2020/04/16 by Krzysztof Barczynski, Krzysztof Barczyński, Guillaume Aulanier +6
Biochemistry, Genetics and Molecular Biology · Physics and Astronomy · #Astrobiology #Astronomy #Astrophysics #Corona (planetary geology) #Coronal mass ejection #Current (fluid) #Electric current #Electric field #Flare #Flux (metallurgy) #Geomagnetism and Paleomagnetism Studies #Ionosphere and magnetosphere dynamics #Magnetic field #Magnetic flux #Magnetic reconnection #Magnetohydrodynamics #Physics #Solar and Space Plasma Dynamics #Solar flare #Solar wind #astro-ph.SR
paper · pdf · doi:10.3847/1538-4357/ab893d
27 pages, 10 figures; Accepted for publication in ApJ (13 April 2020)
arxiv created 2020/04/16 · openalex publication_date 2020/05/01 · arxiv updated 2020/05/27 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/06
Abstract Electric currents play a critical role in the triggering of solar flares and their evolution. The aim of the present paper is to test whether the surface electric current has a surface or subsurface fixed source as predicted by the circuit approach of flare physics, or is the response of the surface magnetic field to the evolution of the coronal magnetic field as the MHD approach proposes? Out of all 19 X-class flares observed by SDO from 2011 to 2016 near the disk center, we analyzed the only nine eruptive flares for which clear ribbon hooks were identifiable. Flare ribbons with hooks are considered to be the footprints of eruptive flux ropes in MHD flare models. For the first time, fine measurements of the time evolution of electric currents inside the hooks in the observations as well as in the OHM 3D MHD simulation are performed. Our analysis shows a decrease of the electric current in the area surrounded by the ribbon hooks during and after the eruption. We interpret the decrease of the electric currents as due to the expansion of the flux rope in the corona during the eruption. Our analysis brings a new contribution to the standard flare model in 3D.