Physics
Scientific paper
May 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007agusmsa33b..03t&link_type=abstract
American Geophysical Union, Spring Meeting 2007, abstract #SA33B-03
Physics
2437 Ionospheric Dynamics, 2447 Modeling And Forecasting, 2467 Plasma Temperature And Density, 2481 Topside Ionosphere
Scientific paper
Electron temperature (Te) in the topside ionosphere and plasmasphere is an important parameter because thermal electrons play a key role in the energy balance of these regions. There are two principal sources of Te measurements - in-situ satellite and ground based Incoherent Scatter Radar (ISR). Since the mid-nineteensixties when radars and satellite instruments began observing Te a large volume of data has been collected by these two techniques. Occasional comparisons of results of these two methods showed agreements but also disagreements. We have built a large database of electron temperature based on all available satellite measurements, the greatest volume of which is represented by DMSP data. Especially DMSP data statistically show surprisingly high values for low solar activity and daytime (Bilitza, 2006). To investigate this discrepancy we have compared Millstoen Hill incoherent scatter measurements with simultaneous satellite measurements during DMSP overflights of the station. Results of this study are shown, discussion is presented and possible implications on empirical Te modeling are pointed out. Bilitza D., Truhlik V., Richards P.G., Abe T., and Triskova L.: Solar Variations of Mid-Latitude Electron Density and Temperature: Satellite Measurements Model Calculations, Advances in Space Research, in press, 2006.
Bilitza Dieter
Triskova Ludmila
Truhlik Vladimir
Zhang Sheng
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