1 This is how it looks like… Magnetic helicity at the solar surface and in the solar wind Axel Brandenburg (Nordita, Stockholm) Properties of magn helicity.
Voyager 2 Observations of Magnetic Waves due to Interstellar Pickup Ions Colin J. Joyce Charles W. Smith, Phillip A. Isenberg, Nathan A. Schwadron, Neil.
Magnetic field generation on long time scales Axel Brandenburg (Nordita/Stockholm) Kemel+12 Ilonidis+11Brandenburg+11Warnecke+11 Käpylä+12.
Magnetic field generation on long time scales
1 Forced – decaying Helical – nonhelical. 2 Points of the talk Resistive effects during inverse transfer B-field does not care about irrotational part.
Scale-dependence of magnetic helicity in the solar wind
