Solar wind composition depends strongly on source distance from the open-closed boundary, with enhanced variability and slow-wind signatures concentrated within ~25 Mm of the boundary.
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2 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.SR 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
A multi-ion solar wind simulation with reflection-driven turbulence reproduces observed preferential heating of oxygen ions when compared to UVCS and SWICS data.
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Solar Wind Dependence on Source Distance from the Open-Closed Boundary
Solar wind composition depends strongly on source distance from the open-closed boundary, with enhanced variability and slow-wind signatures concentrated within ~25 Mm of the boundary.
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Global Multi-ion Solar Wind Model. I. Ion Temperatures
A multi-ion solar wind simulation with reflection-driven turbulence reproduces observed preferential heating of oxygen ions when compared to UVCS and SWICS data.