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  1. The Journal of the Astronautical Sciences
  2. The Journal of the Astronautical Sciences : Volume 62
  3. The Journal of the Astronautical Sciences : Volume 62, Issue 3, September 2015
  4. Low Eccentricity Earth Satellite KAM Tori
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The Journal of the Astronautical Sciences : Volume 65
The Journal of the Astronautical Sciences : Volume 64
The Journal of the Astronautical Sciences : Volume 63
The Journal of the Astronautical Sciences : Volume 62
The Journal of the Astronautical Sciences : Volume 62, Issue 4, December 2015
The Journal of the Astronautical Sciences : Volume 62, Issue 3, September 2015
Low Eccentricity Earth Satellite KAM Tori
Global Search Capabilities of Indirect Methods for Impulsive Transfers
Touchless Electrostatic Three-dimensional Detumbling of Large Axi-symmetric Debris
Reaction Wheel Friction Telemetry Data Processing Methodology and On-Orbit Experience
The Journal of the Astronautical Sciences : Volume 62, Issue 2, June 2015
The Journal of the Astronautical Sciences : Volume 62, Issue 1, March 2015
The Journal of the Astronautical Sciences : Volume 61
The Journal of the Astronautical Sciences : Volume 60
The Journal of the Astronautical Sciences : Volume 59
The Journal of the Astronautical Sciences : Volume 58
The Journal of the Astronautical Sciences : Volume 57
The Journal of the Astronautical Sciences : Volume 56
The Journal of the Astronautical Sciences : Volume 55
The Journal of the Astronautical Sciences : Volume 54

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Low Eccentricity Earth Satellite KAM Tori

Content Provider Springer Nature Link
Author Wiesel, William E.
Copyright Year 2015
Abstract The accuracy of a new theory of Earth satellite motion is assessed across inclination and orbital altitude. This theory is based on periodic orbits in the zonal potential, with a Floquet solution for nearby motion, augmented by perturbation solutions for other perturbing forces. It is completely numerical and well adapted to the rich computational environments of today. Its root mean square error is generally in the tens of meters over a one day data arc, for eccentricities less than e = 0.1. The perturbation methods fail near geopotential resonances, but the theory has been adapted to handle the vicinity of a resonance without significant loss of accuracy. The geometric structure of the solution is also explored, and it is shown that most orbits in the full geopotential are static structures that rotate with the Earth’s rotation. Geopotential KAM tori shrink down to a two dimensional surface as the analog of zero eccentricity orbits. A first attempt is made at visualizing the torus over the Earth’s surface. Precision calculation of low eccentricity KAM tori may lead to much decreased stationkeeping costs for Walker constellations.
Starting Page 197
Ending Page 211
Page Count 15
File Format PDF
ISSN 00219142
Journal The Journal of the Astronautical Sciences
Volume Number 62
Issue Number 3
e-ISSN 21950571
Language English
Publisher Springer US
Publisher Date 2015-12-14
Publisher Place New York
Access Restriction One Nation One Subscription (ONOS)
Subject Keyword KAM tori Extraterrestrial Physics, Space Sciences Mathematical Applications in the Physical Sciences Aerospace Technology and Astronautics Earth orbits
Content Type Text
Resource Type Article
Subject Aerospace Engineering Space and Planetary Science
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