Magnetic signatures in the Galileo Earth flyby data: Can solar wind interactions and auroral substorm processes explain the dynamics of the magnetotail?

M. G. Kivelson, R. L. McPherron, V. Angelopoulos, K. K. Khurana, C. M. Hammond, C. F. Kennel, C. T. Russell, D. J. Southwood, and A. J. Lazarus
Institute of Geophysics and Planetary Physics, University of California, Los Angeles, and
CSR, MIT, Cambridge, MA.

COSPAR Symposium, B. 3-S

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