A dynamical model of plasma turbulence in the solar wind
GG Howes - … Transactions of the Royal Society A …, 2015 - royalsocietypublishing.org
A dynamical approach, rather than the usual statistical approach, is taken to explore the
physical mechanisms underlying the nonlinear transfer of energy, the damping of the …
physical mechanisms underlying the nonlinear transfer of energy, the damping of the …
Numerical magneto-hydrodynamics for relativistic nuclear collisions
G Inghirami, L Del Zanna, A Beraudo… - The European Physical …, 2016 - Springer
We present an improved version of the ECHO-QGP numerical code, which self-consistently
includes for the first time the effects of electromagnetic fields within the framework of …
includes for the first time the effects of electromagnetic fields within the framework of …
Evolution of large-amplitude Alfvén waves and generation of switchbacks in the expanding solar wind
Abstract Motivated by recent Parker Solar Probe (PSP) observations of" switchbacks"(abrupt,
large-amplitude reversals in the radial magnetic field, which exhibit Alfvénic correlations) …
large-amplitude reversals in the radial magnetic field, which exhibit Alfvénic correlations) …
On the 1/f spectrum in the solar wind and its connection with magnetic compressibility
L Matteini, D Stansby, TS Horbury… - The Astrophysical …, 2018 - iopscience.iop.org
On the 1/f Spectrum in the Solar Wind and Its Connection with Magnetic Compressibility -
IOPscience This site uses cookies. By continuing to use this site you agree to our use of cookies …
IOPscience This site uses cookies. By continuing to use this site you agree to our use of cookies …
New observations of solar wind 1/f turbulence spectrum from Parker Solar Probe
The trace magnetic power spectrum in the solar wind is known to be characterized by a
double power law at scales much larger than the proton gyro-radius, with flatter spectral …
double power law at scales much larger than the proton gyro-radius, with flatter spectral …
A self-consistent model of the coronal heating and solar wind acceleration including compressible and incompressible heating processes
We propose a novel one-dimensional model that includes both shock and turbulence
heating and qualify how these processes contribute to heating the corona and driving the …
heating and qualify how these processes contribute to heating the corona and driving the …
Alfvénic fluctuations in the expanding solar wind: Formation and radial evolution of spherical polarization
We investigate properties of large-scale solar wind Alfvénic fluctuations and their evolution
during radial expansion. We assume a strictly radial background magnetic field B∥ R, and …
during radial expansion. We assume a strictly radial background magnetic field B∥ R, and …
Frequency-dependent Alfvén-wave propagation in the solar wind: onset and suppression of parametric decay instability
Using numerical simulations we investigate the onset and suppression of parametric decay
instability (PDI) in the solar wind, focusing on the suppression effect by the wind acceleration …
instability (PDI) in the solar wind, focusing on the suppression effect by the wind acceleration …
Alfvén-wave-driven magnetic rotator winds from low-mass stars. I. Rotation dependences of magnetic braking and mass-loss rate
Observations of stellar rotation show that low-mass stars lose angular momentum during the
main sequence. We simulate the winds of sunlike stars with a range of rotation rates …
main sequence. We simulate the winds of sunlike stars with a range of rotation rates …
Expanding-box quasilinear model of the solar wind
J Seough, PH Yoon, Y Nariyuki… - The Astrophysical …, 2023 - iopscience.iop.org
The expanding-box model of the solar wind has been adopted in the literature within the
context of magnetohydrodynamics, hybrid, and full particle-in-cell simulations to investigate …
context of magnetohydrodynamics, hybrid, and full particle-in-cell simulations to investigate …