SOLAR FLARE Definition & Meaning

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solar flare

Astronomy.

solar flare

Sometimes shortened to: flare.��a brief powerful eruption of particles and intense electromagnetic radiation from the sun's surface, associated with sunspots and causing disturbances to radio communication on earth See also solar wind

solar flare

A sudden eruption of hydrogen gas in the chromosphere of the Sun, usually associated with sunspots. Solar flares may last between several hours and several days, and have temperatures ranging from 20 to 100 million degrees K. The energy of a solar flare, which consists primarily of charged particles and x-rays, is comparable to tens of millions of hydrogen bombs, but is less than one-tenth the total energy emitted by the Sun every second. First observed in 1859, solar flares dramatically affect the Sun's weather and the solar wind, and are correlated with the appearance of auroras on the Earth.
See also prominence

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First recorded in 1935–40

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Examples have not been reviewed.

During this phase there is an increase in the number of eruptions from the Sun, including solar flares and coronal mass ejections.

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But solar storms, solar flares and coronal mass ejections routinely impact Earth's weather.

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It was a solar flare, starting somewhere deep inside of him and growing into a full-blown emoji.

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Activity on the Sun has remained high since one of the largest solar flares in seven years last week.

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The X9 solar flare emitted is the largest categorised by Nasa.

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