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Solar Storms: Flares, CMEs and SEPS

Solar Storms: Flares, CMEs and SEPS. Aim of the splinter, some recent advances in the understanding of 1- particle acceleration and transport processes at the Sun and in the inner heliosphere

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Solar Storms: Flares, CMEs and SEPS

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  1. Solar Storms: Flares, CMEs and SEPS Aim of the splinter, some recent advances in the understanding of 1- particle acceleration and transport processes at the Sun and in the inner heliosphere 2-onset of CMES, propagation in the interplanetary medium and subsequent interactions with the Earth's magnetosphere. 3- the impact of flares (UV radiation) and particles on the Earth’s atmosphere which is still a field under development N. Vilmer (LESIA, Paris Observatory), O. Malandraki (NOA), N. Crosby (BIRA-IASB)

  2. ThanassisPapaioannou (National Observatory of Athens) • 'SolarEnergeticparticleswithin the STEREO era : 2007-2012' • Bernd Heber (Christian-Albrechts-Universitätzu Kiel) • ‘A statisticalsurvey of wide-spreadsolarelectroneventsobservedwith STEREO and ACE' • NeusAgueda (Universitat de Barcelona) • ‘Numerical simulations of the propagation of SEPs’ • Francesco Zucarello (KU Leuven) • ‘Numerical simulations of CME’s in the interplanetary medium’ • Jan MaikWissing (University of Osnabrück) • ‘Modellingparticleprecipitation in the Earth’satmosphere’ Solar Storms: Flares, CMEs and SEPS

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