Comparison of O + /H + and O + /(H + +He + ) transition levels

Advances in Space Research

Volumn 22, Issue 6, 1998, Pages 895-898

  Triskova L ^a   Truhlik V ^a   Smilauer J ^a   Shultchishin, Yu A ^b  

^a INSTITUTE OF ATMOSPHERIC PHYSICS   (Czech Republic)

^b Russian Acad Sci ^*  (Russian Federation)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0040017629     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0273-1177(98)00119-7     Document Type: Article

References (6)

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2. Bilitza D., The Use of Transition Heights for Representation of Ion Composition, Adv. Space Res., 10, (11)183 (1991).
3. + at Middle and Equatorial Latitudes during Solar Maximum, J. Geophys. Res., 95, 10,313(1990).
4. + Ion Transition Surface for Use in IRI, Adv. Space Res., 14, (12)135-(12)138(1994).
5. 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).
6. Truhlík, V., J. Šmilauer, L. Třísková, Y.A. Shultchishin, and N.F. Smirnova, Manifestation of Ionospheric Storms in the Upper Transition Height, 31st Scientific Assembly COSPAR, Birmingham, July 1996. Symposium C4.2.