Radiation effects on the Gaia CCDs after 30 months at L2
Cian Crowley, Asier Abreu, Ralf Kohley, Thibaut Prod'homme, Thierry, Beaufort

TL;DR
This study assesses the radiation effects on Gaia's CCDs over 30 months at L2, comparing in-flight measurements with pre-flight predictions, and finds lower than expected damage due to solar activity and cosmic rays.
Contribution
It provides an in-flight analysis of radiation-induced damage on Gaia CCDs, validating and comparing with pre-flight models, and explores factors influencing radiation effects at L2.
Findings
Radiation damage is less than pre-flight predictions.
Solar activity has been relatively low, reducing damage.
Correlations found between solar events and CTI changes.
Abstract
Since the launch of ESA's Gaia satellite in December 2013, the 106 large-format scientific CCDs onboard have been operating at L2. Due to a combination of the high-precision measurement requirements of the mission and the predicted proton environment at L2, the effect of non-ionizing radiation damage on the detectors was early identified pre-launch as potentially imposing a major limitation on the scientific value of the data. In this paper we compare pre-flight radiation-induced Charge Transfer Inefficiency (CTI) predictions against in-flight measurements, focusing especially on charge injection diagnostics, as well as correlating these CTI diagnostic results with solar proton event data. We show that L2-directed solar activity has been relatively low since launch, and radiation damage (so far) is less than originally expected. Despite this, there are clear cases of correlation between…
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