Evolution of a coronal mass ejection from the Sun to Saturn
Dr. Erika Palmerio1, K Emilia J Kilpua2, Andrei Zhukov3, David Barnes4, Marilena Mierla5, Olivier G Witasse6, Teresa Nieves-Chinchilla7, Beatriz Sanchez-Cano8, Christian Moestl9, Luciano Rodriguez5, Elias Roussos10, Jingnan Guo11, Adam Masters12, Alexey Isavnin13, Gabrielle Provan14, Neel Savani15 and Lucile Turc16, (1)Predictive Science Inc., San Diego, CA, United States, (2)University of Helsinki, Department of Physics, Helsinki, Finland, (3)SIDC, Royal Observatory of Belgium, Brussels, Belgium, (4)United Kingdom Research and Innovation - Science & Technology Facilities Council, Rutherford Appleton Laboratory, RAL Space, Didcot, United Kingdom, (5)SIDC, Royal Observatory of Belgium, Uccle, Belgium, (6)European Space Agency, ESTEC, Villanueva De La Can, Spain, (7)NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, MD, United States, (8)University of Leicester, Leicester, LE1, United Kingdom, (9)Institute of Physics, University of Graz, Graz, Austria, (10)Max Planck Institute for Solar System Research, Göttingen, Germany, (11)University of Science and Technology of China, School of Earth and Space Sciences, Hefei, China, (12)Imperial College London, Blackett Laboratory, London, United Kingdom, (13)Katholieke Universiteit Leuven, Leuven, Belgium, (14)University of Leicester, School of Physics and Astronomy, Leicester, United Kingdom, (15)University of Maryland Baltimore County, Baltimore, MD, United States, (16)LPP - CNRS - Ecole polytechnique - UPMC, Palaiseau, France
