Abstracts for SHINE 2026
Authors: Marcel Corchado Albelo (University of Colorado, Boulder) In this talk we review recent observations that challenge the applicability of the CSHKP 2D standard flareView More
Authors: Lulu Zhao (University of Michigan), Tamas Gombosi (University of Michigan), and the CLEAR Team The Space Weather Center of Excellence CLEAR: All-CLEAR Solar EnergeticView More
Authors: Alessandro Bruno (NASA/GSFC & CUA) The solar eruptions of 11 November 2025 and 18 January 2026 produced two of the most remarkable space weatherView More
Authors: L. A. Fisk Observations and analysis of the behavior of the open magnetic field of the Sun, the component of the solar magnetic fieldView More
Authors: Jack M. Schroeder (University of Wisconsin-Madison), Jan Egedal (University of Wisconsin-Madison) Observations show particles are efficiently heated at astrophysical shocks. However, the relative contributionView More
Authors: Nada Al-Haddad (UNH), Noe Lugaz (SSC, EOS, UNH), Bin Zhuang (SSC, EOS, UNH), Sahanaj Banu (SSC, EOS, UNH), Charlie Farrugia (SSC, EOS, UNH) CoronalView More
Authors: Lidiya Ahmed; Michael Stevens; Samuel Badman; Aileen Niesta Most solar-wind prediction methods rely on boundary conditions specified at a fixed inner radius, typically derivedView More
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: William Taranto (University of Delaware), Riddhi Bandyopadhyay (University of Delaware) We analyze nearly three solar cycles of magnetic field observations from the Wind spacecraftView More
Authors: Katelyn Youngjohn, Ivan Vasko, Xi Lu, Vadim Roytershteyn We present a statistical analysis of 287 electrostatic solitary waves observed by the Magnetospheric Multiscale SpacecraftView More
Authors: Xiaohan Ma (BU), Lingling Zhao (UAH), Merav Opher(BU) The shape and structure of the heliosphere remain subjects of ongoing debate, particularly regarding the extentView More
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: David Galarza (University of Florida), Alicia Petersen (University of Florida) Pitch angle distributions (PADs) of suprathermal electrons serve as vital topological tracers of theView 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: M. B. Khan (University of Delaware), M. A. Shay (University of Delaware) Magnetic reconnection plays an important role in the turbulent relaxation of space andView More
Authors: Andrew M Leisner (George Mason University), Matt Dupertuis (George Mason University), Jie Zhang (George Mason University), Charles N. Arge (NASA/GSFC) Potential Field Source SurfaceView More
Authors: Anna Fitzmaurice (UMCP), James Drake (UMCP), Marc Swisdak (UMCP) Extreme enhancements of 3He are commonly observed during impulsive SEP events, suggesting the presence ofView More
Authors: Samuel Fordin (NASA GSFC, Greenbelt, MD), Jaye Verniero (NASA GSFC, Greenbelt, MD), Adam Szabo (NASA GSFC, Greenbelt, MD), Yeimy Rivera (Harvard-Smithsonian Center for Astrophysics,View More
Authors: Dinesha V. Hegde (Center for Space Plasma and Aeronomic Research (CSPAR), the University of Alabama in Huntsville (UAH)), Sujit Roy (Earth System Science CenterView More
Authors: Arpita Roddanavar (NJIT), Satoshi Inoue (NJIT), Keitarou Matsumoto (NJIT, Nagoya University), Haimin Wang (NJIT) Magnetic flux ropes (MFRs) are widely regarded as fundamental structuresView More
Authors: Samuel Granovsky (Department of Physics, New Jersey Institute of Technology, Newark, NJ 07102, USA), Alexander G. Kosovichev (Department of Physics, New Jersey Institute ofView More
Authors: Joel Dahlin (University of Maryland, College Park) A major unsolved problem in solar physics is understanding what determines whether a solar flare remains confinedView 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: B. L. Alterman (NASA/GSFC), Yogesh (UIowa), F. Carcaboso (NASA/GSFC), A. Weiss (NASA/GSFC), M. Martinovic (UArizona), J. M. Laming (NRL), B. Maruca (UDel), M. StevensView More
Authors: Mia Mancuso (NJIT), Ju Jing (NJIT), Haimin Wang (NJIT) As instrument resolution has increased our ability to study small scale features on the sunView 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: Meiqi Wang(NJIT), Matsumoto Keitarou(NJIT), Sijie Yu(NJIT), Bin Chen(NJIT), and Wickline, Mallory(NJIT) The acceleration and transport of flare-related solar energetic electrons (SEEs) remain unresolved problemsView More
Authors: Matthias Rempel (HAO/NSF NCAR), Georgios Chintzoglou (LMSAL) We present a data-inspired simulation of NOAA active region AR 11158. To this end we simulate theView More
Authors: Shreya Dwivedi (UW-Madison), Joe Olson (UW-Madison), Jeremiah Kirch (UW-Madison), Paul Gradney (UW-Madison), Hui Li (LANL), Ellen Zweibel (UW-Madison), Jan Egedal (UW-Madison) and Cary ForestView 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: Arman Manookian (New Jersey Institute of Technology), Alexander Kosovichev (New Jersey Institute of Technology), Samuel Granovsky (New Jersey Institute of Technology), Irina Kitiashvili (NASAView More
Authors: Rudra Kafle (Worcester Polytechnic Institute), Cutter Beck (Worcester Polytechnic Institute), Evan Smith (Worcester Polytechnic Institute), Jacob Whitehill (Worcester Polytechnic Institute), and Khagendra Katuwal (NewView More
Authors: Jesse Wilson (Florida Instititute of Technology), Juan Carlos Palacios (Florida Institute of Technology), Jean Perez (Florida Institute of Technology), Sofianne Bourouaine (Florida Institute ofView 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: Vamsee Krishna Jagarlamudi (JHUAPL), Nour Rawafi (JHUAPL) By December 2025, the Parker Solar Probe (PSP) had completed 26 orbits around the Sun. During thisView More
Authors: Alaa Fayad (Department of Physics, The University of Texas at Austin, Austin, TX 78712, USA) , Anna Tenerani (Department of Physics, The University ofView More
Authors: Alvin J. G. Angeles (University of New Hampshire), Harlan E. Spence (University of New Hampshire), Charles W. Smith (University of New Hampshire) Solar-terrestrial interactionsView More
Authors: Mari Paz Miralles, Garrett Keating, Katharine Reeves, Chad Madsen, Mark Gurwell (Center for Astrophysics | Harvard & Smithsonian) The Solar Submillimeter Array (Solar SMA)View More
Authors: Dipanwita Misra(Graduate Student at West Virginia University), Dr. Giulia Murtas(Assistant Professor, Center for KINETIC Plasma Physics, West Virginia University) Current sheet collapse is aView More