Following the evolution of coronal mass ejections across the heliosphere

Erika Palmerio1, Olivier G Witasse2, Teresa Nieves-Chinchilla3, David Barnes4, Marilena Mierla5, Andreas J Weiss6, Christian Moestl7, Andrei Zhukov8, Lan Jian3, Beatriz Sanchez-Cano9, Luciano Rodriguez5, Jingnan Guo10, Elias Roussos11, Adam Masters12, Gabrielle Provan13, Alexey Isavnin14, Patrick J Lowrance15, Lucile Turc16 and K Emilia J Kilpua1, (1)University of Helsinki, Helsinki, Finland, (2)European Space Agency, Noordwijk, Netherlands, (3)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (4)Rutherford Appleton Laboratory, Didcot, OX11, United Kingdom, (5)SIDC, Royal Observatory of Belgium, Uccle, Belgium, (6)Space Research Institute, Austrian Academy of Sciences, Graz, Austria, (7)Institute of Physics, University of Graz, Graz, Austria, (8)Skobeltsyn Institute of Nuclear Physics, Moscow State University, Moscow, Russia, (9)University of Leicester, Leicester, LE1, United Kingdom, (10)University of Kiel, Institute of Experimental and Applied Physics, Kiel, Germany, (11)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (12)JAXA Japan Aerospace Exploration Agency, Sagamihara, Japan, (13)University of Leicester, Leicester, United Kingdom, (14)Rays of Space Oy, Vantaa, Finland, (15)IPAC–Spitzer, California Institute of Technology, Pasadena, CA, United States, (16)LPP - CNRS - Ecole polytechnique - UPMC, Palaiseau, France