Venusian atmospheric and Magellan properties from attitude control data

Details Venusian atmospheric and Magellan properties from attitude control data Venusian atmospheric and Magellan properties from attitude control data

Aug 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994gwu..rept.....c&link_type=abstract

M.S. Thesis George Washington Univ., Hampton, VA. Joint Inst. for Advancement of Flight Sciences.

Computer Science

Aerodynamic Coefficients, Attitude Control, Magellan Spacecraft (Nasa), Moment Distribution, Stability Derivatives, Venus Atmosphere, Angular Velocity, Atmospheric Density, Reaction Kinetics, Reaction Wheels, Scale Height, Stellar Mass, Torque, Variability

Scientific paper

Results are presented of the study of the Venusian atmosphere, Magellan aerodynamic moment coefficients, moments of inertia, and solar moment coefficients. This investigation is based upon the use of attitude control data in the form of reaction wheel speeds from the Magellan spacecraft. As the spacecraft enters the upper atmosphere of Venus, measurable torques are experienced due to aerodynamic effects. Solar and gravity gradient effects also cause additional torques throughout the orbit. In order to maintain an inertially fixed attitude, the control system counteracts these torques by changing the angular rates of three reaction wheels. Model reaction wheel speeds are compared to observed Magellan reaction wheel speeds through a differential correction procedure. This method determines aerodynamic, atmospheric, solar pressure, and mass moment of inertia parameters. Atmospheric measurements include both base densities and scale heights. Atmospheric base density results confirm natural variability as measured by the standard orbital decay method. Potential inconsistencies in free molecular aerodynamic moment coefficients are identified. Moments of inertia are determined with a precision better than 1 percent of the largest principal moment of inertia.

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