Alfvenic current system in Saturn's magnetosphere and time variation of the magnetic field in the outer Saturn magnetosphere.
Abstract
We describe all toroidal and poloidal currents connected by each to other through the ratio of the Pedersen and Hall ionospheric conductivities as parts of the total current system. We added the azimuthal field B_phi created by the field-aligned currents to the global paraboloid model of the magnetic field in the Kronian magnetospheres
- Publication:
-
European Planetary Science Congress
- Pub Date:
- September 2018
- Bibcode:
- 2018EPSC...12.1134A