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A prospective new diagnostic technique for distinguishing eruptive and noneruptive active regions

2019

This research has received funding from the Science and Technology Facilities Council (UK) through the consolidated grant ST/N000609/1 and the European Research Council (ERC) under the European Union Horizon 2020 research and innovation program (grant agreement No. 647214). This work used the DiRAC@Durham facility managed by the Institute for Computational Cosmology on behalf of the STFC DiRAC HPC Facility (www.dirac.ac.uk). The equipment was funded by BEIS capital funding via STFC capital grants ST/P002293/1, ST/R002371/1, and ST/S002502/1, Durham University and STFC operations grant ST/R000832/1. DiRAC is part of the National e-Infrastructure. S.L.Y. would like to acknowledge STFC for sup…

Solar coronal mass ejections (310)010504 meteorology & atmospheric sciencesSpace weatherSolar magnetic fieldsSolar activityT-NDASLibrary scienceFOS: Physical sciencesSpace weather (2037)Solar coronaSolar activity (1475)Solar flares (1496)01 natural sciencesSolar coronal mass ejectionsSolar corona (1483)0103 physical sciencesmedia_common.cataloged_instanceAstrophysics::Solar and Stellar AstrophysicsQB AstronomyEuropean union010303 astronomy & astrophysicsQCSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesmedia_commonQBPhysicsEuropean researchSolar active region magnetic fieldsAstronomy and AstrophysicsSolar active region magnetic fields (1975)Solar magnetic fields (1503)Solar active regionsSolar active regions (1974)QC PhysicsAstrophysics - Solar and Stellar Astrophysics13. Climate actionSolar flaresSpace and Planetary SciencePhysics::Space Physics
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