Objetivo Our project precedes the established cooperation and provide a bridge for future space missions aimed to micro scales in a study of magnetosphere plasma transport processes. It can provide a guideline for transport processes in astrophysical and laboratory plasma as well.The main goal is to find evidences for presence of the ion and electron micro-scales in the modern data sets (e.g. in Cluster and Interball ones). Comparison with the dynamics of simulated kinetic current sheets and usage of the Gas Dynamic Convection Field model for gathering together multi-point measurements promises a step towards designing of the future small-scale missions. Historically the respective ROY Project had been proposed by the famous Soviet space physicist Yury Galperin in seventies, which has been revived in the modern Russian Space Program. We prove our approach to the problem by comparison of the different indirect methods.One of the indirect methods is based on the Maxwellian equation: curl B ~ j , which provides in a plane quasi-stationary geometry a scale L estimate: |B|/ |j| ~ L.Another one uses different spectral properties of the ion and electron moments at the respective scales (which correspond to fraction of Hz for the ion scales and to several Hz for the electron ones, while a spacecraft crosses corresponding structures in magnetosphere boundary layers). Modern wavelet coherence and bi-coherence analysis would facilitate our research. We plan to prove and/or modify the existed approaches for the comprehensive statistical mapping of the small-scale disturbances in the magnetosphere boundary layers (e.g. at the outer polar cusp border, in plasma sheet boundary layer and auroral regions), elaborate recommendations for strategic and methods of the future missions, and do a step in evaluating of the nonlinear cascade-like interactions into the plasma transport, as compared with the laminar reconnection of anti-parallel magnetic fields. For the developed turbulence at high-latitude magnetopause the nonlinear cascades should transfer energy down to electron skin-scales in wide regions, for the classical laminar reconnections they should be limited in very narrow diffusion regions. We are aimed to distinguish those extreme cases and to simulate multi-spacecraft tomography on the basis of the highest-resolution data in hands. Palabras clave comparison with kinetic modelling small scale nonlinear processes tomography in future missions Programa(s) IC-INTAS - International Association for the promotion of cooperation with scientists from the independent states of the former Soviet Union (INTAS), 1993- Tema(s) BELARUS - BELARUS Convocatoria de propuestas Data not available Régimen de financiación Data not available Coordinador Polish Academy of Sciences Space Research Center Aportación de la UE Sin datos Dirección Bartycka 18A 00716 Warsaw Polonia Ver en el mapa Coste total Sin datos Participantes (6) Ordenar alfabéticamente Ordenar por aportación de la UE Ampliar todo Contraer todo Academy of Education of Republic Belarus Mogilev State University Bielorrusia Aportación de la UE Sin datos Dirección Kosmonavtov 1 Mogilev Ver en el mapa Coste total Sin datos C.N.R. Istituto di Fisica dello Spazio Interplanetario Italia Aportación de la UE Sin datos Dirección Via del fosso del cavaliere 100 00133 Roma Ver en el mapa Coste total Sin datos CNRS /LPCE Laboratoire de Physique et Chimie, de l'Environnement Francia Aportación de la UE Sin datos Dirección Ave. de la Recherche Scientifique 3A F-45071 Orleans Ver en el mapa Coste total Sin datos Max-Planck-Institut fur Aeronomie Alemania Aportación de la UE Sin datos Dirección Max-Planck-Str. 2 37191 Katlenburg-Lindau Ver en el mapa Coste total Sin datos Moscow State University, Faculty of Physics Rusia Aportación de la UE Sin datos Dirección Vorobjevy Gory 1 119992 Moscow Ver en el mapa Coste total Sin datos Russian Academy of Sciences Space Research Institute Rusia Aportación de la UE Sin datos Dirección Profsoyuznaya 84/32 117997 Moscow Ver en el mapa Coste total Sin datos
