The solar wind is a magnetized plasma and as such exhibits collective plasma behavior
associated with its characteristic spatial and temporal scales. The characteristic length …

In this review we will focus on a topic of fundamental importance for both astrophysics and
plasma physics, namely the occurrence of large-amplitude low-frequency fluctuations of the …

This paper summarises some of the recent progress that has been made in understanding
astrophysical plasma turbulence in the solar wind, from in situ spacecraft observations. At …

This paper presents a theoretical framework for understanding plasma turbulence in
astrophysical plasmas. It is motivated by observations of electromagnetic and density …

Modelling the transport of cosmic rays (CRs) in the heliosphere represents a global
challenge in the field of heliophysics, in that such a study, if it were to be performed from first …

Coronal holes are the darkest and least active regions of the Sun, as observed both on the
solar disk and above the solar limb. Coronal holes are associated with rapidly expanding …

We present a quantitative estimate of the anisotropic power and scaling of magnetic field
fluctuations in inertial range magnetohydrodynamic turbulence, using a novel wavelet …

This paper studies the turbulent cascade of magnetic energy in weakly collisional
magnetized plasmas. A cascade model is presented, based on the assumptions of local …

The 2D+ slab superposition model of solar wind turbulence has its theoretical foundations in
nearly incompressible magnetohydrodynamics (NI MHD) in the plasma beta∼ 1 or≪ 1 …

The significant influences of turbulence in neutral fluid hydrodynamics are well accepted but
the potential for analogous effects in space and astrophysical plasmas is less widely …