Author:
Bruno Roberto,Carbone Vincenzo
Publisher
Springer International Publishing
Reference68 articles.
1. B. Bavassano, R. Bruno, Evidence of local generation of Alfvénic turbulence in the solar wind. J. Geophys. Res. 94 (13), 11977–11982 (1989). doi:10.1029/JA094iA09p11977
2. B. Bavassano, M. Dobrowolny, G. Fanfoni, F. Mariani, N.F. Ness, Statistical properties of MHD fluctuations associated with high-speed streams from Helios 2 observations. Solar Phys. 78, 373–384 (1982). doi:10.1007/BF00151617
3. L. Bianchini, E. Pietropaolo, R. Bruno, An improved method for local intermittency recognition, in Magnetic Fields and Solar Processes, ed. by A. Wilson. ESA Conference Proceedings, vol. SP-448 (ESA Publications Division, Noordwijk, 1999), pp. 1141–1146
4. J.E. Borovsky, Flux tube texture of the solar wind: Strands of the magnetic carpet at 1 AU? J. Geophys. Res. 113 (2008). doi:10.1029/2007JA012684
5. R. Bruno, B. Bavassano, Origin of low cross-helicity regions in the solar wind. J. Geophys. Res. 96, 7841–7851 (1991). doi:10.1029/91JA00144