Page 3: Research news on solar wind

Solar wind is a continuous, supersonic outflow of ionized plasma from the solar corona into interplanetary space, consisting primarily of electrons, protons, and alpha particles embedded in the interplanetary magnetic field. It arises from coronal heating and open magnetic field structures, with typical speeds of ~300–800 km/s and densities of a few particles per cubic centimeter at 1 AU. Solar wind exhibits distinct regimes, notably fast and slow wind with differing composition and turbulence properties, and drives key heliophysical phenomena including the formation of the heliosphere, bow shocks, and magnetospheric dynamics such as geomagnetic storms and auroral activity.

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. ...

PUNCH mission images huge solar eruption

Southwest Research Institute's Dr. Craig DeForest discussed the latest accomplishments of NASA's PUNCH (Polarimeter to Unify the Corona and Heliosphere) mission during a media event at the 246th American Astronomical Society ...

PUNCH mission instruments collect first images

The Southwest Research Institute-led Polarimeter to Unify the Corona and Heliosphere (PUNCH) mission collected its first images following its March 11 launch into polar orbit around Earth. The mission's four small suitcase-sized ...

NASA experiment shows solar wind might make water on the moon

Scientists have hypothesized since the 1960s that the sun is a source of ingredients that form water on the moon. When a stream of charged particles known as the solar wind smashes into the lunar surface, the idea goes, it ...

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