MODEL OF DISTURBANCE OF GLOBAL ELECTROMAGNETIC RESONANCE DURING EXTRA-GALACTIC GAMMA RAY FLARE ON DECEMBER 27, 2004

A. P. Nickolaenko; Masashi Hayakawa

doi:10.1615/TelecomRadEng.v70.i1.80

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Home > Journals > Telecommunications and Radio Engineering > Volume 70, 2011 Issue 1 > MODEL OF DISTURBANCE OF GLOBAL ELECTROMAGNETIC RESONANCE DURING EXTRA-GALACTIC GAMMA RAY FLARE ON DECEMBER 27, 2004

ISSN Print: 0040-2508
ISSN Online: 1943-6009

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Telecommunications and Radio Engineering

DOI: 10.1615/TelecomRadEng.v70.i1.80
pages 73-85

MODEL OF DISTURBANCE OF GLOBAL ELECTROMAGNETIC RESONANCE DURING EXTRA-GALACTIC GAMMA RAY FLARE ON DECEMBER 27, 2004

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

Masashi Hayakawa
Hayakawa Institute of Seismo Electromagnetics Co. Ltd.(Hi-SEM), The University of Electro-Communications (UEC) Alliance Center #521, Advanced & Wireless and Communications Research Center, UEC, Chofu, Tokyo, 182-8585, Japan

ABSTRACT

The possible effect is discussed on the Schumann resonance records of the giant γ -ray flare from Sagittarius constellation (SGR 1806-20). We show that the dayside ionosphere modification is able to cause noticeable abrupt change in the power spectra global electromagnetic resonance. Spectral modifications gradually fade in time, so that usual spectra patterns are recovered in some time after the burst. A technique is proposed for measurements, which emphasizes the gamma burst effect.

KEY WORDS: the Schumann resonance, gamma-burst, the lower ionosphere