Comparison of the auroral E region neutral winds derived with the EuropeanIncoherent Scatter radar and predicted by the National Center for Atmospheric Research Thermosphere-Ionosphere-Mesosphere-Electrodynamics general circulation model

Citation
S. Nozawa et al., Comparison of the auroral E region neutral winds derived with the EuropeanIncoherent Scatter radar and predicted by the National Center for Atmospheric Research Thermosphere-Ionosphere-Mesosphere-Electrodynamics general circulation model, J GEO R-S P, 106(A11), 2001, pp. 24691-24700
Citations number
39
Categorie Soggetti
Space Sciences
Journal title
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
ISSN journal
21699380 → ACNP
Volume
106
Issue
A11
Year of publication
2001
Pages
24691 - 24700
Database
ISI
SICI code
0148-0227(20011101)106:A11<24691:COTAER>2.0.ZU;2-V
Abstract
A comparison study of the auroral E region neutral wind has been conducted using the European Incoherent Scatter (EISCAT) radar observations and Therm osphere-Ionosphere-Mesosphere-Electrodynamics general circulation model (TI ME GCM) predictions. The daily mean wind data as well as diurnal and semidi urnal tidal wind data. are compared for the three seasons summer, equinox, and winter between 95 and 119 km. Fairly good agreement is found in the alt itude profile of the mean zonal wind between the EISCAT observation and the TIME GCM prediction for summer, indicating the parameterization of gravity waves employed in the TIME GCM is adequate for this feature. The meridiona l mean wind amplitude predicted by the TIME GCM is considerably smaller tha n that observed by EISCAT, and the predicted wind is slightly northward for all the seasons above 100 km. Generally good agreement is found for the am plitude of the diurnal tide, especially the summer prediction, while disagr eements between the model and observational results are found for the corre sponding phases. The semidiurnal amplitude predicted by the TIME GCM is muc h smaller than that observed by EISCAT, and relatively large differences of the semidiurnal phase between the observations and predictions are found f or all seasons. These comparison results suggest that further advancements in the gravity wave parameterization. as well as the addition of planetary wave effects, are needed to predict more realistic lower thermospheric wind s at high latitude.