Physics
Scientific paper
Apr 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997jgr...102.7485b&link_type=abstract
Journal of Geophysical Research, Volume 102, Issue A4, p. 7485-7492
Physics
16
Ionosphere: Equatorial Ionosphere, Ionosphere: Modeling And Forecasting, Ionosphere: Plasma Temperature And Density, Ionosphere: Topside Ionosphere
Scientific paper
A study of the thermal structure of the low-latitude (30°N to 30°S) ionosphere under equinoctial conditions at low, medium, and high solar activity has been carried out using the Sheffield University plasmasphere-ionosphere model (SUPIM) and Hinotori satellite observations. The study reveals the existence of an anomaly in the plasma (electron and ion) temperature in the topside ionosphere during the evening-midnight period. The anomaly, called the equatorial plasma temperature anomaly (EPTA), is characterized by a trough around the magnetic equator with crests on either side. The trough develops before the crests. The model results show that the anomaly occurs between 1900 and 0100 LT at altitudes between 450 and 1250 km; the strongest anomaly occurs around 2130 LT at 950 km altitude during high solar activity. The temperature trough of the anomaly arises from the adiabatic expansion of the plasma and an increase in plasma density caused by the prereversal strengthening of the upward vertical
Abdu Mangalathayil Ali
Bailey Graham J.
Balan Nanan
Fukao Shoichiro
Oyama Koh-Ichiro
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