Please note that this session was withdrawn and is no longer available in the respective programme. This withdrawal might have been the result of a merge with another session.
ST2.3 | Particle Precipitation: Drivers, Properties, and Impacts on Atmosphere, Ionosphere, Magnetosphere Coupling
Particle Precipitation: Drivers, Properties, and Impacts on Atmosphere, Ionosphere, Magnetosphere Coupling
Precipitation of particles into planetary atmospheres is a fundamental heliophysics process. At Earth, precipitation transfers energy from the solar wind and magnetosphere into the ionosphere and upper atmosphere. This dynamic coupling between plasma regimes leads to a variety of impacts on the upper atmosphere; from vibrant auroral displays, to generation of ionospheric current systems, changes in atmospheric chemistry and impacts on satellite infrastructure through increased satellite drag. This session takes a system-science perspective on particle precipitation across wide ranging energies and impacts on and in the atmosphere. We invite presentations which focus on links between the drivers and their relative importance in generating particle precipitation; the spatiotemporal dynamics of large-scale system processes; and the impacts of particle precipitation on atmospheric conductivity, chemistry, and dynamics.
Please decide on your access
Please use the buttons below to download the supplementary material or to visit the external website where the presentation is linked. Regarding the external link, please note that Copernicus Meetings cannot accept any liability for the content and the website you will visit.
You are going to open an external link to the asset as indicated by the session. Copernicus Meetings cannot accept any liability for the content and the website you will visit.
