Kepler accuracy model for co-periodic satellite separation extrema
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Publication:468561
DOI10.1007/s10569-014-9534-yzbMath1298.70043OpenAlexW2092604318WikidataQ59318191 ScholiaQ59318191MaRDI QIDQ468561
Publication date: 7 November 2014
Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10569-014-9534-y
co-periodic orbitsconfiguration manifoldestimated condition numberproper relative extremasatellite relative motion
Constrained dynamics, Dirac's theory of constraints (70H45) Celestial mechanics (70F15) Orbital mechanics (70M20)
Uses Software
Cites Work
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- Computing the critical points of the distance function between two Keplerian orbits via rigorous global optimization
- Distance in the space of energetically bounded Keplerian orbits
- Extrema and nowhere differentiable functions
- On the distance function between two Keplerian elliptic orbits
- Metric spaces of Keplerian orbits
- Introduction to Interval Analysis
- Accuracy and Stability of Numerical Algorithms
- The Discrete Sine Transform and the Spectrum of the Finiteq-ary Tree
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