HR: 1330h
AN: SA23A-06 [Abstracts]
TI: Solar Activity Variations of Electron Temperature in the Topside Ionosphere
AU: * Bilitza, D
EM: bilitza@mail630.gsfc.nasa.gov
AF: Raytheon, GSFC, Code 612.4, Greenbelt, MD 20771 United States
AU: Richards, P G
EM: philip.g.richards@nasa.gov
AF: NASA, Earth-Sun Systems Division, Science Mission Directorate, 300 E Street SW, Washington, DC 20546 United States
AU: Truhlik, V
EM: vtr@ufa.cas.cz
AF: Institute of Atmospheric Physics, Bocni II, Praha, 14131 Czech Republic
AB:
Over the past three decades a large volume of electron temperature (Te) and density (Ne) measurements has been accumulated by satellite insitu instruments as well as ground-based incoherent scatter radars. We have established a data base with the
most important of the satellite measurements reaching from the early Explorers to the recent KOMPSAT and DMSP satellites and including close to 7 million data points. Using this database we have studied the variation of Te with solar activity at
different altitudes, latitudes, and seasons. Whereas the electron density generally increases with solar activity at all
studied altitudes, latitudes and seasons, the electron temperature can either increase, decrease or stay constant depending
on the specific altitude, latitude, and season. We have compared these variations patterns with those found with incoherent
scatter radar data and with those predicted by the FLIP model. Our comparisons show overall good agreement thus (i)
confirming the variation patterns established by this study, (ii) showing the compatibility of the two measurement
techniques, and (iii) validating the solar cycle Te predictions of the FLIP model. An important goal of this work is the
inclusion of an accurate representation of Te solar cycle variations in the International Reference Ionosphere (IRI) model.
UR: http://nssdc.gsfc.nasa.gov/space/model/ionos/iri.html
DE: 2400 IONOSPHERE
DE: 2443 Midlatitude ionosphere
DE: 2447 Modeling and forecasting
DE: 2481 Topside ionosphere
SC: SPA-Aeronomy [SA]
MN: 2005 Joint Assembly