SM006
Causes and consequences of energetic particle losses in the coupled ionosphere-thermosphere-magnetosphere system
Causes and consequences of energetic particle losses in the coupled ionosphere-thermosphere-magnetosphere system
Session ID#: 77217
Session Description:
Particle losses act as one of the dominant processes contributing to the dynamic variations of energetic particles in the magnetosphere. These loss processes take place over a wide range of spatial scales from local wave-particle interactions to large system-scales, and on timescales from seconds to tens of days. With growing observations from space- and ground-based missions and development of sophisticated models, advances have been made on improved understanding of the context, causes, and consequences of magnetospheric particle losses. This session solicits presentations that feature recent progress made from ground-based and satellite observations and theoretical investigations to comprehend the losses of energetic particles and their effects on the ionosphere-thermosphere-magnetosphere coupled system. We encourage results utilizing measurements from Heliophysics System Observatory (e.g., Van Allen Probes, Arase, MMS, THEMIS, GOES) in conjunction with low-altitude and/or ground-based measurements (e.g., BARREL, POES, FIREBIRD, CubeSats, ground-based imagers, riometers and magnetometers) and coordinated modeling and theoretical efforts.
Index Terms:
2764 Plasma sheet [MAGNETOSPHERIC PHYSICS]
2774 Radiation belts [MAGNETOSPHERIC PHYSICS]
7859 Transport processes [SPACE PLASMA PHYSICS]
7867 Wave/particle interactions [SPACE PLASMA PHYSICS]
Primary Convener: Hong Zhao, University of Colorado at Boulder, Boulder, CO, United States
Conveners: Binbin Ni, Wuhan University, Wuhan, China, Jacob Bortnik, University of California Los Angeles, Atmospheric and Oceanic Sciences, Los Angeles, CA, United States and Allison N Jaynes, University of Colorado at Boulder, LASP, Boulder, CO, United States
Primary Liaison: Binbin Ni, Wuhan University, Wuhan, China
See more of: SPA-Magnetospheric Physics
