EGU2020-4108, updated on 10 Dec 2020
https://doi.org/10.5194/egusphere-egu2020-4108
EGU General Assembly 2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.

Transport ratios of the kinetic Alfvén mode in space plasmas

Yasuhito Narita1, Zoltan Vörös1, Owen Wyn Roberts1, and Masahiro Hoshino2
Yasuhito Narita et al.
  • 1Space Research Institute, Austrian Academy of Sciences, Graz, Austria
  • 2Graduate School of Science, The University of Tokyo, Tokyo, Japan

Electric field properties of the kinetic Alfvén mode are analytically studied by constructing the dielectric tensor of the plasma using the linear Vlasov theory and reducing (and identifying) the tensor elements into that of the fluid picture such as the polarization drift, the Hall current, and the diamagnetic current. Off-diagonal dielectric responses do not primarly contribute to the dispersion relation of the kinetic Alfvén mode, but play an important role in the electric field polarization (field rotation sense around the mean magnetic field) and parallel component of the field. The polarization becomes more circular and the parallel component enhances at larger perpendicular wavenumbers. Analytic expression of fluctuation sense serves as a tool to identify the kinetic Alfvén mode in space plasma observations.

How to cite: Narita, Y., Vörös, Z., Roberts, O. W., and Hoshino, M.: Transport ratios of the kinetic Alfvén mode in space plasmas, EGU General Assembly 2020, Online, 4–8 May 2020, EGU2020-4108, https://doi.org/10.5194/egusphere-egu2020-4108, 2020