SH016
Interstellar Medium Traces in the Time-Varying Heliosphere
Interstellar Medium Traces in the Time-Varying Heliosphere
Session ID#: 157057
Session Description:
The local interstellar medium in the solar neighborhood contains plasma, magnetic fields, neutral atoms, and cosmic rays, which influence the heliosphere through interconnected time-dependent and multi-scale processes. The plasma and magnetic field determine the heliospheric boundary where neutral atoms and cosmic rays are filtered. The neutral atoms penetrate the heliosphere, where they are ionized, becoming pickup ions, which are subsequently energized and neutralized, creating energetic neutral atoms. These different components are observed through a combination of in situ sampling and remote imaging by, e.g., Voyager, New Horizons, IBEX, Cassini, and the upcoming IMAP mission. Physical interpretation of these observations requires theories and models on scales from interplanetary shocks to the global heliosphere. In this session, we invite presentations on observations, theory, and modeling concerning plasma, magnetic fields, neutral atoms, pickup ions, and cosmic rays in the time-varying heliosphere and the very local interstellar medium.
Index Terms:
2126 Heliosphere/interstellar medium interactions [INTERPLANETARY PHYSICS]
2151 Neutral particles [INTERPLANETARY PHYSICS]
2152 Pickup ions [INTERPLANETARY PHYSICS]
7536 Solar activity cycle [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
Primary Convener: Pawel Swaczyna, Princeton University, Department of Astrophysical Sciences, Princeton, NJ, United States
Conveners: Elena Provornikova, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States and Federico Fraternale, University of Alabama in Huntsville, Center for Space Plasma and Aeronomic Research, Huntsville, AL, United States
See more of: SPA-Solar and Heliospheric Physics
