Sophia A. Sánchez-Maes,1 Johnny Hohttps://orcid.org/0000-0003-4119-4262,1 Isaac Anderson,1 Elias Aguirre-Contreras,1 Carl Barcroft,1 Juliana Barstow,2 David Caldwell,1 Brendan D’Aquino,1,3 Gabriel Dubinsky,1 Thomas M. Gauron,1 Jaesub Hong,1 Almus T. Kenter,1 Christopher S. Moore,1 Rachel Nere,4 Ritesh Pandohie,5 Crisel Suarez1,6
1Ctr. for Astrophysics of Harvard College Observatory and Smithsonian Astrophysical Observatory (United States) 2New Mexico Institute of Mining and Technology (United States) 3Northeastern Univ. (United States) 4Univ. of Massachusetts (United States) 5Cornell Univ. (United States) 6Vanderbilt Univ. (United States)
PERSONAL Sign in with your SPIE account to access your personal subscriptions or to use specific features such as save to my library, sign up for alerts, save searches, etc.
Current-generation solar observatories employ CCD image sensors to observe the Sun in the soft x-ray (SXR) and extreme ultraviolet (EUV) regimes. However, these observations are often compromised by pixel saturation and charge blooming in the CCD image sensors when observing large solar flares. To address these limitations, the Swift Solar Activity x-ray Imager Rocket (SSAXI-Rocket) program is developing CMOS image sensors (CIS) with low noise and high-speed readout (greater than 5Hz) for next-generation solar observatories. These CIS aim to enable the observation of large solar flares while significantly reducing the effects of pixel saturation and charge blooming. As a part of NASA’s 2024 solar flare sounding rocket campaign, the SSAXI-Rocket program demonstrated delta-doped CIS technology in a space environment by operating a novel camera as a sub-payload on board the High-Resolution Coronal Imager (Hi-C) sounding rocket. This paper describes the pre-launch laboratory tests performed with the SSAXI-Rocket CIS to characterize its linearity and soft x-ray spectral resolution.
Conference Presentation
(2024) Published by SPIE. Downloading of the abstract is permitted for personal use only.
PERSONAL Sign in with your SPIE account to access your personal subscriptions or to use specific features such as save to my library, sign up for alerts, save searches, etc.
The alert did not successfully save. Please try again later.
Sophia A. Sánchez-Maes, Johnny Ho, Isaac Anderson, Elias Aguirre-Contreras, Carl Barcroft, Juliana Barstow, David Caldwell, Brendan D’Aquino, Gabriel Dubinsky, Thomas M. Gauron, Jaesub Hong, Almus T. Kenter, Christopher S. Moore, Rachel Nere, Ritesh Pandohie, Crisel Suarez, "SSAXI-Rocket delta-doped CMOS sensors," Proc. SPIE 13103, X-Ray, Optical, and Infrared Detectors for Astronomy XI, 131030N (27 August 2024); https://doi.org/10.1117/12.3020261