Page 2: 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.

New Horizons watches the solar wind as it slows down

Where does the solar system end and interstellar space begin? That's a question scientists have been working to answer using spacecraft traveling beyond the sun's influence. A team of researchers from the Southwest Research ...

Video: Preparing Smile for space

Before Smile can begin studying how Earth responds to the streams of particles and bursts of radiation from the sun, the spacecraft had to complete an extraordinary journey here on Earth.

ESA's Proba 3 is unlocking secrets of the solar wind

It has been a dream of astronomers and solar scientists for ages. A new mission gives solar researchers a powerful new tool in their arsenal: on-demand, total solar eclipses. Launched in 2024, The European Space Agency's ...

Why stars spin down, or up, before they die

From birth to death, stars generally slow by 100 to 1,000 times their initial rotation rates; in other words, they "spin down." The sun's total angular momentum has declined as material is gradually blown off at the surface ...

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