Considering the future long-term space mission programs, many scientific targets will require a payload that includes an UV imager spectrograph. For instance, future missions on gas or ice giant planets will require imaging spectroscopy for a comprehensive study of the aurora footprints and polar magnetosphere as well as the characteristics of the upper atmosphere or exosphere of their satellites.
MIRA: A Low-Noise Pixelated ASIC for Photon Counting Applications
Fabbrica, Edoardo;Carminati, Marco;Fiorini, Carlo
2023-01-01
Abstract
Considering the future long-term space mission programs, many scientific targets will require a payload that includes an UV imager spectrograph. For instance, future missions on gas or ice giant planets will require imaging spectroscopy for a comprehensive study of the aurora footprints and polar magnetosphere as well as the characteristics of the upper atmosphere or exosphere of their satellites.File in questo prodotto:
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Capitolo_MIRA.pdf
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