Physics
Scientific paper
Dec 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003agufmsa21b0093t&link_type=abstract
American Geophysical Union, Fall Meeting 2003, abstract #SA21B-0093
Physics
2419 Ion Chemistry And Composition (0335), 2447 Modeling And Forecasting, 2467 Plasma Temperature And Density, 2481 Topside Ionosphere, 2499 General Or Miscellaneous
Scientific paper
Response of electron temperature (Te) and density (Ne) to solar activity variation in solar maximum is studied. The 27 day period in solar activity is characterized by the F10.7 index. The Te and log Ne response was approximated by a linear dependence. The manifestation of solar flux variation in Ne is rather small. The Te dependence on the solar flux was included in an empirical model based on the Intercosmos satellites data. The model values were compared with Hinotori (altitude 600 km) and ISIS-1 (altitude 2500 km) Te data. The best agreement was found at equatorial and low latitudes. The possible mechanisms are discussed.
Smilauer Ja.
Triskova Ludmila
Truhlik Vladimir
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