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. 2017 Dec 29;9(8):3069–3081. doi: 10.1002/2017MS001109

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© 2017. The Authors.

This is an open access article under the terms of the Creative Commons Attribution‐NonCommercial‐NoDerivs License, which permits use and distribution in any medium, provided the original work is properly cited, the use is non‐commercial and no modifications or adaptations are made.

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Temporal evolution of the energy ratios of VIS and NIR account for GR at the Gobi field observation site during the IOP, (a) each measured energy ratio and (b) the daily‐averaged energy ratio, respectively.