Alexander Mishev, University of Oulu, Finland (Team leader) – analysis of NM data, analysis of historical event, quantification of terrestrial and space weather effects
Alessandro Bruno, NASA/GSFC & CUA, Heliophysics Science Division, USA- AMS02 and PAMELA data analysis. Coordination of space–borne data analysis.
Athanasios Papaioannou, National Observatory of Athens, Greece – space-borne (SOHO, GOES, SO) data analysis.
Bernd Heber, Institut fur Experimentelle und Angewandte Physik, Christian-AlbrechtsUniversitat zu Kiel, Germany – space-borne data analysis, SOHO/EPHIN data analysis, data interpretation and bridging space and ground data analysis.
Charlotte Waterfall, University of Central Lancashire, UK – GLE analysis.
Cristina Consolandi, University of Hawaii at Manoa, Honolulu, USA – AMS 02 data analysis.
Hisashi Hayakawa, Nagoya University, Japan – historical archive data on solar storms.
Ilya Usoskin, University of Oulu, Finland – analysis of NM data, quantification of terrestrial and space weather effects, analysis of historical events.
Keith Ryden, University of Surrey, UK- quantification of terrestrial and space weather effects.
Monica Laurenza, INAF-Istituto di Astrofisica e Planetologia Spaziali, Italy – data interpretation and bridging space and ground data analysis
Sergey Koldobskiy, University of Oulu, Finland – PAMELA and NM data analysis, analysis of historical with cosmogenic imprints SEP events.
Rami Vainio, University of Turku, Finland – data interpretation and bridging space and ground data analysis
Juan V. Rodriguez, University of Colorado Boulder, USA – GOES data analysis
Young scientists:
Lisa Romaneehsen, Ph.D student, University of Kiel, Germany – AMS 02, GOES/HEPAD data analysis.
Nicholas Larsen Ph.D. student, University of Oulu, Finland, magnetospheric modeling, necessary for the data analysis of GLEs and assessment of terrestrial effects.
Self-supported experts:
Rolf Buetikofer, High Altitude Research Stations (Jungfraujoch & Gornergast), Switzerland – NM data analysis, space weather and terrestrial effects.