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Robust Digital Control of Drag-Free Satellites
IFAC Proceedings Volumes, 2003Abstract A drag-free satellite is a small proof-mass (PM) shielded by a spacecraft cavity and moving only subject to gravitational forces. This can be accomplished by a drag-free control keeping the PM centered in the cavity and compensating the non-gravitational forces acting on the spacecraft. A constellation of drag-free satellites can be employed
CANUTO, Enrico, ANDREIS D.
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Drag coefficients for tumbling satellites.
Journal of Spacecraft and Rockets, 1967Figure 3 shows how typical PLOT results are presented. For illustrative purposes, ROD is plotted as a function of normal countdown time, which is extended by the programmed hold. Gain in PLOT is plotted as a function of programmed hold-time; the gain is referenced to RCD for the normal countdown.
LEE H. SENTMAN, STANFORD E. NEICE
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Journal of Geophysical Research: Solid Earth, 1990
The average drag on the LAGEOS satellite appears to be well understood. It consists of three types of drag: Yarkovsky thermal, neutral particle, and charged particle. Yarkovsky thermal drag depends on the LAGEOS spin axis position. The spin axis in the decade since launch appears to have stayed near where the engineering telemetry data put it at apogee
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The average drag on the LAGEOS satellite appears to be well understood. It consists of three types of drag: Yarkovsky thermal, neutral particle, and charged particle. Yarkovsky thermal drag depends on the LAGEOS spin axis position. The spin axis in the decade since launch appears to have stayed near where the engineering telemetry data put it at apogee
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New Satellite Drag Modeling Capabilities
44th AIAA Aerospace Sciences Meeting and Exhibit, 2006This paper reviews the operational impacts of satellite drag, the historical and current capabilities, and requirements to deal with evo lving higher accuracy requirements. Modeling of satellite drag variations showed little improvement from the 1960’s to the late 1990’s. After three decades of essentially no quantitative progress, the problem is being
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Capacitive sensing for drag-free satellites
Classical and Quantum Gravity, 1997We report the key results of a study of the optimization of capacitive sensing for LISA. This work was a component of an ESA study into drag-free satellite control. We discuss the problems associated with the capacitive sensing and control of a proof mass which is electrically isolated and develop models for candidate non-resonant and resonant ...
Clive C Speake, Peter L Andrews
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Interferometric sensing for drag-free satellites
SPIE Proceedings, 2004ABSTRACT We discuss a polarisation based homodyne interferometer that demonstrates a promising sensitivity of approximately. This performance figure is limited above 10 Hz by the resolution of the current analogue-to-digitalconverter (ADC). Sensitivity below 10 Hz is influenced by environmental factors a nd / or noise inherent in the laser.
Clive C. Speake, Stuart M. Aston
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2008
Scientific satellite missions trying to investigate questions regarding geodesy and fundamental physics have become increasingly dependent on ultra low disturbance environments. The precision demanded by the experiments has risen continuously as experimenters strive to deepen their understanding.
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Scientific satellite missions trying to investigate questions regarding geodesy and fundamental physics have become increasingly dependent on ultra low disturbance environments. The precision demanded by the experiments has risen continuously as experimenters strive to deepen their understanding.
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Towards Next Level Satellite Drag Modeling
AIAA Atmospheric and Space Environments Conference, 2010Orbital drag errors adversely impact many space missions including providing collision avoidance warnings for manned spaceflight and other high-value assets, accurately cataloging of all orbiting objects, predicting reentry times and estimating satellite lifetimes, on-board fuel requirements and attitude dynamics.
Frank Marcos +6 more
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Satellite Formation Control using Differential Drag
53rd AIAA Aerospace Sciences Meeting, 2015The ability to operate in formations is a great advantage of small satellites as many small satellites can be built and launched for the cost of one large satellite. Formation operations are valuable because they allow for an observational resolution in time and space not possible with a single large satellite. However, traditional methods of formation
Sanny R. Omar, J. M. Wersinger
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Design considerations for drag free satellites
AIP Conference Proceedings, 1998Missions dictate the implementation of drag free satellites. A variety of missions are used to illustrate the various technologies associated with the TRIAD flight of 1972 and current and past proposed flights.
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