solar wind

American  

noun

1. an emanation from the sun's corona consisting of a flow of charged particles, mainly electrons and protons, that interacts with the magnetic field of the earth and other planetary bodies.

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solar wind British  

/ wɪnd /

noun

1. the constant stream of charged particles, esp protons and electrons, emitted by the sun at high velocities, its density and speed varying during periods of solar activity. It interacts with the earth's magnetic field, some of the particles being trapped by the magnetic lines of force, and causes auroral displays See also Van Allen belt magnetosphere

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solar wind Scientific  

1. A continuous stream of plasma ejected by the Sun, flowing outward from the corona. This plasma, which consists mostly of protons and electrons, has enough energy to escape the Sun's gravitational field at speeds ranging from about 300 to 800 km (186 to 496 mi) per second and averaging 1,610,000 km (1,000,000 mi) per hour, which allows the solar wind to reach Earth in about 3.9 days. The speed and intensity of the solar wind depends on magnetic activity at different regions of the Sun. The solar wind spreads out from the Sun in a pinwheel pattern as a result of the Sun's rotation, pushing back the interstellar medium to the boundary known as the heliopause. The tails of comets, which always extend away from the Sun regardless of the direction of the comet's motion, are a result of the impact of solar wind, which dislodges ice and other particles from the comet's surface. Similar winds flowing from other stars are called stellar winds.

2. See also aurora

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solar wind Cultural  

1. A stream of particles (mostly protons) emitted by the sun and permeating the solar system.

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Discover More

Particularly strong bursts of particles can penetrate the upper atmosphere and disrupt radio communications on Earth.

Etymology

Origin of solar wind

First recorded in 1955–60

Example Sentences

The crisis couldn’t have come at a better time, as the costs of solar, wind, and batteries have fallen dramatically.

From Salon • May 16, 2026

They found that interactions between the magnetosphere and the solar wind at its outer boundary closely resemble processes observed at Jupiter.

From Science Daily • Apr. 3, 2026

“You are going to get more solar, wind, batteries, and nuclear,” he said.

From Barron's • Mar. 28, 2026

Red aurora tends to appear during particularly powerful geomagnetic storms, when the solar wind is strong enough to push particles to extreme heights.

From BBC • Mar. 24, 2026

And I imagine the solar wind blowing the stardust around, trillions of energized particles bombarding the earth, radiation I can't see or feel.

From "Things Not Seen" by Andrew Clements