solar wind

Sun's particle stream

Solar wind is the continuous stream of charged particles—mostly protons and electrons—flowing outward from the sun into space.

It travels at hundreds of kilometers per second, carrying the sun's magnetic field throughout the solar system.

Solar wind interacts with planetary magnetic fields, causing phenomena like the aurora borealis on Earth.

During solar storms, intensified solar wind can disrupt satellites and power grids.

Related

shock wave · protons · aurora · northern lights · electrons · interplanetary · space weather · storm · flare · geomagnetic · Voyager · ions · charged · magnetic field lines · flux · borealis · streaming · luminous

Categories
Opposites
origin/source

solar windcosmic rays

Energetic particles from beyond

stellar wind

energy transfer type

solar windsunlight

Radiance from our star

solar radiation · photons · solar heat · light · thermal radiation

Family

wind, windy, solar, windmill, solstice, sol, solarize, solarized, solarizing

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