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Multi-scale Anti-correlation Between Electron Density and Magnetic Field Strength in the Solar Wind
DOI: 10.1088/0004-637X/728/2/146 Bibcode: 2011ApJ...728..146Y

Tu, C. -Y.; Marsch, E.; Rème, H. +4 more

This work focuses on the relation between the electron density and the magnetic field strength in the solar wind, and aims to reveal its compressive nature and to determine the level of compressibility. For this purpose, we choose a period of quiet solar wind data obtained at 1 AU by the Cluster C1 satellite. The electron density is derived with a…

2011 The Astrophysical Journal
Cluster 73
The Dissipation of Solar Wind Turbulent Fluctuations at Electron Scales
DOI: 10.1088/0004-637X/730/2/114 Bibcode: 2011ApJ...730..114C

Burgess, David; Camporeale, Enrico

We present two-dimensional fully kinetic particle-in-cell simulations of decaying electromagnetic fluctuations. The computational box is such that wavelengths ranging from electron to ion gyroradii are resolved. The parameters used are realistic for the solar wind, and the ion-to-electron mass ratio is physical. The dissipation of turbulent fluctu…

2011 The Astrophysical Journal
Cluster 56
Detection of Current Sheets and Magnetic Reconnections at the Turbulent Leading Edge of an Interplanetary Coronal Mass Ejection
DOI: 10.1088/2041-8205/733/2/L34 Bibcode: 2011ApJ...733L..34C

Chian, Abraham C. -L.; Muñoz, Pablo R.

The relation between current sheets, turbulence, and magnetic reconnections at the leading edge of an interplanetary coronal mass ejection detected by four Cluster spacecraft on 2005 January 21 is studied. We report the observational evidence of two magnetically reconnected current sheets in the vicinity of a front magnetic cloud boundary layer wi…

2011 The Astrophysical Journal
Cluster 47