Kinetic scale turbulence and dissipation in the solar wind: key observational results and future outlook
Turbulence is ubiquitous in the solar wind. Turbulence causes kinetic and magnetic energy
to cascade to small scales where they are eventually dissipated, adding heat to the plasma …
to cascade to small scales where they are eventually dissipated, adding heat to the plasma …
Nature of subproton scale turbulence in the solar wind
The nature of subproton scale fluctuations in the solar wind is an open question, partly
because two similar types of electromagnetic turbulence can occur: kinetic Alfvén turbulence …
because two similar types of electromagnetic turbulence can occur: kinetic Alfvén turbulence …
Kinetic cascade in solar-wind turbulence: 3D3V hybrid-kinetic simulations with electron inertia
Understanding the nature of the turbulent fluctuations below the ion gyroradius in solar-wind
(SW) turbulence is a great challenge. Recent studies have been mostly in favor of kinetic …
(SW) turbulence is a great challenge. Recent studies have been mostly in favor of kinetic …
Collisionless shocks in partly ionized plasma with cosmic rays: microphysics of non-thermal components
AM Bykov, MA Malkov, JC Raymond… - Space Science …, 2013 - Springer
In this review we discuss some observational aspects and theoretical models of
astrophysical collisionless shocks in partly ionized plasma with the presence of non-thermal …
astrophysical collisionless shocks in partly ionized plasma with the presence of non-thermal …
Subproton-scale cascades in solar wind turbulence: driven hybrid-kinetic simulations
ABSTRACT A long-lasting debate in space plasma physics concerns the nature of
subproton-scale fluctuations in solar wind (SW) turbulence. Over the past decade, a series of …
subproton-scale fluctuations in solar wind (SW) turbulence. Over the past decade, a series of …
[图书][B] Classical kinetic theory of weakly turbulent nonlinear plasma processes
PH Yoon - 2019 - books.google.com
Kinetic theory of weakly turbulent nonlinear processes in plasma helped form the foundation
of modern plasma physics. This book provides a systematic overview of the kinetic theory of …
of modern plasma physics. This book provides a systematic overview of the kinetic theory of …
Transition from kinetic to MHD behavior in a collisionless plasma
The study of kinetic effects in heliospheric plasmas requires representation of dynamics at
sub-proton scales, but in most cases the system is driven by magnetohydrodynamic (MHD) …
sub-proton scales, but in most cases the system is driven by magnetohydrodynamic (MHD) …
The origin of non-Maxwellian solar wind electron velocity distribution function: Connection to nanoflares in the solar corona
H Che, ML Goldstein - The Astrophysical Journal Letters, 2014 - iopscience.iop.org
The formation of the observed core-halo feature in the solar wind electron velocity
distribution function is a long-time puzzle. In this Letter, based on the current knowledge of …
distribution function is a long-time puzzle. In this Letter, based on the current knowledge of …
On the Fourier Contribution of Strong Current Sheets to the High‐Frequency Magnetic Power SpectralDensity of the Solar Wind
JE Borovsky, BL Burkholder - Journal of Geophysical Research …, 2020 - Wiley Online Library
The hypothesis is explored that the high‐frequency magnetic spectral power of the solar
wind is associated with the spatial profiles of strong current sheets (directional …
wind is associated with the spatial profiles of strong current sheets (directional …
Spectral breaks of Alfvénic turbulence in a collisionless plasma
Recent observations reveal that magnetic turbulence in the nearly colisionless solar wind
plasma extends to scales smaller than the plasma microscales, such as ion gyroradius and …
plasma extends to scales smaller than the plasma microscales, such as ion gyroradius and …