I point out that the objection of Györi et al. to my finding that neglect of small spots could explain much of the puzzling difference between Royal Greenwich Observatory and Solar Optical Observation Network spot areas is not valid because their analysis was limited to only 1974–76, when activity was low. The 40%–50% difference occurs only at higher activity levels.

中文翻译：

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忽视小光斑仍然是 SOON 和 RGO 光斑区域之间差异的解释

我指出 Györi 等人的反对意见。根据我的发现，忽略小斑点可以解释皇家格林威治天文台和太阳光学观测网络斑点区域之间的大部分令人费解的差异，但这一发现是无效的，因为他们的分析仅限于 1974-76 年，当时活动较低。 40%–50% 的差异仅出现在较高的活动水平下。