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.

Magnetic 'switchback' detected near Earth for the first time

In recent years, NASA's Parker Solar Probe has given us a close-up look at the sun. Among the probe's revelations was the presence of numerous kinks, or "switchbacks," in magnetic field lines in the sun's outer atmosphere. ...

NASA's Parker Solar Probe snaps closest-ever images to sun

On its record-breaking pass by the sun late last year, NASA's Parker Solar Probe captured stunning new images from within the sun's atmosphere. These newly released images—taken closer to the sun than we've ever been before—are ...

NASA's CODEX captures unique views of sun's outer atmosphere

Scientists analyzing data from NASA's CODEX (Coronal Diagnostic Experiment) investigation have successfully evaluated the instrument's first images, revealing the speed and temperature of material flowing out from the sun. ...

The dynamic battle between Mars's atmosphere and solar wind

Qi Zhang, a doctoral student at the Swedish Institute of Space Physics and Umeå University, explores in her doctoral thesis the interaction between Mars and the stream of charged particles from the sun, the solar wind. Her ...

Mars's rare disappearing solar wind event explained

Mars's atmosphere and climate are impacted by interactions with solar wind, a stream of plasma comprised of protons and electrons that flows from the sun's outermost atmosphere (corona), traveling at speeds of 400–1,000 kilometers ...

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