Dynamic model and observation of the equatorial ionosphere

Details Dynamic model and observation of the equatorial ionosphere Dynamic model and observation of the equatorial ionosphere

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995adspr..15..109w&link_type=abstract

Advances in Space Research (ISSN 0273-1177), vol. 15, no. 2, p. 109-112

Computer Science

Sound

6

Dynamic Models, Electron Energy, F Region, Ionospheric Electron Density, Ionospheric Sounding, Plasma Density, Plasma Drift, Reference Atmospheres, Solar Terrestrial Interactions, Anomalies, Computerized Simulation, Geomagnetism, Japanese Spacecraft, Satellite Sounding, Scientific Satellites, Time Dependence

Scientific paper

The Hinotori satellite observed the electron density and temperature around the equatorial anomaly region at approximately 600 km altitude during high solar activity. The observed electron temperature in the equatorial F region ionosphere was compared with the International Reference Ionosphere (IRI) model. The results showed the large difference between observation and model. Time dependent three dimensional computer simulations of the equatorial ionospheric F region have been carried out to investigate the electron temperature anomaly. These simulations coincide with the equatorial electron density and temperature structure observed by the Hinotori satellite.

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