Single event effect characterization of the mixed-signal ASIC developed for CCD camera in space use

We present the single event effect (SEE) tolerance of a mixed-signal application-specific integrated circuit (ASIC) developed for a charge-coupled device camera onboard a future X-ray astronomical mission. We adopted proton and heavy ion beams at HIMAC/NIRS in Japan. The particles with high linear e...

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Published inNuclear instruments & methods in physics research. Section A, Accelerators, spectrometers, detectors and associated equipment Vol. 731; pp. 166 - 171
Main Authors Nakajima, Hiroshi, Fujikawa, Mari, Mori, Hideki, Kan, Hiroaki, Ueda, Shutaro, Kosugi, Hiroko, Anabuki, Naohisa, Hayashida, Kiyoshi, Tsunemi, Hiroshi, Doty, John P., Ikeda, Hirokazu, Kitamura, Hisashi, Uchihori, Yukio
Format Journal Article
LanguageEnglish
Published Elsevier B.V 01.12.2013
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Summary:We present the single event effect (SEE) tolerance of a mixed-signal application-specific integrated circuit (ASIC) developed for a charge-coupled device camera onboard a future X-ray astronomical mission. We adopted proton and heavy ion beams at HIMAC/NIRS in Japan. The particles with high linear energy transfer (LET) of 57.9MeVcm2/mg is used to measure the single event latch-up (SEL) tolerance, which results in a sufficiently low cross-section of σSEL<4.2×10−11cm2/(Ion×ASIC). The single event upset (SEU) tolerance is estimated with various kinds of species with wide range of energy. Taking into account that a part of the protons creates recoiled heavy ions that have higher LET than that of the incident protons, we derived the probability of SEU event as a function of LET. Then the SEE event rate in a low-earth orbit is estimated considering a simulation result of LET spectrum. SEL rate is below once per 49years, which satisfies the required latch-up tolerance. The upper limit of the SEU rate is derived to be 1.3×10−3events/s. Although the SEU events cannot be distinguished from the signals of X-ray photons from astronomical objects, the derived SEU rate is below 1.3% of expected non-X-ray background rate of the detector and hence these events should not be a major component of the instrumental background.
Bibliography:ObjectType-Article-2
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content type line 23
ISSN:0168-9002
1872-9576
DOI:10.1016/j.nima.2013.05.146