Solar wind as a research area focuses on the plasma outflow from the solar corona and its interaction with the heliosphere and planetary environments. It encompasses characterization of its composition, velocity distributions, turbulence, and magnetic structure, including fast and slow streams, coronal mass ejections, and associated shock waves. The field integrates in situ spacecraft measurements, remote sensing, and magnetohydrodynamic and kinetic modeling to study acceleration and heating mechanisms, magnetic reconnection, and wave–particle interactions. Solar wind research is central to understanding heliophysics, space weather forecasting, particle transport, and the coupling between solar activity and magnetospheres throughout the solar system.
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