2014
DOI: 10.1016/j.actaastro.2014.06.012
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Experimental results of debris orbit predictions using sparse tracking data from Mt. Stromlo

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Cited by 20 publications
(7 citation statements)
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“…To make the transition from the optical tracking to the DLR as fast as possible, one would demand the OD use as little angular data of the object as possible. It is well known, however, when only angular data over a short orbit arc is available, the OD computation would not converge because of the poor distribution of tracking data and the unknown ballistic coefficient of the object [ 20 , 21 , 22 ]. To achieve the OD convergence, extra information has to be used in the OD computation.…”
Section: Methodsmentioning
confidence: 99%
“…To make the transition from the optical tracking to the DLR as fast as possible, one would demand the OD use as little angular data of the object as possible. It is well known, however, when only angular data over a short orbit arc is available, the OD computation would not converge because of the poor distribution of tracking data and the unknown ballistic coefficient of the object [ 20 , 21 , 22 ]. To achieve the OD convergence, extra information has to be used in the OD computation.…”
Section: Methodsmentioning
confidence: 99%
“…The following perturbation models will be employed in the OD and OP process; the gravity effect modeled using the EGM 2008 (70 × 70) gravity model; the solid tide model corresponding to the international Earth rotation service (IERS) conventions was used [18]; the gravitational accelerations by Sun and Moon are only considered for the third body perturbations; and the Jacchia-Bowman 2008 atmospheric density will be used in the drag model. When computing the solar radiation force, the area-to-mass ratio of the space debris will first be determined as B C /C D where B C is the initial value of the ballistic coefficient and C D begin the drag coefficient, respectively [19]. Fixing the solar radiation pressure reflectivity coefficient C R , 1.0 (solar radiation is absorbed) [20], and taking its product with the pre-determined area-to-mass simply gives the solar radiation force exerted on the space debris of interest for this study.…”
Section: Ballistic Coefficient Application To the Od/op Processmentioning
confidence: 99%
“…Research related to the initial orbit determination of space objects using shortarc or sparse measurements from different observation sources is studied in depth (DeMars et al, 2012;Li et al, 2012;Ansalone & Curti, 2013;Bennett et al, 2014;Sang et al, 2014). To the orbit determination using GPS measurements, a large number of studies and effectual methods have been carried out in the past (Montenbruck et al, 2005;Bock et al, 2007;Choi et al, 2010;Gu & Yi, 2011;Chicharro et al, 2013;Wang Xin, 2013).…”
Section: . . . .Introductionmentioning
confidence: 98%