In-Flight Hot Pixels and Random Telegraph Signal in Aeolus Accumulation CCDs Operated at Low Temperature

The European Space Agency’s (ESA) Aeolus mission utilized a space-based light detection and ranging (LiDAR) instrument for atmospheric wind measurements. These measurements were derived from signals collected by accumulation charge-coupled Devices (ACCDs), which showed unexpected behavior in flight. During the nearly five-year operation of the exploratory mission, hot pixels in the silicon detectors appeared at an almost-linear rate, most of which exhibited random telegraph signal (RTS) behavior, contrary to predictions based on pre-flight testing. The discrepancy highlights a gap between ground-based radiation tests, typically conducted at room temperature, and in-flight silicon detector conditions of low temperature and low readout noise levels. In-flight dark current activation energies and RTS phenomena observed in ACCD pixels are analysed, including suspected electric field enhancement (EFE) effects. This study compares these in-flight anomalies with literature models that forecast displacement damage dose (DDD)-induced dark current rates to determine if space radiation effects could be the primary cause of the hot pixels.

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Publication Details

Journal
IEEE Transactions on Nuclear Science
Published
2025-04-14
DOI
https://doi.org/10.1109/tns.2025.3558611
Citations
1
Primary Topic
Infrared Target Detection Methodologies
Type
article
Field-Weighted Citation Impact
4.99
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In-Flight Hot Pixels and Random Telegraph Signal in Aeolus Accumulation CCDs Operated at Low Temperature

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In-Flight Hot Pixels and Random Telegraph Signal in Aeolus Accumulation CCDs Operated at Low Temperature

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article en
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Abstract

The European Space Agency’s (ESA) Aeolus mission utilized a space-based light detection and ranging (LiDAR) instrument for atmospheric wind measurements. These measurements were derived from signals collected by accumulation charge-coupled Devices (ACCDs), which showed unexpected behavior in flight. During the nearly five-year operation of the exploratory mission, hot pixels in the silicon detectors appeared at an almost-linear rate, most of which exhibited random telegraph signal (RTS) behavior, contrary to predictions based on pre-flight testing. The discrepancy highlights a gap between ground-based radiation tests, typically conducted at room temperature, and in-flight silicon detector conditions of low temperature and low readout noise levels. In-flight dark current activation energies and RTS phenomena observed in ACCD pixels are analysed, including suspected electric field enhancement (EFE) effects. This study compares these in-flight anomalies with literature models that forecast displacement damage dose (DDD)-induced dark current rates to determine if space radiation effects could be the primary cause of the hot pixels.

IEEE Transactions on Nuclear ScienceVol. 72(8)
Airbus (France) (FR), Institut Superieur de l'Aeronautique et de l'Espace (ISAE-SUPAERO) (FR), Teledyne e2v (United Kingdom) (GB)
Affordable and clean energy
Openalex Percentile: Top 7%
Infrared Target Detection Methodologies
4.99
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