Recent advances in topside profile modeling

被引：20

作者：

Pulinets, SA ^{[1
]}

Depuev, VH

Karpachev, AT

Radicella, SM

Danilkin, NP

机构：

[1] Russian Acad Sci, IZMIRAN, Inst Terr Magnetism Ionosphere & Radiowave Propag, Troitsk 142190, Moscow Region, Russia

[2] Abdus Salam Int Ctr Theoret Phys, I-34014 Trieste, Italy

[3] Inst Appl Geophys, Moscow 129226, Russia

来源：

MODELLING THE TOPSIDE IONOSPHERE AND PLASMASPHERE | 2002年 / 29卷 / 06期

关键词：

D O I：

10.1016/S0273-1177(02)00037-6

中图分类号：

V [航空、航天];

学科分类号：

08 ; 0825 ;

摘要：

A parameterized model for topside profile was developed based on the Epstein function approximation, Using the Intercosmos-19 database, model parameters were obtained for different geophysical conditions, including strong magnetic storms. In some specific conditions the F3 layer was observed on topside ionograms. A physical explanation is proposed as well as results based on modeling approach. Topside ionograms from the sounder on MIR Space Station were studied. Some exotic cases are presented including oblique propagation, station position under the peak height etc. Peak height global distribution is described as well as neutral wind parameters derived from the topside peak height values. (C) 2002 COSPAR. Published by Elsevier Science Ltd. All rights reserved.

引用

页码：815 / 823

页数：9

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