Author/Authors :
Nakajima، نويسنده , , Hiroshi and Fujikawa، نويسنده , , Mari and Mori، نويسنده , , Hideki and Kan، نويسنده , , Hiroaki and Ueda، نويسنده , , Shutaro and Kosugi، نويسنده , , Hiroko and Anabuki، نويسنده , , Naohisa and Hayashida، نويسنده , , Kiyoshi and Tsunemi، نويسنده , , Hiroshi and Doty، نويسنده , , John P. and Ikeda، نويسنده , , Hirokazu and Kitamura، نويسنده , , Hisashi and Uchihori، نويسنده , , Yukio، نويسنده ,
Abstract :
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 57.9 MeV cm 2 / mg is used to measure the single event latch-up (SEL) tolerance, which results in a sufficiently low cross-section of σ SEL < 4.2 × 10 − 11 cm 2 /(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 49 years, which satisfies the required latch-up tolerance. The upper limit of the SEU rate is derived to be 1.3×10−3 events/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.
Keywords :
X-Ray , CCD camera , Single event effect , ASIC