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- SH51B-06: A Statistical Survey of Faint Solar X-ray Transients Observed by NuSTAR
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NOLA CC
Author(s):Generic 'disconnected' Message
Reed Masek, University of Minnesota Twin Cities (First Author, Presenting Author)
Lindsay Glesener, University of Minnesota Twin Cities
Jessie Duncan, Marshall Space Flight Center
Mary Davenport, Gustavus Adolphus College
Kekoa Lasko, University of Minnesota Twin Cities
Ian Markano, University of Minnesota Twin Cities
Zasha Avery, University of Minnesota Twin Cities
Marianne Peterson, University of Minnesota Twin Cities
Natalia Bajnokova, University of Glasgow
Kristopher Cooper, University of Minnesota Twin Cities
Iain Hannah, University of Glasgow
Brian Grefenstette, California Institute of Technology
Stephen White, Air Force Research Laboratory
Hugh Hudson, University of Glasgow
Sam Krucker, FHNW
David Smith, University of California Santa Cruz
Sarah Paterson, University of Glasgow
The frequency of lower energy solar flares can be extrapolated by studying of higher energy. These smaller flares are of interest as they are to have a major role in answering the coronal heating problem - one the major open problems in astrophysics of explaining why the solar the outermost layer of the Sun, has a temperature on the order of of degrees. The NuSTAR telescope, while an astrophysics is the most sensitive X-ray telescope to ever look at the Sun. This
presentation showcases an automated flare finding algorithm developed for use with NuSTAR and its application in constraining the frequency of some of the smallest flares ever observed through X-rays.
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