Solar-type stars Halpha line
收藏B2FIND2026-04-04 收录
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https://b2find.eudat.eu/dataset/950ec315-31bc-5307-b1d1-a154a1e2f264
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Excess chromospheric emissions within deep photospheric lines are effective proxies of stellar magnetism for FGK stars. This emission decays with stellar age and is a potential...
