The formation of an additional layer in the equatorial topside ionosphere

被引:1
|
作者
Jenkins, B [1 ]
Bailey, GJ
Abdu, MA
Batista, IS
Balan, N
机构
[1] Univ Sheffield, Sch Math & Stat, Upper Atmospher Modelling Grp, Sheffield S3 7RH, S Yorkshire, England
[2] Inst Nacl Pesquisas Espaciais, BR-12201970 Sao Jose Dos Campos, SP, Brazil
[3] Kyoto Univ, Ctr Radio Atmospher Sci, Kyoto 611, Japan
关键词
D O I
10.1016/S0273-1177(97)00758-8
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
Calculations using the Sheffield University plasmasphere ionosphere model have shown that under certain conditions an additional layer can form in the low latitude topside ionosphere, This layer (the F3 layer) has subsequently been observed in ionograms recorded at Fortaleza in Brazil, It has not been observed in ionograms recorded at the neighbouring station, Sao Luis, Model calculations have shown that the F3 layer is most likely to form in summer at Fortaleza due to a combination of the neutral wind and the E x B drift acting to raise the plasma, At Fortaleza the horizontal wind moves the plasma up the inclined field lines; at Sao Luis the field lines are nearly horizontal and the wind cannot raise the plasma further. (C) 1997 COSPAR. Published by Elsevier Science Ltd.
引用
收藏
页码:1137 / 1140
页数:4
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