Energy-conserving numerics in CME simulations yield >2x higher kinetic energy by extending flare reconnection duration compared to non-conservative schemes.
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4 Pith papers cite this work. Polarity classification is still indexing.
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Polytropic stellar wind models are extended beyond extreme adiabatic cases to non-adiabatic localized heating, with added energy shown plausible relative to flares and relevant to solar wind observations.
A multi-ion solar wind simulation with reflection-driven turbulence reproduces observed preferential heating of oxygen ions when compared to UVCS and SWICS data.
citing papers explorer
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The Effects of Energy Conservation in Simulating Solar Eruptions
Energy-conserving numerics in CME simulations yield >2x higher kinetic energy by extending flare reconnection duration compared to non-conservative schemes.
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Polytropic stellar wind models with strongly localized heating
Polytropic stellar wind models are extended beyond extreme adiabatic cases to non-adiabatic localized heating, with added energy shown plausible relative to flares and relevant to solar wind observations.
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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.
- On the Nature of Candle-Flame-Shaped Solar Flares and Sub-Alfv\'enic Supra-Arcade Plasma Downflows