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Storms on our<br />

sun, new sun<br />

formation -<br />

so what?<br />

For anyone working with even a passing interest in solar astronomy,<br />

the so-called Carrington event constitutes a defining moment. It<br />

occurred on the afternoon of 1st September 1859, when amateur<br />

British astronomer Richard Carrington pointed the brass telescope<br />

in his private observatory outside London skywards. What he saw<br />

when he trained his attention on the sun surprised him and he began<br />

to sketch a cluster of large spots which appeared to pock-mark its<br />

surface. As Carrington was doing this, to his astonishment, ‘two<br />

patches of intensely bright and white light erupted’ in a brilliant, if<br />

short-lived, display. Within minutes, these fireballs had faded, but<br />

over the hours that followed a series of peculiar phenomena were<br />

observed in various parts of the world: telegraphic services were<br />

interrupted, paper spontaneously caught fire and night-time skies<br />

were illuminated – as if it were daylight – by colourful auroras.<br />

discovery Ireland 36,37<br />

An ultraviolet image of the solar atmosphere. The bright areas are known as 'active regions' and are<br />

composed of twisted and stressed magnetic fields that can produce violent releases of energy. This<br />

energy release can heat the solar atmosphere up to temperatures of well over 10 million degrees<br />

celsius. The heating and energy release is known as a 'solar flare' (Solar Dynamic Observatory)<br />

What Carrington had observed was a ‘solar storm’, explains Dr. Eoin<br />

Carley, a Trinity College Dublin (TCD) solar physicist who is currently<br />

an Irish Research Council Marie Skłodowska-Curie Fellow based at<br />

the prestigious Paris Observatory. These solar storms arise, he says,<br />

because the sun, as well as radiating light and heat, has also been<br />

found to discharge huge eruptions of hot gas, which can hurtle<br />

billions of tons of matter in the direction of the earth. In the 156<br />

years since the Carrington event, these solar storms have been<br />

keenly observed, as have their effects, in the form of radio-wave<br />

disruptions, on the earth. Until relatively recently, however, what<br />

eluded scientists was a fundamental understanding of how these<br />

explosions on the sun were created.

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