Associated with SHINE 2026 Session 7
Authors: Jia Huang (SSL/UCB), Davin E. Larson (SSL/UCB), Orlando Romeo (SSL/UCB), Mingzhe Liu (SSL/UCB), Roberto Livi (SSL/UCB), Ali Rahmati (SSL/UCB), Phyllis Whittlesey (SSL/UCB), Samer T.View 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: Christina Kay (JHU APL) Remote imaging of the Sun, corona, and interplanetary space allow us to observe structures as they develop and how theyView More
Authors: Phillip Hess (NRL), Erika Palmerio (PSI), Robin Colaninno (NRL), Mark Linton (NRL), Volker Bothmer (Institut für Astrophysik und Geophysik, Georg-August-Universität, Göttingen, Germany) Coronal massView More
Authors: Robin Colaninno (U.S. Naval Research Laboratory), Phillip Hess (U.S. Naval Research Laboratory), Eleni Nikou (NRC Research Associate, U.S. Naval Research Laboratory), Teresa Nieves-Chinicilla (NASAView More
Authors: C. Gilly (NWRA) The PUNCH mission images the young solar wind across a field of view that spans several orders of magnitude in heliocentricView More
Authors: Evangelia Samara (NASA/GSFC and The Catholic University of America), C. Nick Arge (NASA/GSFC), Samuel J. Schonfeld (AFRL), Alison Farrish (NASA/GSFC and George Mason University),View More
Authors: Yeimy J. Rivera (Center for Astrophysics | Harvard & Smithsonian), Parker Solar Probe & Solar Orbiter team Parker Solar Probe (Parker) has completed multipleView 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: 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
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.