Objective The objective of the proposed project is to study and to model the strongest (Ap>100nT, Dst<-100 nT) geo-effective disturbances in the corona and inner heliosphere that occurred during solar cycle 23, i.e. from 1997-2005. It is expected that the developed project methods and software products be used to reliably monitor space weather conditions on short-term (2-5 days) basis in 3D. The new data/methods will be made available for future use based on the selection of adequate software packages and data formats. Storage will be done on CD-ROM and DVD media as well as on special institute's Internet servers (computers) to serve the scientific community. A direct comparison and collaboration will take place in 2006 in connection to the STEREO mission data analysis. Programme(s) IC-INTAS - International Association for the promotion of cooperation with scientists from the independent states of the former Soviet Union (INTAS), 1993- Topic(s) OPEN - OPEN Call Call for proposal Data not available Funding Scheme Data not available Coordinator Max-Planck-Institut für Sonnensystemforschung (Formerly Max-Planck-Institut für Aeronomie) EU contribution No data Address Max-Planck-Str. 2 D-37191 Katlenburg-Lindau Germany See on map Total cost No data Participants (4) Sort alphabetically Sort by EU Contribution Expand all Collapse all Academy of Sciences of the Czech Republic Astronomical Institute Czechia EU contribution No data Address Bocni II 1401 14131 Praha See on map Total cost No data Moscow State University Skobelt'syn Institute of Nuclear Physics State Russia EU contribution No data Address Vorob'evy Gory 1 119992 Moscow See on map Total cost No data Royal Observatory of Belgium Belgium EU contribution No data Address Ringlaan 3 B-1180 Brussels See on map Total cost No data Russian Academy of Sciences Institute of Terrestrial Magnetism (IZMIRAN) Russia EU contribution No data Address IZMIRAN 1 142190 Troitsk See on map Total cost No data
