Telecommunications and Radio Engineering

ISSN for PRINT: 0040-2508

For Online Access

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2008, Volume67

Issue 5

93 pages

DOI: 10.1615/TelecomRadEng.v67.i5

Issue price - $271.00

L. M. Rabinowicz
A. Usikov Institute of Radio Physics and Electronics, National Academy of Sciences of Ukraine, 12, Academician Proskura St.; and Institute of Radio Astronomy, National Academy of Sciences of Ukraine 4, Chervonopraporna St., Kharkov 61002, Ukraine

A. V. Shvets
A. Usikov Institute of Radio Physics and Electronics, National Academy of Sciences of Ukraine 12, Academician Proskura St., Kharkov 61085, Ukraine

A. P. Nickolaenko
A. Usikov Institute of Radio Physics and Electronics, National Academy of Sciences of Ukraine, 12, Academician Proskura St., Kharkov 61085, Ukraine

We perform the formal analysis and present the numerical modeling data showing that a polar non-uniformity of the lower ionosphere arises during powerful Solar proton events (SPE), which is able to noticeably change the spectra of the global electromagnetic (Schumann) resonance. Modifications are discussed of resonance spectra, their dependence on the source and observer position. Computational data are compared with observations performed in 2000 − 2003. An interpretation is given for the experimental data. Polar-uniformity parameter is evaluated from the Schumann resonance.

DOI: 10.1615/TelecomRadEng.v67.i5.30 Download article, 413-435 pages

Article price - $65.00

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