The consequences of these phenomena on the solar-terrestrial environment and on Space Weather are nowadays clearly recognized, even if not yet fully understood.
* Corresponding author: magnetism is responsible for the several active phenomena that occur in the solar atmosphere. Udaipur Solar Observatory, Physical Research laboratory, Udaipur 313001, IndiaĬentre for mathematical Plasma Astrophysics, KU Leuven, Celestijnenlaan 200B, 3001 Leuven, Belgium Atomistilor 405, 077125 Magurele-Ilfov, Romaniaĭepartment of Physics, POB 64, 00014 University of Helsinki, Finland Research Center for Atomic Physics and Astrophysics, Faculty of Physics, University of Bucharest, Str. Institute of Geodynamics of the Romanian Academy, Jean-Louis Calderon 19–21, Bucharest-37 020032, Romania Solar – Terrestrial Center of Excellence – SIDC, Royal Observatory of Belgium, Av. LPC2E/CNRS (UMR 7328) and University of Orléans, 3A avenue de la Recherche Scientifique, 45071 Orléans Cedex 2, France UJF-Grenoble 1/CNRS-INSU, Institut de Planétologie et d’Astrophysique de Grenoble (IPAG) UMR 5274, 38041 Grenoble, France INAF – Osservatorio Astrofisico di Catania, Via S. Universidad Tecnológica Nacional – Facultad Regional Mendoza/CONICET, Rodríguez 273, M5502AJE, Mendoza, Argentina Physical-Meteorological Observatory/World Radiation Center, Davos, Switzerland España Sur 1512, J5402DSP, San Juan, Argentina Instituto de Ciencias Astronómicas, de la Tierra y el Espacio, ICATE-CONICET, Av. Astrofisica, Università di Catania, Via S.
Zuccarello 13ĭipartimento di Fisica e Astronomia, Sez.
Lopez 2, Marilena Mierla 8 ,9 ,10, Susanna Parenti 8, Jens Pomoell 11, Paolo Romano 5, Luciano Rodriguez 8, Nandita Srivastava 12, Rami Vainio 11, Matt West 8 and Francesco P. Guglielmino 5, Jean Lilensten 6, Thierry Dudok de Wit 7, Matthieu Kretzschmar 7, Fernando M. Francesca Zuccarello 1 *, Laura Balmaceda 2, Gael Cessateur 3, Hebe Cremades 4, Salvatore L.
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