Search Publications

Local Kinetic Effects in Two-Dimensional Plasma Turbulence
DOI: 10.1103/PhysRevLett.108.045001 Bibcode: 2012PhRvL.108d5001S

Veltri, P.; Califano, F.; Servidio, S. +1 more

Using direct numerical simulations of a hybrid Vlasov-Maxwell model, kinetic processes are investigated in a two-dimensional turbulent plasma. In the turbulent regime, kinetic effects manifest through a deformation of the ion distribution function. These patterns of non-Maxwellian features are concentrated in space nearby regions of strong magneti…

2012 Physical Review Letters
Cluster 181
Intermittent Dissipation at Kinetic Scales in Collisionless Plasma Turbulence
DOI: 10.1103/PhysRevLett.109.195001 Bibcode: 2012PhRvL.109s5001W

Matthaeus, W. H.; Chapman, S. C.; Daughton, W. +6 more

High resolution kinetic simulations of collisionless plasma driven by shear show the development of turbulence characterized by dynamic coherent sheetlike current density structures spanning a range of scales down to electron scales. We present evidence that these structures are sites for heating and dissipation, and that stronger current structur…

2012 Physical Review Letters
Cluster 164
Detection of Small-Scale Structures in the Dissipation Regime of Solar-Wind Turbulence
DOI: 10.1103/PhysRevLett.109.191101 Bibcode: 2012PhRvL.109s1101P

Perri, S.; Sahraoui, F.; Goldstein, M. L. +1 more

Recent observations of the solar wind have pointed out the existence of a cascade of magnetic energy from the scale of the proton Larmor radius ρp down to the electron Larmor radius ρe scale. In this Letter we study the spatial properties of magnetic field fluctuations in the solar wind and find that at small scales the magne…

2012 Physical Review Letters
Cluster 118
Particle Acceleration in Turbulence and Weakly Stochastic Reconnection
DOI: 10.1103/PhysRevLett.108.241102 Bibcode: 2012PhRvL.108x1102K

Lazarian, A.; Kowal, Grzegorz; de Gouveia Dal Pino, Elisabete M.

In this Letter we analyze the energy distribution evolution of test particles injected in three dimensional (3D) magnetohydrodynamic (MHD) simulations of different magnetic reconnection configurations. When considering a single Sweet-Parker topology, the particles accelerate predominantly through a first-order Fermi process, as predicted in and de…

2012 Physical Review Letters
Cluster 109
Lower Hybrid Drift Waves: Space Observations
DOI: 10.1103/PhysRevLett.109.055001 Bibcode: 2012PhRvL.109e5001N

Khotyaintsev, Yuri V.; Vaivads, Andris; André, Mats +1 more

Lower hybrid drift waves (LHDWs) are commonly observed at plasma boundaries in space and laboratory, often having the strongest measured electric fields within these regions. We use data from two of the Cluster satellites (C3 and C4) located in Earth’s magnetotail and separated by a distance of the order of the electron gyroscale. These conditions…

2012 Physical Review Letters
Cluster 86
Secondary Magnetic Islands Generated by the Kelvin-Helmholtz Instability in a Reconnecting Current Sheet
DOI: 10.1103/PhysRevLett.108.255005 Bibcode: 2012PhRvL.108y5005F

Drake, J. F.; Swisdak, M.; Fermo, R. L.

Magnetic islands or flux ropes produced by magnetic reconnection have been observed on the magnetopause, in the magnetotail, and in coronal current sheets. Particle-in-cell simulations of magnetic reconnection with a guide field produce elongated electron current layers that spontaneously produce secondary islands. Here, we explore the seed mechan…

2012 Physical Review Letters
Cluster 71
Spontaneous Chiral Symmetry Breaking of Hall Magnetohydrodynamic Turbulence
DOI: 10.1103/PhysRevLett.109.194501 Bibcode: 2012PhRvL.109s4501M

Galtier, Sébastien; Meyrand, Romain

Hall magnetohydrodynamics (MHD) is investigated through three-dimensional direct numerical simulations. We show that the Hall effect induces a spontaneous chiral symmetry breaking of the turbulent dynamics. The normalized magnetic polarization is introduced to separate the right- (R) and left-handed (L) fluctuations. A classical k-7/3 s…

2012 Physical Review Letters
Cluster 61
Dispersive Nature of High Mach Number Collisionless Plasma Shocks: Poynting Flux of Oblique Whistler Waves
DOI: 10.1103/PhysRevLett.108.025002 Bibcode: 2012PhRvL.108b5002S

Bale, S. D.; Krasnoselskikh, V.; Schwartz, S. J. +3 more

Whistler wave trains are observed in the foot region of high Mach number quasiperpendicular shocks. The waves are oblique with respect to the ambient magnetic field as well as the shock normal. The Poynting flux of the waves is directed upstream in the shock normal frame starting from the ramp of the shock. This suggests that the waves are an inte…

2012 Physical Review Letters
Cluster 38
Entropy Generation across Earth's Collisionless Bow Shock
DOI: 10.1103/PhysRevLett.108.061102 Bibcode: 2012PhRvL.108f1102P

Dandouras, I.; Cao, J. B.; Parks, G. K. +9 more

Earth’s bow shock is a collisionless shock wave but entropy has never been directly measured across it. The plasma experiments on Cluster and Double Star measure 3D plasma distributions upstream and downstream of the bow shock allowing calculation of Boltzmann’s entropy function H and his famous H theorem, dH/dt≤0. The collisionless Boltzmann (Vla…

2012 Physical Review Letters
Cluster 20
Observations of Ionospheric Electron Beams in the Plasma Sheet
DOI: 10.1103/PhysRevLett.109.205001 Bibcode: 2012PhRvL.109t5001Z

Parks, G. K.; Fu, S. Y.; Pu, Z. Y. +3 more

Electrons streaming along the magnetic field direction are frequently observed in the plasma sheet of Earth’s geomagnetic tail. The impact of these field-aligned electrons on the dynamics of the geomagnetic tail is however not well understood. Here we report the first detection of field-aligned electrons with fluxes increasing at ∼1keV forming a “…

2012 Physical Review Letters
Cluster 19