Radiation damage to the Hubble Space Telescope during two Solar cycles, and correction of Charge Transfer Inefficiency using ArCTIc

Fuente: arXiv
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Autores principales: Massey, Richard, Kegerreis, Jacob A., Barrios, Juan Paolo Lorenzo Gerardo, Nightingale, James W., Hayes, Richard G., Lagattuta, David, Lentz, Zane D., Leroy, Gavin, Skottfelt, Jesper, Vecchi, Felix, von Wietersheim-Kramsta, Maximilian
Formato: Preprint
Publicado: 2025
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author Massey, Richard
Kegerreis, Jacob A.
Barrios, Juan Paolo Lorenzo Gerardo
Nightingale, James W.
Hayes, Richard G.
Lagattuta, David
Lentz, Zane D.
Leroy, Gavin
Skottfelt, Jesper
Vecchi, Felix
von Wietersheim-Kramsta, Maximilian
author_facet Massey, Richard
Kegerreis, Jacob A.
Barrios, Juan Paolo Lorenzo Gerardo
Nightingale, James W.
Hayes, Richard G.
Lagattuta, David
Lentz, Zane D.
Leroy, Gavin
Skottfelt, Jesper
Vecchi, Felix
von Wietersheim-Kramsta, Maximilian
contents From 2002 to 2025, the Hubble Space Telescope's Advanced Camera for Surveys has suffered in the harsh radiation environment above the protection of the Earth's atmosphere. We track the degradation of its image quality, as Solar protons and galactic cosmic rays have damaged its photosensitive charge-coupled device (CCD) imaging sensors. The rate of damage in low Earth orbit is modulated by $18.5^{+4.5}_{-0.5}$ per cent during an 11 year Solar cycle, peaking $430^{+11}_{-5}$ days after Solar minimum as recorded in the number of sunspots. The type of damage is consistent with defects in the silicon lattice that have all stabilised into one of three configurations. We also present the open-source Algorithm for Charge Transfer Inefficiency correction (ArCTIc) v7. This models the (instantaneous or gradual) capture of photoelectrons into lattice defects, and their release after (a discrete set or continuum of) characteristic time delays, which creates spurious trailing in an image. Calibrated using the trailing of hot pixels, and applied during post-processing of astronomical images, ArCTIc can correct 99.5% of Charge Transfer Inefficiency trailing averaged over the camera's lifetime, and 99.9% of trailing in the worst-affected recent data.
format Preprint
id arxiv_https___arxiv_org_abs_2509_05057
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Radiation damage to the Hubble Space Telescope during two Solar cycles, and correction of Charge Transfer Inefficiency using ArCTIc
Massey, Richard
Kegerreis, Jacob A.
Barrios, Juan Paolo Lorenzo Gerardo
Nightingale, James W.
Hayes, Richard G.
Lagattuta, David
Lentz, Zane D.
Leroy, Gavin
Skottfelt, Jesper
Vecchi, Felix
von Wietersheim-Kramsta, Maximilian
Instrumentation and Methods for Astrophysics
Earth and Planetary Astrophysics
Astrophysics of Galaxies
Solar and Stellar Astrophysics
From 2002 to 2025, the Hubble Space Telescope's Advanced Camera for Surveys has suffered in the harsh radiation environment above the protection of the Earth's atmosphere. We track the degradation of its image quality, as Solar protons and galactic cosmic rays have damaged its photosensitive charge-coupled device (CCD) imaging sensors. The rate of damage in low Earth orbit is modulated by $18.5^{+4.5}_{-0.5}$ per cent during an 11 year Solar cycle, peaking $430^{+11}_{-5}$ days after Solar minimum as recorded in the number of sunspots. The type of damage is consistent with defects in the silicon lattice that have all stabilised into one of three configurations. We also present the open-source Algorithm for Charge Transfer Inefficiency correction (ArCTIc) v7. This models the (instantaneous or gradual) capture of photoelectrons into lattice defects, and their release after (a discrete set or continuum of) characteristic time delays, which creates spurious trailing in an image. Calibrated using the trailing of hot pixels, and applied during post-processing of astronomical images, ArCTIc can correct 99.5% of Charge Transfer Inefficiency trailing averaged over the camera's lifetime, and 99.9% of trailing in the worst-affected recent data.
title Radiation damage to the Hubble Space Telescope during two Solar cycles, and correction of Charge Transfer Inefficiency using ArCTIc
topic Instrumentation and Methods for Astrophysics
Earth and Planetary Astrophysics
Astrophysics of Galaxies
Solar and Stellar Astrophysics
url https://arxiv.org/abs/2509.05057