E3S Web Conf.
Volume 62, 2018IX International Conference “Solar-Terrestrial Relations and Physics of Earthquake Precursors”
|Number of page(s)||4|
|Section||Atmosphere Physics and Solar-Terrestrial Relations|
|Published online||07 November 2018|
Schumann resonance parameters at Kuju station during solar flares
1 National Institute of Technology, Kagoshima College, Japan
2 International Center for Space Weather Science and Education, Kyushu University, Japan
3 Kyushu Institute of Technology, Japan
1 Corresponding author: firstname.lastname@example.org
We examined the Schumann resonance (SR) at low-latitude station KUJ by comparing with solar X-ray flux and solar proton flux at a geostationary orbit. For intense solar activity in October-November 2003, the reaction of the SR frequency to X-ray enhancement and SPEs was different. The SR frequency in H component increased at the time of the Xray enhancement. The response of SR seems to be caused by the increase of the electron density in the ionospheric D region which ionized by the enhanced solar X-ray flux. In the case of the SPEs, the SR frequency in D component decreased with enhancement of solar proton flux. We suggest that the SPEs caused the decrease of altitude on the ionopheric D region at high-latitude region, and the SR frequency decreased.
© The Authors, published by EDP Sciences, 2018
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