The Carruthers Geocorona Observatory is NASA’s first mission dedicated to investigating the fundamental nature of Earth’s outermost atmospheric layer known as the exosphere. The Carruthers mission’s primary payload is the GeoCoronal Imager, which consists of two co-aligned imagers (channels) for simultaneous, column-volume sensing of ultraviolet emission by exospheric hydrogen atoms. These images will be used to determine the spatial structure and temporal variability of the exosphere on global scales, but a prerequisite of that analysis is isolation of the target emission from instrument and scene backgrounds as well as calibration of the absolute photometric sensitivity of the cameras. This thesis develops the calibration algorithms that will be used for mission data analysis, including: (i) bias and dark current estimation and subtraction, (ii) estimation and subtraction of energetic particle radiation backgrounds, (iii) background photon scene gradient detection and removal, and (iv) flat-fielding. The algorithms are validated using a synthetic image model to measure their accuracy and precision, while laboratory calibration data is used to verify instrument performance against design requirements.
Use this login method if you
don't
have an
@illinois.edu
email address.
(Oops, I do have one)
IDEALS migrated to a new platform on June 23, 2022. If you created
your account prior to this date, you will have to reset your password
using the forgot-password link below.