Research news on Solar wind

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.

Solar Orbiter catches the sun's missing high-speed vibrations

The sun's magnetic fields are a twisty, curvy, ever-changing mess. In particular, our star's polar regions host areas called polar coronal holes, which contain invisible magnetic highways that stretch into interplanetary ...

NASA's PUNCH sharpens solar storm forecasting in first test

Using continuous imagery from NASA's PUNCH (Polarimeter to Unify the Corona and Heliosphere) mission, scientists predicted the near-Earth arrival of a solar eruption to within 30 minutes in an initial proof-of-concept test. ...

NASA science soars during August total solar eclipse

Each time the moon covers the sun during a total solar eclipse—darkening daytime skies and briefly revealing the sun's ethereal outer atmosphere, the corona—it presents new opportunities to better understand our star and ...

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