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The SWAP EUV Imaging Telescope. Part II: In-flight Performance and Calibration

The SWAP EUV Imaging Telescope. Part II: In-flight Performance and Calibration

Publication date: 02 July 2013

Authors: Halain, J.-P. [2013]

Journal: Solar Physics
Volume: 286
Issue: 1
Page: 67
Year: 2013

Copyright: Springer Netherlands

The Sun Watcher with Active Pixel System detector and Image Processing (SWAP) telescope was launched on 2 November 2009 onboard the ESA PROBA2 technological mission and has acquired images of the solar corona every one to two minutes for more than two years. The most important technological developments included in SWAP are a radiation-resistant CMOS-APS detector and a novel onboard data-prioritization scheme. Although such detectors have been used previously in space, they have never been used for long-term scientific observations on orbit. Thus SWAP requires a careful calibration to guarantee the science return of the instrument. Since launch we have regularly monitored the evolution of SWAP's detector response in-flight to characterize both its performance and degradation over the course of the mission. These measurements are also used to reduce detector noise in calibrated images (by subtracting dark-current). Because accurate measurements of detector dark-current require large telescope off-points, we also monitored straylight levels in the instrument to ensure that these calibration measurements are not contaminated by residual signal from the Sun. Here we present the results of these tests and examine the variation of instrumental response and noise as a function of both time and temperature throughout the mission.

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Last Update: Sep 1, 2019 8:44:46 AM
18-May-2022 15:48 UT

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