Solar wind is probably the best laboratory to study turbulence in astrophysical plasmas. In
addition to the presence of magnetic field, the differences with neutral fluid isotropic …

The theory of nearly incompressible magnetohydrodynamics (NI MHD) was developed
largely in the early 1990s, together with an important extension to inhomogeneous flows in …

Solar wind is a highly turbulent medium exhibiting fluctuations ranging from the solar
sidereal rotation period to proton and electron gyroperiods. Their amplitudes show …

Previous research on anticipatory behaviors has found that the fractal scaling of human
behavior may attune to the fractal scaling of an unpredictable signal [Stephen DG, Stepp N …

Advanced spectral and statistical data analysis techniques have greatly contributed to
shaping our understanding of microphysical processes in plasmas. We review some of the …

Incompressible magnetohydrodynamics is often assumed to describe solar wind turbulence.
We use extended self-similarity to reveal scaling in the structure functions of density …

The properties of inertial-and kinetic-range solar wind turbulence have been investigated
with the arbitrary-order Hilbert spectral analysis method, applied to high-resolution density …

Context. The recently released spacecraft potential measured by the RPW instrument on
board Solar Orbiter has been used to estimate the solar wind electron density in the inner …

The solar wind is a highly turbulent medium, with a high level of field fluctuations throughout
a broad range of scales. These include an inertial range where a turbulent cascade is …

We present a novel method for stochastic interpolation of sparsely sampled time signals
based on a superstatistical random process generated from a multivariate Gaussian scale …