Dual-spacecraft observations of a November 2021 CME confirm that the CAAP method reliably estimates instantaneous expansion speed from single-point data while revealing unexpected evolution in shock strength and magnetic flux.
V., M "o stl C., Vennerstrom S., Vrbanec D.
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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Validating a Non-conventional Method for Expansion of Coronal Mass Ejections (CMEs) and Investigating the Evolution of a CME Substructures Using Solar Orbiter and Wind Observations
Dual-spacecraft observations of a November 2021 CME confirm that the CAAP method reliably estimates instantaneous expansion speed from single-point data while revealing unexpected evolution in shock strength and magnetic flux.
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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.