• Bulletin of the Korean Chemical Society
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• v.33 no.7
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• pp.2341-2344
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• 2012

A molecular orbital study is presented of the magnetic coupling in the one-dimensional vanadium oxide $Ba_2V_3O_9$ with a bridge formed by two different types of $VO_4$ tetrahedra. The concept of complementary versus counter-complementary effect has been used to explain the structural origin of the magnetic behavior of the compound. Namely, the observed antiferromagnetic coupling is dominated by the orbital complementarity of the V(1) tetrahedra sharing only one oxygen corner with two adjacent $VO_6$ octahedra. The second type of V(2) tetrahedra does not provide a noticeable contribution to the magnetic coupling due to the orbital counter-complementarity of the bridging ligand.

• Journal of the Korean Society of Propulsion Engineers
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• v.9 no.3
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• pp.145-152
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• 2005

Worldwide there is strong interest in the field of commercial space business, especially 100km altitude sub-orbital Space Tourism. This was soared to by the two-times flight success of SpaceShipOne by Scaled Composites Inc. It reached an altitude of 100km at Oct. 4, 2004. This demonstrates a paradigm change from government-driven space challenge and exploration to commercial space business. Therefore this report provides various insights into the commercial space tourism market, such as current demand for space travel, size of the market, growth potential of the market, technology, etc.

• Journal of Astronomy and Space Sciences
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• v.28 no.1
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• pp.37-54
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• 2011

Two semi-analytic solutions for a perturbed two-body problem known as Lagrange planetary equations (LPE) were compared to a numerical integration of the equation of motion with same perturbation force. To avoid the critical conditions inherited from the configuration of LPE, non-singular orbital elements (EOE) had been introduced. In this study, two types of orbital elements, classical Keplerian orbital elements (COE) and EOE were used for the solution of the LPE. The effectiveness of EOE and the discrepancy between EOE and COE were investigated by using several near critical conditions. The near one revolution, one day, and seven days evolutions of each orbital element described in LPE with COE and EOE were analyzed by comparing it with the directly converted orbital elements from the numerically integrated state vector in Cartesian coordinate. As a result, LPE with EOE has an advantage in long term calculation over LPE with COE in case of relatively small eccentricity.

• Bulletin of the Korean Chemical Society
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• v.32 no.2
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• pp.467-471
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• 2011

Spin exchange interactions of $(C_2N_2H_{10})[Fe(HPO_3)F_3]$ were examined by performing a spin dimer analysis based on extended Huckel tight binding method and a mapping analysis based on first principles density functional theory. Spin exchange interactions occur through the super-superexchange paths $J_1$ and $J_2$ in $(C_2N_2H_{10})[Fe(HPO_3)F_3]$. In the super-superexchange path $J_2$ magnetic orbital interactions between eg-block levels are much stronger than those from $t_{2g}$-block levels. Both electronic structure calculations show that the spin exchange interaction through the super-superexchange path $J_2$ is much stronger than that of $J_1$.

• Proceedings of the Korean Society of Propulsion Engineers Conference
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• 2005.11a
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• pp.272-277
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• 2005

전 세계적으로 우주로의 여행 (우주여행, Space Tourism)에 대한 많은 관심이 일어나고 있다. 특히 2004년 10월 4일 Scaled Composites사(社)의 SpaceShipOne이 2주 연속하여 지상 100km 정도의 지구 저궤도 (Sub-Orbital) 비행에 성공함으로써 이러한 관심은 폭발적으로 증가하고 있다. 이것은 우주여행이라는 것이 민간에 의한 우주 개발의 노력으로 시도된다는 측면에서 기존의 패러다임, 즉, 우주 개발은 국가 주도 하에서만 가능하다는 기존의 패러다임을 부정하는 상당히 획기적인 사건이기 때문이었다. 따라서 민간주도의 우주여행 사업에 대해 미국을 중심으로 한 민간업체의 개발 동향과 함께 지구 저궤도 우주비행체에 대한 (응용) 시장의 (창출) 가능성, 법적인 측면, 사업적 관점, 그리고 기술적 관점에서 바라보고자 한다.

• Progress in Superconductivity and Cryogenics
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• v.25 no.2
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• pp.1-4
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• 2023

Over the past decade, the exploration of high-temperature superconductivity and the discovery of a wide range of exotic superconducting states in Fe-based materials have propelled condensed matter physics research to new frontiers. These materials exhibit intriguing phenomena arising from their multiband electronic structure, strongly orbital-dependent effects, extremely small Fermi energy, electronic nematicity, and topological aspects. Among the various factors influencing their superconducting properties, high magnetic fields play a crucial role as a control knob capable of disrupting the subtle balance between the spin, charge, lattice, and orbital degrees of freedom, leading to the emergence of various exotic superconducting states. In this review, we provide an overview of the current understanding of the exotic superconducting states observed in Fe-based superconductors, with a particular focus on FeSe and Sr₂VO₃FeAs, under the influence of high magnetic fields.

• Journal of the Korean Chemical Society
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• v.46 no.3
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• pp.179-186
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• 2002

A molecular orbital analysis based on the extended Huckel calculations has been carried out to study the OH bond activation of water on the $TiO_2$(110) surface. $H_2O$ binds with its axis perpendicular to the surfac on top of the five-coordinate $Ti^{4+}$ atom via its $3a_1$ orbital. In this bonding situation, the two-coordinated bridging $O^{2-}$ atom ($O_b$, basic site) on $TiO_2$(110) is too distant from an H atom of water to form hydrogen-bondig interactions with water that facilitate O-H bond cleavage. It has been elucidated that the O-H bond is appreciably weakened when the water molecule is tilted to give a hydrogen bond with the $O_b$ atom. This mechanism includes mutual transfer of electron density from the $3a_1$ orbital of the water molecule to the $Ti^{4+} 3d_{z2}$ orbital and from the $O_b$ P orbitals to the $2b_1$ of the adsorbed water molecule This should result in lengthening of the O-H bond in the surface complex and the subsequent dissociation into the fragments OH and H.

• Korean Journal of Radiology
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• v.25 no.8
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• pp.742-748
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• 2024

Objective: ¹⁸F-N-(2-(Diethylamino)ethyl)-5-(2-(2-(2-fluoroethoxy)ethoxy)ethoxy) picolinamide (¹⁸F-PFPN) is a novel positron emission tomography (PET) probe designed to specifically targets melanin. This study aimed to evaluate the diagnostic feasibility of ¹⁸F-PFPN in patients with ocular or orbital melanoma. Materials and Methods: Three patients with pathologically confirmed ocular or orbital melanoma (one male, two females; age 41-59 years) were retrospectively reviewed. Each patient underwent comprehensive ¹⁸F-PFPN and ¹⁸F-fluorodeoxyglucose (¹⁸F-FDG) PET scans. The maximum standardized uptake value (SUV_max) of the lesion and the interference caused by background tissue were compared between ¹⁸F-PFPN and ¹⁸F-FDG PET imaging. In addition, the effect of intrinsic pigments in the uvea and retina on the interpretation of the results was examined. The contralateral non-tumorous eye of each patient served as a control. Results: All primary tumors (3/3) were detected using ¹⁸F-PFPN PET, while only two primary tumors were detected using ¹⁸F-FDG PET. Within each lesion, the SUV_max of ¹⁸F-PFPN was 2.6 to 8.3 times higher than that of ¹⁸F-FDG. Regarding the quality of PET imaging, the physiological uptake of ¹⁸F-FDG PET in the brain and periocular tissues limited the imaging of tumors. However, ¹⁸F-PFPN PET minimized this interference. Notably, intrinsic pigments in the uvea and retina did not cause abnormal concentrations of ¹⁸F-PFPN, as no anomalous uptake of ¹⁸F-PFPN was detected in the healthy contralateral eyes. Conclusion: Compared to ¹⁸F-FDG, ¹⁸F-PFPN demonstrated higher detection rates for ocular and orbital melanomas with minimal interference from surrounding tissues. This suggests that ¹⁸F-PFPN could be a promising clinical diagnostic tool for distinguishing malignant melanoma from benign pigmentation in ocular and orbital melanomas.

• The Bulletin of The Korean Astronomical Society
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• v.44 no.2
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• pp.64.1-64.1
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• 2019

The first high-resolution spectroscopic and new multiband photometric observations of the semi-detached Algol type binary XZ CMi were performed at the Bohyunsan Optical Astronomy Observatory (BOAO) and the Sobaeksan Optical Astronomy Observatory (SOAO), respectively. A total of 34 spectra were obtained using the 1.8 m reflector of the BOAO equipped with the Bohyunsan Optical Echelle Spectrograph to construct the radial velocity (RV) curves of the eclipsing pair. New BVRI photometric light curves were also covered by using the SOAO 61cm reflector and a CCD camera. A detailed analysis of all eclipse timings shows that the orbital period of XZ CMi has varied in an upward parabolic variation superposed on a sinusoidal oscillation with a period of 38.0 yr and a semi-amplitude of 0.0071 days. From the spectral analysis, the effective temperature and the projected rotational velocity of the primary component were determined to be T_eff,1 = 7387±161 K and v₁sini = 122±6 km s^-1, respectively. Our simultaneous synthesis of the double-lined RV and BVRI light curves gives the reliable system parameters of XZ CMi with a mass ratio (q) of 0.314, an orbital inclination (i) of 81.9 deg and a large temperature difference (∆T) of 2481 K. The individual masses and radii of both components are M₁ = 1.91±0.08M_⊙, M₂ = 0.60±0.02M_⊙, R₁ = 1.60±0.02R_⊙, R₂ = 1.13±0.02R_⊙, respectively. Although the primary component is located inside the δ Sct and γ Dor instability strips, no evidence of pulsation in the system was detected. The possible evolutionary status of XZ CMi is discussed.

• Proceeding of EDISON Challenge
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• 2015.03a
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• pp.40-47
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• 2015

본 연구에서는 일치환된 방향족 화합물의 $NO_2{^+}$ 치환반응에서의 반응성 (reactivity)과 지향성 (regioselectivity)에 대해 분석하였다. 기존의 연구에 따르면, 방향족 고리와 치환체 사이의 ${\sigma}$ 결합을 통한 유발효과와 ${\pi}$ 결합을 통한 공명효과로 인해 벤젠 고리의 전자 분포가 증가하게 되면 반응성이 증가하는 것으로 알려져 있다. 또한 반응중간생성물인 탄소양이온의 안정성을 통해 지향성을 확인할 수 있는 것으로 알려진 바가 있다. 이에 따라, 본 연구에서는 반응성과 지향성이 실험적으로 잘 알려진 7가지의 치환기 (OH, $OCH_3$, $CH_3$, Cl, COOH, CN, $NO_2$)를 선정하여 DFT functional인 B3LYP를 사용하여 natural bond orbital (NBO) 계산을 하였고, 각각의 일치환된 벤젠 고리가 갖는 전자 분포를 ${\sigma}$와 ${\pi}$ 전자로 나누어서 보기로 했다. 그 결과, 일치환된 방향족 고리 치환반응의 반응성과 지향성은 ${\sigma}$ 결합을 통한 유발효과에 의해서는 영향을 받지 않고, 공명 효과로 인한 반응물의 ${\pi}$ 전자 분포에 의해 결정되는 것을 확인할 수 있었다. 이외에도 반응성을 비교 하기 위해 친핵체로 작용하는 일치환된 방향족 고리의 highest occupied molecular orbital(HOMO) 에너지와 친전자체인 $NO_2{^+}$의 lowest unoccupied molecular orbital (LUMO) 에너지의 차이를 비교하였으며, 친핵체의 HOMO 에너지가 높을수록 반응성이 커짐을 알 수 있었다.