The SMILE Soft X-ray Imager (SXI) CCD design and development

被引:16
|
作者
Soman, M. R. [1 ]
Hall, D. J. [1 ]
Holland, A. D. [1 ]
Burgon, R. [1 ]
Buggey, T. [1 ]
Skottfelt, J. [1 ]
Sembay, S. [2 ]
Drumm, P. [2 ]
Thornhill, J. [2 ]
Read, A. [2 ]
Sykes, J. [2 ]
Walton, D. [3 ]
Branduardi-Raymont, G. [3 ]
Kennedy, T. [3 ]
Raab, W. [4 ]
Verhoeve, P. [4 ]
Agnolon, D. [4 ]
Woffinden, C. [5 ]
机构
[1] Open Univ, Walton Hall, Milton Keynes MK7 6AA, Bucks, England
[2] Univ Leicester, Leicester LE1 7RH, Leics, England
[3] Univ Coll London, Mullard Space Sci Lab, Surrey RH5 6NT, England
[4] Estec, Directorate Sci European Space Agcy, NL-2201 AZ Noordwijk, Netherlands
[5] Teledyne E2v, Chelmsford CM1 2QU, Essex, England
来源
关键词
Solid state detectors; Space instrumentation; X-ray detectors; X-ray detectors and telescopes; CHARGE-COUPLED-DEVICES; SOLAR-WIND; MAGNETOSPHERE; DAMAGE;
D O I
10.1088/1748-0221/13/01/C01022
中图分类号
TH7 [仪器、仪表];
学科分类号
0804 ; 080401 ; 081102 ;
摘要
SMILE, the Solar wind Magnetosphere Ionosphere Link Explorer, is a joint science mission between the European Space Agency and the Chinese Academy of Sciences. The spacecraft will be uniquely equipped to study the interaction between the Earth's magnetosphere-ionosphere system and the solar wind on a global scale. SMILE's instruments will explore this science through imaging of the solar wind charge exchange soft X-ray emission from the dayside magnetosheath, simultaneous imaging of the UV northern aurora and in-situ monitoring of the solar wind and magnetosheath plasma and magnetic field conditions. The Soft X-ray Imager (SXI) is the instrument being designed to observe X-ray photons emitted by the solar wind charge exchange process at photon energies between 200 eV and 2000 eV. X-rays will be collected using a focal plane array of two custom-designed CCDs, each consisting of 18 mu m square pixels in a 4510 by 4510 array. SMILE will be placed in a highly elliptical polar orbit, passing in and out of the Earth's radiation belts every 48 hours. Radiation damage accumulated in the CCDs during the mission's nominal 3-year lifetime will degrade their performance (such as through decreases in charge transfer efficiency), negatively impacting the instrument's ability to detect low energy X-rays incident on the regions of the CCD image area furthest from the detector outputs. The design of the SMILE-SXI CCDs is presented here, including features and operating methods for mitigating the effects of radiation damage and expected end of life CCD performance. Measurements with a PLATO device that has not been designed for soft X-ray signal levels indicate a temperature-dependent transfer efficiency performance varying between 5 x 10(5) and 9 x 10(4) at expected End of Life for 5.9 keV photons, giving an initial set of measurements from which to extrapolate the performance of the SXI CCDs.
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页数:11
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