• Proceedings of the Korea Information Processing Society Conference
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• 2012.11a
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• pp.212-214
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• 2012

분산 컴퓨팅 자원의 효율적인 관리기술은 많은 기업, 연구소, 표준기관이 연구해온 분야로 최근까지도 관련된 개방형 프로젝트가 진행되고 있다. 대표적으로 DMTF는 선도적인 기업체를 중심으로 학계와 협력하여 객체지향 방법을 통한 다양한 컴퓨팅 하드웨어 및 소프트웨어 관리 시스템의 정보를 CIM기반의 객체로 정의하고 있다. 또한 SNIA에서는 DMTF의 CIM 표준을 기반으로 개방형 스토리지 관리 표준인 SMI-S 규격을 제공하고 있다. 본 논문에서는 SNIA에서 제공하는 SMI-S CIIM 스키마를 이용하여 상용 가상화 소프트웨어 인 Citrix Storagelink를 통해 Third Party 스토리지 시스템을 관리하기 위한 기술에 대해 설명한다.

• Bulletin of the Korean Space Science Society
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• 2009.10a
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• pp.34.1-34.1
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• 2009

After SNIa and WMAP observations during the last decade, the discovery of the accelerated expansion of the universe is a major challenge to particle physics and cosmology. There are currently three candidates for the dark energy which results in this accelerated expansion: $\cdot$ a non-zero cosmological constant, $\cdot$ a dynamical cosmological constant (quintessence scalar field), $\cdot$ modifications of Einstein's theory of gravity. The scalar field model like quintessence is a simple model with time-dependent w, which is generally larger than -w1. Because the different w lead to a different expansion history of the universe, the geometrical measurements of cosmic expansion through observations of SNIa, CMB and baryon acoustic oscillations (BAO) can give us tight constraints on w. One of the interesting ways to study the scalar field dark-energy models is to investigate the coupling between the dark energy and the other matter fields. In fact, a number of models which realize the interaction between dark energy and dark matter, or even visible matter, have been proposed so far. Observations of the effects of these interactions will offer an unique opportunity to detect a cosmological scalar field. In this talk, after briefly reviewing the main idea of the three possible candidates for dark energy and their cosmological phenomena, we discuss the interactinng dark-energy model, paying particular attention to the interacting mechanism between dark energy with a hot dark matter (neutrinos). In this so-called mass-varying neutrino (MVN) model, we calculate explicitly the cosmic microwave background (CMB) radiation and large-scale structure (LSS) within cosmological perturbation theory. The evolution of the mass of neutrinos is determined by the quintessence scalar field, which is responsible for the cosmic acceleration today.

• Journal of Nuclear Fuel Cycle and Waste Technology(JNFCWT)
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• v.21 no.1
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• pp.175-182
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• 2023

APro, a modularized process-based total system performance assessment framework, was developed at the Korea Atomic Energy Research Institute (KAERI) to simulate radionuclide transport considering coupled thermal-hydraulic-mechanical-chemical processes occurring in a geological disposal system. For reactive transport simulation considering geochemical reactions, COMSOL and PHREEQC are coupled with MATLAB in APro using an operator splitting scheme. Conventionally, coupling is performed within a MATLAB interface so that COMSOL stops the calculation to deliver the solution to PHREEQC and restarts to continue the simulation after receiving the solution from PHREEQC at every time step. This is inefficient when the solution is frequently interchanged because restarting the simulation in COMSOL requires an unnecessary setup process. To overcome this issue, a coupling scheme that calls PHREEQC inside COMSOL was developed. In this technique, PHREEQC is called through the "MATLAB function" feature, and PHREEQC results are updated using the COMSOL "Pointwise Constraint" feature. For the one-dimensional advection-reaction-dispersion problem, the proposed coupling technique was verified by comparison with the conventional coupling technique, and it improved the computation time for all test cases. Specifically, the more frequent the link between COMSOL and PHREEQC, the more pronounced was the performance improvement using the proposed technique.

• Korean Journal of Materials Research
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• v.7 no.2
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• pp.107-113
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• 1997

$SrBi_{2}Ta_{2}O_{9}(SBT)$ thin films wcre prepared on $Pt/Ti/SiO_{2}/Si$ suhsrrate by pL~snia-enhanced chemical vapor deposition. Sr and Ta huhhling temperatures were kept ,it $120^{\circ}C$ Iron1 X- ray tiiffriict!on. n~icrostruc~ure. and composjrional analysis of SH7' films, respectivels Hi I~ut~t~lmg tempcl.arure was varied SR'I' thin tilrns dcpositcd ar i3i buhbling temperature of $130^{\circ}C$ have dielccrric constanr of 150 anti dissipation factor of 0 02 at IOOkFic. I .eakagc wrrent density of films was ahour $1.0{\times}10^{-8}A/cm^2$ at 20kV/cm. 1.eakage current i11amcrc1istic.s of Sli'l' films nras c.ontrolled by I'oole Frcnkel emission Kenianent polariziit~on and mercivc field oi SR\ulcorner' films annealed at $550^{\circ}C$ were $9{\mu}C/cm^2$ and 70kV/cm, respectively.

• Journal of Advanced Navigation Technology
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• v.13 no.6
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• pp.957-963
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• 2009

It is necessary for the resource management system to manage for the resource in distributed networking environment. Because of increasing the complexity of vast computer system and business environment, needs of RMS is increasing. Based on the common information model to use of objected oriented technology, through analysis of the reference model for the resource management system of the SNIA, we intend to implement the application program to manage the NGS system that consist of SSD and DRAM. To visualize, it is use the GUI Interface. It is possible for application program(Client) to detect and manage the system that consist of the NGS system. Also, status information that is divided into three cataloges(Minor/Major/Critical) can be displayed and it provide support of configuration functionality to manage devices.