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 …

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 …

The angular momentum (AM) evolution of stellar interiors, along with the resulting rotation
rates of stellar remnants, remains poorly understood. Asteroseismic measurements of red …

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

The Evolution and Role of Solar Wind Turbulence in the Inner Heliosphere - IOPscience This
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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 …

We study the effects of turbulence on magnetic reconnection using three-dimensional direct
numerical simulations. This is the first attempt to test a model of fast magnetic reconnection …

This review of scaling theories of magnetohydrodynamic (MHD) turbulence aims to put the
developments of the last few years in the context of the canonical time line (from Kolmogorov …

We develop a one-dimensional solar-wind model that includes separate energy equations
for the electrons and protons, proton temperature anisotropy, collisional and collisionless …

Wavelet analysis can be used to measure the power spectrum of solar-wind fluctuations
along a line in any direction (θ, ϕ) with respect to the local mean magnetic field B 0. This …