Solar wind turbulence and the role of ion instabilities
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 …
addition to the presence of magnetic field, the differences with neutral fluid isotropic …
Theory and transport of nearly incompressible magnetohydrodynamic turbulence
The theory of nearly incompressible magnetohydrodynamics (NI MHD) was developed
largely in the early 1990s, together with an important extension to inhomogeneous flows in …
largely in the early 1990s, together with an important extension to inhomogeneous flows in …
Intermittency in solar wind turbulence from fluid to kinetic scales
R Bruno - Earth and Space Science, 2019 - Wiley Online Library
Solar wind is a highly turbulent medium exhibiting fluctuations ranging from the solar
sidereal rotation period to proton and electron gyroperiods. Their amplitudes show …
sidereal rotation period to proton and electron gyroperiods. Their amplitudes show …
Strong anticipation: Multifractal cascade dynamics modulate scaling in synchronization behaviors
DG Stephen, JA Dixon - Chaos, Solitons & Fractals, 2011 - Elsevier
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 …
behavior may attune to the fractal scaling of an unpredictable signal [Stephen DG, Stepp N …
Methods for characterising microphysical processes in plasmas
Advanced spectral and statistical data analysis techniques have greatly contributed to
shaping our understanding of microphysical processes in plasmas. We review some of the …
shaping our understanding of microphysical processes in plasmas. We review some of the …
Compressibility in solar wind plasma turbulence
B Hnat, SC Chapman, G Rowlands - Physical review letters, 2005 - APS
Incompressible magnetohydrodynamics is often assumed to describe solar wind turbulence.
We use extended self-similarity to reveal scaling in the structure functions of density …
We use extended self-similarity to reveal scaling in the structure functions of density …
Arbitrary-order Hilbert spectral analysis and intermittency in solar wind density fluctuations
F Carbone, L Sorriso-Valvo, T Alberti… - The Astrophysical …, 2018 - iopscience.iop.org
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 …
with the arbitrary-order Hilbert spectral analysis method, applied to high-resolution density …
Statistical study of electron density turbulence and ion-cyclotron waves in the inner heliosphere: Solar Orbiter observations
F Carbone, L Sorriso-Valvo, YV Khotyaintsev… - Astronomy & …, 2021 - aanda.org
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 …
board Solar Orbiter has been used to estimate the solar wind electron density in the inner …
Multifractal analysis of high resolution solar wind proton density measurements
L Sorriso-Valvo, F Carbone, E Leonardis… - Advances in Space …, 2017 - Elsevier
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 …
a broad range of scales. These include an inertial range where a turbulent cascade is …
Stochastic interpolation of sparsely sampled time series by a superstatistical random process and its synthesis in Fourier and wavelet space
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 …
based on a superstatistical random process generated from a multivariate Gaussian scale …