Empirical modeling of the upper transition height for low and middle latitudes

Advances in Space Research

Volumn 27, Issue 1, 2001, Pages 111-114

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

^a INSTITUTE OF ATMOSPHERIC PHYSICS   (Czech Republic)

Author keywords

[No Author keywords available]

Indexed keywords

COMPOSITION; IONS; MASS SPECTROMETERS; SATELLITES;

SOLAR ACTIVITY;

SPACE RESEARCH;

IONIC COMPOSITION; SOLAR CYCLE;

EID: 0034979884     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0273-1177(00)00145-9     Document Type: Article

References (12)

1. The use of transition heights for representation of ion composition
2. Satellite measurements of ion composition and temperatures in the topside ionosphere during medium solar activity
3. + at middle and equatorial latitudes during solar maximum
4. An approximation of the height of the O+-H+ transition level for use in IRI
5. Ion transition height distribution obtained with satellite Taiyo
6. Intercosmos-24: Helium ion predominance during equinox at low and middle latitudes in the 22nd solar activity cycle
7. Ion transition heights from topside electron density profiles
8. Manifestation of ionospheric storms in the upper transition height
9. Improved electron temperature model and comparison with satellite data
10. Contribution to modelling the electron density and temperature in the disturbed low latitude topside ionosphere
11. + ) transition levels
12. Study of major ions distribution in the outer ionosphere in the solar maximum