Ring Current Structure and Dynamics: Local Measurements (CLUSTER/CIS and FGM) and Global Observations (IMAGE/HENA) Claire Vallat (CESR, Toulouse cedex 4, France, 31028), Iannis Dandouras, Pontus C:son Brandt, Malcolm Dunlop, George K. Parks, Mark Wilber ClusterÕs highly eccentric polar orbit at around 4 Re perigee permits sampling of the ring current population, and gives its latitudinal profile evolution. The CIS (Cluster Ion Spectrometry) experiment onboard Cluster is capable of obtaining full three-dimensional ion distributions (from about 5eV/q to 40 keV/q) with one spacecraft spin time resolution (4 sec) and with mass-per-charge composition determination. The CIS data reveal new and very interesting structures on the ion spectrograms: the presence, for all the major ion species, of different features in energy bands, all along the CLUSTER pass inside the diffuse auroral zone. The highly structured pitch-angle distributions, which are energy dependent, confirm the presence of distinct populations. The latitudinal profile of the ring current is also analysed. The magnetic field measurements on board the 4 CLUSTER spacecraft by the FGM (Flux Gate Magnetometer) instrument allow for the first time to calculate the ring current density profile along the spacecraft orbit, using the curlometer technique. The combination of high time and energy resolution, good mass per charge discrimination, and favorable orbits has enabled Cluster to discern inner magnetospheric populations that have not been well-characterized in previous observations. Events have also been selected for which the CLUSTER spacecraft are within the field of view of the HENA (High Energy Neutral Atom) imager onboard IMAGE. HENA provides energetic neutral atom images with a high geometric factor and with a 120 degree x 360 degree field of view over the spin. The H+ ion distribution functions obtained in situ by CIS are then compared to the ones deduced by inverting the HENA hydrogen neutral atom images for the overlapping energy range of the two instruments (27-39 keV). The results show the complementarity of the two approaches, i.e. local measurements providing the full distribution function and giving the 'ground truth', and ENA imaging which allows to put the local measurements into a global context. _______________ Presented at the August 2003 AGU Chapman Conference, Helsinki, Finland