Associated with SHINE 2026 Session 10
Authors: Anthony Atkinson (Rice University), David Alexander (Rice University) Observations of magnetic fields in extrasolar environments are critical to the current theories of planetary formation,View More
Authors: Chip Manchester (University of Michigan), Igor Sokolov (University of Michigan), Gergely Koban (University of Michigan), Nishtha Sachdeva (University of Michigan), Lulu Zhao (University ofView More
Authors: Samuel J. Schonfeld (AFRL/Space Warfare Directorate), Laura Balmaceda (George Mason University, NASA Goddard Space Flight Center), Alison Farrish (George Mason University, NASA Goddard SpaceView More
Authors: Evangelos Paouris (JHUAPL), Samantha Wallace (Department of Physical Sciences, Embry-Riddle Aeronautical University), Angelos Vourlidas (JHUAPL), Charles Nick Arge (GSFC, NASA) We present a 3DView More
Authors: Julian Toczylowski (Andrews University), Jay Johnson (Andrews University), Simon Wing (Johns Hopkins University), and Thierry Dudok de Wit (ISSI) To better understand the dynamicsView More
Authors: Andres Munoz-Jaramillo (Southwest Research Institute), Isabel Tejada-Sanchez (Universidad de los Andes), Phoebe Mahlin (Universidad de California – Berkeley), Claudia Holland (Universidad de California –View More
Authors: Abhinav G. Iyer (The University of Sydney), Michael S. Wheatland (The University of Sydney) Solar flares and coronal mass ejections (CMEs) are energetic eventsView More
Authors: Cooper Downs (PSI) Modern studies of coronal heating often involve conducting magnetohydrodynamic (MHD) or field-aligned hydrodynamic (HD) simulations of realistic magnetic field configurations inView More
Length of magnetic field lines for an area at the 1 A.U. surface. A Poincaré map shows the intersections of 3 field lines with the surface.
Authors: Ronald M. Caplan (Predictive Science Inc.), Tinatin Baratashvili (KU Leuven), Evangelia Samara (NASA Goddard Space Flight Center), Talwinder Singh (Georgia State University), Elena ProvornikovaView More