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.
C., Bonfond B., Bunce E
2 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.EP 2years
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A descriptive overview of the atmospheric structure, chemistry, and dynamics of the four giant planets in the Solar System.
citing papers explorer
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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.
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Giant Planet Atmospheres
A descriptive overview of the atmospheric structure, chemistry, and dynamics of the four giant planets in the Solar System.