Abstract
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An implementation of the ideal frame formulation of perturbed Keplerian motion is presented which only requires the integration of a differential system of dimension 7, contrary to the 8 variables traditionally integrated with this approach. The new formulation is based on the integration of a scaled version of the Eulerian set of redundant parameters and slightly improves runtime performance with respect to the 8-dimensional case while retaining comparable accuracy. | |
International
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Si |
JCR
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Si |
Title
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Celestial Mechanics & Dynamical Astronomy |
ISBN
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0923-2958 |
Impact factor JCR
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1,584 |
Impact info
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Volume
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129 |
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10.1007/s10569-017-9778-z |
Journal number
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1-2 |
From page
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137 |
To page
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151 |
Month
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SEPTIEMBRE |
Ranking
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