Statistical properties of solar wind discontinuities, intermittent turbulence, and rapid emergence of non-Gaussian distributions
Recent studies have compared properties of the magnetic field in simulations of Hall MHD turbulence with spacecraft data, focusing on methods used to identify classical discontinuities and intermittency statistics. Comparison of ACE solar wind data and simulations of 2D and 3D turbulence shows good...
Autor principal: | Dmitruk, Pablo Ariel |
---|---|
Publicado: |
2010
|
Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0094243X_v1216_n_p202_Greco http://hdl.handle.net/20.500.12110/paper_0094243X_v1216_n_p202_Greco |
Aporte de: |
Ejemplares similares
-
Statistical properties of solar wind discontinuities, intermittent turbulence, and rapid emergence of non-Gaussian distributions
por: Greco, A., et al.
Publicado: (2010) -
Statistical properties of solar wind discontinuities, intermittent turbulence, and rapid emergence of non-Gaussian distributions
por: Greco, A., et al. -
Statistical properties of solar wind discontinuities, intermittent turbulence, and rapid emergence of non-Gaussian distributions
por: Greco, A., et al.
Publicado: (2010) -
Statistical analysis of discontinuities in solar wind ace data and comparison with intermittent mhd turbulence
por: Dmitruk, Pablo Ariel
Publicado: (2009) -
Statistical analysis of discontinuities in solar wind ace data and comparison with intermittent mhd turbulence
por: Greco, A., et al.
Publicado: (2009)