Evolution of Alfvénic Magnetic Deflections and Energy Flux Densities from Sub- to Super-Alfvénic Solar Wind Environments
Evolution of Alfvénic Magnetic Deflections and Energy Flux Densities from Sub- to Super-Alfvénic Solar Wind Environments
Dominic Payne1, Mojtaba Akhavan-Tafti2, Samuel Timothy Badman3, Yeimy Rivera4, Michael Louis Stevens4, Kristoff W Paulson4,5, Gary P Zank6, Chen Shi7, Riddhi Bandyopadhyay8 and Prof. William H Matthaeus9, (1)University of Michigan Ann Arbor, Department of Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (2)University of Michigan Ann Arbor, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (3)Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States, (4)Harvard-Smithsonian Center for Astrophysics, Cambridge, United States, (5)University of New Hampshire, Chelmsford, United States, (6)Center for Space Plasma and Aeronomic Research, Department of Space Science, The University of Alabama in Huntsville, Huntsville, United States, (7)University of California, Los Angeles, Los Angeles, United States, (8)Princeton University, Department of Astrophysical Sciences, Princeton, NJ, United States, (9)University of Delaware, Department of Physics and Astronomy, Newark, United States