Paper
13 December 2018 The analysis of the solar spectra dynamics under x-ray superflares in September 2017 for the geophysical applications
Julia A. Korsunskaya, Andrey N. Lyakhov
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Proceedings Volume 10833, 24th International Symposium on Atmospheric and Ocean Optics: Atmospheric Physics; 108339X (2018) https://doi.org/10.1117/12.2504399
Event: XXIV International Symposium, Atmospheric and Ocean Optics, Atmospheric Physics, 2018, Tomsk, Russian Federation
Abstract
We present the results of the analysis for the GOES-15 and SDO satellites data under the extra strong solar X-class flares X9.3 September 06 2017 and X8.2 September 10 2017. It is shown that X9.3 flare was accompanied by the significant increasing of the UV flux and by the growth of the extremely hard X-ray part of the spectrum. The evidence from ionosondes, GPS receiver and Schumann resonance monitoring has shown different response to these neighbor flares. The flare classification based on the peak flux value is not sufficient for the geophysical applications. The interpretation of the ionosphere response requires the full spectrum analysis.
© (2018) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Julia A. Korsunskaya and Andrey N. Lyakhov "The analysis of the solar spectra dynamics under x-ray superflares in September 2017 for the geophysical applications", Proc. SPIE 10833, 24th International Symposium on Atmospheric and Ocean Optics: Atmospheric Physics, 108339X (13 December 2018); https://doi.org/10.1117/12.2504399
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KEYWORDS
Ultraviolet radiation

X-rays

Absorption

Global Positioning System

Hard x-rays

Wave propagation

Receivers

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