Publication Date:
2017
abstract:
The description of the Moffatt and Parker problem recently revisited by O. Pezzi et al. [Astrophys. J. 834, 166 (2017)] is here extended by analyzing the features of the turbulence produced by the interaction of two colliding Alfvenic wave packets in a kinetic plasma. Although the approach based on the presence of linear modes features is still helpful in characterizing some low-energy fluctuations, other signatures, which go beyond the pure linear modes analysis, are recovered, such as the significant weakening of clear dispersion relations and the production of zero frequency fluctuations.
Iris type:
01.01 Articolo in rivista
Keywords:
magnetohydrodynamic turbulence; plasma turbulence; solar wind; Fokker-Planck and Vlasov model; plasma physics
List of contributors:
Pezzi, Oreste
Published in: