SunCET: A compact EUV instrument to fill a critical observational gap
James Paul Mason, Phillip C. Chamberlin, Daniel Seaton, Joan, Burkepile, Robin Colaninno, Karin Dissauer, Francis G. Eparvier, Yuhong Fan,, Sarah Gibson, Andrew R. Jones, Christina Kay, Michael Kirk, Richard Kohnert,, W. Dean Pesnell, Barbara J. Thompson, Astrid M. Veronig

TL;DR
SunCET is a compact EUV instrument designed to track coronal mass ejections in the middle corona, utilizing innovative detector technology for simultaneous high dynamic range imaging and spectroscopy, suitable for CubeSat deployment.
Contribution
The paper introduces SunCET, a novel compact EUV instrument with simultaneous high dynamic range imaging and spectroscopy, eliminating the need for an opaque occulter and enabling efficient CME tracking.
Findings
Innovative detector technology enables simultaneous high dynamic range imaging.
SunCET's compact design suits CubeSat deployment.
Successful Phase A development for NASA CubeSat mission.
Abstract
The Sun Coronal Ejection Tracker (SunCET) is an extreme ultraviolet imager and spectrograph instrument concept for tracking coronal mass ejections through the region where they experience the majority of their acceleration: the difficult-to-observe middle corona. It contains a wide field of view (0-4~\Rs) imager and a 1~\AA\ spectral-resolution-irradiance spectrograph spanning 170-340~\AA. It leverages new detector technology to read out different areas of the detector with different integration times, resulting in what we call "simultaneous high dynamic range", as opposed to the traditional high dynamic range camera technique of subsequent full-frame images that are then combined in post-processing. This allows us to image the bright solar disk with short integration time, the middle corona with a long integration time, and the spectra with their own, independent integration time.…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Stellar, planetary, and galactic studies · CCD and CMOS Imaging Sensors
