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- SH21C-07: CATE 2024: Novel one-hour continuous observations of polarized structure and dynamics of the inner and middle corona during the 2024 total solar eclipse
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Daniel Seaton, Southwest Research Institute Boulder (First Author, Presenting Author)
Amir Caspi, Southwest Research Institute
Sarah Kovac, Southwest Research Institute
Paul Bryans, NSF National Center for Atmospheric Research
Joan Burkepile, National Center for Atmospheric Research
Sarah Davis, Independent Researcher
Craig DeForest, Southwest Research Institute Boulder
David Elmore, National Solar Observatory
Sanjay Gusain, National Solar Observatory
Rebecca Haacker, NSF National Center for Atmospheric Research
James Hughes, Southwest Research Institute
Jason Jackiewicz, New Mexico State University
Derek Lamb, Southwest Research Institute
Valentin Martinez-Pillet, National Solar Observatory
Ritesh Patel, Southwest Research Institute
Kevin Reardon, National Solar Observatory
Willow Reed, University of Colorado Boulder
Anna Tosolini, University of California Berkeley
Andrei Ursache, Independent Researcher
John Williams, National Center for Atmospheric Research
Padma Yanamandra-Fisher, Space Science Institute
Daniel Zietlow, Provare Media and NSF NCAR
Citizen CATE 2024 was a network of individual observatories distributed along the path of the total eclipse on April 8 2025 and operated by community volunteers. Because these observatories were spaced along the whole eclipse path, their observations can be combined into a single, hour-long movie of the solar corona during the time of the eclipse — except for a few stations that were clouded out. Here we report on the first detailed analysis of the data, providing information about the shape, fine structure, and evolution of the sun's million degree atmosphere, the corona, during the eclipse.
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