Statistical analysis of ionospheric responses to solar flares in the solar cycle 23

In this study, we studied the ionospheric responses to solar flares during 1999–2006 by using GOES 0.1–0.8 nm X‐ray, 26–34 nm EUV, and GPS/total electron content (TEC). The solar zenith angle (SZA) dependence was quantitatively investigated by analyzing global TEC enhancements during about 100 X‐cla...

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Veröffentlicht in:Journal of geophysical research. Space physics 2013-01, Vol.118 (1), p.576-582
Hauptverfasser: Le, Huijun, Liu, Libo, Chen, Yiding, Wan, Weixing
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Sprache:eng
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