SH011
Instabilities and Their Role in Modifying Plasma Dynamics
Instabilities and Their Role in Modifying Plasma Dynamics
Session ID#: 75936
Session Description:
Plasma throughout the heliosphere is subject to a large variety of instabilities driven by processes ranging from differential flows and temperature anisotropies to large amplitude waves. While the temperature anisotropy and drift-driven instabilities are often invoked when discussing the global evolution of plasmas such as the solar wind, these instabilities can also have a dramatic effect on the local dynamics of the plasma, modifying momentum transport and heating, and efficiently scattering particles. In this session, we hope to examine the interplay between instabilities and other fundamental plasma processes at work in the heliosphere, such as turbulence, reconnection, and shocks, through the use of observational data and numerical simulations. This interplay is particularly timely due to the availability of low-beta, near-Sun plasma data from Parker Solar Probe and high resolution and cadence field and particle data from the Magnetospheric Multiscale mission.
Index Terms:
2772 Plasma waves and instabilities [MAGNETOSPHERIC PHYSICS]
7829 Kinetic waves and instabilities [SPACE PLASMA PHYSICS]
7836 MHD waves and instabilities [SPACE PLASMA PHYSICS]
7839 Nonlinear phenomena [SPACE PLASMA PHYSICS]
Primary Convener: Jason M TenBarge, Princeton University, Princeton, NJ, United States
Conveners: Kristopher G. Klein, University of Arizona, Lunar and Planetary Laboratory, Tucson, AZ, United States and Bennett Maruca, University of Delaware, Department of Physics and Astronomy, Newark, DE, United States
Primary Liaison: Jason M TenBarge, Princeton University, Princeton, NJ, United States
See more of: SPA-Solar and Heliospheric Physics
