SM010
Heavy Ions as Tracers and Regulators of Plasma Processes in the Solar System
Heavy Ions as Tracers and Regulators of Plasma Processes in the Solar System
Session ID#: 248740
Session Description:
Heavy ions (i.e., not protons) within planetary environments serve as important tracers for a multitude of plasma phenomena, such as ionospheric outflow, moon-magnetosphere and surface-plasma interactions, mass loading and transport, magnetic reconnection, and wave instabilities. This session solicits studies focusing on (1) data-driven analyses to reveal the sources, evolution and controlling factors of heavy ion flows, (2) the use of theoretical models and numerical simulations to investigate how heavy ions contribute to plasma dynamics, and (3) new mission or instrumentation concepts that can measure the properties of heavy ion flows. We invite researchers from solar, magnetospheric and ionospheric physics, as well as planetary science. We highly encourage comparative studies of different planetary environments throughout the solar system, including but not limited to the inner planets, outer planets and their moons.
Co-Sponsor(s):
- P - Planetary Sciences
Index Terms:
7845 Particle acceleration [SPACE PLASMA PHYSICS]
7846 Plasma energization [SPACE PLASMA PHYSICS]
7859 Transport processes [SPACE PLASMA PHYSICS]
7867 Wave/particle interactions [SPACE PLASMA PHYSICS]
Primary Convener: Kathleen Gwen Hanley, Space Sciences Laboratory, University of California Berkeley, Berkeley, United States
Conveners: Mei-Yun Lin, University of California Berkeley, Berkeley, United States, Weijie Sun, University of California Berkeley, Space Science Laboratory, Berkeley, CA, United States and Jamey R Szalay, Princeton University, Department of Astrophysical Sciences, Princeton, United States
See more of: SPA-Magnetospheric Physics