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Analysis of a Simulated Optical GSO Survey Observation for the Effective Maintenance of the Catalogued Satellites and the Orbit Determination Strategy KCI 등재 SCOPUS

  • 언어ENG
  • URLhttps://db.koreascholar.com/Article/Detail/305912
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한국우주과학회 (The Korean Space Science Society)
초록


A strategy is needed for a regional survey of geosynchronous orbits (GSOs) to monitor known space objects and detect uncataloged space objects. On the basis of the Inter-Agency Debris Committee’s recommendation regarding the protected region of geosynchronous Earth orbit (GEO), target satellites with perigee and apogee of GEO ± 200 km and various inclinations are selected for analysis. The status of the GSO region was analyzed using the satellite distribution based on the orbital characteristics in publicly available two-line element data. Natural perturbation effects cause inactive satellites to drift to two stable longitudinal points. Active satellites usually maintain the designed positions as a result of regular or irregular maneuver operations against their natural drift. To analyze the detection rate of a single optical telescope, 152 out of 412 active satellites and 135 out of 288 inactive satellites in the GSO region were selected on the basis of their visibility at the observation site in Daejeon, Korea. By using various vertical view ranges and various numbers of observations of the GSO region, the detection efficiencies were analyzed for a single night, and the numbers of follow-up observations were determined. The orbital estimation accuracies were also checked using the arc length and number of observed data points to maintain the GSO satellite catalog.

목차
1. INTRODUCTION
 2. STATUS OF GSO REGION
 3. SIMULATION OF OPTICAL SURVEYOBSERVATION
 4. ORBIT DETERMINATION STRATEGY
 5. DISCUSSION AND SUMMARY
 ACKNOWLEDGEMENTS
 REFERENCES
저자
  • Jin Choi(Korea Astronomy and Space Science Institute,Korea University of Science and Technology)
  • Jung Hyun Jo(Korea Astronomy and Space Science Institute,Korea University of Science and Technology) Corresponding Author
  • Hong-Suh Yim(Korea Astronomy and Space Science Institute)
  • Young-Jun Choi(Korea Astronomy and Space Science Institute,Korea University of Science and Technology)
  • Ju-Young Son(Korea Astronomy and Space Science Institute,Korea University of Science and Technology,Korea Air Force) | Ju-Young Sonv
  • Sun-youp Park(Korea Astronomy and Space Science Institute)
  • Young-Ho Bae(Korea Astronomy and Space Science Institute)
  • Dong-Goo Roh(Korea Astronomy and Space Science Institute) | Dong-Goo Roh1
  • Sungki Cho(Korea Astronomy and Space Science Institute)