• 전기학회논문지
• /
• 제61권1호
• /
• pp.80-84
• /
• 2012

Recently, the small scale photovoltaic (PV) electronic devices are drawing attention as the upcoming PV generation system. The PV system is commonly used in small scale PV applications such as LED lighting and cell phone. This paper proposes photovoltaic output sensorless (POS) maximum power point tracking (MPPT) control for a small scale charging system of PV-nickel metal hydride battery using field-programmable gate array (FPGA) controller. A converter is connected to a small scale PV cell and battery, and performs the POS MPPT at the battery terminal current instead of being at the PV cell output voltage and current. The FPGA controller and converter operate based on POS MPPT method. The experimental results show that the nickel metal hydride battery is charged by the maximum PV output power.

• 한국전산구조공학회논문집
• /
• 제19권3호
• /
• pp.233-238
• /
• 2006

이 논문에서는 소형 다층 구조물의 진동제어에 적용하기 위한 복합모드의 자기유변유체(MR) 감쇠기를 개발하였다. 우선, 도식적으로 전단, 유동, 복합모드 MR감쇠기의 형태를 설계조건과 함께 표현하였고, 각각의 모드에 대하여 자기장에 따른 감쇠력을 예측하기 위한 해석모델을 유도하였다. 다음으로 적당한 크기의 복합모드 MR감쇠기를 제작하고 자기장에 따른 감쇠특성을 시간영역에서 평가하였다. 마지막으로 지진하중을 받는 소형구조물에 제작된 MR감쇠기가 준능동 제어기로 제어하였을 때의 성능을 수치적으로 평가하였다.

• 천문학회보
• /
• 제42권2호
• /
• pp.81.3-81.3
• /
• 2017

In this paper, we report a small-scale emerging island and double arc loops, which are associated with a M6.5 flare, in Active Region 12371. We investigate the spatial and temporal changes of both photospheric magnetic fields using SDO/HMI data and coronal magnetic structures obtained from nonliner force-free field (NLFFF) extrapolation. From the vector magnetograms, we find a small-scale emerging island near the main polarityy inversion line about three hours before the flare. The island has a strong shear angle, which is determined by difference between transverse component of observed field and potential field, of around 90 degrees. Furthermore, the NLFFF well reproduces a sigmoidal structure seen in SDO/AIA 94, which is consistent with the double arc loops configuration suggested by Ishiguro and Kusano (2017) who introduced a magnetic configuration showing the double arc instability. The observed emerging island is located among the double arc loops, which is also supproted by their model. Finally, there was an eruption (M6.5 flare) associated with the loops. We discuss a possible role of the double arc instability for the eruption.

• Journal of Advanced Marine Engineering and Technology
• /
• 제30권4호
• /
• pp.494-504
• /
• 2006

It is well known that the two-parameter $J-A_2$ solution can well characterize the crack-tip fields and quantify the crack-tip constraint for different flawed geometries in variety of loading conditions. However, this solution fails to do so for bending dominated specimens or geometries at large deformation because of the influence of significant global bending stress on the crack-tip field. To solve this issue, a modified $J-A_2$ solution is developed in this paper by introducing an additional term to address the global bending influence. Using the $J_2$ flow theory of plasticity and within the small-strain framework detailed finite element analyses are carried out for the single edge notched bend (SENB) specimen with a deep crack in A533B steel at different deformation levels ranging from small-scale Yielding to large-scale Yielding conditions. The numerical results of the crack-tip stress field are then compared with those determined from the $J-A_2$ solution and from the modified $J-A_2$ solution at the same level of applied loading Results indicate that the modified $J-A_2$ solution largely improves the $J-A_2$ solution, and match very well with the numerical results in the region of interest at all deformation levels. Therefore, the proposed solution can effectively describe the crack-tip field and the constraint for bending dominated specimens or geometries.

• 천문학회보
• /
• 제39권2호
• /
• pp.74.2-74.2
• /
• 2014

Magnetohydrodynamics(MHD) dynamo depends on many factors such as viscosity ${\gamma}$, magnetic diffusivity ${\eta}$, magnetic Reynolds number $Re_M$, external driving source, or magnetic Prandtl number $Pr_M$. $Pr_M$, the ratio of ${\gamma}$ to ${\eta}$ (for example, galaxy ${\sim}10^{14}$), plays an important role in small scale dynamo. With the high PrM, conductivity effect becomes very important in small scale regime between the viscous scale ($k_{\gamma}{\sim}Re^{3/4}k_fk_f$:forcing scale) and resistivity scale ($k_{\eta}{\sim}PrM^{1/2}k_{\gamma}$). Since ${\eta}$ is very small, the balance of local energy transport due to the advection term and nonlocal energy transfer decides the magnetic energy spectra. Beyond the viscous scale, the stretched magnetic field (magnetic tension in Lorentz force) transfers the magnetic energy, which is originally from the kinetic energy, back to the kinetic eddies leading to the extension of the viscous scale. This repeated process eventually decides the energy spectrum of the coupled momentum and magnetic induction equation. However, the evolving profile does not follow Kolmogorov's -3/5 law. The spectra of EV (${\sim}k^{-4}$) and EM (${\sim}k^0$ or $k^{-1}$) in high $Pr_M$ have been reported, but our recent simulation results show a little different scaling law ($E_V{\sim}k^{-3}-k^{-4}$, $EM{\sim}k^{-1/2}-k^{-1}$). We show the results and explain the reason.

• 한국벤처창업학회:학술대회논문집
• /
• 한국벤처창업학회 2006년도 추계학술발표회
• /
• pp.275-299
• /
• 2006

This study aims at examining the early-stage financing scale for entrepreneur to build small & medium business. The data was collected from the DART (Data Analysis, Retrieval and Transfer System) of Korean Financial Supervisory Service(FSS) in the main. The results of this study show that small & medium business needs equipment & operation financing for about 37 months extent to reach Break-Even Point. The limitations of this study are data collections from registered firms on Korean FSS primarily and no showing about the early stage financing scale for building small & Medium Business concretely. Small & Medium business entrepreneur have to make a early stage finance plan according to a necessary equipment and operating cost in their business field for 37 months extent.

• 천문학회보
• /
• 제38권2호
• /
• pp.61.1-61.1
• /
• 2013

Turbulence is a common phenomenon in astrophysical fluids such as the interstellar medium (ISM) and the intracluster medium (ICM). In turbulence studies it is customary to assume that fluid powered by an energy injection on a single scale. However, in astrophysical fluids, there can be many different driving mechanisms that act on different scales simultaneously. In this work, we assume multiple energy injection scale (2${\surd}$12 and 15

• 생태와환경
• /
• 제44권3호
• /
• pp.253-263
• /
• 2011

본 연구는 인공 조성된 둠벙의 물리 화학적 및 생물학적 특성을 분석하여 둠벙의 복원 및 관리를 위한 기초 자료를 얻고자 수행한 연구로 다음과 같은 결론을 도출하였다. 연구대상지 둠벙의 면적은 4.6~14.1 $m^2$였으며 모양은 원형과 사각형 모양이 대부분이었다. 조사 둠벙 중 가장 자리에 석축이나 목축을 두르지 않은 둠벙들은 주변 둑이 매몰되어 수심이 얕아져 둠벙의 기능을 잃을 수 있다. 따라서 지속적인 둠벙 기능 유지를 위해서는 주변에 석축이나 목축 등을 둘러 매몰되는 것을 방지할 필요가 있다. 연구대상지의 수질환경은 COD, TN, TP의 경우 농업용수 기준을 초과한 수질등급을 보였으며 특히 TN의 농도는 평균 8.03 mg $L-1$로 농업용수 수질기준을 약 8.0배를 초과하는 농도분포를 보였다. 조사지역 둠벙의 질소농도가 높은 원인으로는 홍성지역의 높은 축산 밀도, 농경지 주변 산재해 있는 축사 시설과 축산폐수를 이용한 저장 액비 사용에 의한 것으로 판단된다. 오히려 농촌지역에서 둠벙과 같은 작은 저류지가 하천으로 유출되는 영양물질을 저감시켜 주는 소규모 침전지 역할도 할 수 있을 것으로 사료된다. 연구대상지 둠벙의 평균적인 모래함량, 유기물 함량, 유효인산 함량은 각각 53.4${\pm}$16.6%, 21.8${\pm}$9.74 g $kg^{-1}$, 12.8${\pm}$7.59 mg $kg^{-1}$로 나타났다. 둠벙의 토양 특성 조사결과 모래함량과 유효인산 농도는 둠벙 안정화를 위한 식생정착에 적합한 농도분포였으나 신규로 조성된 5곳의 둠벙에서는 유기물 함량이 높지 않아 식생 정착에 다소 시간이 소요될 것으로 판단된다. 연구 대상지 둠벙의 어류상은 붕어, 미꾸리, 미꾸라지, 드렁허리 4종이 출현하였으며 군집구조 분석결과 군집 안정도와 다양도 지수가 불량하게 나타났다. 이와 같이 단순한 어류상 구조는 둠벙이 주변 하천과 고립된 구조를 가지고 있기 때문에 논과 정수지역, 농수로 등 연중 수위와 환경변화가 큰 환경에 적응한 어종들만이 서식할 수 있기 때문으로 판단된다. 요인분석에서 도출된 요인점수(Facter score)를 바탕으로 조사한 둠벙을 구분한 결과, 요인점수 1에서 양의 값을 보이는 둠벙은 다른 둠벙에 비해 둠벙의 크기가 큰 것들로 구성되었으며 (Group I), 요인점수 2에서 양의 값을 보인 Group III은 다른 둠벙에 비해 유기물 농도가 높은 둠벙들로(S5, S6) 구성되었다(Fig. 4). 본 연구를 바탕으로 향후 농촌지역 둠벙의 복원 및 효율적 관리를 위해서는 둠벙과 주변하천과의 연계성, 둠벙의 크기를 비롯한 구조적 특성을 잘 고려해야 할 것으로 판단된다. 본 연구에서 거론하지 못한 둠벙 용수의 유 출입량, 둠벙 수체내 먹이 연쇄 구조 등 세부적인 부분에 대한 연구를 추가적으로 진행해야 할 것으로 판단된다.

• 지역사회간호학회지
• /
• 제12권3호
• /
• pp.647-660
• /
• 2001

Forming health care management model in small-scale enterprises was the purpose of this study. For the purpose, we tried to investigate the characteristics of small-scale enterprises and analyzed the pattern of their health care management. The results are as follow: 1. The strength of health managing agency and technical supporting program lies in team approach by specialized manpower. However, if the liaison between each part of the organization is not smooth, the overall management will be very difficult. 2. Small scale enterprises are characterized by their short life after the establishment, use of rental building, lack of welfare facilities, weakness in sanitary management and aggregation of factories of similar type of industry. Because of these characteristics, it is very difficult to solve problem basically, such as improvement of working environment. Therefore, it is important to focus on health education and community based approach. 3. Many workers in small-scale factories are in middle and old age. They have health problems mainly related to personal habits. Implementation of an appropriate health promotion program is needed. 4. The number of workplaces, which should be managed by health managing agent. is increasing rapidly. But the number of health managing agent is limited. In the aspect of the requirement of manpower and equipment, training personal agent is more urgent than founding institutional agent. 5. The uniform method of health management hampers the choice of employer and workers. The types of provision of health management should be diversified. 6. For an efficient management, a frequent visit of personal agent and the following referral to a specialist should be done. The specialists in charge of secondary management are from the field of occupational medicine, occupational hygiene, ergonomics, etc. 7. The health management of small-scale facilities should have six components. They are community-based approach, multi-disciplinary cooperative system, program based on the need of recipient, forming partnership of employer and worker, change of lifestyle, and evidence-based program.

• 천문학회지
• /
• 제37권5호
• /
• pp.553-556
• /
• 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.