2A geopotential expressed in, 'terms of a nonsingular set of orbital eleme~nts is used to iteratively compute Kozai mean orbital elements from either Broiwer mean orbital elemntsor iertal scuiaiing Cartesian position and velocity vecOrs.Atog th computational procedure is general in nature, KMEC has been t ijored to generate Kozai mean elemenis afrm4-hti-dretly-appliable-hir-use-fidie MX 1 502-DS and modified TRANET II geoceivers. a-IC/6
2A geopotential expressed in, 'terms of a nonsingular set of orbital eleme~nts is used to iteratively compute Kozai mean orbital elements from either Broiwer mean orbital elemntsor iertal scuiaiing Cartesian position and velocity vecOrs.Atog th computational procedure is general in nature, KMEC has been t ijored to generate Kozai mean elemenis afrm4-hti-dretly-appliable-hir-use-fidie MX 1 502-DS and modified TRANET II geoceivers. a-IC/6
“…We begin with writing the geopotential and the Lagrange equations with respect to the non-singular elements for eccentricity. Several authors have already expressed the Lagrange equations in non-singular elements: for example (Giacaglia, 1977;Nacozy and Dallas, 1977;Wytrzyszczak, 1986). Here, we write the equations again not only to be self-consistent, but also to give an explicit expression of the coefficients involved in the expansion as power series of the eccentricity of the main differential system.…”
“…- (78) This set only presents a singularity for i " 180˝, a case that is often not interesting for practical applications. The expression for the osculating equations of motion in Lagrange form is provided by Giacaglia [42]. Letting γ " ?…”
Section: E T H O D O F Av E R a G I N G A N D I N T E G R At I O N mentioning
confidence: 99%
“…In the practical calculation of the A i,1 , we have to take into account their dependence from the total disturbing function R " R C`R 1 . After eliminating the short-periodic terms included in their expansions by setting q " 2p´l, we plug them in Equation 95 [42]:…”
Section: Averaged Equations Of Motionmentioning
confidence: 99%
“…We show the equations of motion for the set of equinoctial elements E as presented by Giacaglia [42] and Nacozy and Dallas [74], which is expressed in terms of the classical orbital elements as We recall that the components of the incoming (pre-encounter) asymptotic velocity U " v Ast´vC in the pX, Y, Zq frame defined in subsection 3.1.1 are defined by the quantities U, θ, φ:…”
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