3 February 2004 Ground performance of the High-Energy Focusing Telescope (HEFT) attitude control system
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The High Energy Focusing Telescope (HEFT) is a balloon-borne, hard x-ray/gamma ray (20-70 keV) astronomical experiment. HEFT's 10 arcminute field of view and 1 arcminute angular resolution place challenging demands on its attitude control system (ACS). A microprocessor-based ACS has been developed to manage target acquisition and sidereal tracking. The ACS consists of a variety of sensors and actuators, with provisions for 2-way ground communication, all controlled by an on-board computer. Ground based pointing performance measurements indicate 1σ jitter of 7" and gyro drift rates of <1" s-1. Jitter is expected to worsen in the flight environment, but star tracker data are expected to reduce drift rates significantly, enabling a predicted 1σ absolute attitude determination of ≥4.7". HEFT is scheduled for flight in Spring 2004.
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Kurt S. Gunderson, Kurt S. Gunderson, C. M. Hubert Chen, C. M. Hubert Chen, Finn Erland Christensen, Finn Erland Christensen, William W. Craig, William W. Craig, Todd A. Decker, Todd A. Decker, Charles James Hailey, Charles James Hailey, Fiona A. Harrison, Fiona A. Harrison, Ryan McLean, Ryan McLean, Ronald E. Wurtz, Ronald E. Wurtz, Klaus Ziock, Klaus Ziock, } "Ground performance of the High-Energy Focusing Telescope (HEFT) attitude control system", Proc. SPIE 5165, X-Ray and Gamma-Ray Instrumentation for Astronomy XIII, (3 February 2004); doi: 10.1117/12.513439; https://doi.org/10.1117/12.513439


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