DocumentCode :
2713302
Title :
The role of excited molecular ions in the variation of the E-layer peak height caused by the solar activity
Author :
Zhivolup, Taras G.
Author_Institution :
Inst. of Ionosphere, Acad. of Sci., Kharkov, Ukraine
Volume :
2
fYear :
2000
fDate :
2000
Firstpage :
647
Abstract :
The data obtained by the Kharkov incoherent scatter radar show a monotonous linear decrease of the E-layer peak height (hmE) in the transition from the low to medium solar activity. Such behavior of the E-layer peak height is accounted for by the influence of oscillation-excited ions O2+ on the hmE variations depending on the level of solar activity. The theoretical dependences hmE(F10.7) are in a good agreement with the experimental data
Keywords :
E-region; atmospheric structure; oxygen; positive ions; remote sensing by radar; solar-terrestrial relationships; sunlight; E-layer peak height; Kharkov incoherent scatter radar; O2; O2+; excited molecular ions; oscillation-excited ions; solar activity; Acceleration; Equations; Large Hadron Collider; Petroleum; Solar radiation; Temperature dependence;
fLanguage :
English
Publisher :
ieee
Conference_Titel :
Mathematical Methods in Electromagnetic Theory, 2000. MMET 2000. International Conference on
Conference_Location :
Kharkov
ISSN :
1
Print_ISBN :
0-7803-6347-7
Type :
conf
DOI :
10.1109/MMET.2000.890524
Filename :
890524
Link To Document :
https://search.ricest.ac.ir/dl/search/defaultta.aspx?DTC=49&DC=2713302
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