Analysis of Linear and Nonlinear Relative Orbit Dynamics for Satellite Formation Flying

Relative dynamic models of satellites which describe the relative motion between two satellites is fundamental for research on the formation flying. The accuracy of various linearized or nonlinear models of relative motion is analyzed and compared. A `Modeling Error Index (MEI)` is defined for evalu...

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Main Authors: Han-Earl Park, Sang-Young Park, Sang-Jin Lee, Kyu-Hong Choi
Format: Article
Language:English
Published: Korean Space Science Society (KSSS) 2009-09-01
Series:Journal of Astronomy and Space Sciences
Subjects:
Online Access:http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2009/v26n3/OJOOBS_2009_v26n3_317.pdf
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spelling doaj-32be6d499d5f465fa02e7d8af6b694872020-11-24T21:34:26ZengKorean Space Science Society (KSSS)Journal of Astronomy and Space Sciences2093-55872093-14092009-09-0126331732810.5140/JASS.2009.26.3.317Analysis of Linear and Nonlinear Relative Orbit Dynamics for Satellite Formation FlyingHan-Earl Park0Sang-Young Park1Sang-Jin Lee2Kyu-Hong Choi3Dept. of Astronomy, Yonsei University, Seoul 120-749, KoreaDept. of Astronomy, Yonsei University, Seoul 120-749, KoreaDept. of Astronomy, Yonsei University, Seoul 120-749, KoreaDept. of Astronomy, Yonsei University, Seoul 120-749, KoreaRelative dynamic models of satellites which describe the relative motion between two satellites is fundamental for research on the formation flying. The accuracy of various linearized or nonlinear models of relative motion is analyzed and compared. A `Modeling Error Index (MEI)` is defined for evaluating the accuracy of models. The accuracy of the relative dynamic models in various orbit circumstance are obtained by calculating the modeling error with various eccentricities of the chief orbit and distances between the chief and the deputy. It is found that the modeling errors of the relative dynamic models have different values according to the eccentricity, J2 perturbation, and the distance between satellites. Since the evaluated accuracy of various models in this paper means the error of dynamic models of the formation flying, the results of this paper are very useful for choosing the appropriate relative model of the formation flying mission.http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2009/v26n3/OJOOBS_2009_v26n3_317.pdfformation flyingrelative motionmodeling error
collection DOAJ
language English
format Article
sources DOAJ
author Han-Earl Park
Sang-Young Park
Sang-Jin Lee
Kyu-Hong Choi
spellingShingle Han-Earl Park
Sang-Young Park
Sang-Jin Lee
Kyu-Hong Choi
Analysis of Linear and Nonlinear Relative Orbit Dynamics for Satellite Formation Flying
Journal of Astronomy and Space Sciences
formation flying
relative motion
modeling error
author_facet Han-Earl Park
Sang-Young Park
Sang-Jin Lee
Kyu-Hong Choi
author_sort Han-Earl Park
title Analysis of Linear and Nonlinear Relative Orbit Dynamics for Satellite Formation Flying
title_short Analysis of Linear and Nonlinear Relative Orbit Dynamics for Satellite Formation Flying
title_full Analysis of Linear and Nonlinear Relative Orbit Dynamics for Satellite Formation Flying
title_fullStr Analysis of Linear and Nonlinear Relative Orbit Dynamics for Satellite Formation Flying
title_full_unstemmed Analysis of Linear and Nonlinear Relative Orbit Dynamics for Satellite Formation Flying
title_sort analysis of linear and nonlinear relative orbit dynamics for satellite formation flying
publisher Korean Space Science Society (KSSS)
series Journal of Astronomy and Space Sciences
issn 2093-5587
2093-1409
publishDate 2009-09-01
description Relative dynamic models of satellites which describe the relative motion between two satellites is fundamental for research on the formation flying. The accuracy of various linearized or nonlinear models of relative motion is analyzed and compared. A `Modeling Error Index (MEI)` is defined for evaluating the accuracy of models. The accuracy of the relative dynamic models in various orbit circumstance are obtained by calculating the modeling error with various eccentricities of the chief orbit and distances between the chief and the deputy. It is found that the modeling errors of the relative dynamic models have different values according to the eccentricity, J2 perturbation, and the distance between satellites. Since the evaluated accuracy of various models in this paper means the error of dynamic models of the formation flying, the results of this paper are very useful for choosing the appropriate relative model of the formation flying mission.
topic formation flying
relative motion
modeling error
url http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2009/v26n3/OJOOBS_2009_v26n3_317.pdf
work_keys_str_mv AT hanearlpark analysisoflinearandnonlinearrelativeorbitdynamicsforsatelliteformationflying
AT sangyoungpark analysisoflinearandnonlinearrelativeorbitdynamicsforsatelliteformationflying
AT sangjinlee analysisoflinearandnonlinearrelativeorbitdynamicsforsatelliteformationflying
AT kyuhongchoi analysisoflinearandnonlinearrelativeorbitdynamicsforsatelliteformationflying
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