2016 35th Chinese Control Conference (CCC) 2016
DOI: 10.1109/chicc.2016.7554179
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Autonomous orbit determination and observability analysis for formation satellites

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Cited by 5 publications
(2 citation statements)
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“…The Keplerian elements are defined as the semi-major axis a , eccentricity e , inclination i , right ascension of ascending node Ω, argument of perigee ω, and mean argument of latitude u . In Equation (1), five description parameters are used to determine the relative motion in the LVLH frame (Zeng et al, 2012; Hu et al, 2013; Ou et al, 2016). Based on the orbit elements of the chief, the relative orbit elements are obtained with these parameters.…”
Section: Formation Configuration Designmentioning
confidence: 99%
“…The Keplerian elements are defined as the semi-major axis a , eccentricity e , inclination i , right ascension of ascending node Ω, argument of perigee ω, and mean argument of latitude u . In Equation (1), five description parameters are used to determine the relative motion in the LVLH frame (Zeng et al, 2012; Hu et al, 2013; Ou et al, 2016). Based on the orbit elements of the chief, the relative orbit elements are obtained with these parameters.…”
Section: Formation Configuration Designmentioning
confidence: 99%
“…Spacecraft cooperation, taking the advantage of inter-satellite measurements, has been widely used to aid navigation performance [1][2][3][4] . Usually, cooperative navigation relies on a main satellite which processes all measurements collected by other spacecraft and estimates the states of all spacecraft [5][6][7] . This centralized system introduces notable challenges, such as the single-point failure of that one spacecraft on constellation navigation, coupled with an increasing computation burden as the amount of satellites increases.…”
Section: Introductionmentioning
confidence: 99%