Abstracts for WG2 for the SHINE 2025 Workshop
Authors: Christopher Rowell (Florida Institute of Technology), Ming Zhang (Florida Institute of Technology) The solar wind is a continuous stream of hot plasma emanating fromView More
Authors: Noé Lugaz (University of New Hampshire), Bin Zhuang (University of New Hampshire), Nada Al-Haddad University of New Hampshire), Sahanaj Banu (University of New Hampshire),View More
Authors: Evangelia Samara (NASA/GSFC), Elena Provornikova (JHU/APL), C. Nick Arge (NASA/GSFC), Viacheslav Merkin (JHU/APL) In this work, we use the coupled WSA model of theView More
Authors: Rubaiya Khondoker Shikha (Dept. of Space Science, UAH), Jakobus A. le Roux (Dept. of Space Science, UAH, CSPAR) The acceleration and transport of solarView More
Authors: Zubair I. Shaikh (UTD, TX), Ivan Y. Vasko (UTD, TX), Tai Phan (SSL, UC Berkeley), Stanislav Boldyrev (University of Wisconsin-Madison, USA) Interplanetary Coronal MassView More
Authors: Jakobus A. le Roux (University of Alabama in Hunstville), Rubaiya K. Shikha (University of Alabama in Huntsville) Solar wind magnetic turbulence, being intermittent, canView More
Authors: Eric Zirnstein (Princeton University) The IBEX mission is currently in its 17th year of taking measurements of energetic neutral atom (ENA) emissions from theView More
Authors: Qiang Hu (UAH) Interplanetary coronal mass ejections (ICMEs) are large-scale structures in the solar wind, corresponding to the counterparts of CMEs when they propagateView More
Authors: Roberto Lionello (PSI), Cooper Downs (PSI), Jon A. Linker (PSI), Emily I. Mason (PSI), Pete Riley (PSI) The Time-Dependent Corona and Heliosphere Roberto LionelloView More
Authors: B. L. Alterman (NASA | GSFC), R. D’Amicis (INAF) The two-state solar wind paradigm is based on observations showing that slow and fast solarView More