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Abstract: Correlation Scale Turbulence as the Driver of Magnetic Reconnection (AGU25)

Correlation Scale Turbulence as the Driver of Magnetic Reconnection

Muhammad Bilal Khan1, Michael A. Shay1, Sean Oughton2, Mr. Subash Adhikari, PhD3, Colby C Haggerty4, Riddhi Bandyopadhyay1, Prof. William H Matthaeus1, Daniel O'Donnell1, Samuel Fordin1, Yan Yang3, Sohom Roy3, Julia E Stawarz5, Paul Cassak6, Francesco Pecora7 and Tai Phan8, (1)University of Delaware, Department of Physics and Astronomy, Newark, United States, (2)Univ of Waikato, Hamilton, New Zealand, (3)University of Delaware, Department of Physics and Astronomy, Newark, DE, United States, (4)University of Chicago, Department of Astronomy and Astrophysics, Chicago, United States, (5)Northumbria University, Space and Atmospheric Physics, London, United Kingdom, (6)West Virginia University, Department of Physics and Astronomy, Morgantown, United States, (7)University of Delaware, Newark, United States, (8)University of California, Berkeley, United States