Changes of the first Schumann resonance frequency during relativistic solar proton precipitation in the 6 November 1997 event

The variations of the first mode of Schumann resonance are analyzed using data from Kola peninsula stations during the solar proton event of 6 November 1997. On this day the intensive flux of energetic protons on GOES-8 and the 10% increase of the count rate of the neutron monitor in Apatity between...

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Bibliographic Details
Published in:Annales Geophysicae
Main Authors: V. C. Roldugin, Ye. P. Maltsev, A. N. Vasiljev, E. V. Vashenyuk
Format: Article in Journal/Newspaper
Language:English
Published: Copernicus Publications 1999
Subjects:
Science
Q
Physics
QC1-999
Geophysics. Cosmic physics
QC801-809
Apatity
Kola Peninsula
Schumann
kola peninsula
Online Access:https://doi.org/10.1007/s00585-999-1293-9
https://doaj.org/article/e1f648a1ead04a4bbc67d39f97049a5c
Description
Summary:The variations of the first mode of Schumann resonance are analyzed using data from Kola peninsula stations during the solar proton event of 6 November 1997. On this day the intensive flux of energetic protons on GOES-8 and the 10% increase of the count rate of the neutron monitor in Apatity between 1220 and 2000 UT were preceded by a solar X-ray burst at 1155 UT. This burst was accompanied by a simultaneous increase of the Schumann frequency by 3.5%, and the relativistic proton flux increase was accompanied by 1% frequency decrease. These effects are explained by changes of the height and dielectric permeability of the Earth-ionosphere cavity. Key words. Ionosphere (ionospheric disturbances; solar radiation and cosmic ray effects) · Radio science (ionospheric propagation)

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