Citations:gyroscale


 * 2005 A.A.Schekochihin et al, "Plasma instabilities and magnetic-field growth in clusters of galaxies" arXiv
 * However, their growth rates are proportional to the wavenumber down to the ion gyroscale, so MHD equations with Braginskii viscosity are not well posed and a fully kinetic treatment is necessary.
 * 2009 C. H. K. Chen et al, "Interpreting Power Anisotropy Measurements in Plasma Turbulence" arXiv
 * If fluctuations are anisotropic in shape then the ion gyroscale break point in spectra in the directions parallel and perpendicular to the magnetic field would not occur at the same frequency, and similarly for the electron gyroscale break point.
 * 2010 R. T. Wicks et al, "Power and spectral index anisotropy of the entire inertial range of turbulence in the fast solar wind" arXiv
 * We measure the power and spectral index anisotropy of high speed solar wind turbulence from scales larger than the outer scale down to the ion gyroscale, thus covering the entire inertial range.