Tag: 2026 Session 10. Data-driven Time-Dependent Inner Heliospheric Modeling: Methods and Uncertainties

Associated with SHINE 2026 Session 10

June 1, 2026 cdowns@predsci.com

Magnetic Field Line Mappings and Field-Aligned Integrals as a Dimensionality-Reducing Tool to Analyze 3D Models of Coronal Heating and Loop Hydrodynamics

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

May 7, 2026 lionel@predsci.com

Spheromaks in The Time-Dependent Corona and Heliosphere

Authors: Roberto Lionello (PSI), Viacheslav S. Titov (PSI), Cooper Downs (PSI), Jon A. Linker (PSI), Emily I. Mason (PSI), Tibor Török (PSI) Spheromaks or detachedView More

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