SM034
Plasma Convection in the Subauroral Ionosphere and Coupled Inner Magnetosphere
Plasma Convection in the Subauroral Ionosphere and Coupled Inner Magnetosphere
Session ID#: 83712
Session Description:
Plasma convection in the subauroral region is influenced by different driving forces such as the neutral winds, penetration electric fields, and polarization electric fields (SAPS). Ionospheric conductivity plays an important role in modulating the relative importance of these different drivers. The electric fields interact with the inner magnetosphere, affecting plasma dynamics over a broad energy range. Significant increase in observations from several instruments, such as Van Allen Probes, AMPERE, GPS TEC, and radars, as well as advances in modeling techniques, such as self-consistent coupling between the ionosphere, thermosphere and magnetosphere, provide an outstanding opportunity to study the subauroral region. This session solicits theoretical, numerical, and/or experimental contributions that address the (1) physics of convection in the subauroral ionosphere and/or conjugate inner magnetosphere, (2) influence of ionospheric conductivity and the neutral winds in modulating convection, and (3) significance of convection in terms of plasma dynamics across the energy spectrum.
Index Terms:
2443 Midlatitude ionosphere [IONOSPHERE]
2463 Plasma convection [IONOSPHERE]
2712 Electric fields [MAGNETOSPHERIC PHYSICS]
2730 Magnetosphere: inner [MAGNETOSPHERIC PHYSICS]
Primary Convener: J. Michael Ruohoniemi, Virginia Polytechnic Institute and State University, Blacksburg, VA, United States
Conveners: Naomi Maruyama, University of Colorado, Boulder, CO, United States, Solene Lejosne, Space Sciences Laboratory, Berkeley, CA, United States and Bharat Kunduri, Virginia Tech, Blacksburg, VA, United States
Primary Liaison: J. Michael Ruohoniemi, Virginia Polytechnic Institute and State University, Blacksburg, VA, United States
See more of: SPA-Magnetospheric Physics
