Comparative Planetary Magnetospheric Processes
Comparative Planetary Magnetospheric Processes
Session ID#: 279419
Session Description:
Planetary magnetospheres across the Solar System provide a unique opportunity to investigate fundamental plasma processes under a wide range of physical conditions. This session invites contributions that explore and compare key mechanisms across planetary magnetospheres, including (but not limited to) magnetotail dynamics, current systems, radiation belts, plasma waves, solar wind-magnetosphere interaction, and magnetosphere-ionosphere coupling. By examining both the similarities and distinctions among these systems, we aim to identify universal processes as well as unique drivers shaped by each planet’s environment. While presentations focused on individual planets (including Earth) are welcome, we especially encourage studies that leverage multi-mission observations, theory and modeling to explore magnetospheric processes from a comparative perspective and address broader, cross-planetary scientific questions.
Co-Sponsor(s):
- P - Planetary Sciences
- SA - SPA-Aeronomy
Index Terms:
2437 Ionospheric dynamics [IONOSPHERE]
6207 Comparative planetology [PLANETARY SCIENCES: SOLAR SYSTEM OBJECTS]
7845 Particle acceleration [SPACE PLASMA PHYSICS]
7867 Wave/particle interactions [SPACE PLASMA PHYSICS]
Primary Convener: Wen Li, Boston University, Astronomy, Boston, MA, United States
Conveners: George B Clark, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States and Robert Andrew Marshall, University of Colorado at Boulder, Ann & H.J. Smead Department of Aerospace Engineering Sciences, Boulder, United States
Student/Early Career Convener: Ryan M. Dewey, Laboratory for Atmospheric and Space Physics, Boulder, United States
See more of: SPA-Magnetospheric Physics