The NOAA Goes-12 Solar X-Ray Imager (SXI) 1. Instrument, Operations, and Data

The Solar X-ray Imager (SXI) was launched 23 July 2001 on NOAA’s GOES-12 satellite and completed post-launch testing 20 December 2001. Beginning 22 January 2003 it has provided nearly uninterrupted, full-disk, soft X-ray solar images, with a continuous frame rate significantly exceeding that for previous similar instruments. The SXI provides images with a 1 min cadence and a single-image (adjustable) dynamic range near 100. A set of metallic thin-film filters provides temperature discrimination in the 0.6 – 6.0 nm bandpass. The spatial resolution of approximately 10 arcsec FWHM is sampled with 5 arcsec pixels. Three instrument degradations have occurred since launch, two affecting entrance filters and one affecting the detector high-voltage system. This work presents the SXI instrument, its operations, and its data processing, including the impacts of the instrument degradations. A companion paper (Pizzo et al., this issue) presents SXI performance prior to an instrument degradation that occurred on 5 November 2003 and thus applies to more than 420000 soft X-ray images of the Sun.

[1]  Haimin Wang,et al.  Active-Region Monitoring and Flare Forecasting – I. Data Processing and First Results , 2002 .

[2]  Eric L. Corder Development of the solar x-ray imager (SXI) camera , 1994, Defense, Security, and Sensing.

[3]  Alphonse C. Sterling,et al.  Observational Plasma Astrophysics: Five Years of Yohkoh and Beyond , 1998 .

[4]  Richard Grubb,et al.  Monitoring space weather with the GOES magnetometers , 1996, Optics & Photonics.

[5]  Barbara B. Poppe,et al.  New scales help public, technicians understand space weather , 2000 .

[6]  W. Neupert,et al.  EIT: Extreme-ultraviolet Imaging Telescope for the SOHO mission , 1995 .

[7]  Richard Grubb,et al.  Operational uses of the GOES energetic particle detectors , 1996, Optics & Photonics.

[8]  Martin E. Smithers,et al.  Solar X-ray Imager (SXI) optical performance analysis , 1996, Optics & Photonics.

[9]  David F. Webb,et al.  Results from OSO-IV: The long term behavior of X-ray emitting regions , 1972 .

[10]  John H. Chappell,et al.  Solar x-ray imager (SXI) detector calibration and characterization , 1996, Optics & Photonics.

[11]  John M. Davis,et al.  Metalized polyimide filters for x-ray astronomy and other applications , 1997, Optics & Photonics.

[12]  Allen S. Krieger,et al.  Identification and analysis of structures in the corona from X-ray photography , 1973 .

[13]  R. Rosner,et al.  Recent advances in coronal physics. , 1978 .

[14]  Frank Zimmermann,et al.  Accommodation of the Solar X-Ray Imager (SXI) on the GOES 12 spacecraft , 2004, SPIE Optics + Photonics.

[15]  J. Owens,et al.  The Soft X-ray Telescope for the SOLAR-A mission , 1991 .

[16]  S. Freeland,et al.  Data Analysis with the SolarSoft System , 1998 .