Solar Flares Explained: What You Need to Know

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Solar Flares Explained: What You Need to Know
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On May 13, 2013, an X2.8-class flare erupted from the sun -- the strongest flare of 2013 to date. This NASA image shows a close-up of the flare as seen by the Solar Dynamics Observatory in the 131 angstrom wavelength.

The sun has unleashed two colossal flares since Sunday night, firing off its most powerful eruptions of 2013 in less than a day.

The first flare peaked Sunday (May 12) at 10:17 p.m. EDT (0217 GMT), registering as an X1.7-class eruption. The second flare, which occurred at midday on Monday (May 13), was even stronger, clocking in at X2.8, scientists said.

X-class flares are the most powerful type. Here's a brief rundown on solar flares, their classification and their potential impacts on Earth. [Sun Unleashes Biggest Flares of 2013 (Photos)]

Classifying solar flares

Solar flares occur when a buildup of magnetic energy on the sun is suddenly released. They usually erupt from sunspots, temporary dark and relatively cool patches on our star's surface where the local magnetic field is very strong.

Flares generate a burst of radiation across a wide range of the electromagnetic spectrum. They're often accompanied by coronal mass ejections (CMEs), which hurl enormous clouds of super-heated plasma into space.

Scientists classify strong solar flares into one of three categories: C, M or X (with A and B classes, too, for weaker eruptions). There's a tenfold increase in power from one class to the next, so an X flare is 10 times stronger than an M flare, and 100 times more powerful than a C.

There's also a finer gradation within each class, from 1 to 9 in the case of C and M flares. But the number goes higher for X flares, because it's the top of the scale and the sun occasionally fires off eruptions more than 10 times stronger than an X-1. For example, in 2003, the sun let loose a flare that registered as an X28 before overwhelming the sensors that measured it. It remains the most powerful solar flare ever recorded.

Effects on Earth

Flares that are C-class and weaker don't affect Earth in any meaningful way. M-class eruptions can generate brief radio blackouts at the poles and minor radiation storms that could endanger orbiting astronauts.

X-class flares, on the other hand, can have consequences on a planet-wide scale, triggering widespread radio blackouts and long-lasting radiation storms.

The CMEs that often accompany solar flares have even more destructive potential. When a CME's charged particles interact with Earth's magnetic field, they can spawn geomagnetic storms powerful enough to disrupt GPS signals, radio communications and power grids.

In March 1989, for example, a CME caused a power blackout in Quebec, leaving 5 million Canadians in the dark in cold weather for hours. The event caused about $2 billion in damages and lost business, scientists say.

We should expect more activity from the sun over the coming months. Solar activity waxes and wanes on an 11-year cycle, and researchers think the current cycle, known as Solar Cycle 24, will peak later this year.

Follow Mike Wall on Twitter @michaeldwall and Google+. Follow us @Spacedotcom, Facebook or Google+. Originally published on SPACE.com.

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