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SAMI3 ICON: MODEL OF THE IONOSPHERE/PLASMASPHERE SYSTEM
Summary
The NRL ionosphere/plasmasphere model SAMI3 was updated for NASA ICON, integrating data from TIEGCM-ICON and AMIE. This provides daily ionosphere and thermosphere data, including electron densities and total electron content (TEC).
Area of Science:
- Space Physics
- Atmospheric Science
- Aeronomy
Background:
- The ionosphere and plasmasphere are critical regions of Earth's upper atmosphere, influencing radio communications and satellite operations.
- Accurate modeling of these regions is essential for understanding space weather and its impacts.
- The Naval Research Laboratory (NRL) ionosphere/plasmasphere model, SAMI3, is a key tool for such studies.
Purpose of the Study:
- To modify the SAMI3 model to support the NASA Ionospheric Connection Explorer (ICON) mission.
- To enable daily runs of the SAMI3 ICON model for providing real-time ionosphere and thermosphere data.
- To enhance the scientific community's access to critical ionospheric and plasmaspheric parameters.
Main Methods:
- The SAMI3 model was adapted, creating a version named SAMI3 ICON.
- SAMI3 ICON was enhanced to import thermospheric composition, temperature, and winds from the Thermosphere-Ionosphere-Electrodynamics General Circulation Model (TIEGCM-ICON).
- High-latitude electric potential data from the Assimilative Model of Ionospheric Electrodynamics (AMIE) were incorporated.
Main Results:
- The modified SAMI3 ICON model is operational and ready for daily use during the ICON mission.
- The model will provide essential ionospheric and plasmaspheric parameters, including electron and ion densities, temperatures, and velocities.
- Key outputs will include total electron content (TEC), peak ionospheric electron density (NmF2), and the height of the F layer at NmF2 (hmF2).
Conclusions:
- The SAMI3 ICON model represents a significant advancement in simulating the ionosphere and plasmasphere.
- Daily data provision will greatly benefit the NASA ICON mission and the broader space science community.
- This enhanced modeling capability will improve our understanding of upper atmospheric dynamics and space weather.
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