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 …
Shell models of magnetohydrodynamic turbulence
Shell models of hydrodynamic turbulence originated in the seventies. Their main aim was to
describe the statistics of homogeneous and isotropic turbulence in spectral space, using a …
describe the statistics of homogeneous and isotropic turbulence in spectral space, using a …
Ion‐scale spectral break of solar wind turbulence at high and low beta
The power spectrum of magnetic fluctuations in the solar wind at 1 AU displays a break
between two power laws in the range of spacecraft‐frame frequencies 0.1 to 1 Hz. These …
between two power laws in the range of spacecraft‐frame frequencies 0.1 to 1 Hz. These …
Solar wind turbulent spectrum at plasma kinetic scales
O Alexandrova, C Lacombe, A Mangeney… - The Astrophysical …, 2012 - iopscience.iop.org
The description of the turbulent spectrum of magnetic fluctuations in the solar wind in the
kinetic range of scales is not yet completely established. Here, we perform a statistical study …
kinetic range of scales is not yet completely established. Here, we perform a statistical study …
Evidence for electron Landau dam** in space plasma turbulence
How turbulent energy is dissipated in weakly collisional space and astrophysical plasmas is
a major open question. Here, we present the application of a field-particle correlation …
a major open question. Here, we present the application of a field-particle correlation …
Spectrum of kinetic-Alfvén turbulence
S Boldyrev, JC Perez - The Astrophysical Journal Letters, 2012 - iopscience.iop.org
ABSTRACT A numerical study of strong kinetic-Alfvén turbulence at scales smaller than the
ion gyroscale is presented, and a phenomenological model is proposed that argues that …
ion gyroscale is presented, and a phenomenological model is proposed that argues that …
Scaling of the electron dissipation range of solar wind turbulence
Electron scale solar wind (SW) turbulence has attracted great interest in recent years.
Considerable evidence exists that the turbulence is not fully dissipated near the proton …
Considerable evidence exists that the turbulence is not fully dissipated near the proton …
Nature of subproton scale turbulence in the solar wind
CHK Chen, S Boldyrev, Q ** in kinetic plasma turbulence
JM TenBarge, GG Howes - The Astrophysical Journal Letters, 2013 - iopscience.iop.org
We present the first study of the formation and dissipation of current sheets at electron scales
in a wave-driven, weakly collisional, three-dimensional kinetic turbulence simulation. We …
in a wave-driven, weakly collisional, three-dimensional kinetic turbulence simulation. We …
Wave‐particle interaction of Alfvén waves in Jupiter's magnetosphere: Auroral and magnetospheric particle acceleration
We investigate spatial and temporal scales at which wave‐particle interaction of Alfvén
waves occurs in Jupiter's magnetosphere. We consider electrons, protons, and oxygen ions …
waves occurs in Jupiter's magnetosphere. We consider electrons, protons, and oxygen ions …