The role of EEP forcing and background dynamics on the seasonal NO variability in the MLT region
- 1Birkeland Centre for Space Science, University of Bergen, Norway
- 2Atmospheric Chemistry Observations and Modeling, National Center for Atmsopheric Research, USA
- 3School of Physics and Astronomy / School of Chemistry, University of Leeds, UK
Energetic electron precipitation (EEP) ionizes the Earth's atmosphere and leads to production of nitric oxide (NO) from 50 to 150 km altitude. In this study we investigate the direct and indirect NO response to EEP using the Whole Atmosphere Community Climate Model (WACCM). In comparison to observations from SOFIE / AIM (Solar Occultation For Ice Experiment / Aeronomy of Ice in the Mesosphere), we find that EEP production of NO in the D-region is well simulated when both medium energy electron precipitation and negative and cluster ion chemistry is included in the model. However, the main EEP production of NO occurs in the E-region, and there the observed and modeled production differ. This discrepancy impacts also the D-region, and is seasonally dependent with the highest underestimate of D-region NO occuring during winter. The modeled transport across the mesopause during winter is generally weak, but strengthens with increased gravity wave activity. Increased eddy diffusion, increases NO at all altitudes through the polar MLT region
How to cite: Smith-Johnsen, C., Tyssøy, H. N., Marsh, D., and Smith, A.: The role of EEP forcing and background dynamics on the seasonal NO variability in the MLT region, EGU General Assembly 2020, Online, 4–8 May 2020, EGU2020-4946, https://doi.org/10.5194/egusphere-egu2020-4946, 2020
This abstract will not be presented.