Marsch, Eckart MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society; Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;
He, J., Tu, C., Marsch, E., & Yao, S. (2012). Do oblique Alfven/ion-cyclotron or fast-mode/whistler waves dominate the dissipation of solar wind turbulence near the proton inertial length? Astrophysical Journal, 745: L8. doi:10.1088/2041-8205/745/1/L8.