Home
General Overview
Online Documents
Flight
Performance
 
Access to Data
 
Daily Observation History
Photo Gallery
Related Sites
Personnel
Intranet
Rules of the Road
Contact Us
The Final Word
Stellar Alignment of the High Resolution Doppler Imager
A. R. Marshall, D. A. Gell, J. H. Yee, D. A. Ortland, M. D. Burrage, W. R. Skinner, and P. B. Hays (1995), Stellar Alignment of the High Resolution Doppler Imager, Journal of Spacecraft and Rockets, VOL. 32, NO. 6, pages 1039-1043, Nov-Dec 1995.

Abstract:

A method is described for determining the angular misalignment between the High Resolution Doppler Imager instrument and its spacecraft, the Upper Atmospheric Research Satellite, using observations of stars by the instrument. Roll, pitch, and yaw misalignments have been measured to within 0.0025 deg (1 σ), which is an order of magnitude better than the largest tolerable alignment error. The misalignment results are validated using observations of the nighttime 5577-Å O(1S) green line emission. In addition, the long-term behavior of the derived alignment offsets, which shows a clear dependence of the alignment on the solar β angle, is presented.

 
Hrdi_web_support@umich.edu