New Synchronous Orbits Using the Geomagnetic Lorentz Force
- 1 November 2007
- journal article
- Published by American Institute of Aeronautics and Astronautics (AIAA) in Journal of Guidance, Control, and Dynamics
- Vol. 30 (6), 1677-1690
- https://doi.org/10.2514/1.29080
Abstract
Repeat groundtrack orbit is any orbit whose sub-satellite point traces out a recurring pattern in some integer numbers of orbits. Traditionally, these orbits are achieved by adjusting the period of a satellite such that it completes an integer number of orbits in exactly an integer number of sidereal Earth days. Geostationary and Geosynchronous orbits are perhaps the most familiar and useful examples. These orbits have a mean motion equal to the spin rate of the Earth. We shall refer to orbits that repeat their groundtrack every orbit as GT-1 orbits. Thus all GEO orbits are in the GT-1 class. We define a general notation of a GT-x class orbit repeats its groundtrack every x orbits. For example, satellites in the GPS constellation are in 12 sidereal hour orbits, and can thus be considered GT-2 satellites. Many LEO imaging satellites designed for full-Earth coverage also use repeat track orbits. Landsat 7 covers the full Earth every 233 orbits making it a GT-233 satellite: every 16 days, the satellite completes exactly 233 orbits.1 Dedicated weather satellites and both government and commercial communications satellites are just a few of the numerous uses for GT-1 orbits. However GT-1 systems are currently limited to GEO orbits. The altitude of these satellites, roughly 36000km, requires high-power communications and impacts the aperture requirements for Earth-imaging satellites. An ideal arrangement would be a GT-1 orbit at a low Earth altitude. We propose a method of obtaining a low Earth, polar GT-1 orbit with the help of a new propellantless propulsion concept called Lorentz Augmented Orbits (LAO). The Lorentz force experienced by a particle of charge q (Coulombs) moving through a magnetic field ~ BKeywords
This publication has 14 references indexed in Scilit:
- Stabilization of Satellite Motion Relative to a Coulomb Spacecraft FormationJournal of Guidance, Control, and Dynamics, 2005
- Prospects and Challenges for Lorentz-Augmented OrbitsPublished by American Institute of Aeronautics and Astronautics (AIAA) ,2005
- The superposition of rotating and stationary magnetic sources: Implications for the auroral regionPhysics of Plasmas, 2003
- Spacecraft charging, an updateIEEE Transactions on Plasma Science, 2000
- Charged dust in planetary magnetospheres: Hamiltonian dynamics and numerical simulations for highly charged grainsJournal of Geophysical Research, 1994
- Motion of Dust in a Planetary Magnetosphere: Orbit-Averaged Equations for Oblateness, Electromagnetic, and Radiation Forces with Application to Saturn's E RingIcarus, 1993
- An overview of electron and ion beam effects in charging and discharging to spacecraftIEEE Transactions on Nuclear Science, 1989
- The dynamics of weakly charged dust: Motion through Jupiter's gravitational and magnetic fieldsJournal of Geophysical Research, 1987
- SCATHA survey of high‐level spacecraft charging in sunlightJournal of Geophysical Research, 1986
- Lorentz force perturbations of a charged ballistic missilePublished by American Institute of Aeronautics and Astronautics (AIAA) ,1982