SHINE 2026 abstracts associated with WG1
Authors: Sayak Bose (Princeton University, Princeton Plasma Physics Laboratory), Troy Carter (Oak Ridge National Laboratory), Michael Hahn (Columbia University), Daniel Wolf Savin (Columbia University) andView More
Authors: Isaac Asante (Georgia State University), Viacheslav Sadykov (Georgia State University), Irina Kitiashvili (NASA Ames Research Center) Solar oscillations are reliable diagnostic tools for understandingView More
Authors: Alan Hsu (Harvard University), Jenna Samra (Smithsonian Astrophysical Observatory), Steven Tomczyk (Solar Scientific LLC), Daniel Durusky (Smithsonian Astrophysical Observatory), Jacob Hawthorne (Smithsonian Astrophysical Observatory),View More
Authors: Marc DeRosa (Lockheed Martin Solar and Astrophysics Laboratory), Soumyaranjan Dash (National Solar Observatory), Sushant Mahajan (Stanford University) The evolution of the photospheric magnetic fieldsView More
Authors: Richard Frazin (UMich), Federico Nuevo (CONICET, AR), Alberto Vásquez (CONICET, AR), Enrico Landi (UMich), Ward Manchester (UMich) Solar Rotational Tomography (SRT) of the coronaView More
Authors: Aidan Nakhleh (University of Michigan), Nicholeen Viall (NASA Goddard Space Flight Center), Sue Lepri (University of Michigan), Jim Raines (University of Michigan) Density andView 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
Authors: Elizabeth Wraback (HAO/NSF NCAR), Samaiyah Faird (Alabama A&M University), Thomas Schad (NSO), Urszula Bak-Steslicka (University of Wroclaw), Giuliana de Toma (HAO/NSF NCAR), Yuhong FanView More
Authors: D. Lloveras1,2, L. Balmaceda1,2, F. Iglesias3,4, Y. Machuca3,4, M. Sánchez Toledo3, H. Cremades3,4, C. Sasso5, P. Sahani5, Y. de Leo6,7 & T. Nieves-Chinchilla1 1View More
Authors: Yuhong Fan (NSF NCAR) We present a magnetohydrodynamic simulation of the evolution of a prominence-forming coronal flux rope from quasi-equilibrium to eruption beneath aView More
Authors: Dominic Payne (University of Michigan), Mojtaba Akhavan-Tafti (University of Michigan) Using data from Parker Solar Probe encounters 13-23, we analyze the statistics of switchbacksView More
Authors: Jihyeon Son (Korea Astronomy & Space Science Institute, South Korea), Yong-Jae Moon (Kyung Hee University, South Korea), Young-Sil Kwak (Korea Astronomy & Space ScienceView More
Authors: Jon A. Linker (Predictive Science Inc.), Cooper Downs (Predictive Science Inc.), Ronald M. Caplan (Predictive Science Inc.), James Turtle (Predictive Science Inc.), Pete RileyView More
Authors: KD Leka (NWRA), Karin Dissauer (U. Graz, NWRA), Graham Barnes (NWRA) Solar flares are often “eruptive”, sending mass into the corona and often intoView More
Authors: John T. Stefan (New Jersey Institute of Technology) & Alexander G. Kosovichev (New Jersey Institute of Technology) With the increasing focus on space weatherView More
Authors: Krishnendu Mandal (New Jersey Institute of Technology), Alexander G. Kosovichev (New Jersey Institute of Technology) The precise location of the solar dynamo remains anView More
Authors: Peijin Zhang (Center for Solar-Terrestrial Research, New Jersey Institute of Technology, Newark, NJ 07102, USA), Bin Chen (Center for Solar-Terrestrial Research, New Jersey InstituteView More
Authors: Kelly Victor-French (U.S. Naval Research Laboratory), Brian E. Wood (U.S. Naval Research Laboratory), Karl Battams (U.S. Naval Research Laboratory) The publication, “The Relationship BetweenView More
Authors: Eleni Nikou (NRC Research Associate, U.S. Naval Research Laboratory), Evangelos Paouris (The Johns Hopkins University Applied Physics Laboratory), Norberto Romanelli (Department of Astronomy, UniversityView More
Authors: Marcel F. Corchado Albelo (University of Colorado Boulder/LASP/NSO), Maria D. Kazachenko (Univeristy of Colorado Boulder/LASP/NSO), Joel T. Dahlin (Univeristy of Maryland/GSFC), Ryan J. FrenchView More
Authors: Chris Jia (Stanford University), Aimee Norton (Stanford University) We study the flux emergence of active regions from 10^20-10^23 Mx and correlated their flux emergenceView More
Authors: Mehmet Sarp Yalim (The University of Alabama in Huntsville), Clayton Reece (University of Georgia), Christian Beck (National Solar Observatory), Sanjiv K. Tiwari (SETI Institute),View More
Authors: Dana Longcope (Montana State University), Roger Scott (Montana State University) A key element of the CSHKP eruptive flare model is a current sheet (CS)View More
Authors: Jenny M Rodríguez-Gómez (The Catholic University of America and NASA Goddard Space Flight Center), Laura Balmaceda (George Mason University), Alison Farrish (George Mason University)View More
Authors: Satyam Agarwal (CSPAR, UAH, USA), Alphonse C. Sterling (NASA Marshall Space Flight Center, USA), Shibu K. Mathew (Udaipur Solar Observatory, PRL, India), Ronald LView More
Authors: Caroline L. Evans (Univeristy of Colorado Boulder, CIRES, NSO), Cooper Downs (Predictive Science Inc.), Donald Schmit (CIRES) The magnetic field of the Sun isView More
Authors: Sarah Bruce (University of Colorado Boulder), Kevin Reardon (NSO) Measuring the temperature of the different constituents of the coronal plasma can provide information onView More
Authors: Chris Lowder (Southwest Research Institute), William Ashfield IV (Southwest Research Institute) , Charles Kankelborg (Montana State University) , and Sean-Eowyn Brannon (Montana State University)View More
Authors: Vasyl Yurchyshyn (Big Bear Solar Observatory), Seth Garland (Sagamore Hill Solar Observatory) We present an investigation of the 3D coronal magnetic field evolution associatedView More
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
Authors: Cole Tamburri (CU Boulder, LASP, NSO), Maria Kazachenko (CU Boulder, LASP, NSO), Ryan French (LASP), Adam Kowalski (CU Boulder, LASP, NSO), Rahul Yadav (LASP,View More
Authors: Ziyang Zhang (NJIT), Qin Li (NJIT), Vasyl Yurchyshyn (BBSO), Kangwoo Yi (NJIT), Haimin (BBSO & NJIT), Bo Shen (NJIT) Strong chromospheric absorption lines suchView More
Authors: Talwinder Singh (Department of Physics & Astronomy, Georgia State University, Atlanta, GA 30303, USA), Timothy S. Newman (Department of Computer Science, University of AlabamaView More
Authors: Jialiang Li (Institute for Space Weather Sciences, New Jersey Institute of Technology), Vasyl Yurchyshyn (Big Bear Solar Observatory, New Jersey Institute of Technology), JasonView More