Associated with SHINE 2024 Session 5
Authors: Georgios Chintzoglou Solar Active Regions (ARs) are produced by the emergence of strong magnetic fields generated in the solar interior. ARs can be furtherView More
Authors: Peter W. Schuck (NASA/GSFC) Currents are a much maligned observable in solar physics. There are many advantages to understanding solar phenomena through the evolutionView More
Authors: Brian T. Welsch (Univ. Wisc. – Green Bay), Yang Liu (Stanford University) Energy released in solar flares and coronal mass ejections (CMEs) is believedView More
Authors: Wei Liu (LMSAL/BAERI), Thomas Berger (Univ. Colorado), Andrei Afanasev (Univ. Colorado), and Yuhong Fan (UCAR/HAO) Solar prominences are large-scale plasma structures embedded in non-potentialView More
Authors: Silvina Guidoni (American University), Rebecca Bonness (American University) During solar eruptions, massive amounts of energy stored in the coronal magnetic field are converted intoView More
Authors: Bin Chen (NJIT), Dale Gary (NJIT), Gelu Nita (NJIT), Sijie Yu (NJIT), Pascal Saint-Hilaire (UC Berkeley), Gregg Hallinan (Caltech), and the EOVSA and OVRO-LWAView More
Authors: Nat Mathews (NASA GSFC), Barbara Thompson (NASA GSFC) An increase in machine learning based techniques for solar research has mandated the creation of aView 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: Ying Wang(NJIT), Yan Xu (NJIT), Haimin Wang(NJIT) Previous studies have shown that rotation can impact the orientation of Interplanetary Coronal Mass Ejections (ICMEs) asView 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
Authors: Xu Yang (BBSO/NJIT), Meiqi Wang (NJIT) We carry out high-resolution observations of a filament-eruption-triggered X1.0 white-light flare on October 2, 2022. The Visible ImagingView More
Authors: Dominic Payne (UMD),Marc Swisdak(UMD), James Drake(UMD) Magnetic shear (guide field) has been shown to play an important role in the rapidity and amount ofView More
Authors: Charles Fred Driscoll (UCSD) A model of “charge-electric” energization of the Solar Wind and Corona is developed, including electro-magnetic particle effects precluded by traditionalView More