Kinetic Alfvn Waves Dynamics and Substorm Onset Andreas Keiling Pi2 pulsations in the nearEarth plas

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Kinetic Alfvén Waves Dynamics and Substorm Onset
Andreas KeilingPi2 pulsations in the
near-Earth plasma sheet Andreas KeilingAlfvén
waves during storms Andreas KeilingNear Earth
and Aurora (Eric)Rumi BBFs and connection with
aurora and inner edge of plasma sheet
(Nakamura)Kelvin-Helmholtz instability and hot
dense ions Masaki FujimotoVelocity vorticity
and FAC Larry KepkoNonlinear MHD instabilities
(ballooning first, then tearing) John Samson
Same as AlainThin current sheet / Inner edge of
plasma sheet Andrei Runov Smaller scale size
than in the prime mission, down to ion inertial
length Cluster could not do it. ISEE1/2 was
there. We dont need 4 s/c. Unique region,
unique separations. Clusters innermost location
_at_10Re, but moves fast, and at large
separations (10,000km). Not optimal for current
studies. - High energy particle wall , need X
and Z. Flow braking and thin current sheet
instabilities Tony Lui Z separation benefits
both MaybeConvection crisis/BBF
penetration/thin current sheet build up and
disruption Victor Sergeev