Jupiter's Lyα UV emission and continuum track solar X-ray and sunspot variations over two cycles while Fe II lines do not, and X-ray flares appear 7-15 days after CMEs with post-CME Ne8+ auroral emission.
F., Randall Gladstone G., Cravens T
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A long-term spectro-temporal study of Jovian X-ray and Ultraviolet response to solar activity
Jupiter's Lyα UV emission and continuum track solar X-ray and sunspot variations over two cycles while Fe II lines do not, and X-ray flares appear 7-15 days after CMEs with post-CME Ne8+ auroral emission.