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Effect of Current Sheets on the Solar Wind Magnetic Field Power Spectrum from the Ulysses Observation: From Kraichnan to Kolmogorov Scaling
DOI: 10.1103/PhysRevLett.106.125001 Bibcode: 2011PhRvL.106l5001L

Li, G.; Hu, Q.; Qin, G. +1 more

The MHD turbulence theory developed by Iroshnikov and Kraichnan predicts a k-1.5 power spectrum. Solar wind observations, however, often show a k-5/3 Kolmogorov scaling. Based on 3 years worth of Ulysses magnetic field data where over 28 000 current sheets are identified, we propose that the current sheet is the cause of the …

2011 Physical Review Letters
Ulysses 62