• Y. V. Chugunov, P. A. Bespalov: Institute of Applied Physics, Russian Academy of Sciences (IAP RAS), Nizhny Novgorod, Russia (electrodynamics of co-rotating plasmaspheres of planets)
  • N. V. Erkaev: Institute for Computational Modelling, Russian Academy of Sciences (ICM RAS), and Siberian Federal University, Krasnoyarsk, Russia (formation of magnetodisks; magnetospheric effects of distributed internal current systems)
  • N. Achilleos, P. Guio, S. Miller: University College London (UCL), UK (physical processes in the planetary magnetodisks; modelling of a giant planet magnetodisk formation in the co-rotation region)
  • I. I. Alexeev, E. S. Belenkaya, V. Kalegaev: Laboratory of planetary magnetospheres at Institute of Nuclear Physics of the Moscow State University (SINP, MSU), Moscow, Russia (PMM modelling support for exoplanetary magnetosphere study; study of magnetodisk origin)
  • J.-M. Grießmeier: Laboratoire de Physique et Chimie de l'Environnement et de l'Espace, CNRS, Orleans, France (modelling of exoplanetary magnetospheres and study of planetary magnetospheric protection)
  • M. Holmström: Swedish Institute of Space Physics (IRF), Kiruna, Sveden (planetary magnetospheres interaction with stellar winds, generation of ENA coronas)
  • E. Kallio, S. Dyadechkin: Finnish Meteorological Institute (FMI), Helsinki, Finland (Hybrid numerical model HYB for simulation of exoplanetary plasma environments and possible linkage to PMM)