4 February 2004 Characterization of the flight CCD detectors for the GOES N and O solar x-ray imagers
Author Affiliations +
Abstract
A new Solar X-ray Imager (SXI) using back-illuminated, anti-blooming CCD technology will become part of the instrument complement on NOAA's GOES (Geosynchronous Orbiting Environmental Satellite) N and O spacecraft, with probable launch dates beginning in the 2004-2005 time frame. SXI N and O were developed under a NASA contract by the Solar and Astrophysics Laboratory at the Lockheed Martin Advanced Technology Center, and are currently being integrated into their respective spacecrafts by Boeing Space Systems. SXI N and O will each provide full disk images of the Sun from 0.2 to 1.2 keV (10-60 Å) through the combination of a grazing incidence telescope, bandpass filters, and an X-ray imaging CCD. The custom designed, back-illuminated CCDs were fabricated and initially tested by Marconi Technologies (formerly EEV Ltd, now e2v technologies), screened in visible light by the Mullard Space Science Laboratory, and fully characterized in both visible light and X-rays at LMSAL. By minimizing the field-free region within the CCD, the spatial resolution at low X-ray energies was significantly improved. The SXI CCDs also exhibit only very modest response changes as a result of solar X-ray exposure, based upon extended life tests. The flight CCDs meet or surpass all specifications for quantum efficiency (QE), spatial uniformity, defects, charge transfer efficiency, QE stability in vacuum, read noise, linearity, full well and dark current. A QE model based on earlier work with ion-implanted, laser-annealed CCDs provides a consistent picture of the CCD response from soft X-rays through far UV wavelengths.
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Robert A. Stern, Robert A. Stern, Lawrence Shing, Lawrence Shing, Paul R. Catura, Paul R. Catura, Mons D. Morrison, Mons D. Morrison, Dexter W. Duncan, Dexter W. Duncan, James R. Lemen, James R. Lemen, Tim Eaton, Tim Eaton, Peter J. Pool, Peter J. Pool, Roy Steward, Roy Steward, Dave M. Walton, Dave M. Walton, Alan Smith, Alan Smith, } "Characterization of the flight CCD detectors for the GOES N and O solar x-ray imagers", Proc. SPIE 5171, Telescopes and Instrumentation for Solar Astrophysics, (4 February 2004); doi: 10.1117/12.506346; https://doi.org/10.1117/12.506346
PROCEEDINGS
12 PAGES


SHARE
RELATED CONTENT

Information Storage Requirements In Radiology
Proceedings of SPIE (December 25 1979)
XEUS wide field imager first experimental results with the...
Proceedings of SPIE (February 02 2004)
CCD development and characterization for the GOES N and O...
Proceedings of SPIE (October 21 1999)
High-accuracy x-ray imaging: screen, lens, and CCD
Proceedings of SPIE (September 13 1993)
Soft x-ray cathode and its application in Lixiscope
Proceedings of SPIE (February 01 2006)

Back to Top