Slide 1NSF Site Visit Madison, May 1-2, 2006 Magnetic Helicity Conservation and Transport R. Kulsrud and H. Ji for participants of the Center for Magnetic Self-organization…
Slide 1 1. Background2. Flux variation3. Polarity reversal4. Electron evolution5. Conclusions The role of coronal mass ejections in the solar cycle evolution of the heliospheric…
1. How much helicity isneeded to drivelarge-scale dynamos? (submitted to Phys. Rev. E) Simon Candelaresi Axel Brandenburg 2. Closed alpha^2 DynamoMomentum equation: forcing…