Corpus Viewer
太陽之氣，有色球焉，亦曰色球層
。其在大氣中為三者之次，厚約二千里，居於光球之上，
過渡之下。
其密甚微，始於色球底下，其密僅光球之十分之一萬四；較地氣，惟十分之一萬八。是以常不見，唯日全之時，稍見赭色，其色猶紅粉間。然非特殊之具，以光球之明亮蓋遮其矣。
IDS:
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If a component is awkward to type directly, choose its total stroke count and then its first stroke. This is an input aid, not a judgement about how difficult the component is to learn. The five first-stroke classes follow the IRG system.