yielded an increased d(Fe-Np) (1 $.98\AA)$ and Debye-Wailer factor $(0.005\AA^2).$ The formation of $[Fe(II)PC(-3)]^-$, however, produced a shorter d(Fe-$N_p$) of $1.91\AA$ the same as that of crystalline FePC within experimental error, and about the same DebyeWaller $factor(0.006\AA^2)$.

• 미술이론과 현장
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• 제7호
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• pp.165-188
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• 2009

In the development of linear perspective, Brook Taylor's theory has achieved a special position. With his method described in Linear Perspective(1715) and New Principles of Linear Perspective(1719), the subject of linear perspective became a generalized and abstract theory rather than a practical method for painters. He is known to be the first who used the term 'vanishing point'. Although a similar concept has been used form the early stage of Renaissance linear perspective, he developed a new method of British perspective technique of measure points based on the concept of 'vanishing points'. In the 15th and 16th century linear perspective, pictorial space is considered as independent space detached from the outer world. Albertian method of linear perspective is to construct a pavement on the picture in accordance with the centric point where the centric ray of the visual pyramid strikes the picture plane. Comparison to this traditional method, Taylor established the concent of a vanishing point (and a vanishing line), namely, the point (and the line) where a line (and a plane) through the eye point parallel to the considered line (and the plane) meets the picture plane. In the traditional situation like in Albertian method, the picture plane was assumed to be vertical and the center of the picture usually corresponded with the vanishing point. On the other hand, Taylor emphasized the role of vanishing points, and as a result, his method entered the domain of projective geometry rather than Euclidean geometry. For Taylor's theory was highly abstract and difficult to apply for the practitioners, there appeared many perspective treatises based on his theory in England since 1740s. Joshua Kirby's Dr. Brook Taylor's Method of Perspective Made Easy, Both in Theory and Practice(1754) was one of the most popular treatises among these posterior writings. As a well-known painter of the 18th century English society and perspective professor of the St. Martin's Lane Academy, Kirby tried to bridge the gap between the practice of the artists and the mathematical theory of Taylor. Trying to ease the common readers into Taylor's method, Kirby somehow abbreviated and even omitted several crucial parts of Taylor's ideas, especially concerning to the inverse problems of perspective projection. Taylor's theory and Kirby's handbook reveal us that the development of linear perspective in European society entered a transitional phase in the 18th century. In the European tradition, linear perspective means a representational system to indicated the three-dimensional nature of space and the image of objects on the two-dimensional surface, using the central projection method. However, Taylor and following scholars converted linear perspective as a complete mathematical and abstract theory. Such a development was also due to concern and interest of contemporary artists toward new visions of infinite space and kaleidoscopic phenomena of visual perception.

• 한국지구물리탐사학회:학술대회논문집
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• 한국지구물리탐사학회 2009년도 학술대회 초록집
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• pp.167-173
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• 2009

2009년 국립해양조사원은 백령도 부근 해역에 대해 바다로 1호에 장착된 Simrad EM3000 다중빔 음향측심기를 이용한 수심측량조사를 실시하였으며 정확한 음속보정을 위해 1일 $7{\sim}10$회 이상의 음속을 관측하였다. 백령도 주변해역은 계절에 따라 여러 질 수괴(쿠로시오 난류, 황해 연안수 등)가 복잡하게 분포하여 여러 형태의 수온 전선이 형성되어 수층 음속 깊이가 최대 10m/s 이상의 차이를 나타냈다. 또한 난수괴 유입으로 인해 수온약층의 깊이가 지역별로 다르게 분포 하였다. 이러한 음속의 국지적 변화는 다중빔을 이용한 수심측량 자료의 정확도를 저하시키는 요인으로 작용한다. 따라서 다중빔을 이용한 수심측량 자료의 정확도를 저하시키는 요인으로 작용한다. 따라서 백령도 주변해역 수심측량 자료의 수평 수직 변화를 음선추적 이론을 이용하여 확인하였다.

• Bulletin of the Korean Chemical Society
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• 제35권8호
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• pp.2311-2316
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• 2014

Conformations and vibrational frequencies of the racemic (2RS,3RS)-5-amino-3-(4-phenylpiperazin-1-yl)-1,2,3,4-tetrahydronaphthalen-2-ol-(I) [(2RS,3RS)-(I)], a precursor of benzovesamicol analogues, have been carried out using various DFT methods (M06-2X, B3LYP, B3PW91, PBEPBE, LSDA, and B3P86) with basis sets of 6-31G(d), 6-31+G(d,p), 6-311+G(d,p), 6-311++G(d,p), cc-pVTZ, and TZVP. The LSDA/6-31G(d) level of theory shows the best performance in reproducing the X-ray powder structure. However, the PBEPBE/cc-pVTZ level of theory is the best method to predict the vibrational frequencies of (2RS,3RS)-(I). The potential energy surfaces of racemic pairs (2RS,3RS)-(I) and -(II) are obtained at the LSDA/6-31G(d) level of theory in the gas phase and in water. The results indicate that (2RS,3RS)-(I) are more stable by ~0.75 kcal/mol in energy than (2RS,3RS)-(II) in water, whereas conformer AIIg and BIIg are more stable by ~0.04 kcal/mol than AIg in gas phase. In particular, the hydrogen bond distances between the N of piperazine and the OH of tetrahydronaphthalen become longer in gas, compared with those in the water phase. Vibrational frequencies calculated at the PBEPBE/cc-pVTZ level of theory in the gas phase are larger than those in water, whereas their intensities in the gas phase are weaker than those in water.

• 한국음향학회지
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• 제21권8호
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• pp.679-685
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• 2002

천해에서의 저주파 단상태 잔향음 모델 (L-HYREV: Low-frequency Hanyang univ. Reverberation model)을 개발하였다. 음선이론 (ray-theory)에 기초한 전파모델은 해저 내로 투과되는 음파에 대한 효과를 적절하게 고려할 수 없으므로, 해저 내 상호작용을 계산할 수 있는 전파모델이 필요하다. 따라서 본 논문에서는 RAM(Range dependent Acoustic Model)을 이용해서 전달손실을 계산 후, 다중경로 확장모델 (multi-path expansion model)을 이용해서 산출한 전달손실을 보정하였다. 모델의 검증을 위하여 GSM (generic sonar model) 잔향음 모의 신호 및 실측 잔향음 신호와 비교하였으며, 비교 결과 GSM보다 L-HYREV 모델이 저주파 잔향음 예측에 적합함을 확인할 수 있다.

• 통합자연과학논문집
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• 제8권1호
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• pp.19-29
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• 2015

In view of the growing medicinal importance of chromene and its derivatives, the single crystal X-ray diffraction study was carried out for the potential active 4,6-dimethyl-9-phenyl-8,12-dioxa-4,6-diazatetracyclo [8.8.0.02,7.013,18]octadeca-2(7),13,15,17-tetraene-3,5,11-trione-2-ethoxyphenyl (2E)-but-2-enoate ($C_{18}H_{20}N_2O_5$). In the title compound are two molecules exist in the asymmetric unit. It crystallizes in the monoclinic space group $P2_1/c$ with unit cell dimension a=14.608(3) ${\AA}$, b=12.845(3) and c= 17.781(4) [alpha & gamma=$90^{\circ}$ beta=$91.233(5)^{\circ}$]. Both pyran and pyran ring of the chromene moiety adopts sofa conformation in the molecule A & B. The crystal structure is stabilized by intramolecular C-H...O hydrogen bond interaction.

• 한국자기학회지
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• 제18권2호
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• pp.63-66
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• 2008

초상자성 코발트 페라이트 나노입자를 제조하여 자화 및 자기엔트로피 변화를 조사하였다. 제조된 시료는 전형적인 입방 스피넬 구조를 띠고 있었다. 5K와 300K에서의 최대 자화는 덩어리 상태에서의 최대 자화보다 작은 값을 가졌다. 시료의 초상자성적 거동은 M vs. H/T 곡선의 겹침에 의해 확인되었다. 열역학적 이론을 바탕으로 자기엔트로피의 변화에 대한 온도 의존성을 도출한 결과, 온도가 높을수록 자기엔트로피의 변화는 더 크게 감소하는 것으로 나타났다.

• Journal of Astronomy and Space Sciences
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• 제19권1호
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• pp.1-6
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• 2002

Recently, one interesting possibility is proposed that a magnetar can be a progenitor of short and hard gamma-ray bursts (GRBs). If this is true, one may expect that the short and hard GRBs, at least some of GRBs in this class, are distributed in the Euclidean space and that the angular position of these GRBs is correlated with galaxy clusters. Even though it is reported that the correlation is statistically marginal, the observed value of < $V/V_{max}$ > deviates from the Euclidean value. The latter fact is often used as evidence against a local extragalactic origin for short GRB class. We demonstrate that GRB sample of which the value of < $V/V_{max}$ > deviates from the Euclidean value can be spatially confined within the low value of z. We select very short bursts (TgO < 0.3 sec) from the BATSE 4B catalog. The value of < $V/V_{max}$ > of the short bursts is 0.4459. Considering a conic-beam and a cylindrical beam for the luminosity function, we deduce the corresponding spatial distribution of the GRB sources. We also calculate the fraction of bursts whose redshifts are larger than a certain redshift z', i.e. f>z'. We find that GRBs may be distributed near to us, despite the non-Euclidean value of < $V/V_{max}$ >. A broad and uniform beam pattern seems compatible with the magnetar model in that the magnetar model requires a small $z_{max}$.