Intermittency, nonlinear dynamics and dissipation in the solar wind and astrophysical plasmas
An overview is given of important properties of spatial and temporal intermittency, including
evidence of its appearance in fluids, magnetofluids and plasmas, and its implications for …
evidence of its appearance in fluids, magnetofluids and plasmas, and its implications for …
Magnetohydrodynamic and kinetic scale turbulence in the near-Earth space plasmas: a (short) biased review
The near-Earth space is a unique laboratory to explore turbulence and energy dissipation
processes in magnetized plasmas thanks to the availability of high-quality data from various …
processes in magnetized plasmas thanks to the availability of high-quality data from various …
Kinetic instabilities in the solar wind driven by temperature anisotropies
PH Yoon - Reviews of Modern Plasma Physics, 2017 - Springer
The present paper comprises a review of kinetic instabilities that may be operative in the
solar wind, and how they influence the dynamics thereof. The review is limited to collective …
solar wind, and how they influence the dynamics thereof. The review is limited to collective …
Observations of turbulence in a Kelvin‐Helmholtz event on 8 September 2015 by the Magnetospheric Multiscale mission
Spatial and high‐time‐resolution properties of the velocities, magnetic field, and 3‐D electric
field within plasma turbulence are examined observationally using data from the …
field within plasma turbulence are examined observationally using data from the …
The role of proton cyclotron resonance as a dissipation mechanism in solar wind turbulence: a statistical study at ion-kinetic scales
We use magnetic field and ion moment data from the MFI and SWE instruments on board the
Wind spacecraft to study the nature of solar wind turbulence at ion-kinetic scales. We …
Wind spacecraft to study the nature of solar wind turbulence at ion-kinetic scales. We …
Compressible Magnetohydrodynamic Turbulence in the Earth's Magnetosheath: Estimation of the Energy Cascade Rate Using in situ Spacecraft Data
The first estimation of the energy cascade rate| ε C| of magnetosheath turbulence is obtained
using the Cluster and THEMIS spacecraft data and an exact law of compressible isothermal …
using the Cluster and THEMIS spacecraft data and an exact law of compressible isothermal …
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 …
Solar wind turbulence around Mars: Relation between the energy cascade rate and the proton cyclotron waves activity
The first estimation of the incompressible energy cascade rate at magnetohydrodynamic
(MHD) scales in the plasma upstream of the Martian bow shock is obtained, making use of …
(MHD) scales in the plasma upstream of the Martian bow shock is obtained, making use of …
Observations of heating along intermittent structures in the inner heliosphere from PSP data
RA Qudsi, BA Maruca, WH Matthaeus… - The Astrophysical …, 2020 - iopscience.iop.org
The solar wind proton temperature at 1 au has been found to be correlated with small-scale
intermittent magnetic structures, ie, regions with enhanced temperature are associated with …
intermittent magnetic structures, ie, regions with enhanced temperature are associated with …
Nonlinear and linear timescales near kinetic scales in solar wind turbulence
The application of linear kinetic treatments to plasma waves, damping, and instability
requires favorable inequalities between the associated linear timescales and timescales for …
requires favorable inequalities between the associated linear timescales and timescales for …