Study of major ions distribution in the outer ionosphere in the solar maximum

Advances in Space Research

Volumn 25, Issue 1, 2000, Pages 193-196

  Triskova L ^a   Truhlik V ^a   Smilauer J ^a  

^a INSTITUTE OF ATMOSPHERIC PHYSICS   (Czech Republic)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 17144461845     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0273-1177(99)00917-5     Document Type: Article

References (5)

1. Bilitza D., The Use of Transition Heights for Representation of Ion Composition, Adv. Space Res., 10, (11)183 (1991).
2. + at middle and equatorial latitudes during solar maximum, J. Geophys. Res., 95, 10,313(1990).
3. Gonzales, S.A., B.G. Fejer, R.A. Heelis, and W.B. Hanson, Ion composition of the topside equatorial ionosphere during solar minimum, J. Geophys. Res., 97, 4299(1992).
4. Shultchishin, Yu.A., V.V. Afonin, K.V. Grechnev, V.A. Ershova, V.A. Kochnev, O. Z. Roste, N. F. Smirnova, and J. Šmilauer, Intercosmos-24: Helium Ion Predominance during Equinox at Low and Middle Latitudes in the 22nd Solar Activity Cycle, Adv. Space Res., 18, (3)15-(3)18(1996).
5. + ) transition levels, Adv. Space Res., 22, (6)895-(6)898(1998).