• 충청수학회지
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• 제26권4호
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• pp.869-878
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• 2013

We study boundedness of solutions of dynamic equations on time scales by using Lyapunov-type functions.

• 소성∙가공
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• 제13권1호
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• pp.72-77
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• 2004

An Fe-25Cr steel was oxidized in Ar atmosphere at 973K with and without applying external stress of 30∼35 MPa. A 0.1$\mu\textrm{m}$ thick $Cr_2O_3$ scales formed during pre-treatment in Ar atmosphere. Initiation of cracking on the oxide scales took place at grain boundaries during the end of second creep stage, in which cracks were found nearly perpendicular to the tensile directions. On the contrary, a scale developed in $N_2$-0.1%$SO_2$ displaced a poor adherence on the metal substrate. In this sample, a fast grown of scales was observed during creep deformation, and the strength of materials was much lower than in Ar. The creep strain rate of $1.5{\times}10^{-7}/s$ and $5.8{\times}10^{-7}/s$ was determined in Ar and in $N_2$-0.1%$SO_2$ under 30MPa, respectively.

• 천문학회지
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• 제46권1호
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• pp.41-47
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• 2013

I present a simple scheme for the treatment of gravitational interactions on galactic scales. In anal- ogy with known mechanisms of quantum field theory, I assume ad hoc that gravitation is mediated by virtual exchange particles-gravitons-with very small but non-zero masses. The resulting den- sity and mass profiles are proportional to the mass of the gravitating body. The mass profile scales with the centripetal acceleration experienced by a test particle orbiting the central mass, but this comes at the cost of postulating a universal characteristic acceleration $a_0{\approx}4.3{\times}10^{-12}msec^{-2}$ (or $8{\pi}a_0{\approx}1.1{\times}10^{-10}msec^{-2}$). The scheme predicts the asymptotic flattening of galactic rotation curves, the Tully-Fisher/Faber-Jackson relations, the mass discrepancy-acceleration relation of galaxies, the surface brightness-acceleration relation of galaxies, the kinematics of galaxy clusters, and "Renzo's rule" correctly; additional (dark) mass components are not required. Given that it is based on various ad-hoc assumptions and given further limitations, the scheme I present is not yet a consistent theory of gravitation; rather, it is a "toy model" providing a convenient scaling law that simplifies the description of gravity on galactic scales.

• 설비공학논문집
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• 제29권10호
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• pp.530-537
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• 2017

Scales generated inside pipes cause negative effects on heat transfer performance, pressure loss and flow rate due to increased thermal resistance and reduced flow cross-sectional area. If these scales are not prevented or eliminated, thermal-fluid performance of the facilities can be deteriorated, or in extreme cases, accidents such as explosion due to overheating can occur. There are two ways to remove the scales, physically and chemically. Removing the scales physically needs specific machines which are expensive, and removing them chemically may provoke corrosion or shorten the age of the facilities. In this study, an eco-friendly pipe scale cleaner using natural organic acid is developed by applying the concept of a limestone cave generation. The manufactured scale cleaner is applied to remove the scales in industrial, water heating and urinal pipes. The results show that this cleaner removes scales more effectively and safely compared to existing scale treatments. Scale removal efficiencies of this work is 1.2~10.7 times for industrial pipes and 1.8~15.5 times for boiler water heating pipes higher than those of conventional cleaners.

• 천문학회지
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• 제37권5호
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• pp.553-556
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• 2004

We present a new model for the generation of magnetic fields on large scales occurring at the end of cosmological reionisation. The inhomogeneous radiation provided by luminous sources and the fluctuations in the matter density field are the major ingredients of the model. More specifically, differential radiation pressure acting on ions and electrons gives rise to electric currents which induce magnetic fields on large scales. We show that on protogalactic scales, this process is highly efficient, leading to magnetic field amplitudes of the order of $10^{-1l}$ Gauss. While remaining of negligible dynamical impact, those amplitudes are million times higher than those obtained in usual astrophysical magnetogenesis models. Finally, we derive the relation between the power spectrum of the generated field and the one of the matter density fluctuations. We show in particular that magnetic fields are preferably created on large (galactic or cluster) scales. Small scale magnetic fields are strongly disfavoured, which further makes the process we propose an ideal candidate to explain the origin of magnetic fields in large scale structures.

• 전기전자학회논문지
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• 제19권3호
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• pp.392-399
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• 2015

본 논문에서는 HEVC와 VP9 코덱의 계수 변환 (Transform)을 수행하는 통합형 아키텍쳐를 제안하여 하드웨어 크기를 줄이고자 한다. 제안하는 아키텍쳐는 HEVC $4{\times}4$ IDCT, HEVC $4{\times}4$ IDST, VP9 $4{\times}4$ IDCT, VP9 $4{\times}4$ IADST를 통합 하드웨어에서 처리가 가능하다. HEVC $4{\times}4$ IDCT와 VP9 $4{\times}4$ IDCT는 계수의 스케일만 다를 뿐 동일한 IDCT 연산을 사용하며, 마찬가지로 HEVC $4{\times}4$ IDST와 VP9 $4{\times}4$ IADST도 계수의 스케일만 다를 뿐 동일한 IDST 연산을 사용한다. 더욱이 IDCT 연산과 IDST 연산에는 상당히 많은 유사점이 있어 일부 하드웨어를 공동으로 사용할 수 있다. 따라서 제안하는 하드웨어는 4가지 연산에 대해 곱셈기의 계수는 각각 다르지만 버터플라이 덧셈기등은 공통으로 사용하여 통합적으로 수행한다. 0.18um 공정에서 합성했을 때 게이트 수가 약 6,679 게이트로 기존 아키텍처 대비 25.3% 감소함을 확인하였다.

• Journal of Acupuncture Research
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• 제41권1호
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• pp.53-62
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• 2024

Background: The aim of this study is to determine the correlation between clinical assessment scales, self-assessment scales, and surface electromyography (SEMG) for facial nerve palsy. Methods: This study assessed 32 cases of facial nerve palsy on the first visit, 11 cases on the second visit, and 9 cases on the third visit to the Korean medicine hospital, university. This study was conducted from October 22, 2022, to December 22, 2022. The patients were evaluated using SEMG, clinical assessment scales, and self-assessment scales 3 times. The House-Brackmann grading systems (HBGS), Yanagihara unweighted grading system (Y-score), facial disability index, numerous rating scale, and accompanying symptoms of facial nerve palsy were used for assessment. Moreover, statistical correlation was analyzed using Pearson correlation. Results: On Visit 1, Significant correlations were observed between the results of SEMG and other clinical assessment scales as well as between SEMG-F (frontalis) and different parts of the Y-score. On Visit 2, significant correlations were observed between the results of SEMG and HBGS as well as between SEMG-F and the detailed parts of the Y-score. On Visit 3, significant correlations were observed only between SEMG-F and the detailed parts of the Y-score. A significant correlation was also observed between the changes in the clinical assessment scales on Visits 1 and 3 and between the changes in SEMG-F and those in the patient self-assessment scales. Conclusion: These findings suggest that SEMG can be used to evaluate facial nerve palsy in conjunction with the use of other clinical assessment scales.

• 천문학회지
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• 제29권spc1호
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• pp.215-216
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• 1996

The wind-formed features observed in the early SNe spectra type II and Ia give an evidence of the existence of an ellipsoidal shell formed by the stellar wind prior to the explosion. Such non-spherical shell can occur not only at scales of parsec (the case of SN 1987 A progenitor), but at the scales of 1000 times less. Such shells can be the result of the radial pulsation. The prolate multi-shell structures are interpreted as a result of a pulsation processes with recurrent wind ejections with velocity increasing.

• 충청수학회지
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• 제25권2호
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• pp.349-357
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• 2012

In this paper we introduce the C-delta integral which generalize the McShane delta integral and investigate some properties of these integrals.

• 식물조직배양학회지
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• 제26권2호
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• pp.103-107
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• 1999

Lilium oriental hybrid 'Casa Blanca'의 기내인편에서 자구를 대량생산하기 위하여 MS배지의 염류농도 및 당, 광조건 등이 자구의 형성 및 비대에 미치는 영향을 조사하였다. MS배지의 1/2～2배 염류농도에서 자구의 형성은 차이를 나타내지 않았으나 3배 염류농도에서 자구의 형성이 현저히 억제되었다 자구의 비대는 MS기본배지에서 가장 촉진되었다. 배지의 NH$_4$$^{+}$ : NO$_3$의 비율이 1 : 2와 1 : 3일 때, 또는 MS기본배지 (NH$_4$$^{+}$ : NO$_3$= 약 1 : 2)가 인편에서 자구의 형성 및 비대에 적절하였다. 따라서 MS 기본배지가 자구의 형성 및 비대에 양호한 것으로 나타났다. 당의 농도가 높아지면 자구형성은 억제되고 자구비대는 촉진되었으며, 당 9~12% 첨가배지에서 자구비대가 양호하였다. 배지내 활성탄의 첨가는 인편에서 자구의 형성을 억제하였으나 형성된 자구의 비대는 촉진하였다. 특히 활성탄 1 g/L를 첨가한 배지가 자구의 비대에 가장 효과적이었다. 자구의 형성 및 형성된 자구의 비대는 명, 암간에 차이를 나타내지 않았다. 따라서 L. Oriental Hybrid 'Casa Blanca'의 기내 대량번식은 당 9%와 활성탄 1 g/L가 첨가된 MS기본배지에서 기내인편을 배양하여 자구를 형성 및 비대시키고 형성된 자구의 인편을 계대배양하는 것이 효율적이었다.