Improvements of the International Reference Ionosphere model for the topside electron density profile

被引:81
作者
Bilitza, D
Reinisch, BW
Radicella, SM
Pulinets, S
Gulyaeva, T
Triskova, L
机构
[1] NASA, Goddard Space Flight Ctr, Raytheon Intelligence & Informat Syst, Greenbelt, MD 20771 USA
[2] Univ Massachusetts, Ctr Atmospher Res, Lowell, MA 01854 USA
[3] Abdus Salam Int Ctr Theoret Phys, Aeron & Radiopropagat Lab, I-34014 Trieste, Italy
[4] Univ Nacl Autonoma Mexico, Inst Geophys, Mexico City 04150, DF, Mexico
[5] Inst Terr Magnetism Ionosphere & Radio Wave P, Moscow, Russia
[6] Polish Acad Sci, Space Res Ctr, PL-01237 Warsaw, Poland
[7] Acad Sci, Inst Atmospher Phys, Prague 14131 4, Czech Republic
关键词
D O I
10.1029/2005RS003370
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
[ 1] Shortcomings of the representation of the topside electron density profile in the International Reference Ionosphere (IRI) model have been noted in comparison with recently analyzed topside sounder data and also with total electron content (TEC) data. Various studies have proposed corrections of the IRI formulas or have introduced a new formalism. This paper reviews the different approaches, their implications for IRI, and their current status. An important challenge for topside modeling is the truthful representation of profiles in the equatorial anomaly (EA) region over the whole range of the EA fountain. This means that the latitudinal representation has to reproduce the merging of the double- peak signature at F region heights into a single peak at the top of the fountain. In this context, special emphasis is given to the coupling between topside and plasmaspheric models.
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页数:8
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