SCALING OF THE ELECTRON DISSIPATION RANGE OF SOLAR WIND TURBULENCE
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 scale, but continues cascading down to electron scales. However, the scaling of the magnetic energy spectra as well as the nature of the plasma …