Paper
20 September 2007 GOES-13 SXI initial on-orbit performance results
S. M. Hill, V. J. Pizzo, A. A. Reinard, D. A. Biesecker, J. Lemen, P. Catura, M. Morrison, T. Rink, D. Sabolish, R. Stern
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Abstract
On 2006 May 24 NOAA's Geostationary Operational Environmental Satellite (GOES) 13 satellite was launched with the next generation Solar X-ray Imager (SXI) aboard. This instrument represents a significant step forward in performance over the previous SXI flown on GOES-12, even before that instrument suffered serious degradation. Like the previous instrument, the new instrument uses a grazing incidence optical design, but with a new detector and other improvements, it has about 10 times the sensitivity, twice the spatial resolution, and greatly reduced wide-angle scattering compared to the GOES-12 SXI. The GOES-13 SXI completed its 6 month checkout period in December 2006. Performance tests included dark current, flat-field, spatial response, scattered light, pointing stability and jitter. We present initial analyses and results of these tests as well as comparisons to ground test results. In addition, GOES-13 solar observations are compared to solar observations by other instruments. When it enters operations, the GOES-13 SXI will provide continuous, real-time observations of the X-ray Sun at 1-minute cadence.
© (2007) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
S. M. Hill, V. J. Pizzo, A. A. Reinard, D. A. Biesecker, J. Lemen, P. Catura, M. Morrison, T. Rink, D. Sabolish, and R. Stern "GOES-13 SXI initial on-orbit performance results", Proc. SPIE 6689, Solar Physics and Space Weather Instrumentation II, 66890H (20 September 2007); https://doi.org/10.1117/12.734738
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KEYWORDS
Sun

Scattering

Sensors

X-rays

Coronagraphy

Image filtering

Satellites

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