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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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
3D MHD modeling of candle-flame solar flares reveals Y-points do not coincide with apparent cusp tips and observed downflow speeds underestimate reconnection Alfvén speeds by 2-10x.
citing papers explorer
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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.
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On the Nature of Candle-Flame-Shaped Solar Flares and Sub-Alfv\'enic Supra-Arcade Plasma Downflows
3D MHD modeling of candle-flame solar flares reveals Y-points do not coincide with apparent cusp tips and observed downflow speeds underestimate reconnection Alfvén speeds by 2-10x.