Page 2: 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.

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. ...

An AI model can forecast harmful solar winds days in advance

Scientists at NYU Abu Dhabi (NYUAD) have developed an artificial intelligence (AI) model that can forecast solar wind speeds up to four days in advance, significantly more accurately than current methods. The study is published ...

UK space weather prediction system goes operational

The impacts of space weather such as extreme solar winds and magnetic waves are not limited to outer space. Bursts of plasma emanating from the sun, for instance, can temporarily intensify electric and magnetic fields on ...

A better way to turn solar sails

Solar sails represent one of the most elegant concepts in space exploration: using sunlight itself to propel spacecraft through the cosmos without any fuel. But these thin, light giants face a stubborn engineering challenge ...

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