Associated with SHINE 2024 Session 3
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: Ayla Weitz (University of Colorado, NSO), Sanjiv Tiwari (LMSAL, BAERI), Bart De Pontieu (LMSAL, University of Oslo), Gianna Cauzzi (NSO), Kevin Reardon (University ofView More
Authors: Karin Dissauer (NorthWest Research Associates, 3380 Mitchell Lane, Boulder, CO 80301, USA), KD Leka (NorthWest Research Associates, 3380 Mitchell Lane, Boulder, CO 80301, USA,View 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: Nian Liu (NJIT), Satoshi Inoue (NJIT), Ju Jing (NJIT, BBSO), Haimin Wang (NJIT, BBSO) We conducted both data-constrained and data-driven magnetohydrodynamic (MHD) simulations ofView More
Authors: Zhuo Liu, Caio Silva, Lucio M. Milanese, Noah R. Mandell, Nuno F. Loureiro Electron-only reconnection is a type of magnetic reconnection occurring in sufficientlyView 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: 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: Hamilton, J. (Georgia State University); Sadykov, V.M. (Georgia State University); Kitiashvili, I.N. (NASA Ames Research Center); Wray, A.A. (NASA Ames Research Center) The abilityView 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: Alin Razvan Paraschiv (NSO) With the commissioning of new generation instrumentation and the recent advances in understanding the theoretical aspects of solar coronal polarization,View More
Authors: Mehmet Sarp Yalim (University of Alabama in Huntsville), Sanjiv Tiwari (Bay Area Environmental Research Institute), Debi Prasad Choudhary (California State University, Northridge), Christian BeckView 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