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We investigate the spectral properties of plasma turbulence from fluid tosub-ion scales by means of high-resolution three-dimensional (3D) numericalsimulations performed with the hybrid particle-in-cell (HPIC) code CAMELIA. Weproduce extended turbulent spectra with well-defined power laws for themagnetic, ion bulk velocity, density, and electric fluctuations. The presentresults are in good agreement with previous two-dimensional (2D) HPICsimulations, especially in the kinetic range of scales, and reproduce severalfeatures observed in solar wind spectra. By providing scaling tests on manydifferent architectures and convergence studies, we prove CAMELIA to representa very efficient, accurate and reliable tool for investigating the develpomentof the turbulent cascade in the solar wind, being able to cover simultaneouslyseveral decades in wavenumber, also in 3D.

Three-dimensional simulations of solar wind turbulence with the hybrid code CAMELIA