Compressive hydrodynamic fluctuations amplify fusion power in plasmas via hydrodynamic, two-temperature, and kinetic mechanisms, often exceeding the gain from using the same energy for heating.
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Review of helioseismic inversions shows the solar modelling problem remains unsolved with broad implications for stellar seismology and fields relying on precise stellar parameters.
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Fusion-power amplification by compressive hydrodynamic fluctuations
Compressive hydrodynamic fluctuations amplify fusion power in plasmas via hydrodynamic, two-temperature, and kinetic mechanisms, often exceeding the gain from using the same energy for heating.
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Progress in global helioseismology: a new light on the solar modelling problem and its implications for solar-like stars
Review of helioseismic inversions shows the solar modelling problem remains unsolved with broad implications for stellar seismology and fields relying on precise stellar parameters.