SA008
Energetic Precipitation Effects in the Middle and Upper Atmosphere
Energetic Precipitation Effects in the Middle and Upper Atmosphere
Session ID#: 82263
Session Description:
Precipitating energetic particles have been shown to be able to change the mean state of the atmosphere. Energetic precipitation with different origins (magnetosphere plasma sheet, radiation belt, solar energetic protons, cosmic rays) can penetrate into different layers of the atmosphere and affect atmospheric chemistry and dynamics in different ways. For example, the changes of ionospheric conductivity in the upper atmosphere due to auroral precipitation directly affect the electrodynamic coupling between the magnetosphere and the ionosphere, and heating and forcing of the atmosphere at different altitudes. Relativistic precipitation produces nitrogen and hydrogen oxides in the middle atmosphere which have both local and global influences on ozone concentration and radiative heating/cooling. This session addresses issues related to the precipitation effects in the middle and upper atmosphere using observations and models. This topic couples the solar, magnetospheric, ionospheric, and atmospheric physics which will be of interest for both atmospheric and heliospheric communities.
Co-Organized:
- SM - SPA-Magnetospheric Physics
Index Terms:
0341 Middle atmosphere: constituent transport and chemistry [ATMOSPHERIC COMPOSITION AND STRUCTURE]
2716 Energetic particles: precipitating [MAGNETOSPHERIC PHYSICS]
2788 Magnetic storms and substorms [MAGNETOSPHERIC PHYSICS]
3334 Middle atmosphere dynamics [ATMOSPHERIC PROCESSES]
Primary Convener: Dong Lin, Virginia Polytechnic Institute and State University, Blacksburg, VA, United States
Conveners: Wenbin Wang1, Harlan E. Spence2 and Chia-Lin Huang2, (1)NCAR, HAO, Boulder, CO, United States(2)University of New Hampshire, Durham, NH, United States
Primary Liaison: Dong Lin, Virginia Polytechnic Institute and State University, Blacksburg, VA, United States
See more of: SPA-Aeronomy
