• 한국HCI학회:학술대회논문집
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• 2009.02a
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• pp.862-867
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• 2009

The development of internet has changed the realm of life from off-line to on-line, causing not only the overall change in society but also urgently demanding change in the basic concept of museum. Virtual Museums have appeared in line with such changes, and they utilize space regardless of real time and space unlike the traditional museums that collected and preserved works for exhibition in physical space thereby playing a role of catalyst for exhibition in virtual space and for direct exchange with the public. Through relevant literatures and case studies, the present research particularly investigated the exhibition characteristics of virtual reality-based museums out of all types of cyber museum, in an effort to make a comparison with those of offline museums, and eventually to suggest a direction of virtual reality museums that would be established in the future and to consider the possibilities of utilizing them.

• Publications of The Korean Astronomical Society
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• v.29 no.3
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• pp.35-44
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• 2014

In ground-based astronomical spectroscopic observations, there are many telluric absorption lines that are laid on the spectra of celestial objects. To study the physical properties of the celestial objects with these contaminated spectra, the telluric lines should be removed. A conventional method for removing the telluric lines is using the standard stellar spectrum as telluric line. In this paper, we introduce a technique to calculate synthetic telluric spectra and use them to remove telluric lines from a spectrum of a celestial object. We used Line-by-Line Radiative Transfer Model (LBLRTM) for calculating a synthetic spectrum and selected Michelson Interferometer for Passive Atmospheric Sounding (MIPAS) model as atmospheric model. We apply our method to some spectra obtained by Bohyunsan Observatory Echelle Spectrograph (BOES) to show that the telluric lines are well removed from the observed spectra by our model within an accuracy of 2% which is close to the 1-sigma rms of the original spectra.

• Current Optics and Photonics
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• v.1 no.4
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• pp.344-350
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• 2017

We present a new design approach and an example design for an image-space telecentric two-mirror system that has a fast f-number and a wide-field line image. The initial design of the telecentric mirror system is a conventional axially symmetric system, consisting of a flat primary mirror with fourth-order aspheric deformation and an oblate ellipsoidal secondary mirror to correct spherical aberration, coma, and field curvature. Even though in the optimized design the primary mirror is tilted, to avoid ray obstruction by the secondary mirror, the image-space telecentric two-mirror system shows quite good imaging performance, for a line imager.

• International conference on construction engineering and project management
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• 2007.03a
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• pp.573-582
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• 2007

Working spaces in the construction site are much more complicated than completed spaces in the building. There are many researches focus on partition of building spaces. However, few discussed partition sequencing in building construction sites. Space syntax is a set of techniques for analyzing spatial configurations. It has become a useful tool in a variety of researches. Partition sequencing of working spaces should be related to the working direction. However, with convex space and axial line, the partition sequencing became unrelated to the working direction. When critical space is blocked, the partition sequencing with axial line will be changed. It is significant to reveal the impact of the entire spatial structure when some of the working spaces are blocked. This paper discussed the improved partition sequencing theory and highlighted the importance of critical space and analyzed the spatial structure of working space. A real case project was demonstrated in this paper.

• Journal of KIISE:Software and Applications
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• v.33 no.1
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• pp.84-94
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• 2006

The color information in an image changes as the illuminant condition varies. The mechanism to find canonical color of an object by estimating illumination color in an image is generally referred as color constancy. In color constancy, computing robust and precise dichromatic line is most important to estimate illumination chromaticity. In this paper, a novel approach to estimate the color of a single illuminant for noisy and micro-textured images is introduced. An accurate dichromatic line is found by using Dichromatic Line Space (DLS), proposed in this paper. which has information about diffuse chromaticity and illumination chromaticity.

• Proceedings of the KIPE Conference
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• 2010.07a
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• pp.472-473
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• 2010

1kW~10kW급의 UPS 토폴로지로서 Line Interactive UPS가 많이 사용되고 있다. Line Interactive UPS는 Single Stage의 AC/DC 변환기 구조를 갖으며 정상상태에서는 적은 전류로 DC측 에너지 저장장치의 충전상태를 유지만 하면 되므로 운전 효율이 높고 가격이 저렴하다. 그러나 고성능의 전류/전압 제어기술이 요구되므로 제품화하는데 어려움이 많다. 본 논문에서는 MATLAB Simulink와 연동하여 간단히 다양한 제어알고리즘을 구현 할 수 있는 dSPACE 장비를 사용하여 실험 장치를 구축하고 Single Stage UPS의 제어알고리즘을 구현하였다.

• Journal of Astronomy and Space Sciences
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• v.30 no.4
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• pp.307-314
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• 2013

Infrared optical systems are operated at low temperature and vacuum (LT-V) condition, whereas the assembly and alignment are performed at room temperature and non-vacuum (RT-NV) condition. The differences in temperature and pressure between assembly/alignment environments and operation environment change the physical characteristics of optical and opto-mechanical parts (e.g., thickness, height, length, curvature, and refractive index), and the resultant optical performance changes accordingly. In this study, using input relay optics (IO), among the components of the Immersion GRating INfrared Spectrograph (IGRINS) which is an infrared spectrograph, a simulation based on the physical information of this optical system and an actual experiment were performed; and optical performances in the RT-NV, RT-V, and LT-V environments were predicted with an accuracy of $0.014{\pm}0.007{\lambda}$ rms WFE, by developing an adaptive fitting line. The developed adaptive fitting line can quantitatively control assembly and alignment processes below ${\lambda}/70$ rms WFE. Therefore, it is expected that the subsequent processes of assembly, alignment, and performance analysis could not be repeated.

• The Bulletin of The Korean Astronomical Society
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• v.35 no.1
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• pp.58.1-58.1
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• 2010

We carried out simultaneous 22GHz $H_2O$ and 44GHz $CH_3OH$ maser line surveys of about 1000 galactic YSOs using KVN 21m telescopes. The sources consist of low-mass, intermediate-mass, high-mass YSOs in different evolutionary stages. We will present the preliminary results.

• Bulletin of the Korean Space Science Society
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• 1997.04a
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• pp.38.2-38
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• 1997

No Abstract.See Full-text

• Proceedings of the KIPE Conference
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• 1999.07a
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• pp.333-337
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• 1999

This paper presents the DQ transfomation space space vector modulation method to devel control algorithm of distribu STATCON(STATic CONdenser) for line volt regulation, dc link voltage regulation harmonics compensation. The Performance an of a PI with ramp comparision and synchro reference frame current controller is carried Based on these analysis, the control perform are desirable to compensate the harmonics a regulate dc link and line voltage of Distrib line.