• Title/Summary/Keyword: Science and Technology Space

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DESIGN AND STRUCTURAL ANALYSIS OF DOME ENCLOSURE FOR TRACKING ARTIFICIAL SPACE OBJECTS (인공우주물체 추적용 완전 개폐형 돔의 설계 및 구조해석)

  • Seol, K.H.;Kim, S.J.;Jang, M.;Min, S.W.;Mun, B.S.;Baek, K.M.
    • Publications of The Korean Astronomical Society
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    • v.22 no.4
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    • pp.211-217
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    • 2007
  • We have been making dual dome enclosures which are useful to track artificial space objects at SSNT (Space Science and Technology Lab.) Kyung Hee University. We verified the safety of the dome enclosures using basic design and structure analyses before manufacturing them, and then performed an optimization analysis for economic and safe systems. The dome enclosure has a fully-open type structure to smoothly operate a telescope made in the style of altazimuth mount with very fast tracking. It is also designed to be safe against extreme weather conditions. The general structure of the observatory system consists of the dual dome enclosures at the top of a container. For the structural analyses, we consider the following two methods: (1) gravitational sustain analysis - how the structure supporting the dome withstand the weight of the dome, and (2) wind load analysis that considers the effect of the wind velocity at the region where the observatory is located. The result of overall deformation is found to be less than 0.551mm and the result of equivalent stress is found to be 20.293Mpa, indicating that the dual dome system is reasonably designed. This means structurally to be safe.

FUV Sky Survey Observation of Hot ISM

  • Han Wonyong;Seon Kwang-Il;Park Jang-Hyun;Yuk In-Soo;Nam Uk-Won;Lee Dae-Hee;Min Kyung-Wook;Ryu Kwang-Sun;Shinn Jong-Ho;Edelstein Jerry;Korpela Eric;Nishikida Kaori
    • Bulletin of the Korean Space Science Society
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    • 2005.10a
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    • pp.41-41
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    • 2005
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FIMS Observations of Hot Interstellar Medium

  • Seon Kwang-Il;Kim I. J.;Park J. H.;Shinn J. H.;Lee D. H.;Ryu K. S.;Han W.;Min K. W.;Jin H.;Yuk I. S.;Nam U. W.;Edelstein J.;Nishikida K.
    • Bulletin of the Korean Space Science Society
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    • 2004.10b
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    • pp.49-49
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    • 2004
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Global features of the Cygnus Loop observed with FIMS

  • Seon Kwang-Il;Park Jang-Hyun;Lee Dae-Hee;Jin Ho;Yuk In-Soo;Han Wonyong;Nam Uk-Won;Kim Il-Joong;Shinn Jong-Ho;Ryu Kwang-Sun;Min Kyung W.;Edelstein Jerry;Korpela Erick
    • The Bulletin of The Korean Astronomical Society
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    • v.30 no.1
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    • pp.32.1-32.1
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    • 2005
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A Substorm Injection Event and the Radiation Belt Structure Observed by Space Radiation Detectors onboard Next Generation Small Satellite-1 (NEXTSat-1)

  • Yoo, Ji-Hyeon;Lee, Dae-Young;Kim, Eojin;Seo, Hoonkyu;Ryu, Kwangsun;Kim, Kyung-Chan;Min, Kyoungwook;Sohn, Jongdae;Lee, Junchan;Seon, Jongho;Kang, Kyung-In;Lee, Seunguk;Park, Jaeheung;Shin, Goo-Hwan;Park, SungOg
    • Journal of Astronomy and Space Sciences
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    • v.38 no.1
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    • pp.31-38
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    • 2021
  • In this paper, we present observations of the Space Radiation Detectors (SRDs) onboard the Next Generation Small Satellite-1 (NEXTSat-1) satellite. The SRDs, which are a part of the Instruments for the study of Stable/Storm-time Space (ISSS), consist of the Medium-Energy Particle Detector (MEPD) and the High-Energy Particle Detector (HEPD). The MEPD can detect electrons, ions, and neutrals with energies ranging from 20 to 400 keV, and the HEPD can detect electrons over an energy range from 0.35 to 2 MeV. In this paper, we report an event where particle flux enhancements due to substorm injections are clearly identified in the MEPD A observations at energies of tens of keV. Additionally, we report a specific example observation of the electron distributions over a wide energy range in which we identify electron spatial distributions with energies of tens to hundreds of keV from the MEPD and with energy ranging up to a few MeV from the HEPD in the slot region and outer radiation belts. In addition, for an ~1.5-year period, we confirm that the HEPD successfully observed the well-known outer radiation belt electron flux distributions and their variations in time and L shell in a way consistent with the geomagnetic disturbance levels. Last, we find that the inner edge of the outer radiation belt is mostly coincident with the plasmapause locations in L, somewhat more consistent at subrelativistic energies than at relativistic energies. Based on these example events, we conclude that the SRD observations are of reliable quality, so they are useful for understanding the dynamics of the inner magnetosphere, including substorms and radiation belt variations.

The FUV Sky Survey Map with FIMS

  • Han, Won-Yong;Seon, Kwang-Il;Park, Jang-Hyun;Yuk, In-Soo;Nam, Uk-Won;Lee, Dae-Hee;Min, Kyung-Wook;Ryu, Kwang-Sun;Shinn, Jong-Ho;Edelstein, Jerry;Korpela, Eric;Nishikida, Kaori
    • The Bulletin of The Korean Astronomical Society
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    • v.30 no.2
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    • pp.52.2-52.2
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    • 2005
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