Friday Morning 1
Time	Session	Location	Title
0830	SM51A	CC Hall B	Solar Wind-Magnetosphere Interactions II Posters Presiding: P D Craven, NASA Marshall Space Flight Center; R J Strangeway, Institute of Geophysics and Planetary Physics, University of California, Los Angeles    [Abstracts]
0830	SM51A-01	CC Hall B	The aurora and particle fluxes during the large January 21, 2005 geomagnetic storm *H U Frey, S B Mende, T J Immel, J McFadden, D S Evans POSTER    [details]
0830	SM51A-02	CC Hall B	Cusp-Region Ion Outflows Observed During January 21, 2005 Storm Period *R J Strangeway, J P McFadden POSTER    [details]
0830	SM51A-03	CC Hall B	Magnetospheric response to extreme solar events of January 2005, as observed by the Cluster and Double Star spacecraft *c Vallat, I Dandouras, P Escoubet, H RŠme, J Cao, A Balogh, C Carr POSTER    [details]
0830	SM51A-04	CC Hall B	Prediction of Auroral Electrojet AL Index *A Tan, W Lyatsky POSTER    [details]
0830	SM51A-05	CC Hall B	Contributions from Different Sources to Semiannual Variation of Geomagnetic Activity *S Lyatskaya, W Lyatsky, A Tan POSTER    [details]
0830	SM51A-06	CC Hall B	The Phase Structure of Pc3 Geomagnetic Pulsations at Low Latitudes *I A Ansari POSTER    [details]
0830	SM51A-07	CC Hall B	A Study of the Characteristics and Behavior of the Low Energy Plasma in the Magnetospheric Lobal Wind *P D Craven, M W Liemohn, M O Chandler, T E Moore POSTER    [details]
0830	SM51A-08	CC Hall B	Solar Wind Entry and Plasma Sheet Formation in the Magnetosphere Using a Global Unstructured Hybrid Simulation Model *F Kazeminezhad, A T Lui POSTER    [details]
0830	SM51A-09	CC Hall B	Geomagnetic Activity Forecasting Using Self-Learning Algorithms: Application in Space Weather Studies *A F Khalil, A R Barakat, M McKee POSTER    [details]
0830	SM51A-10	CC Hall B	Equation free projective integration: A novel scheme for modeling multiscale processes in plasmas *M A Shay, B Dorland, J Drake, B Jemella, G Stantchev, S Cowley POSTER    [details]
0830	SM51A-11	CC Hall B	Failure of Dst index fields to represent a ring current *W H Campbell POSTER    [details]