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 …

Unlike the vast majority of astrophysical plasmas, the solar wind is accessible to spacecraft,
which for decades have carried in-situ instruments for directly measuring its particles and …

Recent fully nonlinear, kinetic three-dimensional simulations of magnetic reconnection [W.
Daughton et al., Nat. Phys. 7, 539 (2011)] evolve structures and exhibit dynamics on multiple …

Scale-invariance has rapidly established itself as one of the most used concepts in space
plasmas to uncover underlying physical mechanisms via the scaling-law behavior of the …

ABSTRACT We focus on Hinode Solar Optical Telescope (SOT) calcium II H-line
observations of a solar quiescent prominence (QP) that exhibits highly variable dynamics …

Extended or generalized similarity is a ubiquitous but not well understood feature of
turbulence that is realized over a finite range of scales. The ULYSSES spacecraft solar polar …

We investigate the intermittency of anisotropic magnetohydrodynamic (MHD) turbulence in
high-speed solar wind. Using the data recorded by the Ulysses spacecraft, we apply the …

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The solar wind provides unique opportunities for long duration in situ studies of
magnetohydrodynamic turbulence in a plasma flowing supersonically with high magnetic …

Turbulence is a highly non-linear process ubiquitous in Nature. The nonlinearity is
responsible for the coupling of many degrees of freedom leading to an unpredictable …