High Latitude Thermosphere-Ionosphere Variability During the Solar Minimum IPY Period

Details High Latitude Thermosphere-Ionosphere Variability During the Solar Minimum IPY Period High Latitude Thermosphere-Ionosphere Variability During the Solar Minimum IPY Period

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agufmsa32a..02c&link_type=abstract

American Geophysical Union, Fall Meeting 2008, abstract #SA32A-02

Physics

2400 Ionosphere (6929), 2447 Modeling And Forecasting, 2467 Plasma Temperature And Density, 3367 Theoretical Modeling, 7949 Ionospheric Storms (2441)

Scientific paper

The Thermosphere-Ionosphere Mesosphere Electrodynamics General Circulation Model (TIMEGCM) driven by high latitude inputs from the Assimilative Mapping of Ionospheric Electrodynamics (AMIE) algorithm represents a true space-weather model that captures much of the variability in the global thermosphere and ionosphere. This coupled model has been run for the entire IPY period at solar minimum, and the ability of the model to reproduce thermosphere-ionosphere climate and weather at various locations has been quantified using incoherent scatter radar data and GUVI composition measurements. The differences between the model and the measurements provide insight into how the model might be improved in the future. Analysis of the AMIE results themselves also provides insight into the variability of the high latitude drivers during solar minimum conditions.

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