SHINE 2024 abstracts associated with WG1
Authors: J. Lorincik (BAERI/LMSAL), V. Polito (LMSAL; Department of Physics, Oregon State University), G. Kerr (NASA GSFC; Catholic University of America), L. Hayes (ESTEC) TheView More
Authors: Rohit Chhiber (NASA GSFC & U Delaware) (Draft:) Global inner-heliospheric magnetohydrodynamic (MHD) models aim to represent large-scale properties of the solar wind from theView More
Authors: Surajit Mondal (NJIT), Bin Chen (NJIT) , Dale Gary (NJIT) , Peijin Zhang (NJIT,UCAR), Gregg Hallinan (Caltech) and the OVRO-LWA team The middle coronaView More
Authors: Maria D. Kazachenko (University of Colorado Boulder / National Solar Observatory), Yuhong Fan (High Altitude Observatory), Andrei Afanasev (University of Colorado Boulder / NationalView More
Authors: Gabriela Gonzalez (CU/LASP), Phillip Chamberlin (LASP), Vicki Herde (CU/LASP) The Extreme ultraviolet Variability Experiment (EVE) is one of three instruments onboard the Solar DynamicsView More
Authors: Andrew Leisner (George Mason University), Jie Zhang (George Mason University), Nick Arge (Goddard Space Flight Center), Scarlett Adams (Harvard University), Angela Jin (Phillips AcademyView More
Authors: Peter W. Schuck (NASA/GSFC), Mark G. Linton (NRL), and James E. Leake (NASA/GSFC) Understanding the evolution of electric currents in the solar corona isView More
Authors: Evan P. Shimoun (University of Michigan), Susan T. Lepri (University of Michigan), Jim M. Raines (University of Michigan), Lynn B. Wilson (Goddard Space FlightView More
Authors: Shirsh Lata Soni (CLaSP, University of Michigan), Mojtaba Akhavan-Tafti (CLaSP, University of Michigan) Switchbacks are discrete angular deflections in the solar wind radial magneticView More
Authors: Isaac Kofi Asante The Helioseismic and Magnetic Imager (HMI) onboard the Solar Dynamics Observatory performs full disk observations of the Sun in the FeView More
Authors: M. P. Miralles (Center for Astrophysics | Harvard & Smithsonian), N. Karna (Center for Astrophysics | Harvard & Smithsonian), I. Vivas-Abad (Center for AstrophysicsView More
Authors: Y. J. Rivera (Center for Astrophysics | Harvard & Smithsonian), J. Samra (Center for Astrophysics | Harvard & Smithsonian), S. T. Badman (Center forView More
Authors: Samuel T. Badman (Center for Astrophysics | Harvard & Smithsonian) , Stuart D. Bale (UC Berkeley), Michael L. Stevens (Center for Astrophysics | HarvardView More
Authors: Cooper Downs (PSI), Jon A. Linker (PSI), Peter Riley (PSI), Emily I. Mason (PSI), Ronald M. Caplan (PSI), Roberto Lionello (PSI) In this posterView More
Authors: Tamima Saba (Georgia State University), Viacheslav Sadykov (Georgia State University), Piet Martens (Georgia State University) Understanding the nature of a flare in terms ofView More
Authors: Wei Liu (Lockheed Martin Solar and Astrophysics Laboratory and Bay Area Environmental Research Institute), Meng Jin (Lockheed Martin Solar and Astrophysics Laboratory), Tongjiang WangView More
Authors: Nian Liu (NJIT), Satoshi Inoue (NJIT), Ju Jing (NJIT, BBSO), Haimin Wang (NJIT, BBSO) We conducted data-constrained magnetohydrodynamic (MHD) simulations of consecutive flares (twoView More
Authors: Tyler Eddy (University of Michigan), Susan Lepri (University of Michigan), and Jim Raines (University of Michigan) The frozen-in-flux and frozen-in-charge state theorems are importantView More
Authors: de Nolfo, G.A. (NASA Goddard Space Flight Center, Greenbelt, MD), A. Bruno (Catholic University of America, Washington DC / NASA Goddard Space Flight Center,View More
Authors: Evan Yerger (Space Science Center), Benjamin Chandran (University of New Hampshire), Vincent David (Space Science Center), Romain Meyrand (Space Science Center/University of Otago) PerpendicularView More
Authors: Momchil E. Molnar (HAO), Roberto Casini (HAO) The Helium I 1083 nm atomic line can be utilized to infer properties of the solar coronalView More
Authors: Zhaoming Gan (New Mexico Consortium), Hui Li (Los Alamos National Laboratory), Xiangrong Fu (Los Alamos National Laboratory), Senbei Du (Boston University) and Lingling ZhaoView More
Authors: Milan Gosic (LMSAL/BAERI) The quiet regions of the solar surface are densely populated with small and weak flux patches. They contain an amount ofView More
Authors: Caroline L. Evans (University of Colorado Boulder), Cooper Downs (Predictive Science, Inc.), Don Schmit (Cooperative Institute for Research in Environmental Sciences), James Crowley (UniversityView More
Authors: James Crowley (National Solar Observatory; CU Boulder), Cooper Downs (Predictive Science Inc.), Don Schmit (CIRES), Caroline Evans (National Solar Observatory; CU Boulder) Over theView More
Authors: Jackson R. MacTaggart, Susan T. Lepri, Liang Zhao, Lennard A. Fisk During the solar minima of solar cycles 23 and 24, the heliospheric magneticView More
Authors: MohammadReza EskandariNasab (Utah State University), Shah Muhammad Hamdi (Utah State University), Soukaina Filali Boubrahimi (Utah State University) The accurate prediction of solar flares isView More
Authors: Mariana Jeunon (NASA GSFC/CUA), Sophie Musset (APL), Paloma Jol (Leiden Observatory),Ramana Sankar (, University of Minnesota), Lindsay Glesener (University of Minnesota), Lucy Fortson(University ofView More
Authors: CR. Gilly (Southwest Research Institute), Joe Plowman(Southwest Research Institute) This poster will present the EMToolkit dashboard, which is a new python tool that canView More
Authors: Steven Cranmer (University of Colorado Boulder) Many different physical processes have been suggested to explain the origin of the corona and solar wind. AView More
Authors: Arpita Roddanavar (New Jersey Institute of Technology), Satoshi Inoue (New Jersey Institute of Technology) We conducted magnetohydrodynamic (MHD) simulations to understand the erupting processView More
Authors: Roger K. Ulrich (University of California at Los Angeles) The magnetograph developed by Babcock(1953), \citet{1955ApJ…121..349B}, and \citet{1960ApJ…132..218H} has been used by research groups supervisedView More
Authors: Samuel J. Schonfeld (Air Force Research Laboratory), Lily A. Wood (University of New Mexico), Carl J. Henney (Air Force Research Laboratory) The Solar IndicesView More
Authors: Wenda Cao Big Bear Solar Observatory (BBSO) has operated the 1.6-meter Goode Solar Telescope (GST) for over a decade. GST is one of the highest-resolutionView More
Authors: Niharika Godbole (American University, NASA GSFC), Steve Christe (NASA GSFC), Elliad Peretz (NASA GSFC), Natasha Jeffreys (Northumbria University), Daniel Ryan (University of Applied SciencesView More
Authors: E Johnson (University of Delaware) The solar wind is a plasma that frequently exhibits strong departures from local thermal equilibrium (LTE). Previous studies focusingView More
Authors: Tak Chu Li (Dartmouth College), Yi-Hsin Liu (Dartmouth College), and Yi Qi (University of Colorado Boulder) Electron-only magnetic reconnection was first identified by theView More
Authors: Meng Jin (Lockheed Martin Solar and Astrophysics Lab) Coronal Mass Ejection (CME) driven shocks are widely recognized as key drivers of gradual Solar EnergeticView More
Authors: Liana Y. Zhou(Ann Arbor Skyline High School, MI; University of Michigan), S. Rajavelu-Mohan(Washtenaw Technical Middle College, Michigan), Z. Liu(University of Michigan), E. Schneider(Marquette SeniorView More
Authors: Ryan French (National Solar Observatory), Ritesh Patel (Southwest Research Institute), Maria Kazachenko (University of Colorado Boulder / National Solar Observatory), Joel Dahlin (NASA GSFC),View More