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.

Kissing the sun: Unraveling mysteries of the solar wind

Using data collected by NASA's Parker Solar Probe during its closest approach to the sun, a University of Arizona-led research team has measured the dynamics and ever-changing "shell" of hot gas from where the solar wind ...

Parker Solar Probe spies solar wind 'U-turn'

Images captured by NASA's Parker Solar Probe as the spacecraft made its record-breaking closest approach to the sun in December 2024 have now revealed new details about how solar magnetic fields responsible for space weather ...

Astronomers create first map of the sun's outer boundary

Astronomers have produced the first continuous, two-dimensional maps of the outer edge of the sun's atmosphere, a shifting, frothy boundary that marks where solar winds escape the sun's magnetic grasp. By combining the maps ...

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