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| Wilbert R. Skinner, Paul B. Hays, Heinz J. Grassl, David A. Gell, Mark D. Burrage, Alan R. Marshall, David A. Ortland (1994), Optical Spectroscopic techniques and instrumentation for atmospheric and space research, SPIE-International Society of Optical Engineering, VOL 2266, pages 281-293, July 1994
Abstract:
The High Resolution Doppler Imager (HRDI) on the Upper Atmosphere Research Satellite has been providing measurements of the wind field in the stratosphere, mesosphere and lower thermosphere since November 1991. Examination of various calibration data indicates the instrument has remained remarkably stable since launch. The instrument has a thermal drift of about 30 m/s/˚C (slightly dependent on wavelength) and a long term temporal drift that has amounted to about 80 m/s. The temperature control of the instrument has improved significantly since launch as a new method was implemented. The initial temperature control held the instrument temperature at about ±1˚C. The improved method, which holds constant the temperature of the optical bench instead of the radiator, keeps the instrument at about 0.2˚C. The calibration indicates very little change in the sensitivity of the instrument. The detector response has shown no degradation and the optics have not changed their transmittance.
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