Abstracts associated with SHINE 2026 invited speakers with no poster.
Authors: Tyler Reese (University of Arizona) Joe Giacalone (University of Arizona) The New Horizons mission is expected to cross the Solar Wind Termination Shock withinView More
Authors: Bishwas L. Shrestha (Princeton University) Pickup ions (PUIS) produced by the ionization of interstellar and inner-source neutral atoms and subsequently advected by the solarView More
Authors: Matthias Rempel (HAO/NSF NCAR) In this scene setting talk I will provide an overview of recent 3D flare models. I will focus specifically onView More
Authors: Urszula Bąk-Stęślicka (Astronomical Institute, University of Wrocław, Poland), Sarah E. Gibson (National Center for Atmospheric Research, Boulder, CO 80305, USA), Marek Stęślicki (Space ResearchView More
Authors: Bishwas L. Shrestha (Princeton University) Interplanetary shocks driven by solar wind structures propagate outward, evolving continuously as they sweep through the outer heliosphere. AsView More
Authors: Chen Shi (Department of Physics, Auburn University) The solar wind is highly turbulent, containing fluctuations that span a wide range of spatial and temporalView More
Authors: Georgios Chintzoglou (Lockheed Martin Solar and Astrophysics Lab) Solar magnetic fields appear on a wide range of spatial scales, from the quiet Sun andView More
Authors: Evan Yerger (Space Science Center, University of New Hampshire) The heating and acceleration of the solar wind remain an enduring mysteries in heliophysics. AView More
Authors: S. E. Gibson (NSF NCAR/HAO) In this talk I will discuss CMEs, from their initiation in the lower solar corona to their propagation andView More
Authors: Gregory G. Howes (University of Iowa) The evolution of heliospheric plasmas is strongly influenced by kinetic plasma physics processes that govern the flow ofView More
Authors: Lindsay Glesener The new data from large radio observatories with many antennas will revolutionize the investigations we can perform on the Sun. In thisView More
Authors: Yuhong Fan (HAO/NSF NCAR) We present magnetohydrodynamic simulations of the evolution of a prominence-forming coronal flux rope from quasi-equilibrium to eruption beneath a coronalView More
Authors: Mausumi Dikpati (NSF-NCAR, HAO) Flux emergence is often described as magnetic tubes rising through the convection zone, but the central unresolved issue is whetherView More
Authors: Tams I. Gombosi (University of Michigan) Physics-based simulations of SEP events are one of the computational grand challenges of heliophysics. They are also essentialView More
Authors: Andres Munoz-Jaramillo (Southwest Research Institute) The application of Artificial Intelligence (AI) to solve scientific objectives contains an intrinsic tension between versatility and interpretability. OnView More
Authors: Steven R. Cranmer (CU Boulder) Coronal heating and solar wind acceleration are not “problems” because of an absence of proposed explanations, but because thereView More
Authors: Steven R. Cranmer (CU Boulder) In the parts of the solar corona and solar wind that experience the fewest particle-particle collisions, the various constituentsView More
Authors: S. Raptis (Johns Hopkins Applied Physics Laboratory), D. L. Turner (Johns Hopkins Applied Physics Laboratory), T. Horbury (Imperial College London), D. Chakrabarty (PRL-Gujarat, India),View More
Authors: Katie Whitman (KBR, NASA JSC SRAG), The SRAG Team (NASA JSC SRAG) From https://www.nasa.gov/blogs/missions/2026/04/11/artemis-ii-astronauts-back-in-houston-reunite-with-families/ The Artemis II crew of NASA astronauts – Reid Wiseman, Victor Glover, and Christina Koch, and CSA (Canadian Space Agency)View More