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| Titel |
Electron density profiles in the quiet lower ionosphere based on the results of modeling and experimental data |
| VerfasserIn |
V. Barabash, A. Osepian, P. Dalin, S. Kirkwood  |
| Medientyp |
Artikel
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| Sprache |
Englisch
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| ISSN |
0992-7689
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| Digitales Dokument |
URL |
| Erschienen |
In: Annales Geophysicae ; 30, no. 9 ; Nr. 30, no. 9 (2012-09-13), S.1345-1360 |
| Datensatznummer |
250017267
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| Publikation (Nr.) |
 copernicus.org/angeo-30-1345-2012.pdf |
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| Zusammenfassung |
The theoretical PGI (Polar Geophysical Institute) model for the quiet lower
ionosphere has been applied for computing the ionization rate and electron
density profiles in the summer and winter D-region at solar zenith angles
less than 80° and larger than 99° under steady state conditions. In
order to minimize possible errors in estimation of ionization rates provided
by solar electromagnetic radiation and to obtain the most exact values of
electron density, each wavelength range of the solar spectrum has been
divided into several intervals and the relations between the solar radiation
intensity at these wavelengths and the solar activity index F10.7 have
been incorporated into the model. Influence of minor neutral species (NO,
H2O, O, O3) concentrations on the electron number density at
different altitudes of the sunlit quiet D-region has been examined. The
results demonstrate that at altitudes above 70 km, the modeled electron
density is most sensitive to variations of nitric oxide concentration.
Changes of water vapor concentration in the whole altitude range of the
mesosphere influence the electron density only in the narrow height interval
73–85 km. The effect of the change of atomic oxygen and ozone concentration
is the least significant and takes place only below 70 km.
Model responses to changes of the solar zenith angle, solar activity
(low–high) and season (summer–winter) have been considered. Modeled electron
density profiles have been evaluated by comparison with experimental
profiles available from the rocket measurements for the same conditions. It
is demonstrated that the theoretical model for the quiet lower ionosphere is
quite effective in describing variations in ionization rate, electron number
density and effective recombination coefficient as functions of solar zenith
angle, solar activity and season. The model may be used for solving inverse
tasks, in particular, for estimations of nitric oxide concentration in the
mesosphere. |
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