A weak planetary magnetic field enhances ion escape from a Mars-like planet up to a critical strength set by the stellar wind, after which escape decreases.
E., Howell E., Waite J
2 Pith papers cite this work. Polarity classification is still indexing.
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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.
citing papers explorer
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Planetary Magnetic Field Control of Ion Escape from Weakly Magnetized Planets
A weak planetary magnetic field enhances ion escape from a Mars-like planet up to a critical strength set by the stellar wind, after which escape decreases.
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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.